Short-period variations of the rate of change of solar activity as a possible geoefficiient parameter

Details Short-period variations of the rate of change of solar activity as a possible geoefficiient parameter Short-period variations of the rate of change of solar activity as a possible geoefficiient parameter

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..519v&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, July-Aug. 1983, p. 519-522. In Russian.

Computer Science

1

Cosmic Rays, Geomagnetism, Solar Activity, Interplanetary Medium, Periodic Variations, Solar Wind, Walsh Function

Scientific paper

The periodic structure of cosmic ray intensity, and geomagnetic and solar activity is analyzed in the Walsh-function basis. A marked component in the period range of 6-8 days is shown to exist in the spectra of diurnal variations of the parameters investigated. The dynamics of the quasi-weekly wave in Delta Sp is compared with the dynamics of various parameters of thhe interplanetary medium, solar atmosphere, and solar wind.

Affiliated with

Also associated with

No associations

Rating

Short-period variations of the rate of change of solar activity as a possible geoefficiient parameter 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 Short-period variations of the rate of change of solar activity as a possible geoefficiient parameter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Short-period variations of the rate of change of solar activity as a possible geoefficiient parameter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-742130