Flare observation during Max 1991 balloon campaigns

Details Flare observation during Max 1991 balloon campaigns Flare observation during Max 1991 balloon campaigns

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988fnsm.work..201f&link_type=abstract

In NASA, Goddard Space Flight Center, Max 1991: Flare Research at the Next Solar Maximum. Workshop 1: Scientific Objectives p 20

Mathematics

Probability

Balloon-Borne Instruments, Equipment Specifications, Measuring Instruments, Solar Flares, Solar Maximum Mission, Statistical Distributions, Temporal Distribution

Scientific paper

A brief overview is presented for some of the large flare properties as observed during the prime SMM flare observation interval, 1980 to 1984. Two of these properties, namely their tendency to occur in groups and the strong effects of the 154 day periodicity, can be used to increase the probability of detecting large flares during the limited observing duration of Max 1991 balloon campaigns provided the solar flare characteristics of the 1991 solar cycle follows that observed in 1980 to 1984.

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