Solar-cycle phenomena in cosmic-ray intensity - Differences between even and odd cycles

Details Solar-cycle phenomena in cosmic-ray intensity - Differences between even and odd cycles Solar-cycle phenomena in cosmic-ray intensity - Differences between even and odd cycles

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988em%26p...42..233m&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 42, Sept. 1988, p. 233-244.

Computer Science

10

Cosmic Rays, Radiant Flux Density, Solar Activity, Solar Cycles, Solar Flares, Solar Wind Velocity, Sunspots

Scientific paper

Cosmic-ray intensity data for the period 1964 - 1985 covering two solar cycles are used to investigate the solar activity behaviour in relation to cosmic-ray modulation. A detailed statistical analysis of them shows a large time-lag of about one and half years between cosmic-ray intensity and solar activity during the 21st solar cycle. The account of the solar-wind speed in the 11-year variation significantly decreases the modulation region of cosmic-rays to the value of 40 AU. A comparison with the behaviour of the previous solar cycle establishes a distinction between even and odd solar cycles.

Affiliated with

Also associated with

No associations

Rating

Solar-cycle phenomena in cosmic-ray intensity - Differences between even and odd cycles 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 Solar-cycle phenomena in cosmic-ray intensity - Differences between even and odd cycles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar-cycle phenomena in cosmic-ray intensity - Differences between even and odd cycles will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-913073