An approach to trend analysis in data with special reference to cometary magnitudes

Details An approach to trend analysis in data with special reference to cometary magnitudes An approach to trend analysis in data with special reference to cometary magnitudes

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.256..647d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 256, no. 4, June 15, 1992, p. 647-654.

Astronomy and Astrophysics

Astronomy

2

Brightness Distribution, Comets, Magnitude, Trend Analysis, Data Reduction, Mathematical Models, Normal Density Functions, Solar Orbits

Scientific paper

A novel trend-analysis method is presently developed in association with a Pareto power-law model used by Donnison (1986, 1987, 1990) to model the brightness magnitude distribution of long and short-period comets. Compelling evidence is found for an increase in the brightness indices with the discovery rate of the long-period comets. No trend is discernible as a function of perihelion distance; neither are trends apparent in the brightness distribution of the short-period comets with increased orbital period.

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