Solar activity and cosmic-ray proton fluxes in March--July 1972. [Effects of behind-the-limb flares on proton flux]

Journal Article · Wed Jan 01 00:00:00 EST 1975 · Geomagn. Aeron. (USSR) (Engl. Transl.); (United States)

OSTI ID:7155871

Kontor, N N; Lyubimov, G P; Nikolaev, A G; Pereslegina, N V; Tverskoy, B A; Khotilovskaya, T G

The reasons for seven considerable increases in proton intensity in March--July 1972 are established. It is shown that four out of the seven increases were produced by solar flares in strong active regions behind the limb.

• Research Organization: Moscow State Univ.
• OSTI ID: 7155871
• Journal Information: Geomagn. Aeron. (USSR) (Engl. Transl.); (United States), Vol. 15:5; Other Information: Translated from Geomagn. Aeron.; 15: No. 5, 777-786(1975)
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC PROTONS
COSMIC RAY FLUX
SOLAR FLARES
SOLAR PROTONS
MODULATION
KEV RANGE 100-1000
MEV RANGE 01-10
MEV RANGE 10-100
SOLAR ACTIVITY
VARIATIONS
BARYONS
COSMIC RADIATION
ELEMENTARY PARTICLES
ENERGY RANGE
FERMIONS
HADRONS
IONIZING RADIATIONS
KEV RANGE
MEV RANGE
NUCLEONS
PROTONS
RADIATION FLUX
RADIATIONS
SOLAR PARTICLES
SOLAR RADIATION
STELLAR RADIATION
640101* - Astrophysics & Cosmology- Cosmic Radiation
640104 - Astrophysics & Cosmology- Solar Phenomena