Abstract
A new instrument for direct measurements of the individual energy spectra of heavy cosmic-ray nuclei in the energy range from 1011 to several 1014 eV shall be described. The instrument performance is discussed, using first results from a 28-hour balloon flight and from an accelerator calibration.
| Original language | English |
|---|---|
| Pages (from-to) | 142-145 |
| Number of pages | 4 |
| Journal | Nuclear Physics B - Proceedings Supplements |
| Volume | 97 |
| Issue number | 1-3 |
| DOIs | |
| Publication status | Published - Apr 2001 |
| Externally published | Yes |
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