Transient cosmic ray increase associated with a geomagnetic storm

Details Transient cosmic ray increase associated with a geomagnetic storm Transient cosmic ray increase associated with a geomagnetic storm

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..246k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 246-249 (SEE N85-34991 23-93)

Computer Science

Cosmic Rays, Diurnal Variations, Flux Density, Magnetic Storms, Correlation Detection, Estimates, Geomagnetism, Longitude, Neutron Counters

Scientific paper

On the basis of worldwide network data of cosmic ray nucleonic components, the transient cosmic ray increase due to the depression of cosmic ray cutoff rigidity during a severe geomagnetic storm was investigated in terms of the longitudinal dependence. Multiple correlation analysis among isotropic and diurnal terms of cosmic ray intensity variations and Dst term of the geomagnetic field is applied to each of various station's data. It is shown that the amplitude of the transient cosmic ray increase associated with Dst depends on the local time of the station, and that its maximum phase is found in the evening sector. This fact is consistent with the theoretical estimation based on the azimuthally asymmetric ring current model for the magnetic DS field.

Affiliated with

Also associated with

No associations

Rating

Transient cosmic ray increase associated with a geomagnetic storm 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 Transient cosmic ray increase associated with a geomagnetic storm, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transient cosmic ray increase associated with a geomagnetic storm will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-756847