Other
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36..122c&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 36, no. 2, 1985, p. 122-127.
Other
H Alpha Line, Solar Flares, Field Strength, Histograms, Solar Radio Bursts, Sunspots
Scientific paper
The visual features of the four types of solar H-alpha radio flares were studied in relation to the occurrence of radio bursts, sunspots, and the distribution of flares on the solar disk. Flare types A and T were the most frequent and infrequent types of flares, respectively. Flare types K and U were found to be more durable than K and L types, but K and L types had greater rise times in comparison with the other types of flares. The distribution of A-type flares corresponded to the location of sunspots of the alphap configuration having magnetic fields of 500-200 G. The distribution of the remaining flare types was associated with sunspots in the Alphap, Betap, and Beta and Delta configurations with magnetic field strengths in the range 1000-2000 G. In general, flare types J, K, and U were comparatively burst productive, while G-type bursts were not. Curves showing the cumulative percentage occurrence of the different types of flares are provided.
Chakravorti T.
Das Tapas Kumar
Das Gupta M. K.
No associations
LandOfFree
Studies on some aspects of the solar H-alpha flares of different visual features does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Studies on some aspects of the solar H-alpha flares of different visual features, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Studies on some aspects of the solar H-alpha flares of different visual features will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-821812