| タイトル | The Energetic Trans-Iron Nuclei Experiment (ENTICE) |
| 著者（英） | Denolfo, G. A.; Israel, M. H.; Binns, W. R.; Cummings, A. C.; Leske, R. A.; Hams, T.; Mewaldt, R. A.; Christian, E. R.; Labrador, A. W.; Link, J. T.; Adams, J. H.; Sasaki, M.; Wiedenbeck, M. E.; Waddington, C. J.; Mitchell, J. W.; Stone, E. C. |
| 著者所属（英） | NASA Marshall Space Flight Center |
| 発行日 | 2009-07-07 |
| 言語 | eng |
| 内容記述 | The ENTICE experiment is one of two instruments that comprise the "Orbiting Astrophysical Spectrometer in Space (OASIS)" which is presently undergoing a NASA "Astrophysics Strategic Mission Concept Study". ENTICE is designed to make high precision measurements of the abundances of individual elements from neon through the actinides and, in addition, will search for possible superheavy nuclei in the galactic cosmic rays. The ENTICE instrument utilizes silicon detectors, aerogel and acrylic Cherenkov counters, and a scintillating optical fiber hodoscope to measure the charge and energy of these ultra-heavy nuclei for energies greater than 0.3 GeV/nucleon. It is a large instrument consisting of four modules with a total effective geometrical factor of ~20 m2sr. Measurements made in space for a period of 3 years with ENTICE will enable us to determine if cosmic rays include a component of recently synthesized heavy elements (Pu and Cm), what the age of that component is, and test the model of the OB association origin of galactic cosmic rays. Additionally, it will enable us to study how diffusive shock acceleration of cosmic rays operates differently on interstellar grains and gas. |
| NASA分類 | Astrophysics |
| レポートNO | M09-0351 |
| 権利 | Copyright |
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