Features of cosmic ray variation at the phase of the minimum between the 23rd and 24th solar cycles

Bulletin of the Russian Academy of Sciences: Physics

Volumn 75, Issue 6, 2011, Pages 782-785

  Bazilevskaya, G A ^a   Krainev, M B ^a   Makhmutov, V S ^a   Svirzhevskaya, A K ^a   Svirzhevsky, N S ^a   Stozhkov, Yu L ^a  

^a LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

DIRECT MEASUREMENT; EARTH'S ORBIT; GROUND BASED; HIGH ENERGY; NEUTRON MONITORS; SOLAR ACTIVITY; SOLAR CYCLE; STRATOSPHERIC MEASUREMENTS;

COSMIC RAYS; MAGNETIC FIELDS; SOLAR ENERGY; SOLAR RADIATION; UPPER ATMOSPHERE;

COSMOLOGY;

EID: 79960497178     PISSN: 10628738     EISSN: None     Source Type: Journal    
DOI: 10.3103/S1062873811060074     Document Type: Article

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