X-Ray Telescope for an Orbiting Solar Observatory
The X-ray experiment described here was designed to monitor the intensity, energy distribution, and time variations of solar X-rays, and to measure the intensity and angular distribution of X-rays over the celestial sphere. The detector, which operates between about 7 to 200 Kev, will also monitor l...
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Veröffentlicht in: | IEEE (Inst. Elec. Electron. Engrs.), Trans. Nucl. Sci Trans. Nucl. Sci, 1965-02, Vol.12 (1), p.54-65 |
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