Solar and geomagnetic activity during cycle 21 and implications for cycle 22

Details Solar and geomagnetic activity during cycle 21 and implications for cycle 22 Solar and geomagnetic activity during cycle 21 and implications for cycle 22

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988eostr..69..962h&link_type=abstract

EOS (ISSN 0096-3941), vol. 69, Oct. 18, 1988, p. 962, 972, 973.

Computer Science

3

Magnetic Effects, Solar Activity, Solar Cycles, Solar Terrestrial Interactions, Sunspot Cycle, Energetic Particles, Satellite Drag, Solar Flares, Solar Protons

Scientific paper

The 21st solar cycle is characterized in terms of variations in sunspots, solar radio noise, EUV emission, and episodic phenomena. The data are presented in tables and graphs and compared with measurements obtained during the first years of cycle 22 (beginning September 1986). On the basis of its rapid rise, it has been predicted that cycle 22 will have an amplitude slightly greater than that of the largest recorded cycle (19), with sunspot numbers of about 200 and radio flux F(10.7) of about 250. Estimates based on observations of the end of cycle 21, however, are somewhat lower.

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