Hostname: page-component-848d4c4894-mwx4w Total loading time: 0 Render date: 2024-06-25T20:03:10.574Z Has data issue: false hasContentIssue false

The Nucleus: Panel Discussion

Published online by Cambridge University Press:  12 April 2016

Extract

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.

Almost all information about the physics of the nucleus is based on deductions from observations of the coma and tails. It is well to keep in mind the hierarchy of events on which these deductions are based:

1. The material properties of the constituents of the nucleus and the detailed physical and chemical structure of the nucleus form the basis for the behavior of coma and tails.

2. Interaction of solar radiation with the surface of the nucleus determines the overall temporal development of the coma.

3. The subsequent interaction of solar radiation and solar wind with the coma determine the gross features of the tails.

4. Short term fluctuations primarily in the solar wind (and associated magnetic, field) cause disturbances of comparable duration observable mostly in the tail but also in the coma.

Type
Part II
Copyright
Copyright © NASA 1976

References

Buhl, D., Huebner, W. F., and Snyder, L. E., 1974, “Detection of Molecular Microwave Transitions in the 3 mm Wavelength Range in Comet Kohoutek (1973f).” Proceedings of this conference.Google Scholar
Huebner, W. F., 1971, Bull. Am. Astron. Soc. 3, 500.Google Scholar
Jackson, W. M., Clark, T., and Donn, B., 1974, “Radio Observations of H2O in Comet Bradfield,” Proceedings of this conference.Google Scholar
Lelevier, R., 1965, “Lecture Notes on Hydrodynamics and Shockwaves,” Lawrence Radiation Laboratory report UCRL-4333 Rev. 1.CrossRefGoogle Scholar
Ulich, B. L., and Conklin, E. K., 1974, Nature 248, 121.CrossRefGoogle Scholar