What determines the magnetude of forbush decreases?

Advances in Space Research

Volumn 27, Issue 3, 2001, Pages 625-630

  Belov, A V ^a   Eroshenko, E A ^a   Oleneva, V A ^a   Struminsky, A B ^a   Yanke, V G ^a  

^a PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

COSMIC RAY DETECTORS; GEOMAGNETISM; NEUTRONS; WIND;

CORONAL MASS EJECTIONS;

SPACE RESEARCH;

COSMIC RAY;

EID: 0034925312     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00095-3     Document Type: Article

References (22)

1. The large-scale magnetic field configuration associated with Forbush decreases
2. Causes of Forbush decreases and other cosmic ray variations
3. Forbush-effects in 1978. 1.The role of suddenly disappearing filaments
4. Forbush-effects in 1977-1979
5. Modulation effects in 1991-1994 years
6. Modulation effects in 1991-1992 years
7. Transient effects in the cosmic rays during 1990-1995 (in Russian)
8. Cosmic ray effects caused by the great disturbances of the interplanetary medium in 1990-1996
9. Interplanetary flow systems associated with cosmic ray modulation in 1977-1980
10. Cosmic ray decreases and magnetic clouds
11. CMEs and Forbush decreases
12. Cosmic ray decreases and particle acceleration in 1978-1982 and the associated solar wind structure
13. Postmodern view of M-regions
14. On the effects in the cosmic-ray intensity observed during magnetic storms
15. Coronal hole-active region-current sheet (CHARCS) association with intense interplanetary and geomagnetic activity
16. High speed solar wind streams and galactic cosmic ray modulation
17. Solar sources of the interplanetary plasma streams on the Earth's orbit
18. Transient effects and disturbed conditions