Distribution of cometary parameters over the 11-year cycle of solar activity

Details Distribution of cometary parameters over the 11-year cycle of solar activity Distribution of cometary parameters over the 11-year cycle of solar activity

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...68g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, July-Aug. 1990, p. 68-73. In Russian.

Physics

Comets, Solar Activity, Sunspot Cycle, Ecliptic, Jupiter (Planet), Solar System, Spatial Distribution

Scientific paper

The characteristics of long-period comets (P greater than 200 years) detected in different phases of the 11-year solar cycle are examined. It is shown that there exists a group of comets which manifest high activity after the maximum of the 11-year cycle and which differ greatly from the total set of long-period comets with respect to a whole series of parameters. It is suggested that this group of comets may be connected with Jupiter.

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