3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
Contribution Poster
Merida, Mexico
-
Regency (Hyatt)
SH.2.3
Recurrent variations in the high-energy cosmic ray intensity
Speakers
- Dr. Sardaana GERASIMOVA
Primary authors
- Prof. Germogen KRYMSKY (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS)
Co-authors
- Dr. Velikanida MAMRUKOVA (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS)
- Dr. Prokopii KRIVOSHAPKIN (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS)
- Dr. Sardaana GERASIMOVA (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS)
- Sergey STARODUBTSEV (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS)
Files
Abstract content
Recurrent variations and their relation to the solar activity and solar wind parameters are investigated on the basis of the cosmic ray intensity data for 4 solar cycles by means of the spectral analysis method.
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 1 (SH), pages 381-384