27-Days variations of galactic cosmic rays and changes of solar and geomagnetic activities

Advances in Space Research

Volumn 27, Issue 3, 2001, Pages 619-624

  Alania, M V ^a   Baranov, D G ^c   Tyasto, M I ^d   Vernova, E S ^b  

^a SIEDLCE UNIVERSITY OF NATURAL SCIENCES AND HUMANITIES   (Poland)

^b Georgian Academy of Science MNodia Institute of Geophysics   (Georgia)

^c IOFFE INSTITUTE   (Russian Federation)

^d PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

LIGHT EMISSION; NEUTRONS; OPTIMIZATION;

GALACTIC COSMIC RAYS;

GEOMAGNETISM;

COSMIC RAY;

EID: 0034924108     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00091-6     Document Type: Article

References (16)

1. Features of 27-day variations of galactic cosmic rays and of solar activity
2. A study of the modulation region causing 27-day cosmic ray variations
3. Experimental and modeling investigation of 27-day variation of galactic cosmic rays
4. Some properties of a fully three-dimensional drift model for the modulation of galactic cosmic rays
5. Cosmic ray latitudinal effects predicted by a three-dimensional drift model
6. Effects of drift on the transport of cosmic rays. VI. A three-dimensional model including diffusion
7. The role of corotating interaction regions in cosmic ray modulation
8. The 13.5-day periodicity in the sun, solar wind, and geomagnetic activity: The last three solar cycles
9. The passage of energetic charged particles through interplanetary space
10. 22-year dependence in the size of near ecliptic corotating cosmic ray depressions during five solar minima
11. Evidence of a N-S asymmetry in the heliosphere associated with a southward displacement of the heliospheric current sheet
12. Anomalies of solar activity in 1964-1965
13. The effect of solar activity longitudinal distribution of the northern and southern solar hemispheres on the 27-day galactic cosmic ray variation
14. North-south asymmetry in sudden disappearances of solar prominence