Cosmic ray density gradient and its dependence on the north-south asymmetry in solar activity

Computer Science

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Anisotropy, Cosmic Rays, Density Distribution, Radiant Flux Density, Solar Activity, Solar Magnetic Field, Current Sheets, Geomagnetism, Neutron Counters, Polarity, Solar Wind Velocity, Vertical Orientation

Scientific paper

An analysis of the diurnal anisotropy on geomagnetically quiet days was performed using neutron monitor data at Deep River, Leeds, Rome and Tokyo, well distributed in latitude and longitude for the period 1964-79. The days were separated according to the polarity of IMF on that day. A significant difference in the amplitude and phase was found on towards and away polarity days, particularly during the years of high solar activity and large north-south asymmetry. These results (particularly time of maximum) on geomagnetically quiet days show some better relationship to the expected results as compared to the results obtained using all the days in a year.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cosmic ray density gradient and its dependence on the north-south asymmetry in solar activity 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 Cosmic ray density gradient and its dependence on the north-south asymmetry in solar activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic ray density gradient and its dependence on the north-south asymmetry in solar activity will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-756694

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.