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Observing the Sun with the Atacama Large Millimeter/submillimeter Array – from continuum to magnetic fields

Published online by Cambridge University Press:  24 September 2020

Sven Wedemeyer Open the ORCID record for Sven Wedemeyer [Opens in a new window] ,
Mikolaj Szydlarski ,
Jaime de la Cruz Rodriguez  and
Shahin Jafarzadeh
Sven Wedemeyer
Affiliation:
Rosseland Centre for Solar Physics, University of Oslo, Postboks 1029 Blindern, N-0315 Oslo, Norway Institute of Theoretical Astrophysics, University of Oslo, Postboks 1029 Blindern, N-0315 Oslo, Norway
Mikolaj Szydlarski
Affiliation:
Rosseland Centre for Solar Physics, University of Oslo, Postboks 1029 Blindern, N-0315 Oslo, Norway Institute of Theoretical Astrophysics, University of Oslo, Postboks 1029 Blindern, N-0315 Oslo, Norway
Jaime de la Cruz Rodriguez
Affiliation:
Institute for Solar Physics, Dept. of Astronomy, Stockholm University, Albanova University Center, SE-10691 Stockholm, Sweden
Shahin Jafarzadeh
Affiliation:
Rosseland Centre for Solar Physics, University of Oslo, Postboks 1029 Blindern, N-0315 Oslo, Norway Institute of Theoretical Astrophysics, University of Oslo, Postboks 1029 Blindern, N-0315 Oslo, Norway
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Abstract

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The Atacama Large Millimeter/submillimeter Array offers regular observations of our Sun since 2016. After an extended period of further developing and optimizing the post-processing procedures, first scientific results are now produced. While the first observing cycles mostly provided mosaics and time series of continuum brightness temperature maps with a cadence of 1-2s, additional receiver bands and polarization capabilities will be offered in the future. Currently, polarization capabilities are offered for selected receiver bands but not yet for solar observing. An overview of the recent development, first scientific results and potential of solar magnetic field measurements with ALMA will be presented.

Keywords

Sun: atmosphereSun: chromosphereSun: radio radiationradiation mechanisms: thermalmagnetic fieldspolarizationtechniques: interferometric
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S354: Solar and Stellar Magnetic Fields: Origins and Manifestations , June 2019 , pp. 24 - 37
Copyright
© International Astronomical Union 2020

References

Bastian, T. S., Bárta, M., Brajša, R., et al. 2018, The Messenger, 171, 25Google Scholar
Bastian, T. S., Chintzoglou, G., De Pontieu, B., et al. 2017, Astrophys. J. Lett., 845, L19CrossRefGoogle Scholar
Bogod, V. M. & Gelfreikh, G. B. 1980, Solar Phys., 67, 29CrossRefGoogle Scholar
Brajša, R., Sudar, D., Benz, A. O., et al. 2018, A&A, 613, A17Google Scholar
Carlsson, M., Hansteen, V. H., Gudiksen, B. V., Leenaarts, J., & De Pontieu, B. 2016, A&A, 585, A4Google Scholar
de la Cruz Rodriguez, J., Szydlarski, M., Wedemeyer, S., & et al. in prep., The Advanced Radiative Transfer codeGoogle Scholar
Grebinskij, A., Bogod, V., Gelfreikh, G., et al. 2000, A&AS, 144, 169Google Scholar
Gudiksen, B. V., Carlsson, M., Hansteen, V. H., et al. 2011, A&A, 531, A154+CrossRefGoogle Scholar
Jafarzadeh, S., Wedemeyer, S., Szydlarski, M., et al. 2019, A&A, 622, A150Google Scholar
Kundu, M. R. 1965, Solar radio astronomy (Interscience Publication, New York)Google Scholar
Kuridze, D., Henriques, V. M. J., Mathioudakis, M., et al. 2018, ApJ, 860, 10CrossRefGoogle Scholar
Loukitcheva, M., White, S. M., Solanki, S. K., Fleishman, G. D., & Carlsson, M. 2017, A&A, 601, A43Google Scholar
Loukitcheva, M. A., White, S. M., & Solanki, S. K. 2019, ApJ, 877, L26CrossRefGoogle Scholar
Loukitcheva, M. 2020, Front. Astron. Space Sci., 11 August 2020 (https://doi.org/10.3389/fspas.2020.00045)CrossRefGoogle Scholar
Molnar, M. E., Reardon, K. P., Chai, Y., et al. 2019, ApJ, 881, 99CrossRefGoogle Scholar
Nindos, A., Alissandrakis, C. E., Bastian, T. S., et al. 2018, A&A, 619, L6Google Scholar
Nita, G. M., Fleishman, G. D., Kuznetsov, A. A., Kontar, E. P., & Gary, D. E. 2015, ApJ, 799, 236CrossRefGoogle Scholar
Rodger, A. S., Labrosse, N., Wedemeyer, S., et al. 2019, ApJ, 875, 163CrossRefGoogle Scholar
Selhorst, C. L., Simões, P. J. A., Brajša, R., et al. 2019, ApJ, 871, 45CrossRefGoogle Scholar
Shimojo, M., Bastian, T. S., Hales, A. S., et al. 2017a, Sol. Phys., 292, #87Google Scholar
Shimojo, M., Hudson, H. S., White, S. M., Bastian, T. S., & Iwai, K. 2017b, ApJ, 841, L5CrossRefGoogle Scholar
Wedemeyer, S. 2016, The Messenger, 163, 15Google Scholar
Wedemeyer, S., Bastian, T., Brajša, R., et al. 2016, Space Sci. Rev., 200, 1CrossRefGoogle Scholar
Wedemeyer, S., Szydlarski, M., Jafarzadeh, S., et al. 2020, A&A, 635, A71Google Scholar
White, S. M., Iwai, K., Phillips, N. M., et al. 2017, Sol. Phys., 292, #88Google Scholar
Yokoyama, T., Shimojo, M., Okamoto, T. J., & Iijima, H. 2018, ApJ, 863, 96CrossRefGoogle Scholar