Some trends in perfecting the dynamic models of cosmic ray modulation

Radiation Measurements

Volumn 26, Issue 3 SPEC. ISS., 1996, Pages 477-480

  Nymmik, R A ^a   Suslov, A A ^a  

^a MOSCOW STATE UNIVERSITY   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; MATHEMATICAL MODELS; MODULATION; NUCLEAR PHYSICS; SIMULATION;

COSMIC RAY MODULATION; GALACTIC COSMIC RAY FLUXES; SOLAR MODULATION; WOLF NUMBER;

COSMIC RAYS;

EID: 0030150730     PISSN: 13504487     EISSN: None     Source Type: Journal    
DOI: 10.1016/1350-4487(96)00049-2     Document Type: Article

References (8)

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3. Krainev M. B. (1991) Galactic cosmic ray intensity during the beginning of sun global magnetic field reversal. Izv. AN SSSR Ser. Phys. 55, 1942.
4. Kroeger R. (1986) Measurements of hydrogen and helium isotopes in galactic cosmic rays from 1978 through 1984. Astrophys. J. 303, 816.
5. McDonald F., Moraal H., Reinecke J. P. L., Lal N. and McGuire R. E. (1991) The cosmic radiation in the heliosphere at successive solar minima: observations. Galactic Cosmic Radiation: Constraints on Space Exploration. Naval Research Laboratory Publication 209-4154, 89.
6. Nymmik R. A., Panasyuk M. I., Pervaya T. I. and Suslov A. A. (1992) A model of galactic cosmic ray fluxes. Nucl. Tracks. Radiat. Meas. 20, 427.
7. Stuiver M. and Quay P. (1980) Changes in atmospheric carbon-14 attributed to a variable sun. Science 207, 4426, 11.
8. Suslov A. A. and Nymmik R. A. (1990) A semi-empirical model for large scale modulation of galactic cosmic ray energy spectra. In: Proc. 21st ICRC, Adelaide, Vol. 6, p. 33.