Isotropic background cosmic X-rays in the energy range 50–290 KeV
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Chemistry
Link
http://link.springer.com/content/pdf/10.1007/BF03049343.pdf
Reference11 articles.
1. Bleeker, J. A. M., Burger, J. J., Deerenberg, A. J. M., Swanenburg, B. N. and Tanaka, Y. “Balloon observation of the X-ray sources in the cygnus,”Ap. J., 1967,147, 391–94.
2. Brini, D., Ciriegi, U., Fulgni, F., Gandolfi, A. and Moretti, E. “Evaluation of the X-ray primary omnidirectional flux from measurements at balloon altitudes,”Nuovo Cimento, 1965,38, 4710–20.
3. Chubb, T. A., Kreplin, R. W. and Friedman, H. “Observations of hard X-ray emission from solar flares,”J. Geophys. Research, 1966,71, 3611–22.
4. Edwards, P. J. and McCracken, K. G. “Upper limits to the hard X-ray flux from the quiet sun and Jupiter,” Ibid., 1967,72, 1809–12.
5. Frost, K. J., Rothe, E. D. and Peterson, L. E. “A search for the quet-time solar gamma rays from balloon altitudes,” Ibid., 1966,71, 4079–089.
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1. Diffuse X-ray background measurements in the energy range 2?18 keV;Astrophysics and Space Science;1971-01
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