Intensity fluctuations in the head of comet 1973f

Details Intensity fluctuations in the head of comet 1973f Intensity fluctuations in the head of comet 1973f

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....41....9i&link_type=abstract

Astronomy and Astrophysics, vol. 41, no. 1, June 1975, p. 9-13. In German.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Photometry, Comet Heads, Kohoutek Comet, Luminous Intensity, Brightness Discrimination, Fine Structure, Periodic Variations, Solar Cycles

Scientific paper

Observations are reported which show that short-period variations in the intensity of comet Kohoutek were probably due to changes in its surface brightness, and thus originated in the tail. The period of the oscillations correlates with the 300 sec period of the solar photosphere and corona. Both measurements of the comet's gradual increase in brightness and of its short-period oscillations match functions of sun-comet distance better than functions of earth-comet distance.-

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