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Extraterrestrial Seismology
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Book description

Seismology is a highly effective tool for investigating the internal structure of the Earth. Similar techniques have also successfully been used to study other planetary bodies (planetary seismology), the Sun (helioseismology), and other stars (asteroseismology). Despite obvious differences between stars and planetary bodies, these disciplines share many similarities and together form a coherent field of scientific research. This unique book takes a transdisciplinary approach to seismology and seismic imaging, reviewing the most recent developments in these extraterrestrial contexts. With contributions from leading scientists, this timely volume systematically outlines the techniques used in observation, data processing, and modelling for asteroseismology, helioseismology, and planetary seismology, drawing comparisons with seismic methods used in geophysics. Important recent discoveries in each discipline are presented. With an emphasis on transcending the traditional boundaries of astronomy, solar, planetary and Earth sciences, this novel book is an invaluable resource and reference for undergraduates, postgraduates and academics.


'… extensive, interesting, and useful… This is the most widely embracing discussion of the subject between two covers, and can be useful to anyone involved in extraterrestrial seismology who wishes to improve their expertise by extending the arena of their knowledge beyond their own subdiscipline.'

Douglas Gough Source: The Observatory

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Abramowicz, M. A., and Fragile, P. C. 2013. Foundations of black hole accretion disk theory. Living Rev. Relativity, 16(Jan.), 1.
Acevedo-Arreguin, L. A., Garaud, P., and Wood, T. S. 2013. Dynamics of the solar tachocline: III. Numerical solutions of the Gough and McIntyre model. MNRAS, 434(Sept.), 720–741.
Aerts, C. 2013. Asteroseismology of binary stars and a compilation of core overshoot and rotational frequency values of OB stars. Pages 323–330 of Pavlovski, K., Tkachenko, A., and Torres, G. (eds), Setting a New Standard in the Analysis of Binary Stars. EAS Publications Series, vol. 64.
Aerts, C., Thoul, A., Daszyńska, J., et al. 2003. Asteroseismology of HD 129929: Core overshooting and nonrigid rotation. Science, 300(June), 1926–1928.
Aerts, C., Christensen-Dalsgaard, J., and Kurtz, D. W. 2010. Asteroseismology. Springer.
Afanasiev, M. V., Pratt, G., Kamei, R., and McDowell, G. 2014. Waveform-based simulated annealing of crosshole transmission data: A semi-global method for estimating seismic anisotropy. Geophys. J. Int., 193(3), 1586–1607.
Ahmad, Q. R., Allen, R. C., Andersen, T. C., et al. 2002. Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory. Phys. Rev. Lett., 89(1), 011301.
Aizenman, M., Smeyers, P., and Weigert, A. 1977. Avoided crossing of modes of non-radial stellar oscillations. A&A, 58(June), 41.
Aki, K., and Chouet, B. 1975. Origin of coda waves: Source, attenuation, and scattering effects. J. Geophys. Res., 80, 3322–3342.
Aki, K., and Richards, P. G. 2002. Quantitative Seismology, 2nd edn, Sausalito, CA: University Science Books.
Allain, S. 1998. Modelling the angular momentum evolution of low-mass stars with coreenvelope decoupling. A&A, 333(May), 629–643.
Allred, J. C., Hawley, S. L., Abbett, W. P., and Carlsson, M. 2005. Radiative hydrodynamic models of the optical and ultraviolet emission from solar flares. ApJ, 630(Sept.), 573–586.
Alterman, Z., and Karal, F. 1968. Propagation of elastic waves in layered media by finite difference methods. Bull. Seism. Soc. Am., 58, 367–398.
Alvan, L., Mathis, S., and Decressin, T. 2013. Coupling between internal waves and shearinduced turbulence in stellar radiation zones: The critical layers. A&A, 553(May), A86.
Alvan, L., Brun, A. S., and Mathis, S. 2014. Theoretical seismology in 3D: Nonlinear simulations of internal gravity waves in solar-like stars. A&A, 565(May), A42.
Andersen, J. 1991. Accurate masses and radii of normal stars. A&A Rev., 3, 91–126.
Anderson, D. L. 1972. Internal constitution of Mars. J. Geophys. Res., 77, 789–795.
Anderson, D. L., Miller, W. F., Latham, G. V., et al. 1977. Seismology on Mars. J. Geophys. Res., 82(Sept.), 4524–1546.
Anderson, E. R., Duvall, Jr., T. L., and Jefferies, S. M. 1990. Modeling of solar oscillation power spectra. ApJ, 364(Dec.), 699–705.
Ando, H., and Osaki, Y. 1975. Nonadiabatic nonradial oscillations: An application to the five-minute oscillation of the sun. PASJ, 27, 581–603.
Ando, H., Watanabe, E., Yutani, M., Shimizu, Y., and Nishimura, S. 1988. Search for small-amplitude oscillations in stars by a Fabry-Perot interferometer. PASJ, 40, 249–262.
Antia, H. M., and Basu, S. 1994. Nonasymptotic helioseismic inversion for solar structure. A&AS, 107(Nov.), 421–144.
Antia, H. M., and Basu, S. 2000. Temporal variations of the rotation rate in the solar interior. ApJ, 541(Sept.), 442–448.
Antia, H. M., and Basu, S. 2005. The discrepancy between solar abundances and helioseismology. ApJ, 620(Feb.), L129–L132.
Antia, H. M., and Chitre, S. M. 1999. Limits on the proton-proton reaction cross-section from helioseismology. A&A, 347(July), 1000–1004.
Antia, H. M., Basu, S., and Chitre, S. M. 1998. Solar internal rotation rate and the latitudinal variation of the tachocline. MNRAS, 298(Aug.), 543–556.
Antia, H. M., Basu, S., Hill, F., et al. 2001. Solar-cycle variation of the sound-speed asphericity from GONG and MDI data1995–2000. MNRAS, 327(Nov.), 1029–1040.
Antia, H. M., Chitre, S. M., and Thompson, M. J. 2003. On variation of the latitudinal structure of the solar convection zone. A&A, 399(Feb.), 329–336.
Apollo 11 Mission Report 1969. NASA Manned Spacecraft Center MSC-00171, Houston, Texas.
Apollo 16 Mission Report 1972. NASA Manned Spacecraft Center MSC-07230, Houston, Texas.
Appourchaux, T. 2014. A crash course on data analysis in asteroseismology. In Palle, P. (ed), Asteroseismology. Canary Islands Winter School of Astrophysics, vol. 22. Cambridge: Cambridge University Press.
Appourchaux, T., Catala, C., Catalano, S., et al. 1991. PRISMA: Probing Rotation and Interior of Stars. Microvariability and activity, Assessment study report. In Appourchaux, T. (ed), SCI(91)5.
Appourchaux, T., Catala, C., Cornelisse, J., et al. 1993. PRISMA: Probing Rotation and Interior of Stars. Microvariability and activity. In Appourchaux, T. (ed), Phase-A study report, SCI(93)3, European Space Agency.
Appourchaux, T., Toutain, T., Telljohann, U., et al. 1995. Frequencies and splittings of low-degree solar p modes: results of the Luminosity Oscillations Imager. A&A, 294, L13–L16.
Appourchaux, T., Andersen, B. N., Frohlich, C., et al. 1997. In-flight performance of the Virgo Luminosity Oscillations Imager aboard SOHO. Sol. Phys., 170, 27–41.
Appourchaux, T., Michel, E., Auvergne, M., et al. 2008. CoRoT sounds the stars: P-mode parameters of Sun-like oscillations on HD 49933. A&A, 488(Sept.), 705–714.
Appourchaux, T., Belkacem, K., Broomhall, A.-M., et al. 2010. The quest for the solar g modes. A&A Rev., 18(Feb.), 197–277.
Appourchaux, T., Chaplin, W. J., García, R. A., et al. 2012a. Oscillation mode frequencies of 61 main-sequence and subgiant stars observed by Kepler. A&A, 543(July), A54.
Appourchaux, T., Benomar, O., Gruberbauer, M., et al. 2012b. Oscillation mode linewidths of main-sequence and subgiant stars observed by Kepler. A&A, 537(Jan.), A134.
Araki, H. 2001. Focal processes of deep moonquakes. J. Geod. Soc. Jpn., 47(1), 508–513.
Araki, H., Tazawa, S., Node, H., et al. 2009. Lunar global shape and polar topography derived from Kaguya-LALT laser altimetry. Science, 323, 897–900.
Arentoft, T., Kjeldsen, H., Bedding, T. R., et al. 2008. A multisite campaign to measure solar-like oscillations in Procyon. I. Observations, data reduction, and slow variations. ApJ, 687(Nov.), 1180–1190.
Artru, J., Farges, T., and Lognonné, P. 2004. Acoustic waves generated from seismic surface waves: Propagation properties determined from Doppler sounding observation and normal-modes modeling. Geophys. J. Int., 158, 1067–1077.
Asplund, M., Grevesse, N., and Sauval, A. J. 2005 (Sept.). The solar chemical composition. Page 25 of Barnes, III, T. G., and Bash, F. N. (eds), Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis. Astronomical Society of the Pacific Conference Series, vol. 336.
Asplund, M., Grevesse, N., Sauval, A. J., and Scott, P. 2009. The chemical composition of the Sun. ARA&A, 47(Sept.), 481–522.
Bachmann, K. T., and Brown, T. M. 1993. P-mode frequency variation in relation to global solar activity. ApJ, 411(July), L45–L48.
Bachmann, K. T., Duvall, Jr., T. L., Harvey, J. W., and Hill, F. 1995. Frequencies of high degree solar oscillations. Page 156 of Ulrich, R. K., Rhodes, Jr., E. J., and Dappen, W. (eds), GONG 1994. Helio- and Astro-Seismology from the Earth and Space. Astronomical Society of the Pacific Conference Series, vol. 76.
Baer, J. J. 2010. Development of an observational error model, and astrometric masses of 28 asteroids. Ph.D. thesis, James Cook University, Australia.
Baglin, A., Weiss, W. W., and Bisnovatyi-Kogan, G. 1993 (Jan.). E. V. R. I. S on board MARS 94: the first space experiment devoted to stellar seismology. Page 758 of Weiss, W. W., and Baglin, A. (eds), IAU Colloqium 137: Inside the Stars. Astronomical Society of the Pacific Conference Series, vol. 40.
Baglin, A., Auvergne, M., Barge, P., et al. 2009 (Feb.). CoRoT: Description of the mission and early results. Pages 71–81 of Pont, F., Sasselov, D., and Holman, M. J. (eds), Transiting Planets. IAU Symposium, S253.
Baglin, A., Michel, E., and CoRoT Team. 2012 (Sept.). CoRoT: A few highlights and their impacts on understanding internal stellar structure. Page 492 of Shibahashi, H., Takata, M., and Lynas-Gray, A. E. (eds), Progress in Solar/Stellar Physics with Helio- and Asteroseismology. Astronomical Society of the Pacific Conference Series, vol. 462.
Bahcall, J. N., Pinsonneault, M. H., Basu, S., and Christensen-Dalsgaard, J. 1997. Are standard solar models reliable?Phys. Rev. Lett., 78(Jan.), 171–174.
Bahcall, J. N., Basu, S., and Pinsonneault, M. H. 1998. How uncertain are solar neutrino predictions?Phys. Lett. B, 433, 1–8.
Bahcall, J. N., Basu, S., Pinsonneault, M., and Serenelli, A. M. 2005a. Helioseismological implications of recent solar abundance determinations. ApJ, 618(Jan.), 1049–1056.
Bahcall, J. N., Basu, S., and Serenelli, A. M. 2005b. What is the neon abundance of the Sun?ApJ, 631(Oct.), 1281–1285.
Bahcall, J. N., Serenelli, A. M., and Basu, S. 2006. 10,000 standard solar models: A Monte Carlo simulation. ApJS, 165(July), 400–431.
Baldner, C. S., and Basu, S. 2008. Solar cycle related changes at the base of the convection zone. ApJ, 686(Oct.), 1349–1361.
Baldner, C. S., and Schou, J. 2012. Effects of asymmetric flows in solar convection on oscillation modes. ApJ, 760(Nov.), L1.
Ballot, J., Turck-Chièze, S., and García, R. A. 2004. Seismic extraction of the convective extent in solar-like stars: The observational point of view. A&A, 423(Sept.), 1051–1061.
Ballot, J., García, R. A., and Lambert, P. 2006. Rotation speed and stellar axis inclination from p modes: How CoRoT would see other suns. MNRAS, 369(July), 1281–1286.
Ballot, J., Lignières, F., Reese, D. R., and Rieutord, M. 2010. Gravity modes in rapidly rotating stars: Limits of perturbative methods. A&A, 518(July), A30.
Ballot, J., Lignières, F., Prat, V., Reese, D. R., and Rieutord, M. 2012 (Sept.). 2D computations of g-modes in fast rotating stars. Page 389 of Shibahashi, H., Takata, M., and Lynas-Gray, A. E. (eds), Progress in Solar/Stellar Physics with Helio- andAsteroseis-mology. Astronomical Society of the Pacific Conference Series, vol. 462.
Ballot, J., Lignières, F., and Reese, D. R. 2013. Numerical exploration of oscillation modes in rapidly rotating stars. Page 91 of Goupil, M., Belkacem, K., Neiner, C., Lignières, F., and Green, J. J. (eds), Studying Stellar Rotation and Convection. Lecture Notes in Physics, Berlin: Springer Verlag, vol. 865.
Balmforth, N. J. 1992a. Solar pulsational stability. Part Three: Acoustical excitation by turbulent convection. MNRAS, 255(Apr.), 639–649.
Balmforth, N. J. 1992b. Solar pulsational stability. I: Pulsation-mode thermodynamics. MNRAS, 255(Apr.), 603–631.
Bamberger, A., Chavent, G., Hemon, Ch., and Lailly, P. 1982. Inversion of normal incidence seismograms. Geophysics, 47, 757–770.
Banerdt, W. B, Chui, T., Griggs, C. E., et al. 2007. Using the Moon as a low-noise seismic detector for strange quark nuggets. Nucl. Phys. B Proc. Suppl., 166, 203–208.
Banerdt, W. B., Smrekar, S., Alkalai, L., et al. 2012. InSight: An Integrated Exploration of the Interior of Mars, 43rd Lunar and Planetary Science Conference, March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659.
Barban, C., De Ridder, J., Mazumdar, A., et al. 2004a. Detection of solar-like oscillations in two red giant stars. Page 113 of Danesy, D. (ed), SOHO 14 Helio- and Asteroseis-mology: Towards a Golden Future. ESA Special Publication, vol. 559.
Barban, C., Hill, F., and Kras, S. 2004b. Simultaneous velocity-intensity spectral and cross-spectral fitting of helioseismic data. ApJ, 602(Feb.), 516–527.
Barban, C., Matthews, J. M., De Ridder, J., et al. 2007. Detection of solar-like oscillations in the red giant star ε Ophiuchi by MOST spacebased photometry. A&A, 468(June), 1033–1038.
Barnes, S. A. 2003. On the rotational evolution of solar- and late-type stars, its magnetic origins, and the possibility of stellar gyrochronology. ApJ, 586(Mar.), 464–479.
Bass, H. E., and Chambers, J. P. 2001. Absorption of sound in the Martian atmosphere. J. Acoust. Soc. Am., 109, 3069–3071.
Bates, J. R., Lauderdale, W. W., and Kernaghan, H. 1979. ALSEP Termination Report, NASA reference Publication 1036, NASA Scientific and Technical Information Office.
Bastien, F. A., Stassun, K. G., Basri, G., and Pepper, J. 2013. An observational correlation between stellar brightness variations and surface gravity. Nature, 500(Aug.), 427–430.
Basu, S. 2003. Stellar inversions. Ap&SS, 284, 153–164.
Basu, S., and Antia, H. M. 1995. Helium abundance in the solar envelope. MNRAS, 276(Oct.), 1402–1408.
Basu, S., and Antia, H. M. 1997. Seismic measurement of the depth of the solar convection zone. MNRAS, 287(May), 189–198.
Basu, S., and Antia, H. M. 1999. Large-scale flows in the solar interior: Effect of asymmetry in peak profiles. ApJ, 525(Nov.), 517–523.
Basu, S., and Antia, H. M. 2000. Effect of asymmetry in peak profiles on solar oscillation frequencies. ApJ, 531(Mar.), 1088–1093.
Basu, S., and Antia, H. M. 2004. Constraining solar abundances using helioseismology. ApJ, 606(May), L85–L88.
Basu, S., and Antia, H. M. 2008. Helioseismology and solar abundances. Phys. Rep., 457(Mar.), 217–283.
Basu, S., and Antia, H. M. 2010. Characteristics of solar meridional flows during solar cycle 23. ApJ, 717(July), 488–495.
Basu, S., and Christensen-Dalsgaard, J. 1997. Equation of state and helioseismic inversions. A&A, 322(June), L5–L8.
Basu, S., Antia, H. M., and Narasimha, D. 1994. Helioseismic measurement of the extent of overshoot below the solar convection zone. MNRAS, 267(Mar.), 209.
Basu, S., Christensen-Dalsgaard, J., Chaplin, W. J., et al. 1997. Solar internal sound speed as inferred from combined BiSON and LOWL oscillation frequencies. MNRAS, 292(Dec.), 243.
Basu, S., Däppen, W., and Nayfonov, A. 1999a. Helioseismic analysis of the hydrogen partition function in the solar interior. ApJ, 518(June), 985–993.
Basu, S., Antia, H. M., and Tripathy, S. C. 1999b. Ring diagram analysis of near-surface flows in the Sun. ApJ, 512(Feb.), 458–170.
Basu, S., Pinsonneault, M. H., and Bahcall, J. N. 2000. How much do helioseismological inferences depend on the assumed reference model?ApJ, 529(Feb.), 1084–1100.
Basu, S., Christensen-Dalsgaard, J., and Thompson, M. J. 2002 (Jan.). SOLA inversions for the core structure of solar-type stars. Pages 249–252 of Battrick, B., Favata, F., Roxburgh, I. W., and Galadi, D. (eds), Stellar Structure and Habitable Planet Finding. ESA Special Publication, vol. 485.
Basu, S., Antia, H. M., and Bogart, R. S. 2004. Ring-diagram analysis of the structure of solar active regions. ApJ, 610(Aug.), 1157–1168.
Basu, S., Chaplin, W. J., Elsworth, Y., New, R., and Serenelli, A. M. 2009. Fresh insights on the structure of the solar core. ApJ, 699(July), 1403–1417.
Basu, S., Chaplin, W. J., and Elsworth, Y. 2010. Determination of stellar radii from asteroseismic data. ApJ, 710(Feb.), 1596–1609.
Basu, S., Grundahl, F., Stello, D., et al. 2011. Sounding open clusters: Asteroseismic constraints from Kepler on the properties of NGC 6791 and NGC 6819.ApJ, 729(Mar.), L10.
Basu, S., Broomhall, A.-M., Chaplin, W. J., and Elsworth, Y. 2012. Thinning of the Sun's magnetic layer: The peculiar solar minimum could have been predicted. ApJ, 758(Oct.), 43.
Batalha, N. M., Borucki, W. J., Bryson, S. T., et al. 2011. Kepler's first rocky planet: Kepler-10b. ApJ, 729(Mar.), 27–48.
Baturin, V. A., Däppen, W., Gough, D. O., and Vorontsov, S. V. 2000. Seismology of the solar envelope: Sound-speed gradient in the convection zone and its diagnosis of the equation of state. MNRAS, 316(July), 71–83.
Baudin, F., Barban, C., Belkacem, K., et al. 2011. Amplitudes and lifetimes of solarlike oscillations observed by CoRoT. Red-giant versus main-sequence stars. A&A, 529(May), A84.
Bazot, M., Bourguignon, S., and Christensen-Dalsgaard, J. 2012. A Bayesian approach to the modelling of α Cen A. MNRAS, 427(Dec.), 1847–1866.
Beauduin, R., Lognonnei, P., Montagner, J. P., Cacho, S., Karczewski, J. F. and Morand, M. 1996. The effect of the atmospheric pressure changes on seismic signals or how to improve the quality of a station. Bull. Seismol. Soc. Am., 86, 1760–1769.
Beck, C., Fabbian, D., Moreno-Insertis, F., Puschmann, K. G., and Rezaei, R. 2013. Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations. A&A, 557(Sept.), A109.
Beck, P. G., Bedding, T. R., Mosser, B., et al. 2011. Kepler detected gravity-mode period spacings in a red giant star. Science, 332(Apr.), 205.
Beck, P. G., Montalban, J., Kallinger, T., et al. 2012. Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes. Nature, 481(Jan.), 55–57.
Bedding, T. R. 2014. Solar-like oscillations: An observational perspective. Pages 60–86 in Palle, P. and Esteban, C. (eds), Asteroseismology. Canary Islands Winter School of Astrophysics, vol. 22. Cambridge: Cambridge University Press.
Bedding, T. R., Kjeldsen, H., Bouchy, F., et al. 2005. The non-detection of oscillations in Procyon by MOST: Is it really a surprise?A&A, 432(Mar.), L43–L48.
Bedding, T. R., Kjeldsen, H., Arentoft, T., et al. 2007. Solar-like oscillations in the G2 subgiant β Hydri from dual-site observations. ApJ, 663(July), 1315–1324.
Bedding, T. R., Kjeldsen, H., Campante, T. L., et al. 2010a. A multi-site campaign to measure solar-like oscillations in Procyon. II. Mode frequencies. ApJ, 713(Apr.), 935–949.
Bedding, T. R., Huber, D., Stello, D., et al. 2010b. Solar-like oscillations in low-luminosity red giants: First results from Kepler. ApJ, 713(Apr.), L176–L181.
Bedding, T. R., Mosser, B., Huber, D., et al. 2011. Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars. Nature, 471(Mar.), 608–611.
Behrend, R., Bernasconi, L., and Roy, R., et al. 2006. Four new binary minor planets: (854) Frostia, (1089) Tama, (1313) Berna, (4492) Debussy. A&A, 446(Feb.), 1177–1184.
Belkacem, K., Goupil, M. J., Dupret, M. A., et al. 2011. The underlying physical meaning of the vmax–vc relation. A&A, 530(June), A142.
Belkacem, K., Dupret, M. A., Baudin, F., et al. 2012. Damping rates of solar-like oscillations across the HR diagram: Theoretical calculations confronted to CoRoT and Kepler observations. A&A, 540(Apr.), L7.
Belkacem, K., Samadi, R., Mosser, B., Goupil, M.-J., and Ludwig, H.-G. 2013. On the seismic scaling relations Δv-p and vmax-vc. Page 61 of Shibahashi, H., and Lynas-Gray, A. E. (eds), Progress in Physics ofthe Sun and Stars: A New Era in Helio- and Asteroseismology. Astronomical Society of the Pacific Conference Series, vol. 479.
Belloche, A., Schuller, F., Parise, B., et al. 2011. The end of star formation in Chamaeleon I? A LABOCA census of starless and protostellar cores. A&A, 527(Mar.), A145.
Bellot Rubio, L. R. 2010. The Evershed flow and the brightness of the penumbra. Page 193 of Hasan, S. S., and Rutten, R. J. (eds), Magnetic Coupling between the Interior and Atmosphere ofthe Sun. Springer Astrophysics and Space Science Proceedings.
Belmonte, J. A., Jones, A. R., Palle, P. L., and Roca Cortes, T. 1990a. Acoustic oscillations in the K2 III star Arcturus. Ap&SS, 169(July), 77–84.
Belmonte, J. A., Pérez Hernández, F., and Roca Cortés, T. 1990b. Detection of acoustic oscillations in the F2 V star HD 155543. A&A, 231(May), 383–390.
Belmonte, J. A., Jones, A. R., Palle, P. L., and Roca Cortés, T. 1990c. Global acoustic oscillations on Alpha Bootis. ApJ, 358(Aug.), 595–609.
Ben-Menahem, A. 1975. Source parameters of the Siberian explosion of June 30, 1908, from analysis and synthesis of seismic signal at four stations. Phys. Earth Planet. Inter., 11, 1–35.
Benomar, O., Appourchaux, T., and Baudin, F. 2009. The solar-like oscillations of HD 49933: A Bayesian approach. A&A, 506(Oct.), 15–32.
Bercovici, D., and Schubert, G. 1987. Jovian seismology. Icarus, 69(Mar.), 557–565.
Berthomieu, G., Gonczi, G., Graff, P., Provost, J., and Rocca, A. 1978. Low-frequency gravity modes of a rotating star. A&A, 70(Nov.), 597.
Bills, B. G., and Ferrari, A. J. 1977. A lunar density model consistent with topographic, gravitational, librational, and seismic data. J. Geophys. Res., 82, 1306–1314.
Birch, A. C., and Kosovichev, A. G. 2000. Travel time sensitivity kernels. Sol. Phys., 192(Mar.), 193–201.
Birch, A. C., Kosovichev, A. G., Price, G. H., and Schlottmann, R. B. 2001. The accuracy of the Born and ray approximations in time-distance helioseismology. ApJ, 561(Nov.), L229–L232.
Birch, A. C., Kosovichev, A. G., and Duvall, Jr., T. L. 2004. Sensitivity of acoustic wave travel times to sound-speed perturbations in the solar interior. ApJ, 608(June), 580600.
Birch, A. C., Gizon, L., Hindman, B. W., and Haber, D. A. 2007. The linear sensitivity of helioseismic ring diagrams to local flows. ApJ, 662(June), 730–737.
Birch, A. C., Braun, D. C., and Fan, Y. 2010. An estimate of the detectability of rising flux tubes. ApJ, 723(Nov.), L190–L194.
Bogdan, T. J. 1997. A comment on the relationship between the modal and time-distance formulations of local helioseismology. ApJ, 477(Mar.), 475–484.
Bogdan, T. J., and Cally, P. S. 1995. Jacket modes: Solar acoustic oscillations confined to regions surrounding sunspots and plage. ApJ, 453(Nov.), 919.
Böhm-Vitense, E. 1958. Uber die Wasserstoffkonvektionszone in Sternen verschiedener Effektivtemperaturen und Leuchtkräfte. Mit 5 Textabbildungen. ZAp, 46, 108.
Böhm-Vitense, E. 2007. Chromospheric activity in G and K main-sequence stars, and what it tells us about stellar dynamos. ApJ, 657(Mar.), 486–493.
Bonet, J. A., Márquez, I., Sánchez Almeida, J., Cabello, I., and Domingo, V. 2008. Convectively driven vortex flows in the Sun. ApJ, 687(Nov.), L131–L134.
Bonet, J. A., Márquez, I., Sánchez Almeida, J., et al. 2010. SUNRISE/IMaX observations of convectively driven vortex flows in the Sun.ApJ, 723(Nov.), L139–L143.
Borucki, W. J., Koch, D., Basri, G., et al. 2010. Kepler planet-detection mission: Introduction and first results. Science, 327(Feb.), 977–980.
Bouchy, F., and Carrier, F. 2001. P-mode observations on α Cen A.A&A, 374(July), L5–L8.
Bouchy, F., and Carrier, F. 2002. The acoustic spectrum of alpha Cen A.A&A, 390(July), 205–212.
Bouchy, F., Pepe, F., and Queloz, D. 2001. Fundamental photon noise limit to radial velocity measurements. A&A, 374(Aug.), 733–739.
Bouvier, J. 2013 (Sept.). Observational studies of stellar rotation. Pages 143–168 of Role and Mechanisms of Angular Momentum Transport During the Formation and Early Evolution of Stars. EAS Publications Series, vol. 62.
Bouvier, J., Forestini, M., and Allain, S. 1997. The angular momentum evolution of low-mass stars. A&A, 326(Oct.), 1023–1043.
Bozdag, E., Trampert, J., and Tromp, J. 2011. Misfit functions for full waveform inversion based on instantaneous phase and envelope measurements. Geophys. J. Int., 185, 845–870.
Braithwaite, J. 2006. A differential rotation driven dynamo in a stably stratified star. A&A, 449(Apr.), 451–160.
Braithwaite, J. 2008. On non-axisymmetric magnetic equilibria in stars. MNRAS, 386(June), 1947–1958.
Braithwaite, J., and Spruit, H. C. 2004. A fossil origin for the magnetic field in A stars and white dwarfs. Nature, 431(Oct.), 819–821.
Brandão, I. M., Cunha, M. S., and Christensen-Dalsgaard, J. 2014. On the inference of stellar ages and convective-core properties in main-sequence solar-like pulsators. MNRAS, 438(Feb.), 1751–1761.
Brandenburg, A., Jennings, R. L., Nordlund, Å., et al. 1996. Magnetic structures in a dynamo simulation. J. Fluid Mech., 306(Jan.), 325–352.
Brandt, P. N., Scharmer, G. B., Ferguson, S., Shine, R. A., and Tarbell, T. D. 1988. Vortex flow in the solar photosphere. Nature, 335(Sept.), 238–240.
Braun, D. C. 1995. Scattering of p-modes by sunspots: I. Observations. ApJ, 451(Oct.), 859.
Braun, D. C., and Birch, A. C. 2008. Surface-focused seismic holography of sunspots: I. Observations. Sol. Phys., 251, 267–289.
Braun, D. C., Duvall, Jr., T. L., and Labonte, B. J. 1987. Acoustic absorption by sunspots. ApJ, 319(Aug.), L27–L31.
Braun, D. C., Duvall, Jr., T. L., and Labonte, B. J. 1988. The absorption of high-degree p-mode oscillations in and around sunspots. ApJ, 335(Dec.), 1015–1025.
Braun, D. C., Lindsey, C., Fan, Y., and Jefferies, S. M. 1992. Local acoustic diagnostics of the solar interior. ApJ, 392(June), 739–745.
Braun, D. C., Birch, A. C., Rempel, M., and Duvall, T. L. 2012. Helioseismology of a realistic magnetoconvective sunspot simulation. ApJ, 744(Jan.), 77.
Breger, M. 1993. Accuracy in variable-star work: The three-star single channel technique. Butler, C. J., and Elliott, I. (eds), Stellar Photometry: Current Techniques and Future Developments. IAU Colloquium 136.
Breger, M., Stich, J., Garrido, R., et al. 1993. Nonradial pulsation of the delta-Scuti star Bu-Cancri in the Praesepe cluster. A&A, 271(Apr.), 482.
Brenguier, F., Shapiro, N. M., Campillo, M., Nercessian, A., and Ferrazzini, V. 2007. 3-D surface wave tomography of the Piton de la Fournaise volcano using seismic noise correlations. Geophys. Res. Lett., 34(Jan.), 2305.
Brillouin, L. 1960. Wave Propagation and Group Velocity. New York: Academic Press.
Britt, D. T., Yeomans, D., Housen, K., and Consolmagno, G. 2002. Asteroid density, porosity, and structure. Asteroids III, 485–500.
Brogi, M., Snellen, I. A. G., de Kok, R. J., et al. 2012. The signature of orbital motion from the dayside of the planet τ Boötis b. Nature, 486(June), 502–504.
Brookes, J. R., Isaak, G. R., and van der Raay, H. B. 1978. A resonant-scattering solar spectrometer. MNRAS, 185(Oct.), 1–18.
Broomhall, A.-M., Salabert, D., Chaplin, W. J., et al. 2012a. Misleading variations in estimated rotational frequency splittings of solar p modes: Consequences for helioseismology and asteroseismology. MNRAS, 422(June), 3564–3573.
Broomhall, A.-M., Chaplin, W. J., Elsworth, Y., and Simoniello, R. 2012b. Quasi-biennial variations in helioseismic frequencies: Can the source of the variation be localized?MNRAS, 420(Feb.), 1405–1414.
Brossier, R., Operto, S., and Virieux, J. 2009. Robust elastic frequency-domain fullwaveform inversion using the L-1 norm. Geophys. Res. Lett., 36, L20310.
Brown, P., Spalding, R. E., ReVelle, D. O., Tagliaferri, E., and Worden, S. P. 2002. The flux of small near-Earth objects colliding with the Earth. Nature, 420, 294–296.
Brown, T. 1981. The Fourier tachometer: Principles of operation and current status. Page 150 of Dunn, R. B. (ed), Solar Instrumentation: What's Next?Sunspot, NM: Sacramento Peak National Observatory.
Brown, T. M. 1985. Solar rotation as a function of depth and latitude. Nature, 317(Oct.), 591–594.
Brown, T. M., and Christensen-Dalsgaard, J. 1990. A technique for estimating complicated power spectra from time series with gaps. ApJ, 349(Feb.), 667–674.
Brown, T. M., Gilliland, R. L., Noyes, R. W., and Ramsey, L. W. 1991. Detection of possible p-mode oscillations on Procyon. ApJ, 368(Feb.), 599–609.
Brown, T. M., Kennelly, E. J., Korzennik, S. G., et al. 1997. A radial velocity search for p-mode pulsations in eta Bootis. ApJ, 475(Jan.), 322.
Brown, T. M., Latham, D. W., Everett, M. E., and Esquerdo, G. A. 2011. Kepler Input Catalog: Photometric calibration and stellar classification. AJ, 142(Oct.), 112.
Browning, M. K., Miesch, M. S., Brun, A. S., and Toomre, J. 2006. Dynamo action in the solar convection zone and tachocline: Pumping and organization of toroidal fields. ApJ, 648(Sept.), L157–L160.
Brummell, N. H., Hurlburt, N. E., and Toomre, J. 1998. Turbulent compressible convection with rotation: II. Mean flows and differential rotation. ApJ, 493(Jan.), 955.
Brun, A. S. 2004. On the interaction between differential rotation and magnetic fields in the Sun. Sol. Phys., 220(Apr.), 333–345.
Brun, A. S., and Toomre, J. 2002. Turbulent convection under the influence of rotation: Sustaining a strong differential rotation. ApJ, 570(May), 865–885.
Brun, A. S., and Zahn, J.-P. 2006. Magnetic confinement of the solar tachocline. A&A, 457(Oct.), 665–674.
Brun, A. S., Turck-Chièze, S., and Zahn, J. P. 1999. Standard solar models in the light of new helioseismic constraints: II. Mixing below the convective zone. ApJ, 525(Nov.), 1032–1041.
Brun, A. S., Miesch, M. S., and Toomre, J. 2004. Global-scale turbulent convection and magnetic dynamo action in the solar envelope. ApJ, 614(Oct.), 1073–1098.
Brun, A. S., Miesch, M. S., and Toomre, J. 2011. Modeling the dynamical coupling of solar convection with the radiative interior. ApJ, 742(Dec.), 79.
Brun, A. S., Browning, M. K., Dikpati, M., Hotta, H., and Strugarek, A. 2013. Recent advances on solar global magnetism and variability. Space Sci. Rev., Nov, doi:10.1007/ s11214-013-0028-0.
Bruntt, H., Kjeldsen, H., Buzasi, D. L., and Bedding, T. R. 2005. Evidence for granulation and oscillations in Procyon from photometry with the WIRE satellite. ApJ, 633(Nov.), 440–446.
Bulow, R. C., Johnson, C. L., and Shearer, P. M. 2005. New events discovered in the Apollo lunar seismic data. J. Geophys. Res., 110, E10003, doi:10.1029/2005JE002414.
Bulow, R. C., Johnson, C. L., Bills, B. G., and Shearer, P. M. 2007. Temporal and spatial properties of some deep moonquake clusters. J. Geophys. Res., 112, E09003, doi:10.1029/2006JE002847.
Buzasi, D. L. 2000 (Apr.). Experiment design and data reduction for seismology: Lessons learned from WIRE. Page 9 of Teixeira, T., and Bedding, T. (eds), The Third MONS Workshop: Science Preparation and Target Selection.
Buzasi, D., Catanzarite, J., Laher, R., et al. 2000. The detection of multimodal oscillations on α Ursae Majoris. ApJ, 532(Apr.), L133–L136.
Buzasi, D. L., Bruntt, H., Preston, H. L., and Clausen, J. V. 2004 (Dec.). High precision photometry with WIRE: Converting spectroscopic binaries to eclipsing systems. Bull. AAS, 36, 1369.
Cacciani, A., and Fofi, M. 1978. The magneto-optical filter: II. Velocity field measurements. Sol. Phys., 59(Sept.), 179–189.
Cacciani, A., Dolci, M., Moretti, P. F., et al. 2001. Search for global oscillations on Jupiter with a double-cell sodium magneto-optical filter. A&A, 372(June), 317–325.
Cacciani, A., Jefferies, S. M., Finsterle, W., et al. 2003 (Feb.). A new instrument for sounding the solar atmosphere. Pages 243–245 of Sawaya-Lacoste, H. (ed), GONG+ 2002. Local and Global Helioseismology: the Present and Future. ESA Special Publication, vol. 517.
Caffau, E., Ludwig, H.-G., Steffen, M., Freytag, B., and Bonifacio, P. 2011. Solar chemical abundances determined with a CO5BOLD 3D model atmosphere. Sol. Phys., 268(Feb.), 255–269.
Callen, H. B., and Welton, T. A. 1951. Irreversibility and generalized noise. Phys. Rev., 83, 34–40.
Cally, P. S., and Bogdan, T. J. 1993. Solar p-modes in a vertical magnetic field: Trapped and damped pi-modes. ApJ, 402(Jan.), 721–732.
Cally, P. S., Crouch, A. D., and Braun, D. C. 2003. Probing sunspot magnetic fields with p-mode absorption and phase shift data. MNRAS, 346(Dec.), 381–389.
Cameron, R., Schüssler, M., Vögler, A., and Zakharov, V. 2007. Radiative magnetohydrodynamic simulations of solar pores. A&A, 474(Oct.), 261–272.
Cammarano, F., Lekic, V., Manga, M., Panning, M., and Romanowicz, B. 2006. Longperiod seismology on Europa: 1. Physically consistent interior models. J. Geophys. Res. (Planets), 111(10), 12009.
Campante, T. L., Handberg, R., Mathur, S., et al. 2011. Asteroseismology from multi-month Kepler photometry: The evolved Sun-like stars KIC 10273246 and KIC 10920273.A&A, 534(Oct.), A6.
Canuto, V. M., and Mazzitelli, I. 1991. Stellar turbulent convection: A new model and applications. ApJ, 370(Mar.), 295–311.
Carlsson, M. 1998. Radiative transfer and radiation hydrodynamics. Page 163 of Vial, J. C., Bocchialini, K., and Boumier, P. (eds), Space Solar Physics: Theoretical and Observational Issues in the Context ofthe SOHO Mission. Lecture Notes in Physics, Berlin: Springer Verlag, vol. 507.
Carpenter, K. G., Schrijver, C. J., and Karovska, M. 2009. The Stellar Imager (SI) project: A deep space UV/optical interferometer (UVOI) to observe the Universe at 0.1 milli-arcsec angular resolution. Ap&SS, 320(Apr.), 217–223.
Carpenter, K. G., Schrijver, C. J., Karovska, M., et al. 2010. Stellar Imager (SI): Developing and testing a predictive dynamo model for the Sun by imaging other stars. ArXiv:1011.5214.
Carrier, F., and Bourban, G. 2003. The acoustic spectrum of alpha Cen B. A&A, 406(July), L23.
Carrier, F., Eggenberger, P., and Bouchy, F. 2005. New seismological results on the G0 IV η Bootis. A&A, 434(May), 1085–1095.
Catala, C. 2009. PLATO: PLAnetary Transits and Oscillations of stars. Exp. Astron., 23(Mar.), 329–356.
Catala, C., Mangeney, A., Gautier, D., et al. 1995. COROT: A proposal to study stellar convection and internal rotation. Page 426 of Ulrich, R. K., Rhodes, Jr., E. J., and Dappen, W. (eds), GONG 1994: Helio- and Astro-Seismology from the Earth and Space. Astronomical Society of the Pacific Conference Series, vol. 76.
Ceillier, T., Eggenberger, P., García, R. A., and Mathis, S. 2013. Understanding angular momentum transport in red giants: The case of KIC 7341231.A&A, 555(July), A54.
Červený, V. 1985. The application of ray tracing to the numerical modeling of seismic wavefields in complex structures. Pages 1–124 of Dohr, G. P. (ed), Handbook of Geophysical Exploration, vol. 15A. London: Geophysical Press.
Chaboyer, B., Demarque, P., and Pinsonneault, M. H. 1995. Stellar models with microscopic diffusion and rotational mixing: 1. Application to the Sun. ApJ, 441(Mar.), 865–875.
Chakrabarti, S. K., and Manickam, S. G. 2000. Correlation among quasi-periodic oscillation frequencies and quiescent-state duration in black hole candidate GRS 1915+105. ApJ, 531(Mar.), L41–L44.
Chandrasekhar, S. 1964. A general variational principle governing the radial and the nonradial oscillations of gaseous masses. ApJ, 139(Feb.), 664.
Chaplin, W. J. 2006. Music of the Sun: Story of Helioseismology. London: Oneworld Publications.
Chaplin, W. J., and Miglio, A. 2013. Asteroseismology of solar-type and red-giant stars. ARA&A, 51, 353–392.
Chaplin, W. J., Elsworth, Y., Howe, R., et al. 1996. BiSON performance. Sol. Phys., 168(Sept.), 1–18.
Chaplin, W. J., Elsworth, Y., Isaak, G. R., et al. 1997a. Solar p-mode linewidths from recent BiSON helioseismological data. MNRAS, 288(July), 623–626.
Chaplin, W. J., Elsworth, Y., Howe, R., et al. 1997b. Techniques used in the analysis of data collected by the Birmingham Solar-Oscillations Network (BiSON): II. Frequency domain analysis and data merging. A&AS, 125(Oct.), 195–205.
Chaplin, W. J., Christensen-Dalsgaard, J., Elsworth, Y., et al. 1999. Rotation of the solar core from BiSON and LOWL frequency observations. MNRAS, 308(Sept.), 405–414.
Chaplin, W. J., Elsworth, Y., Isaak, G. R., Miller, B. A., and New, R. 2000. Variations in the excitation and damping of low-l solar p modes over the solar activity cycle. MNRAS, 313(Mar.), 32–42.
Chaplin, W. J., Elsworth, Y., Isaak, G. R., et al. 2001. Changes to low-l solar p-mode frequencies over the solar cycle: Correlations on different time-scales. MNRAS, 322(Mar.), 22–30.
Chaplin, W. J., Sekii, T., Elsworth, Y., and Gough, D. O. 2004. On the detectability of a rotation-rate gradient in the solar core. MNRAS, 355(Dec.), 535–542.
Chaplin, W. J., Appourchaux, T., Baudin, F., et al. 2006. Solar FLAG hare and hounds: On the extraction of rotational p-mode splittings from seismic, Sun-as-a-star data. MNRAS, 369(June), 985–996.
Chaplin, W. J., Appourchaux, T., Arentoft, T., et al. 2008. AsteroFLAG: First results from hare-and-hounds Exercise #1. Astron. Nachr., 329, 549.
Chaplin, W. J., Houdek, G., Karoff, C., Elsworth, Y., and New, R. 2009. Mode lifetimes of stellar oscillations: Implications for asteroseismology. A&A, 500(June), L21–L24.
Chaplin, W. J., Kjeldsen, H., Christensen-Dalsgaard, J., et al. 2011a. Ensemble asteroseismology of solar-type stars with the NASA Kepler mission. Science, 332(Apr.), 213–216.
Chaplin, W. J., Kjeldsen, H., Bedding, T. R., et al. 2011b. Predicting the detectability of oscillations in solar-type stars observed by Kepler. ApJ, 732(May), 54.
Chaplin, W. J., Sanchis-Ojeda, R., Campante, T. L., et al. 2013a. Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65. ApJ, 766(Apr.), 101.
Chaplin, W. J, Kjeldsen, H., Christensen-Dalsgaard, J., et al. 2013b. Kepler white paper: Asteroseismology of solar-like oscillators in a 2-wheel mission. ArXiv:1309.0702.
Chaplin, W. J., Basu, S., Huber, D., et al. 2014. Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler mission. ApJS, 210(Jan.), 1.
Charbonneau, P. 2010. Dynamo models of the solar cycle. Living Rev. Solar Phys., 7(Sept.), 3.
Charbonneau, P., and MacGregor, K. B. 1993. Angular momentum transport in magnetized stellar radiative zones. II. The solar spin-down. ApJ, 417(Nov.), 762.
Charbonneau, P., Christensen-Dalsgaard, J., Henning, R., et al. 1999. Helioseismic constraints on the structure of the solar tachocline. ApJ, 527(Dec.), 445–460.
Charbonnel, C., and Talon, S. 2005. Influence of gravity waves on the internal rotation and Li abundance of solar-type stars. Science, 309(Sept.), 2189–2191.
Chaty, S. 2007. The role of microquasars in astroparticle physics. Page 329 of Giovannelli, F., and Mannocchi, G. (eds), Vulcano Workshop: Frontier Objects in Astrophysics and Particle Physics.
Chaty, S. 2013. Optical/infrared observations unveiling the formation, nature and evolution of high-mass X-ray binaries. Adv. Space Res., 52(Dec.), 2132–2142.
Chen, P., Jordan, T. H., and Zhao, L. 2007. Full three-dimensional tomography: A comparison between the scattering-integral and adjoint-wavefield methods. Geophys. J. Int., 170, 175–181.
Chenet, H., Lognonné, Ph., Wieczorek, M., and Mizutani, H. 2006. Lateral variations of lunar crustal thickness from the Apollo seismic data set. Earth Planet. Sci. Lett., 243, 1–14.
Cheng, C. H., and Toksoz, M. N. 1978. Tidal stresses in the Moon. J. Geophys. Res., 83(Feb.), 845–853.
Cheung, M. C. M., Sdnussler, M., Tarbell, T. D., and Title, A. M. 2008. Solar surface emerging flux regions: A comparative study of radiative MHD modeling and Hinode SOT observations. ApJ, 687(Nov.), 1373–1387.
Chou, D.-Y., and Dai, D.-C. 2001. Solar cycle variations of subsurface meridional flows in the Sun. ApJ, 559(Oct.), L175–L178.
Chou, D.-Y., Sun, M.-T., Huang, T.-Y., et al. 1995. Taiwan Oscillation Network. Sol. Phys., 160(Sept.), 237–243.
Chou, D.-Y., Yang, M.-H., Liang, Z.-C., and Sun, M.-T. 2009a. Measurements of absorption of acoustic waves in sunspots with direction filters and cross correlation. ApJ, 690(Jan.), L23–L26.
Chou, D.-Y., Yang, M.-H., Zhao, H., Liang, Z.-C., and Sun, M.-T. 2009b. Spatial distributions of absorption, local suppression, and emissivity reduction of solar acoustic waves in magnetic regions. ApJ, 706(Nov.), 909–916.
Chicarro, A. F. 2013. INSPIRE: A future European Mars Network Science Mission. 44th Lunar and Planetary Science Conference, March 18–22. 2013 in The Woodlands, Texas. LPI Contribution No. 1719.
Christensen, E. M., Batterson, S. A., Benson, H. E., et al. 1968. Lunar Surface Mechanical Properties. Pages 44-108 of Surveyor VI Mission Report, Part II: Science Results, Jet Propulsion Laboratory, Technical Report 32–1262, Pasadena.
Christensen-Dalsgaard, J. 1984. What will asteroseismology teach us? Page 11 of Mangeney, A., and Praderie, F. (eds), Space Research in Stellar Activity and Variability. Observatoire de Paris-Meudon.
Christensen-Dalsgaard, J. 1989. The effect of rotation on whole-disc Doppler observations of solar oscillations. MNRAS, 239(Aug.), 977–994.
Christensen-Dalsgaard, J. 1993. On the asteroseismic HR diagram. Page 347 of Brown, T. M. (ed), GONG 1992: Seismic Investigation of the Sun and Stars. Astronomical Society of the Pacific Conference Series, vol. 42.
Christensen-Dalsgaard, J. 2002. Helioseismology. Rev. Mod. Phys., 74(Nov.), 1073–1129.
Christensen-Dalsgaard, J. 2004. Physics of solar-like oscillations. Sol. Phys., 220(Apr.), 137–168.
Christensen-Dalsgaard, J. 2012. Stellar model fits and inversions. Astron. Nachr., 333(Dec.), 914.
Christensen-Dalsgaard, J., and Di Mauro, M. P. 2007. Diffusion and helioseismology. Pages 3–16 of Straka, C. W., Lebreton, Y., and Monteiro, M. J. P. F. G. (eds), Stellar Evolution and Seismic Tools for Asteroseismology. EAS Publications Series, vol. 26.
Christensen-Dalsgaard, J., and Frandsen, S. 1983. Stellar 5 min oscillations. Sol. Phys., 82(Jan.), 469–486.
Christensen-Dalsgaard, J., and Gough, D. 0.1976. Towards aheliological inverse problem. Nature, 259(Jan.), 89–92.
Christensen-Dalsgaard, J., and Gough, D. O. 1982. On the interpretation of five-minute oscillations in solar spectrum line shifts. MNRAS, 198(Jan.), 141–171.
Christensen-Dalsgaard, J., and Schou, J. 1988 (Dec.). Differential rotation in the solar interior. Pages 149–153 of Rolfe, E. J. (ed), Seismology of the Sun and Sun-Like Stars. ESA Special Publication, vol. 286.
Christensen-Dalsgaard, J., and Thompson, M. J. 1997. On solar p-mode frequency shifts caused by near-surface model changes. MNRAS, 284(Jan.), 527–540.
Christensen-Dalsgaard, J., Duvall, Jr., T. L.Gough, D. O., Harvey, J. W., and Rhodes, Jr., E. J. 1985. Speed of sound in the solar interior. Nature, 315(May), 378–382.
Christensen-Dalsgaard, J., Thompson, M. J., and Gough, D. O. 1989. Differential asymptotic sound-speed inversions. MNRAS, 238(May), 481–502.
Christensen-Dalsgaard, J., Gough, D. O., and Thompson, M. J. 1991. The depth of the solar convection zone. ApJ, 378(Sept.), 413–137.
Christensen-Dalsgaard, J., Dappen, W., Ajukov, S. V., et al. 1996. The current state of solar modeling. Science, 272(May), 1286–1292.
Christensen-Dalsgaard, J., Kjeldsen, H., and Mattei, J. A. 2001. Solar-like oscillations of semiregular variables. ApJ, 562(Dec.), L141–L144.
Christensen-Dalsgaard, J., di Mauro, M. P., Houdek, G., and Pijpers, F. 2009. On the opacity change required to compensate for the revised solar composition. A&A, 494(Jan.), 205–208.
Christensen-Dalsgaard, J., Monteiro, M. J. P. F. G., Rempel, M., and Thompson, M. J. 2011. A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology. MNRAS, 414(June), 1158–1174.
Claret, A., and Giménez, A. 2010. The apsidal-motion test of stellar structure and evolution: An update. A&A, 519(Sept.), A57.
Claverie, A., Isaak, G. R., McLeod, C. P., van der Raay, H. B., and Cortes, T. R. 1979. Solar structure from global studies of the 5-minute oscillation. Nature, 282(Dec.), 591–594.
Clement, M. J. 1984. Normal modes of oscillation for rotating stars: II. Variational solutions. ApJ, 276(Jan.), 724–736.
Cobden, L. J., Tong, C. H., and Warner, M. R. 2010. Influence of acoustic source density on cross-correlated signals: Implications for amplitude-based tomography in helio-seismology. ApJ, 725, 313–318.
Cobden, L. J., Tong, C. H., and Warner, M. R. 2011. Inversion of full acoustic wavefield in local helioseismology: A study with synthetic data. ApJ, 727, 68.
Coleiro, A., and Chaty, S. 2013. Distribution of high-mass X-ray binaries in the Milky Way. ApJ, 764(Feb.), 185.
Connes, P. 1985. Absolute astronomical accelerometry. Ap&SS, 110(Mar.), 211–255.
Cooley, J. W., and Tukey, J. W. 1965. An algorithm for the machine calculation of complex Fourier series. Math. Comput., 19 297–301.
Cooper, M. R., Kovach, R. L., and Watkins, J. S. 1974. Lunar near-surface structure. Rev. Geophys. Space Phys., 12, 291–308.
Cooper, M. R., and Kovach, R. L. 1975. Energy, frequency, and distance of moonquakes at the Apollo 17 site. Proceedings of the 6th Lunar Science Conference, 2863–2879.
Corsaro, E., Stello, D., Huber, D., et al. 2012. Asteroseismology of the open clusters NGC 6791, NGC 6811, and NGC 6819 from 19 months of Kepler photometry. ApJ, 757(Oct.), 190.
Costa, J. E. S., and Kepler, S. O. 2008. The temporal changes of the pulsational periods of the pre-white dwarf PG 1159–035. A&A, 489(Oct.), 1225–1232.
Couvidat, S., and Birch, A. C. 2006. Optimal Gaussian phase-speed filters in time-distance helioseismology. Sol. Phys., 237(Sept.), 229–243.
Couvidat, S., García, R. A., Turck-Chieze, S., et al. 2003. The rotation of the deep solar layers. ApJ, 597(Nov.), L77–L79.
Couvidat, S., Birch, A. C., Kosovichev, A. G., and Zhao, J. 2004. Three-dimensional inversion of time-distance helioseismology data: Ray-path and Fresnel-zone approximations. ApJ, 607(May), 554–563.
Couvidat, S., Zhao, J., Birch, A. C., et al. 2012a. Implementation and comparison of acoustic travel-time measurement procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager time-distance helioseismology pipeline. Sol. Phys., 275(Jan.), 357–374.
Couvidat, S., Schou, J., Shine, R. A., et al. 2012b. Wavelength dependence of the Helioseis-mic and Magnetic Imager (HMI) instrument onboard the Solar Dynamics Observatory (SDO). Sol. Phys., 275(Jan.), 285–325.
Covas, E., Moss, D., and Tavakol, R. 2005. Dynamo models and differential rotation in late-type rapidly rotating stars. A&A, 429(Jan.), 657–665.
Cowling, T. G., and Newing, R. A. 1949. The oscillations of a rotating star. ApJ, 109(Jan.), 149.
Cranmer, S. R., Bastien, F. A., Stassun, K. G., and Saar, S. H. 2014. Stellar granulation as the source of high-frequency flicker in Kepler light curves. ApJ, 781(Feb.), 124.
Crawford, Jr., F. S. 1968. Waves. New York: McGraw-Hill Book Company.
Creevey, O. L., Monteiro, M. J. P. F. G., Metcalfe, T. S., et al. 2007. The complementary roles of interferometry and asteroseismology in determining the mass of solar-type stars. ApJ, 659(Apr.), 616–625.
Criswell, D. R., and Lindsay, J. F. 1974. Thermal moonquakes and booming dunes (abstract). Lunar Science V, 151–153.
Crouch, A. D., Cally, P. S., Charbonneau, P., Braun, D. C., and Desjardins, M. 2005. Genetic magnetohelioseismology with Hankel analysis data. MNRAS, 363(Nov.), 11881204.
Crouch, A. D., Birch, A. C., Braun, D. C., and Clack, C. T. M. 2011. Helioseismic probing of the subsurface structure of sunspots. Pages 384–388 of Choudhary, D. P., and Strassmeier, K. G. (eds), Physics of Sun and Star Spots. IAU Symposium273.
Cunha, M. S., and Metcalfe, T. S. 2007. Asteroseismic signatures of small convective cores. ApJ, 666(Sept.), 413–122.
Cunha, M. S., Aerts, C., Christensen-Dalsgaard, J., et al. 2007. Asteroseismology and interferometry. A&A Rev., 14(Nov.), 217–360.
Dahlen, F. A., and Tromp, J. 1998. Theoretical Global Seismology. Princeton: Princeton University Press.
Dainty, A. M., and M. N., Toksoz 1981. Seismic codas on the Earth and the Moon: A comparison. Phys. Earth Planet. Inter., 26 250–260.
Dainty, A. M., Toksöz, M. N., Anderson, K. R., et al. 1974. Seismic scattering and shallow structure of the Moon in Oceanus Procellarum. The Moon, 9, 11–29.
Daubar, I. J., McEwen, A. S., Byrne, S., Kennedy, M. R., and Ivanov, B. 2013. The current martian cratering rate. Icarus, 225(July), 506–516.
Davis, P. M. 1993. Meteoroid impacts as seismic sources on Mars. Icarus, 105, 469–478.
De Oliveira Fialho, F. 2007. Définition et impléementation des corrections instrumentales de la mission spatiale CoRoT. Ph.D. thesis, Université Pierre et Marie Curie, Paris, France.
De Ridder, J., Barban, C., Carrier, F., et al. 2006. Discovery of solar-like oscillations in the red giant ε Ophiuchi. A&A, 448(Mar.), 689–695.
De Ridder, J., Barban, C., Baudin, F., et al. 2009. Non-radial oscillation modes with long lifetimes in giant stars. Nature, 459(May), 398–400.
Decressin, T., Mathis, S., Palacios, A., et al. 2009. Diagnoses to unravel secular hydrodynamical processes in rotating main sequence stars. A&A, 495(Feb.), 271–286.
Degroote, P., Briquet, M., Auvergne, M., et al. 2010. Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry. A&A, 519(Sept.), A38.
Deheuvels, S., and Michel, E. 2011. Constraints on the structure of the core of subgiants via mixed modes: The case of HD 49385. A&A, 535(Nov.), A91.
Deheuvels, S., Bruntt, H., Michel, E., et al. 2010. Seismic and spectroscopic characterization of the solar-like pulsating CoRoT target HD 49385. A&A, 515(June), A87.
Deheuvels, S., García, R. A., Chaplin, W. J., et al. 2012. Seismic evidence for a rapidly rotating core in a lower-giant-branch star observed with Kepler. ApJ, 756(Sept.), 19.
Deheuvels, S., Doğan, G., Goupil, M. J., et al. 2014. Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants. A&A, 564(Apr.), A27.
Delahunty, A. K., and Pike, W. T. 2013. Metal-armouring for shock protection of MEMS. Sensors and Actuators, 215, 36–43.
Deming, D., Mumma, M. J., Espenak, F., et al. 1989. A search for p-mode oscillations of Jupiter: Serendipitous observations of nonacoustic thermal wave structure. ApJ, 343(Aug.), 456–467.
Denissenkov, P. A., Pinsonneault, M., Terndrup, D. M., and Newsham, G. 2010. Angular momentum transport in solar-type stars: Testing the timescale for core-envelope coupling. ApJ, 716(June), 1269–1287.
Derr, J. S. 1969. Free oscillations of new lunar models. Phys. Earth Planet. Inter., 2, 61–68.
Deubner, F.-L. 1975. Observations of low wavenumber nonradial eigenmodes of the Sun. A&A, 44(Nov.), 371–375.
Deupree, R. G. 2011. Structure of uniformly rotating stars. ApJ, 735(July), 69.
Dikpati, M., and Charbonneau, P. 1999. A Babcock–Leighton flux transport dynamo with solar-like differential rotation. ApJ, 518(June), 508–520.
Dikpati, M., and Gilman, P. A. 2006. Simulating and predicting solar cycles using a flux-transport dynamo. ApJ, 649(Sept.), 498–514.
Dintrans, B., and Rieutord, M. 2000. Oscillations of a rotating star: A non-perturbative theory. A&A, 354(Feb.), 86–98.
Dintrans, B., Brandenburg, A., Nordlund, A., and Stein, R. F. 2005. Spectrum and amplitudes of internal gravity waves excited by penetrative convection in solar-type stars. A&A, 438(July), 365–376.
Domingo, V., Fleck, B., and Poland, A. I. 1995. The SOHO mission: An overview. Sol. Phys., 162, 1–37.
Donati, J.-F., and Landstreet, J. D. 2009. Magnetic fields of nondegenerate stars. ARA&A, 47(Sept.), 333–370.
Donea, A. 2011. Seismic transients from flares in solar cycle 23. Space Sci. Rev., 158(July), 451–169.
Donea, A.-C., and Lindsey, C. 2005. Seismic emission from the solar flares of 2003 October 28 and 29. ApJ, 630(Sept.), 1168–1183.
Donea, A. C., Lindsey, C., and Braun, D. 1999. Helioseismic holography: A technique for understanding solar flares. Romanian Astron. J., 9, 71.
Dorman, J., Evans, S., Nakamura, Y., and Latham, G. 1978. On the time-varying properties of the lunar seismic meteoroid population. Proceedings of the 9th Lunar and Planetary Science Conference, 3615–3626.
Doschek, G. A., Warren, H. P., and Young, P. R. 2013. Chromospheric evaporation in an M1.8 flare observed by the Extreme-ultraviolet Imaging Spectrometer on Hinode. ApJ, 767(Apr.), 55.
Drummond, R., Vandenbussche, B., Aerts, C., De Oliveira Fialho, F., and Auvergne, M. 2006. Jitter correction algorithms for the COROT satellite mission. PASP, 118(June), 874.
Dubus, G., Hameury, J.-M., and Lasota, J.-P. 2001. The disc instability model for X-ray transients: Evidence for truncation and irradiation. A&A, 373(July), 251271.
Duennebier, F. 1976. Thermal movement of the regolith. Proceedings of the 7th Lunar Science Conference, 1073–1086.
Duennebier, F., and Sutton, G.H. 1974. Thermal moonquakes. J. Geophys. Res., 79(29), 4351–4363.
Duennebier, F., Dorman, J., Lammlein, D., Latham, G., and Nakamura, Y. 1975. Meteoroid flux from passive seismic experiment data. Proceedings of the 6th Lunar Science Conference, 2417–2426.
Duennebier, F. K., Nakamura, Y, Latham, G. V., and Dorman, H. J. 1976. Meteoroid storms detected on the Moon. Science, 192, 1000–1002.
Duez, V., and Mathis, S. 2010. Relaxed equilibrium configurations to model fossil fields: I. A first family. A&A, 517(July), A58.
Duez, V., Braithwaite, J., and Mathis, S. 2010. On the stability of non-force-free magnetic equilibria in stars. ApJ, 724(Nov.), L34–L38.
Dupret, M.-A., Thoul, A., Scuflaire, R., et al. 2004. Asteroseismology of the β Cep star HD 129929: II. Seismic constraints on core overshooting, internal rotation and stellar parameters. A&A, 415(Feb.), 251–257.
Dupret, M.-A., Belkacem, K., Samadi, R., et al. 2009. Theoretical amplitudes and lifetimes of non-radial solar-like oscillations in red giants. A&A, 506(Oct.), 57–67.
Duvall, Jr., T. L. 1982. A dispersion law for solar oscillations. Nature, 300(Nov.), 242.
Duvall, Jr., T. L., and Birch, A. C. 2010. The vertical component of the supergranular motion. ApJ, 725(Dec.), L47–L51.
Duvall, T. L., and Hanasoge, S. M. 2013. Subsurface supergranular vertical flows as measured using large distance separations in time-distance helioseismology. Sol. Phys., 287(Oct.), 71–83.
Duvall, Jr., T. L., and Harvey, J. W. 1983. Observations of solar oscillations of low and intermediate degree. Nature, 302(Mar.), 24–27.
Duvall, Jr., T. L., Dziembowski, W. A., Goode, P. R., et al. 1984. Internal rotation of the sun. Nature, 310(July), 22–25.
Duvall,Jr., T. L., Harvey, J. W., and Pomerantz, M. A. 1986. Latitude and depth variation of solar rotation. Nature, 321(May), 500.
Duvall, Jr., T. L., Jefferies, S. M., Harvey, J. W., Osaki, Y., and Pomerantz, M. A. 1993a. Asymmetries of solar oscillation line profiles. ApJ, 410(June), 829–836.
Duvall, Jr., T. L., Jefferies, S. M., Harvey, J. W., and Pomerantz, M. A. 1993b. Time-distance helioseismology. Nature, 362(Apr.), 430–432.
Duvall, T. L., D'Silva, S., Jefferies, S. M., Harvey, J. W., and Schou, J. 1996. Downflows under sunspots detected by helioseismic tomography. Nature, 379(Jan.), 235–237.
Duvall, Jr., T. L., Kosovichev, A. G., Scherrer, P. H., et al. 1997. Time-distance helioseismology with the MDI instrument: Initial results. Sol. Phys., 170, 63–73.
Dziembowski, W., and Kosovichev, A. 1987. Low frequency oscillations in slowly rotating stars: I. General properties. Acta Astronomica, 37, 313.
Dziembowski, W. A. 1977. Light and radial velocity variations in a nonradially oscillating star. Acta Astron., 27, 203–211.
Dziembowski, W. A., and Goode, P. R. 1992. Effects of differential rotation on stellar oscillations: A second-order theory. ApJ, 394(Aug.), 670–687.
Dziembowski, W. A., and Pamyatnykh, A. A. 1991. A potential asteroseismological test for convective overshooting theories. A&A, 248(Aug.), L11–L14.
Dziembowski, W. A., and Pamyatnykh, A. A. 2008. The two hybrid B-type pulsators: ν Eridani and 12 Lacertae. MNRAS, 385(Apr.), 2061–2068.
Dziembowski, W. A., Goode, P. R., and Libbrecht, K. G. 1989. The radial gradient in the Sun's rotation. ApJ, 337(Feb.), L53–L57.
Dziembowski, W. A., Pamyatnykh, A. A., and Sienkiewicz, R. 1990. Solar model from helioseismology and the neutrino flux problem. MNRAS, 244(June), 542–550.
Dziewonski, A. M., and Anderson, D. L. 1981. Preliminary reference Earth model. Phys. Earth Planet. Inter., 25(June), 297–356.
Dziewonski, A. M., Hager, B. H., and O'Connell, R. J. 1977. Large-scale heterogeneities in the lower mantle. J. Geophys. Res., 82(Jan.), 239–255.
Eckart, C. 1960. Hydrodynamics of Oceans and Atmospheres. New York: Pergamon.
Eddington, A. S. 1925. Circulating currents in rotating stars. The Observatory, 48(Mar.), 73–75.
Edmonds, P. D., and Cram, L. E. 1995. A search for global acoustic oscillations on a1 Cen and α1 and β Hyi. MNRAS, 276(Oct.), 1295.
Edwards, W. N. 2008. Meteor generated infrasound: Theory and observation. Pages 355408 of Le Pichon, A. (ed), Infrasound Monitoring for Atmospheric Studies. New York: Springer.
Edwards, W. N., Eaton, D. W., and Brown, P. G. 2008. Seismic observations of meteors: Coupling theory and observations, Rev. Geophys. 46, RG4007.
Eff-Darwich, A., and Korzennik, S. G. 2013. The dynamics of the solar radiative zone. Sol. Phys., 287(Oct.), 43–56.
Eggenberger, P., Miglio, A., Montalban, J., et al. 2010. Effects of rotation on the evolution and asteroseismic properties of red giants. A&A, 509(Jan.), A72.
Eggenberger, P., Montalbán, J., and Miglio, A. 2012a. Angular momentum transport in stellar interiors constrained by rotational splittings of mixed modes in red giants. A&A, 544(Aug.), L4.
Eggenberger, P., Haemmerlé, L., Meynet, G., and Maeder, A. 2012b. Impact of rotation and disc lifetime on pre-main sequence lithium depletion of solar-type stars. A&A, 539(Mar.), A70.
Elliott, J. R., and Kosovichev, A. G. 1998. The adiabatic exponent in the solar core. ApJ, 500(June), L199–L202.
Elsworth, Y., Howe, R., Isaak, G. R., McLeod, C. P., and New, R. 1990. Evidence from solar seismology against non-standard solar-core models. Nature, 347(Oct.), 536–539.
Endal, A. S., and Sofia, S. 1978. The evolution of rotating stars: II. Calculations with time-dependent redistribution of angular momentum for 7- and 10-solar-mass stars. ApJ, 220(Feb.), 279–290.
Epstein, C. R., and Pinsonneault, M. H. 2014. How good a clock is rotation? The stellar rotation-mass-age relationship for old field stars. ApJ, 780(Jan.), 159.
Espinosa Lara, F., and Rieutord, M. 2013. Self-consistent 2D models of fast-rotating earlytype stars. A&A, 552(Apr.), A35.
Ewing, M., Latham, G., Press, F., et al. 1971. Seismology of the Moon and implications on internal structure, origin and evolution. Pages 155–172 of de Jager, C. (ed), Highlights of Astronomy. Dordrecht: D. Reidel.
Eyer, L., and Mowlavi, N. 2008. Variable stars across the observational HR diagram. J. Phys. Conf. Ser., 118(1), 012010.
Eyer, L., Holl, B., Pourbaix, D., et al. 2013. The Gaia Mission. Central Eur. Astrophys. Bull., 37, 115–126.
Fan, Y., Braun, D. C., and Chou, D.-Y. 1995. Scattering of p-modes by sunspots: II. Calculations of phase shifts from a phenomenological model. ApJ, 451(Oct.), 877.
Fares, R., Donati, J.-F., Moutou, C., et al. 2009. Magnetic cycles of the planet-hosting star τ Bootis: II. A second magnetic polarity reversal. MNRAS, 398(Sept.), 1383–1391.
Favata, F. 2004 (Jan.). The Eddington baseline mission. Pages 3-11 of Favata, F., Aigrain, S., and Wilson, A. (eds), Stellar Structure and Habitable Planet Finding. ESA Special Publication, vol. 538.
Favre, A. 1969. In Statistical equations of turbulent gases, Problems of Hydrodynamics and Continuum Mechanics, Society for Industrial and Applied Mathematics.
Featherstone, N. A., Hindman, B. W., and Thompson, M. J. 2011. Ring-analysis flow measurements of sunspot outflows. J. Phys. Conf. Ser., 271(1), 012002.
Feigelson, E. D., and Montmerle, T. 1999. High-energy processes in young stellar objects. ARA&A, 37, 363–408.
Felipe, T., Braun, D., Crouch, A., and Birch, A. 2012. Scattering of the f-mode by small magnetic flux elements from observations and numerical simulations. ApJ, 757(Oct.), 148.
Fernandes, J., and Monteiro, M. J. P. F. G. 2003. HR diagram and asteroseismic analysis of models for beta Hydri. A&A, 399(Feb.), 243–251.
Fichtner, A., and Trampert, J. 2011. Resolution analysis in full waveform inversion. Geophys. J. Int., 187, 1604–1624.
Fichtner, A., Bunge, H.-P., and Igel, H. 2006. The adjoint method in seismology. Phys. Earth Planet. Inter., 157, 86–104.
Fichtner, A., Kennett, B. L. N., Igel, H., and Bunge, H.-P. 2008. Theoretical background for continental- and global-scale full-waveform inversion in the time-frequency domain. Geophys. J. Int., 175, 665–685.
Fichtner, A., Kennett, B. L. N., Igel, H., and Bunge, H.-P. 2009. Full seismic waveform tomography for upper-mantle structure in the Australasian region using adjoint methods. Geophys. J. Int., 179, 1703–1725.
Fichtner, A., Trampert, J., Cupillard, P., et al. 2013. Multiscale full waveform inversion. Geophys. J. Int., 194, 534–556.
Fisher, G. H., Canfield, R. C., and McClymont, A. N. 1985. Flare loop radiative hydrodynamics: VII. Dynamics of the thick target heated chromosphere. ApJ, 289(Feb.), 434.
Fleming, W. P. 1895. Stars having peculiar spectra: Eleven new variable stars. ApJ, 1(May), 411–415.
Fletcher, S. T., Chaplin, W. J., Elsworth, Y., and New, R. 2009. Efficient pseudo-global fitting for helioseismic data. ApJ, 694(Mar.), 144–150.
Foglizzo, T., García, R. A., Boumier, P., et al. 1998. Are solar acoustic modes correlated?A&A, 330(Feb.), 341–350.
Fogtmann-Schulz, A., Hinrup, B., Van Eylen, V., et al. 2014. Accurate parameters of the oldest known rocky-exoplanet hosting system: Kepler-10 revisited. ApJ, 781(Feb.), 67.
Forbriger, T., Widmer-Schnidrig, R., Wielandt, E., Hayman, M., and Ackerley, N. 2010. Magnetic field background variations can limit the resolution of seismic broad-band sensors. Geophys. J. Int., 183, 303–312.
Forgács-Dajka, E., and Petrovay, K. 2002. Dynamics of the fast solar tachocline: I. Dipolar field. A&A, 389(July), 629–640.
Fortney, J. J., and Nettelmann, N. 2010. The interior structure, composition, and evolution of giant planets. Space Sci. Rev., 152(May), 423–447.
Fossat, E. 1991. The IRIS network for full disk helioseismology: Present status of the programme. Sol. Phys., 133(May), 1–12.
Frandsen, S. 1987. An upper limit on p-mode amplitudes in Beta Hyi. A&A, 181(July), 289–292.
Frandsen, S., Carrier, F., Aerts, C., et al. 2002. Detection of solar-like oscillations in the G7 giant star xi Hya. A&A, 394(Oct.), L5–L8.
Frankel, A., and Clayton, R. W. 1986. Finite difference simulations of seismic scattering: Implications for the propagation of short-period seismic waves in the crust and models of crustal heterogeneity. J. Geophys. Res., 91(May), 6465–6489.
French, S. W., Lekic, V., and Romanowicz, B. 2013. Waveform tomography reveals channeled flow at the base of the oceanic asthenosphere. Science, 334, 783–787.
Fridlund, M., Gough, D. O., Jones, A., et al. 1995. STARS: A proposal for a dedicated space mission to study stellar structure and evolution. Page 416 of Ulrich, R. K., Rhodes, Jr., E. J., and Dappen, W. (eds), GONG 1994: Helio- and Astro-Seismology from the Earth and Space. Astronomical Society of the Pacific Conference Series, vol. 76.
Frohlich, C., and Nakamura, Y. 2006. Possible extra-solar-system cause for certain lunar seismic events. Icarus, 185, 21–28.
Fröhlich, C., and Nakamura, Y. 2009. The physical mechnisms of deep moonquakes and intermediate-depth earthquakes: How similar and how different?Phys. Earth Planet. Inter., 173, 365–374.
Fröhlich, C., Romero, J., Roth, H., et al. 1995. VIRGO: Experiment for helioseismology and solar irradiance monitoring. Sol. Phys., 162, 101–128.
Fröhlich, C., Crommelynck, D. A., Wehrli, C., et al. 1997. In-flight performance of the Virgo solar irradiance instruments on SOHO. Sol. Phys., 175(Oct.), 267–286.
Fröhlich, H.-E., Frasca, A., Catanzaro, G., et al. 2012. Magnetic activity and differential rotation in the young Sun-like stars KIC 7985370 and KIC 7765135. A&A, 543(July), A146.
Fujiwara, A., Kawaguchi, J., D. K., Yeomans, et al. 2006. The rubble-pile asteroid Itokawa as observed by Hayabusa. Science, 312, 1330–1334.
Fuller, J., Lai, D., and Storch, N. I. 2014. Non-radial oscillations in rotating giant planets with solid cores: Application to Saturn and its rings. Icarus, 231(Mar.), 34–50.
Gabriel, A. H., Grec, G., Charra, J., et al. 1995. Global oscillations at low frequency from the SOHO mission (GOLF). Sol. Phys., 162, 61–99.
Gabriel, A. H., Charra, J., Grec, G., et al. 1997. Performance and early results from the GOLF instrument flown on the SOHO mission. Sol. Phys., 175(Oct.), 207–226.
Gagnepain-Beyneix, J., Lognonné, P., Chenet, H., Lombardi, D., and Spohn, T. 2006. A seismic model of the lunar mantle and constraints on temperature and mineralogy. Phys. Earth Planet. Inter., 159 140–166.
Gangi, A. F., and Yen, T. E. 1979. Velocity structure of the shallow lunar crust. The Moon and The Planets, 20, 439–468.
Gallet, F., and Bouvier, J. 2013. Improved angular momentum evolution model for solar-like stars. A&A, 556(Aug.), A36.
Gandorfer, A., Solanki, S. K., Woch, J., et al. 2011. The Solar Orbiter mission and its Polarimetric and Helioseismic Imager (SO/PHI). J. Phys. Conf. Ser., 271(1), 012086.
García, R. A., Pallé, P. L., Turck-Chièze, S., et al. 1998. High-frequency peaks in the power spectrum of solar velocity observations from the GOLF experiment. ApJ, 504(Sept.), L51.
García, R. A., Corbard, T., Chaplin, W. J., et al. 2004. About the rotation of the solar radiative interior. Sol. Phys., 220(Apr.), 269–285.
Garcia, R., Lognonné, P., and Bonnin, X. 2005. Detecting atmospheric perturbations produced by Venus quakes. Geophys. Res. Lett., 32, L16205.
García, R. A., Turck-Chièze, S., Boumier, P., et al. 2005. Global solar Doppler velocity determination with the GOLF/SOHO instrument. A&A, 442(Oct.), 385–395.
García, R. A., Turck-Chièze, S., Jiménez-Reyes, S. J., et al. 2007. Tracking solar gravity modes: The dynamics of the solar core. Science, 316(June), 1591–1593.
García, R. A., Mathur, S., Ballot, J., et al. 2008a. Influence of low-degree high-order p-mode splittings on the solar rotation profile. Sol. Phys., 251(Sept.), 119–133.
García, R. A., Jiménez, A., Mathur, S., et al. 2008b. Update on g-mode research. Astron. Nachr., 329, 476.
García, R. A., Mathur, S., Salabert, D., et al. 2010. CoRoT reveals a magnetic activity cycle in a Sun-like star. Science, 329(Aug.), 1032.
García, R. A., Salabert, D., Ballot, J., et al. 2011. New insights on the solar core. J. Phys. Conf. Ser., 271(1), 012046.
Garcia, R. F., Gagnepain-Beyneix, J., Chevrot, S., and Lognonné, P. 2011. Very preliminary reference Moon model. Phys. Earth Planet. Inter., 188, 96–113.
Garcia, R. F., Gagnepain-Beyneix, J., Chevrot, S., and Lognonne, P. 2012. Erratum to “Very preliminary reference Moon model” by R. F., Garcia, J., Gagnepain-Beyneix, S., Chevrot, P., Lognonné [Phys. Earth Planet. Inter. 188 (2011) 96–113], Phys. Earth Planet. Inter., 202–203, 89–91.
García, R. A., Ceillier, T., Mathur, S., and Salabert, D. 2013 (Dec.). Measuring reliable surface rotation rates from Kepler photometric observations. Page 129 of Shibahashi, H., and Lynas-Gray, A. E. (eds), Progress in Physics of the Sun and Stars: A New Era in Helio-and Asteroseismology. Astronomical Society of the Pacific Conference Series, vol. 479.
García, R. A., Pérez Hernández, F., Benomar, O., et al. 2014a. Study of KIC 8561221 observed by Kepler: An early red giant showing depressed dipolar modes. A&A, 563(Mar.), A84.
García, R. A., Ceillier, T., Salabert, D., et al. 2014b. Towards asteroseismically calibrated age-rotation-activity relations for Kepler solar-like stars. ArXiv:1403.7155.
Garcia, R. F., Gagnepain-Beyneix, J., Chevrot, S., and Lognonné, P. 2011. Very preliminary reference Moon model. Phys. Earth Planet. Inter., 188(Sept.), 96–113.
Gaskell, R., Saito, J., and Ishiguro, M., et al. 2008. Itokawa Shape Model V1.0. HAY-A-AMICA-5-ITOKAWASHAPE-V1.0. Technical Report NASA Planetary Data System.
Gaulme, P., and Mosser, B. 2005. Coupling of acoustic waves to clouds in the jovian troposphere. Icarus, 178 (Nov.), 84–96.
Gaulme, P., Schmider, F.X., Gay, J., et al. 2008. SYMPA, a dedicated instrument for Jovian seismology: II.Real performance and first results. A&A, 490 (Nov.), 859-871.
Gaulme, P., Schmider, F.-X., Gay, J., Guillot, T., and Jacob, C. 2011. Detection of Jovian seismic waves: A new probe of its interior structure. A&.A, 531 (July), A104.
Gaulme, P., McKeever, J., Rawls, M.L., et al. 2013. Red giants in eclipsing binary and multiple-star systems: Modeling and asteroseismic analysis of 70 candidates from Kepler data. ApJ, 767 (Apr.), 82.
Gauthier, O., Virieux, J., and Tarantola, A. 1986. Two-dimensional nonlinear inversion of seismic wave-forms: Numerical results. Geophysics, 51, 1387–1403.
Gelly, B., Gree, G., and Fossat, E. 1986. Evidence for global pressure oscillations in Procyon and Alpha Centauri. A&A, 164 (Aug.), 383–394.
Georgobiani, D., Kosovichev, A.G., Nigam, R., Nordlund, A., and Stein, R.F. 2000. Numerical simulations of oscillation modes of the solar convection zone. ApJ, 530 (Feb.), L139-L142.
Georgobiani, D., Stein, R.F., and Nordlund, Å. 2003.Asymmetry reversal in solar acoustic modes.Pages 279-282 of Sawaya-Lacoste, H. (ed), GONG+ 2002. Local and Global Helioseismology: The Present and Future. ESA Special Publication, vol.517.
Georgobiani, D., Zhao, J., Kosovichev, A.G., et al. 2007. Local helioseismology and correlation tracking analysis of surface structures in realistic simulations of solar convection. ApJ, 657 (Mar.), 1157–1161.
Germano, M., Piomelli, U., Moin, P., and Cabot, W.H. 1991. A dynamic subgrid-scale eddy viscosity model. Phys.Fluids, 3 (July), 1760–1765.
Giacconi, R., Gursky, H., Paolini, F.R., and Rossi, B.B. 1962. Evidence for X-rays from sources outside the Solar System. Phys.Rev.Lett., 9 (Dec.), 439–443.
Giles, P.M., Duvall, T.L., Scherrer, P.H., and Bogart, R.S. 1997. A subsurface flow of material from the Sun's equator to its poles. Nature, 390 (Nov.), 52–54.
Gilliland, R.L. 2008. Photometric oscillations of low-luminosity red giant stars. AJ, 136 (Aug.), 566–579.
Gilliland, R.L., and Brown, T.M. 1988. Time-resolved CCD photometry of an ensemble of stars. PASP, 100 (June), 754–765.
Gilliland, R.L., and Brown, T.M. 1992. Limits to CCD ensemble photometry precision and prospects for asteroseismology. PASP, 104, 582–591.
Gilliland, R.L., Brown, T.M., Duncan, D.K., et al. 1991. Time-resolved CCD photometry of an ensemble of stars in the open cluster M67. AJ, 101 (Feb.), 541–561.
Gilliland, R.L., Brown, T.M., Kjeldsen, H., et al. 1993. A search for solar-like oscillations in the stars of M67 with CCD ensemble photometry on a network of 4 M telescopes. AJ, 106 (Dec.), 2441–2476.
Gilliland, R.L., Brown, T.M., Christensen-Dalsgaard, J., et al. 2010. Kepler asteroseismology program: Introduction and first results. PASP, 122 (Feb.), 131–143.
Gilman, P.A., and Howe, R. 2003.(Feb.).Meridional motion and the slope of isorotation contours.Pages 283-285 of Sawaya-Lacoste, H. (ed), GONG+ 2002.Local and Global Helioseismology: The Present and Future. ESA Special Publication, vol.517.
Gilman, P.A., Morrow, C.A., and Deluca, E.E. 1989. Angular momentum transport and dynamo action in the Sun: Implications of recent oscillation measurements. ApJ, 338 (Mar.), 528–537.
Gizon, L., and Birch, A.C. 2002. Time-distance helioseismology: The forward problem for random distributed sources. ApJ, 571 (June), 966–986.
Gizon, L., and Birch, A.C. 2004. Time-distance helioseismology: Noise estimation. ApJ, 614 (Oct.), 472–489.
Gizon, L., and Birch, A.C. 2005. Local helioseismology. Living Rev.Sol.Phys., 2 (Nov.), 6.
Gizon, L., and Birch, A.C. 2012. Helioseismology challenges models of solar convection. Proc.Nat.Acad.Sci., 109 (July), 1189–1189.
Gizon, L., and Solanki, S.K. 2003. Determining the inclination of the rotation axis of a Sun-like star. ApJ, 589 (June), 1009–1019.
Gizon, L., Duvall, Jr., T., L., and Larsen, R.M. 2000. Seismic tomography of the near solar surface. J.Astrophys.Astron., 21 (June), 339.
Gizon, L., Duvall, T.L., and Schou, J. 2003. Wave-like properties of solar supergranulation. Nature, 421 (Jan.), 43–44.
Gizon, L., Schunker, H., Baldner, C.S., et al. 2009. Helioseismology of sunspots: A case study of NOAA Region 9787. Space Sci.Rev., 144 (Apr.), 249–.273.
Gizon, L., Birch, A.C., and Spruit, H.C. 2010. Local helioseismology: Three-dimensional imaging of the solar interior. ARA&A, 48 (Sept.), 289–338.
Gizon, L., Ballot, J., Michel, E., et al. 2013. Seismic constraints on rotation of Sun-like star and mass of exoplanet. Proc.Nat.Acad.Sci., 110 (Aug.), 1326–1327.
Goins, N.R., and Lazarewicz, A.R. 1979. Martian seismicity. Geophys.Res.Lett., 6, 368-370.
Goins, N.R., Dainty, A.M., and Toksöz, M.N. 1977. The deep seismic structure of the Moon, Proceedings of the 8th Lunar Science Conference, 471–486.
Goins, N.R., Dainty, A.M., and Toksöz, M.N. 1981. Seismic energy release of the Moon. J.Geophys.Res., 86 378–388.
Goins, N.R., Dainty, A.M., and Toksöz, M.N. 1981. Structure of the lunar crust at highland site Apollo Station 16. Geophys.Res.Lett., 8 29–32.
Goins, N.R., Dainty, A.M., and Toksöz, M.N. 1981c. Lunar seismology: The internal structure of the Moon. J.Geophys.Res., 86, 5061–5074.
Gold, T., and Soter, S. 1970. Apollo 12 seismic signal: Indication of a deep layer of powder. Science, 169, 1071–1075.
Goldreich, P., and Keeley, D.A. 1977. Solar seismology: II.The stochastic excitation of the solar p-modes by turbulent convection. ApJ, 212 (Feb.), 243–251.
Goldreich, P., and Nicholson, P.D. 1989. Tides in rotating fluids. ApJ, 342 (July), 1075-1078.
Goldreich, P., Murray, N., Willette, G., and Kumar, P. 1991. Implications of solar p-mode frequency shifts. ApJ, 370 (Apr.), 752–762.
Goldreich, P., Murray, N., and Kumar, P. 1994. Excitation of solar p-modes. ApJ, 424 (Mar.), 466–479.
Golombek, M.P. 2002.A revision of Mars seismicity from surface faulting.Lunar and Planetary Science Conference, XXXIII, Abstract #1244.
Golombek, M.P., Banerdt, W.B., Tanaka, K.L., and Tralli, D.M. 1992. A prediction of Mars seismicity from surface faulting. Science, 258 (Nov.), 979–981.
Goode, P.R., and Thompson, M.J. 1992. The effect of an inclined magnetic field on solar oscillation frequencies. ApJ, 395 (Aug.), 307–315.
Goode, P.R., Gough, D., and Kosovichev, A.G. 1992. Localized excitation of solar oscillations. ApJ, 387 (Mar.), 707–711.
Goodricke, J. 1783. A series of observations on, and a discovery of, the period of the variation of the light of the bright star in the Head of Medusa, called Algol.In a letter from John Goodricke, the Rev.Anthony Shepherd, D.D.F.R.S. and Plumian, Professor at Cambridge. Phil.Trans.R.Soc.London Ser.I, 73, 474–482.
Goodricke, J., and Englefield, H.C. 1785. Observations of a new variable star.By John Goodricke, Esq.; Communicated by Sir H.C., Englefield, Bart, F.R.S. and A., S.Phil.Trans.R.Soc.London Ser.I, 75 153–164.
Gough, D. 2013. What have we learned from helioseismology, what have we really learned, and what do we aspire to learn?Sol.Phys., 287 (Oct.), 9–41.
Gough, D.O. 1984. On the rotation of the Sun. Phil.Trans.R.Soc.London Ser.A, 313 (Nov.), 27–38.
Gough, D.O. 1990.Comments on helioseismic inference.Page 283 of Osaki, Y., and Shibahashi, H. (eds), Progress of Seismology of the Sun and Stars. Lecture Notes in Physics, Berlin: Springer Verlag, vol.367.
Gough, D.O., and Kosovichev, A.G. 1993. Seismic analysis of stellar P-mode spectra.Page 351 of Brown, T.M. (ed), GONG 1992.Seismic Investigation of the Sun and Stars.Astronomical Society of the Pacific Conference Series, vol.42.
Gough, D.O., and McIntyre, M.E. 1998. Inevitability of a magnetic field in the Sun's radiative interior. Nature, 394 (Aug.), 755–757.
Gough, D.O., and Thompson, M.J. 1990. The effect of rotation and a buried magnetic field on stellar oscillations. MNRAS, 242 (Jan.), 25–55.
Gough, D.O., Kosovichev, A.G., Toomre, J., et al. 1996. The seismic structure of the Sun. Science, 272 (May), 1296–1300.
Goulty, N.R. 1979. Tidal triggering of deep moonquakes. Phys.Earth Planet.Int., 19 (May), 52–58.
Goupil, M.J., Dziembowski, W.A., and Fontaine, G. 1998. On some observational consequences of nonlinearities in stellar pulsations. Baltic Astron., 7 (Mar.), 21–41.
Goupil, M.J., Mosser, B., Marques, J.P., et al. 2013. Seismic diagnostics for transport of angular momentum in stars: II.Interpreting observed rotational splittings of slowly rotating red giant stars. A&A, 549 (Jan.), A75.
Gowen, R.A., Smith, A., Fortes, A.D., et al. 2011. Penetrators for in situ subsurface investigations of Europa. Adv.Space Res., 48, 725–742.
Grec, G., Fossat, E., and Vernin, J. 1976. A spectrophotometer for the study of long period solar photospheric oscillations. A&A, 50 (July), 221–225.
Grec, G., Fossat, E., and Pomerantz, M. 1980. Solar oscillations: Full disk observations from the geographic South Pole. Nature, 288 (Dec.), 541–544.
Grec, G., Fossat, E., and Pomerantz, M.A. 1983. Full-disk observations of solar oscillations from the geographic South Pole: Latest results. Sol.Phys., 82 (Jan.), 55–66.
Greenberg, J.M., and Huebner, W.F. 2002. Summary of the Workshop on Geophysical and Geological Properties of NEOs: ‘Know Your Enemy’.Pages 419-432 of International Seminars on Nuclear War and Planetary Emergencies, vol.26.
Grevesse, N., and Sauval, A.J. 1998. Standard solar composition. Space Sci.Rev., 85 (May), 161–174.
Grimm, H.-J., Gilfanov, M., and Sunyaev, R. 2002. The Milky Way in X-rays for an outside observer: Log(N)-Log(S) and luminosity function of X-ray binaries from RXTE/ASM data. A&A, 391 (Sept.), 923–944.
Gruberbauer, M., Kallinger, T., Weiss, W.W., and Guenther, D.B. 2009. On the detection of Lorentzian profiles in a power spectrum: A Bayesian approach using ignorance priors. A&A, 506 (Nov.), 1043–1053.
Gruberbauer, M., Guenther, D.B., and Kallinger, T. 2012. Toward a new kind of asteroseismic grid fitting. ApJ, 749 (Apr.), 109.
Grundahl, F., Kjeldsen, H., Christensen-Dalsgaard, J., Arentoft, T., and Frandsen, S. 2007. Stellar oscillations network group. Commun.Asteroseismol., 150 (June), 300.
Grundahl, F., Christensen-Dalsgaard, J., Gråe Jørgensen, U., et al.2011. SONG: Getting ready for the prototype. J.Phys.Conf.Ser., 271 (1), 01203.
Gruneisen, R. 1998.High precision photometry from space with COROT: Effect of spatial image jitter on the photometric performances of CCDs.Page 217 of Beletic, J., and Amico, P. (eds), Optical Detectors for Astronomy. Astrophysics and Space Science Library, vol.228.
Guasch, L., Warner, M., Nangoo, T., et al. 2012. Elastic 3D full-waveform inversion, 82nd Annual International Meeting, SEG, Expanded Abstracts, SI6.8.
Gudkova, T., Mosser, B., Provost, J., et al. 1995. Seismological comparison of giant planet interior models. A&A, 303 (Nov.), 594.
Gudkova, T., Lognonne, P., and Gagnepain-Beyneix, J. 2011. Large impacts detected by the Apollo seismometers: Impactor mass and source cutoff frequency estimations. Icarus, 211, 1049–1065.
Gudkova, T., Lognonne, P., Miljkovic, K., and Gagnepain-Beyneix, J. 2014. Impact cutoff frequency-momentum scaling law inverted from Apollo seismic data. Earth Planet.Sci.Lett.Guillot, T. 1999.Interior of giant planets inside and outside the Solar System.Science, 286 (Oct.), 72–77.
Guillot, T. 2005. The interiors of giant planets: Models and outstanding questions. Annu.Rev.Earth Planet.Sci., 33 (Jan.), 493–530.
Guillot, T., Stevenson, D.J., Hubbard, W.B., and Saumon, D. 2004.The interior of Jupiter.Pages 35-57 of Bagenal, F., Dowling, T.E., and McKinnon, W.B. (eds), Jupiter: The Planet, Satellites and Magnetosphere.Cambridge: Cambridge University Press.
Haber, D.A., and Hindman, B.W. 2005. Solar meridional flows: Recent findings. Highlights of Astronomy, 13 (Jan.), 431.
Haber, D.A., Hindman, B.W., Toomre, J., et al. 2002. Evolving submerged meridional circulation cells within the upper convection zone revealed by ring-diagram analysis. ApJ, 570 (May), 855–864.
Haber, D.A., Hindman, B.W., Toomre, J., and Thompson, M.J. 2004. Organized subsurface flows near active regions. Sol.Phys., 220 (Apr.), 371–380.
Hall, R.C. 1977. Lunar Impact: A History of Project Ranger, NASA History Series, NASA SP-4210.Washington, D.C.
Hammel, H.B., Beebe, R.F., Ingersoll, A.P., et al. 1995. HST imaging of atmospheric phenomena created by the impact of comet Shoemaker-Levy 91. Science, 267, 1288-1296.
Hammel, H.B., Wong, M.H., Clarke, J.T., et al. 2010. Jupiter after the 2009.impact: Hubble Space Telescope imaging of the impact-generated debris and its temporal evolution. Astron.J.Lett., 715, L150.
Hanasoge, S.M. 2013. The influence of noise sources on cross-correlation amplitudes. Geophys.J.Int., 192 (Jan.), 295–309.
Hanasoge, S.M. 2014. Measurements and kernels for source-structure inversions in noise tomography. Geophys.J.Int., 196 (Feb.), 971–985.
Hanasoge, S.M., Duvall, Jr., T., L., and Couvidat, S. 2007. Validation of helioseismology through forward modeling: Realization noise subtraction and kernels. ApJ, 664 (Aug.), 1234-1243.
Hanasoge, S.M., Duvall, Jr., T., L., and De Rosa, M.L. 2010. Seismic constraints on interior solar convection. ApJ, 712 (Mar.), L98-L102.
Hanasoge, S.M., Birch, A., Gizon, L., and Tromp, J. 2011. The adjoint method applied to time-distance helioseismology. ApJ, 738 (Sept.), 100.
Hanasoge, S., Birch, A., Gizon, L., and Tromp, J. 2012. Seismic probes of solar interior magnetic structure. Phys.Rev.Lett., 109 (10), 101101.
Hanasoge, S.M., Duvall, T.L., and Sreenivasan, K.R. 2012. Anomalously weak solar convection. Proc.Nat.Acad.Sci., 109 (July), 1192–1193.
Handberg, R., and Campante, T.L. 2011. Bayesian peak-bagging of solar-like oscillators using MCMC: A comprehensive guide. A&A, 527 (Mar.), A56.
Hansen, C.J., Kawaler, S.D., and Trimble, V. 2004.Stellar Interiors: Physical Principles, Structure, and Evolution.New York: Springer.
Harlow, F.H., and Welch, J.E. 1965. Numerical calculation of time-dependent viscous incompressible flow of fluid with free surface. Phys.Fluids, 8, 2182–2189.
Hartlep, T., Kosovichev, A.G., Zhao, J., and Mansour, N.N. 2011. Signatures of emerging subsurface structures in acoustic power maps of the Sun. Sol.Phys., 268 (Feb.), 321-327.
Hartlep, T., Zhao, J., Kosovichev, A.G., and Mansour, N.N. 2013. Solar wave-field simulation for testing prospects of helioseismic measurements of deep meridional flows. ApJ, 762 (Jan.), 132.
Harvey, J. 1985.High-resolution helioseismology.Page 199 of Rolfe, E., and Battrick, B. (eds), Future Missions in Solar, Heliospheric & Space Plasma Physics.ESA Special Publication, vol.235.
Harvey, J., Tucker, R., and Britanik, L. 1998.High resolution upgrade of the GONG instruments.Page 209 of Korzennik, S. (ed), Structure and Dynamics of the Interior of the Sun and Sun-like Stars.ESA Special Publication, vol.418.
Harvey, J.W. 1988.Techniques forobserving stellaroscillations.Page 497 of Christensen-Dalsgaard, J., and Frandsen, S. (eds), Advances in Helio- and Asteroseismology. IAU Symposium, vol.123.
Harvey, J.W., Hill, F., Hubbard, R., et al. 1996. The Global Oscillation Network Group (GONG) Project. Science, 272 (May), 1284.
Hathaway, D.H. 2012. Supergranules as probes of the Sun's meridional circulation. ApJ, 760 (Nov.), 84.
Hedman, M.M., and Nicholson, P.D. 2013. Kronoseismology: Using density waves in Saturn's C ring to probe the planet's interior. AJ, 146 (July), 12.
Hekker, S., Barban, C., Baudin, F., et al. 2010. Oscillation mode lifetimes of red giants observed during the initial and first anticentre long run of CoRoT. A&A, 520 (Sept.), A60.
Hekker, S., Gilliland, R.L., Elsworth, Y., et al. 2011. Characterization of red giant stars in the public Kepler data. MNRAS, 414 (July), 2594-2601.
Helled, R., and Guillot, T. 2013. Interior models of Saturn: Including the uncertainties in shape and rotation. ApJ, 767 (Apr.), 113.
Hello, Y., Ogé, A., Sukhovich, A., and Nolet, G. 2011. Modern mermaids: New floats image the deep Earth. EOS Trans., 92 (4 Oct.), 337–338.
Hempel, S., Knapmeyer, M., Jonkers, A.R.T., and Oberst, J. 2012. Uncertainty of Apollo deep moon quake locations andimplications for future network designs. Icarus, 220 (Aug.), 971–980.
Hill, F. 1984. The effects of a nearly 100% duty cycle in observations of solar oscillations. Pages 271-277 of Ulrich, R.K., Harvey, J., Rhodes, Jr., E.J., and Toomre, J. (eds), Solar Seismology from Space. NASA JPL.
Hill, F. 1988. Rings and trumpets: Three-dimensional power spectra of solar oscillations. ApJ, 333 (Oct.), 996–1013.
Hill, F., and Newkirk, Jr., G. 1985. On the expected performance of a solar oscillation network. Sol.Phys., 95 (Feb.), 201–219.
Hill, F., Stark, P.B., and Stebbins, R.T., et al. 1996. The solar acoustic spectrum and eigenmode parameters. Science, 272 (May), 1292-1295.
Hill, F., Anderson, E., Howe, R., et al. 1998.Estimated mode parameters from the fitting of GONG spectra.Page 231 of Korzennik, S. (ed.), Structure and Dynamics of the Interior of the Sun andSun-like Stars. ESA Special Publication, vol.418.
Hill, F., Baldner, C.S., García, R.A., Roth, M., and Schunker, H. 2013.Where to go from here: The future of helio- and astero-seismology.Pages 401-408 of Jain, K., Tripathy, S.C., Hill, F., Leibacher, J.W., and Pevtsov, A.A. (eds), Fifty Years of Seismology of the Sun and Stars. Astronomical Society of the Pacific Conference Series, vol.478.
Hill, H.A., Stebbins, R.T., and Brown, T.M. 1976.Recent oblateness observations: Data, interpretation and significance for earlier work.Page 622 of Sanders, J.H., and Wapstra, A.H. (eds), Atomic Masses and Fundamental Constants, vol.5.New York: Plenum.
Hilton, J.L. 2002. Asteroid masses and densities. Asteroids III, 103–112.
Hopf, T., Kumar, S., Karl, W.J., and Pike, W.T. 2010. Shock protection of penetrator-based instrumentation via a sublimation approach. Adv.Space Res., 45, 460–467.
Horvath, P., Latham, G., Nakamura, Y., and Dorman, H.J. 1980. Lunar near-surface shear wave velocities at the Apollo landing sites as inferred from spectral amplitude ratios. J.Geophys.Res., 85, 6572–6578.
Houdek, G., and Gough, D.O. 2007. An asteroseismic signature of helium ionization. MNRAS, 375 (Mar.), 861–880.
Houdek, G., Balmforth, N.J., Christensen-Dalsgaard, J., and Gough, D.O. 1999. Amplitudes of stochastically excited oscillations in main-sequence stars. A&A, 351 (Nov.), 582–596.
Howe, R. 2009. Solar interior rotation and its variation. Living Rev.Sol.Phys., 6 (Feb.), 1.
Howe, R., and Hill, F. 1998.Estimating low-degree mode parameters from GONG data using the leakage matrix.Page 237 of Korzennik, S. (ed), Structure and Dynamics of the Interior of the Sun and Sun-like Stars.ESA Special Publication, vol.418.
Howe, R., and Thompson, M.J. 1998. A strategy for fitting partially blended ridges in GONG solar p-mode spectra. A&AS, 131 (Sept.), 539–548.
Howe, R., Christensen-Dalsgaard, J., Hill, F., et al. 2000. Dynamic variations at the base of the solar convection zone. Science, 287 (Mar.), 2456–2460.
Howe, R., Christensen-Dalsgaard, J., and Hill, F., et al. 2005. Solar convection-zone dynamics, 1995–2004. ApJ, 634 (Dec.), 1405–1415.
Howe, R., Christensen-Dalsgaard, J., Hill, F., et al. 2009. A note on the torsional oscillation at solar minimum. ApJ, 701 (Aug.), L87-L90.
Howe, R., Christensen-Dalsgaard, J., Hill, F., et al. 2013. The high-latitude branch of the solar torsional oscillation in the rising phase of cycle 24. ApJ, 767 (Apr.), L20.
Howell, S.B., Sobeck, C., Haas, M., et al. 2014. The K2 mission: Characterization and early results. PASP, 126 (Apr.), 398–408.
Hu, H., Tout, C.A., Glebbeek, E., and Dupret, M.-A. 2011. Slowing down atomic diffusion in subdwarf B stars: Mass loss or turbulence?MNRAS, 418 (Nov.), 195–205.
Huber, D., Bedding, T.R., Stello, D., et al. 2011. Testing scaling relations for solar-like oscillations from the main sequence to red giants using Kepler data. ApJ, 743 (Dec.), 143.
Huber, D., Chaplin, W.J., Christensen-Dalsgaard, J., et al. 2013. Fundamental properties of Kepler planet-candidate host stars using asteroseismology. ApJ, 767 (Apr.), 127.
Huber, D., Carter, J.A., Barbieri, M., et al. 2013. Stellar spin-orbit misalignment in a multiplanet system. Science, 342 (Oct.), 331–334.
Huber, D., Silva Aguirre, V., Matthews, J.M., et al. 2014. Revised stellar properties of Kepler targets for the quarter 1-16 transit detection run. ApJS, 211 (Mar.), 2.
Hudson, H.S., Fisher, G.H., and Welsch, B.T. 2008.Flare energy and magnetic field variations.Page 221 of Howe, R., Komm, R.W., Balasubramaniam, K.S., and Petrie, G.J. D.(eds), Subsurface and Atmospheric Influences on Solar Activity.Astronomical Society of the Pacific Conference Series, vol.383.
Huebner, W.F., Cellino, A., Cheng, A.F., and Greenberg, J.M. 2001. NEOs: Physical properties.Pages 309-34 of International Seminars on Nuclear War and Planetary Emergencies, vol.25.
Hueso, R., Sánchez-Lavega, A., and Guillot, T. 2002. A model for large-scale convective storms in Jupiter. J.Geophys.Res.(Planets), 107 (Oct.), 5075.
Hunt, M.L., and Vriend, N.M. 2010.Booming sand dunes.Annu.Rev.Earth Planet.Sci., 2010.38:281-301, doi:10.1146.annurev-earth-040809–152336.
Iben, Jr., I. 1971. Globular cluster stars: Results of theoretical evolution and pulsation studies compared with the observations. PASP, 83 (Dec.), 697.
Ibrahim, M.I. 2012. The elastic properties of carbonaceous chondrites.Ph.D.thesis, University of Calgary, Alberta, Canada.
Ilonidis, S., Zhao, J., and Kosovichev, A.G. 2011. Detection of emerging sunspot regions in the solar interior by helioseismology. AGU Fall Meeting Abstracts, Dec., A1.
Irwin, P.G.J. 2009. Giant Planets of Our Solar System.Springer-Praxis.
Jackiewicz, J., Gizon, L., and Birch, A.C. 2008. High-resolution mapping of flows in the solar interior: Fully consistent OLA inversion of helioseismic travel times. Sol.Phys., 251 (Sept.), 381–415.
Jackiewicz, J., Nettelmann, N., Marley, M., and Fortney, J. 2012. Forward and inverse modeling for jovian seismology. Icarus, 220 (Aug.), 844–854.
Jackiewicz, J., Birch, A.C., Gizon, L., et al. 2012. Multichannel three-dimensional SOLA inversion for local helioseismology. Sol.Phys., 276 (Feb.), 19–33.
Jackson, J.D., and Fox, R.F. 1999. Classical Electrodynamics, 3rd edn.New York: John Wiley & Sons.
Jacoutot, L., Kosovichev, A.G., Wray, A.A., and Mansour, N.N. 2008. Numerical simulation of excitation of solar oscillation modes for different turbulent models. ApJ, 682 (Aug.), 1386–1391.
Jacoutot, L., Kosovichev, A.G., Wray, A., and Mansour, N.N. 2008. Realistic numerical simulations of solar convection and oscillations in magnetic regions. ApJ, 684 (Sept.), L51-L54.
Jain, R., and Haber, D. 2002. Solar p-modes and surface magnetic fields: Is there an acoustic emission? MDI/SOHO observations. A&A, 387 (June), 1092–1099.
Jaupart, C., and Mareschal, J.-C. 2010. Heat Generation and Transport in the Earth.Cambridge: Cambridge University Press.
Jensen, J.M., and Pijpers, F.P. 2003. Sensitivity kernels for time-distance inversion based on the Rytov approximation. A&A, 412 (Dec.), 257–265.
Jensen, J.M., Duvall, Jr., T., L., Jacobsen, B.H., and Christensen-Dalsgaard, J. 2001. Imaging an emerging active region with helioseismic tomography. ApJ, 553 (June), L193-L196.