Cosmic ray variation effects in the temperature of the high-latitudinal atmosphere

Advances in Space Research

Volumn 17, Issue 11, 1996, Pages 165-168

  Pudovkin, M I ^a   Veretenenko, S V ^a   Pellinen, R ^b   Kyro E ^b  

^a ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^b FINNISH METEOROLOGICAL INSTITUTE   (Finland)

Author keywords

[No Author keywords available]

Indexed keywords

ATMOSPHERIC TEMPERATURE PROFILE; CLOUD FORMATION; COSMIC RAY VARIATION; STRATOSPHERE IONIZATION;

FINLAND, LAPI, SODANKYLA;

EID: 0029750019     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00746-2     Document Type: Article

References (5)

1. M.I. Pudovkin and S.V. Veretenenko, this issue.
2. M.I. Pudovkin and S.V. Babushkina, J. Atm. Terr. Phys., 54(7/8), 841-846, (1992).
3. C.J.E. Schuurmans and A.H. Oort, Pure Appl. Geophys., 75, 233-246, (1969).
4. Yu.I. Logachev (ed.), Solar proton events. Catalogue 1980-1986., Soviet geophysical committee of the Academy of Sciences of the USSR, Moscow, 1990 (in Russian).
5. L.T. Matveev, Textbook on meteorology. Physics of atmosphere. Hydrometeoizdat, Leningrad,1976 (in Russian).