Short-lived stellar flares - Identification and evaluation methods

Details Short-lived stellar flares - Identification and evaluation methods Short-lived stellar flares - Identification and evaluation methods

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...61z&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Sept.-Oct. 1991, p. 61-67. In Russian.

Physics

1

Photon Density, Statistical Analysis, Stellar Flares, Stellar Physics, Atmospheric Radiation, Instrument Errors, Root-Mean-Square Errors, Stellar Oscillations

Scientific paper

A method is presented for identifying short-lived stellar flares on the basis of a statistical analysis of group count declinations in Poisson and Gaussian photon fluxes. Estimates of integrated amplitudes and flare duration as well as their rms errors are given. Phantom flares induced both by scintillations of the earth atmosphere and by instrumentation interference are investigated.

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