Rigidity dependence and time response of cosmic rays to the modulation steps in the rising part of solar cycle 23. COSPIN/KET results

Space Science Reviews

Volumn 97, Issue 1-4, 2001, Pages 349-354

  Paizis, C ^a,d   Raviart, A ^b   Heber, B ^c   Falconi, B ^d   Ferrando, Ph ^b   Kunow, H ^e   Muller Mellin R ^e  

^a UNIVERSITY OF MILAN   (Italy)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^d CNR   (Italy)

^e UNIVERSITY OF KIEL   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

ASTRONOMY; ATOMIC PARTICLE; CONFERENCE PAPER; COSMIC RADIATION; ELECTRON; FREQUENCY MODULATION; PARTICLE RADIATION; PHYSICS; RIGIDITY; SUN; TIME;

EID: 0034806063     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1011801722658     Document Type: Conference Paper

References (6)

1. Rigidity dependence of near-Earth latitudinal proton density gradients
2. Spatial variation of >40 MeV/n nuclei fluxes observed during the Ulysses rapid latitude scan
3. Cosmic ray modulation over the poles at solar maximum: Observations
4. Amplitude evolution and rigidity dependence of the 26-day recurrent cosmic ray decreases: COSPIN/KET results
5. The causes of the 11-year and the 22-year cycles in cosmic-ray modulation
6. The Ulysses cosmic ray and solar particle investigation