Abstract
Observations of Ultra-Heavy galactic cosmic rays (GCR) help to distinguish the possible origins of GCRs. The Trans-Iron Galactic Element Recorder (TIGER) measures the charge (Z) and energy of GCRs using a combination of scintillation counters, Cherenkov counters, and a scintillating fiber hodoscope. TIGER has accumulated data on two successful flights from McMurdo, Antarctica: the first launched in December of 2001 with a total flight duration of 31.8 days and the second in December of 2003 with a total flight duration of 18 days. We present a preliminary analysis of the combined data from both flights for Ultra-Heavy GCRs.
| Original language | English |
|---|---|
| Pages | 93-96 |
| Number of pages | 4 |
| State | Published - 2005 |
| Event | 29th International Cosmic Ray Conference, ICRC 2005 - Pune, India Duration: Aug 3 2005 → Aug 10 2005 |
Conference
| Conference | 29th International Cosmic Ray Conference, ICRC 2005 |
|---|---|
| Country/Territory | India |
| City | Pune |
| Period | 08/3/05 → 08/10/05 |