Analysis of spectral characteristics of long-period comets

Details Analysis of spectral characteristics of long-period comets Analysis of spectral characteristics of long-period comets

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...10g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 6, p. 10-13.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Comets, Spectrum Analysis, Solar Activity Effects, Solar System

Scientific paper

The dependence of the number of discoveries of comets with different spectral characteristics on the phase of solar activity is studied. It is shown that comets in which the continuum dominates over emissions are discovered more often near a solar activity phase of 0.550, i.e., after the maximum phase. Discoveries of comets in which emissions dominate over continuum fall at phase intervals near 0.200 and 0.800. A statistical criterion is used to show that these two groups cannot be related to a single population. The results agree well with the conclusions of Guliev (1990) on the heterogeneity of the system of long-period comets.

Affiliated with

Also associated with

No associations

Rating

Analysis of spectral characteristics of long-period comets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Analysis of spectral characteristics of long-period comets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of spectral characteristics of long-period comets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1138361