Abstract
We report a cosmic-ray antiproton spectrum measured with the BESS balloon experiment performed in 2002, which was in an intermediate period between the solar maximum in 2000 and the coming solar minimum. The observed antiproton spectrum and the antiproton to proton ratio are crucial for further development of the drift model of the solar modulation effect which has been generally supported by the previous measurements.
Original language | English |
---|---|
Pages | 13-16 |
Number of pages | 4 |
Publication status | Published - 2005 |
Externally published | Yes |
Event | 29th International Cosmic Ray Conference, ICRC 2005 - Pune, India Duration: Aug 3 2005 → Aug 10 2005 |
Other
Other | 29th International Cosmic Ray Conference, ICRC 2005 |
---|---|
Country/Territory | India |
City | Pune |
Period | 8/3/05 → 8/10/05 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics