Hostname: page-component-5c6d5d7d68-vt8vv Total loading time: 0.001 Render date: 2024-08-06T11:37:55.588Z Has data issue: false hasContentIssue false
  • English
  • Français

Observations of Spatial and Temporal Variations of the Jovian H2 Quadrupole Lines

Published online by Cambridge University Press:  14 August 2015

N. P. Carleton  and
W. A. Traub
N. P. Carleton
Affiliation:
Smithsonian Astrophysical Observatory and Harvard University, Cambridge, Mass., U.S.A.
W. A. Traub
Affiliation:
Smithsonian Astrophysical Observatory and Harvard University, Cambridge, Mass., U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have made high resolution scans of the Jovian H2 4–0 S(1) line at 6367.75 Å and the 3–0 S(1) line at 8150.67 Å, in an attempt to establish improved equivalent widths and to measure any spatial-temporal variations across the disc. Preliminary analysis indicates that temporal changes in the 3–0 S(1) line can be as large as about 40% over a period of about a week; furthermore, this line is systematically weaker at the limb (about 10%) and stronger at the poles (about 20%) than it is at the center of the disc. The 4–0 S(1) line shows very little temporal change, but does have a similar center to limb variation. Current theoretical models of line formation and cloud structure on Jupiter are not able to explain the observed variations although it is clear that some sort of two-layer model is necessary.

Type
Part III Outer Planets and Their Satellites
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 345 - 349
Copyright
Copyright © Reidel 1974 

References

Beckman, J. E.: 1967, Planetary Space Sci. 15, 1211.Google Scholar
Emerson, J. P., Eddy, J. A., and Dulk, G. A.: 1969, Icarus 11, 413.Google Scholar
Fink, U. and Belton, M. J. S.: 1969, J. Atmospheric Sci. 26, 952.Google Scholar
Gehrels, T.: 1969, Icarus 10, 410.Google Scholar
Hunt, G. E.: 1973, Icarus 18, 637.Google Scholar
Hunt, G. E. and Margolis, J. S.: 1973, J. Quant. Spectrosc. Radiat. Transfer 13, 417.Google Scholar
Owen, T. and Mason, H. P.: 1968, Astrophys. J. 154, 317.Google Scholar
Spinrad, H. and Trafton, L. M.: 1963, Icarus 2, 19.Google Scholar
Trafton, L.: 1972, Bull. Am. Astron. Soc. 4, 358.Google Scholar
Trauger, J. T.: 1972, , University of Wisconsin.Google Scholar
Trauger, J. T. and Roesler, F. L.: 1972, Appl. Opt. 11, 1964.Google Scholar
Trauger, J. T., Roesler, F. L., Carleton, N. P., and Traub, W. A.: 1973, Astrophys. J. 184, L137.CrossRefGoogle Scholar