CAOSP abstracts, Volume: 25, year: 1995
- Author(s): ANTALOVA, A.
- Journal: [SUPPLEMENT] Contributions of the Astronomical Observatory Skalnate Pleso,
vol. 25, p. 121-124.
- Date: 09/1995
- Title: Catalogue of LDE-type flares (1993-1994)
- Keyword(s): THE SUN, FLARES
- Pages: 121 -- 124
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 in Table 1. The latter contains the list of LDE flares
observed from July 1993 to June 1994, and ties in timewise with the previous
paper (Antalova 1990); 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. Analysis of the
LDE-type flare occurrence in solar cycles 20, 21 and 22 is published in the
- Periodicities of the LDE-type flare occurrence (1969-1992) in Antalova
- Cosmic-ray modulation and long-duration solar flare events, in Kudela et
- On the correlation between daily GCR intensity values and LDE-type flare
index (1987, 1988, 1990 and 1992) in Antalova et al. (1995). The temporal
changes found in a daily CNI-FI anticorrelation profile reflect the cyclic
magnetic reversal of the Sun as well as the corresponding heliospherical
- E-W distribution of Solar LDE-type Flares and Galactic Cosmic ray modulation
(1969-1972) in Antalova et al. (1994) and Jakimiec et al. (1995).
- Role of LDE-type flares in the GCR Modulation (1969-1972) in Antalova et al.
- The magnetic reversal in the 21st solar cycle and LDE-type flares in
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