Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cosks..25..121a&link_type=abstract
Contributions of the Astronomical Observatory Skalnate Pleso Supplement, Volume 25, p. 121-124
Astronomy and Astrophysics
Astronomy
Solar Flares, Stellar Mass Ejection, Heliosphere, Galactic Cosmic Rays, Statistical Analysis, Astronomical Catalogs, Correlation Coefficients, Solar Prominences, Temporal Distribution, Solar Magnetic Field
Scientific paper
The Catalogue of LDE-type flares covers 25 years of LDE-type flare data (1969-1994). The continuation of the list of long-lasting SXR flares (LDE-type) is given. The latter contains the list of LDE flares observed from July 1993 to June 1994, and ties in timewise with the previous paper; it is only available in a computer-file form. One considers temporal variations of the occurrence of the LDE flares, with SXR duration exceeding 2 hours, throughout the 22-nd cycle. Current studies of the heliosphere regard Coronal Mass Ejections (CMEs) as a principal phenomenon modifying its properties. CMEs are usually accompanied by dynamic activity phenomena (LDE-type flares, DBs and eruptive prominences). That is the reason why CMEs are implicitly incorporated in LDE-type flare list.
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