Computer Science
Scientific paper
Oct 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..722a&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Sept.-Oct. 1985, p. 722-728. In Russian.
Computer Science
Galactic Cosmic Rays, Midlatitude Atmosphere, Radiant Flux Density, Stratosphere Radiation, Amplitudes, Diurnal Variations, Modulation, Pitch (Inclination), Solar Activity Effects, Solar Cycles, Solar Terrestrial Interactions
Scientific paper
Features characterizing the modulation of galactic cosmic rays in the midlatitude stratosphere during 1976-1982 are examined on the basis of data obtained at Erevan, Alma-Ata, and Dal'nerechensk, as well as during sea expeditions. An unusual modulation in the solar cycle was observed; the intensity decreased from the solar minimum (1976) to the solar maximum (1980) in the primary rigidity range of 6-8 GV. Also measured was the diurnal intensity wave; its amplitude (approximately 3 percent) was significantly higher than the amplitude of the diurnal wave in the neutron component. The observed effects can be explained qualitatively by changes in the anisotropic pitch-angle distribution of particles in interplanetary space.
Asatrian G. A.
Stozhkov Iu. I.
No associations
LandOfFree
Modulation of galactic cosmic rays in the midlatitude stratosphere 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 Modulation of galactic cosmic rays in the midlatitude stratosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modulation of galactic cosmic rays in the midlatitude stratosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1546017