Time distribution of flare events on UV CET stars

Details Time distribution of flare events on UV CET stars Time distribution of flare events on UV CET stars

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..77..347p&link_type=abstract

Astrophysics and Space Science, vol. 77, no. 2, July 1981, p. 347-355.

Mathematics

Probability

12

Flare Stars, Stellar Spectrophotometry, Time Dependence, Ultraviolet Astronomy, Autocorrelation, Electrophotometers, Poisson Density Functions, Probability Distribution Functions, Random Variables, Statistical Analysis, Stochastic Processes

Scientific paper

The flare occurrence on UV Cet, EQ Peg, and YZ CMi is studied by a statistical analysis of observational data based on four variables. The variables include: time elapsed from the start of a continuous observation period to the occurrence of the first flare; time interval between consecutive flares; the number of flares occurring in time periods of given duration; and the ratio of the number of flares observed in each continuous observation period to that expected for a Poisson process. Results indicate that the time sequence of flares on the stars studied does not have a Poisson distribution.

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