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Search for galactic γ-rays with energies greater than 500 MeV on board OGO-5

Published online by Cambridge University Press:  14 August 2015

J. A. M. Bleeker ,
J. J. Burger ,
A. J. M. Deerenberg ,
H. C. Van De Hulst ,
A. Scheepmaker ,
B. N. Swanenburg  and
Y. Tanaka
J. A. M. Bleeker
Affiliation:
Cosmic Ray Working Group, Kamerlingh Onnes Laboratorium, Leyden, The Netherlands
J. J. Burger
Affiliation:
Cosmic Ray Working Group, Kamerlingh Onnes Laboratorium, Leyden, The Netherlands
A. J. M. Deerenberg
Affiliation:
Cosmic Ray Working Group, Kamerlingh Onnes Laboratorium, Leyden, The Netherlands
H. C. Van De Hulst
Affiliation:
Cosmic Ray Working Group, Kamerlingh Onnes Laboratorium, Leyden, The Netherlands
A. Scheepmaker
Affiliation:
Cosmic Ray Working Group, Kamerlingh Onnes Laboratorium, Leyden, The Netherlands
B. N. Swanenburg
Affiliation:
Cosmic Ray Working Group, Kamerlingh Onnes Laboratorium, Leyden, The Netherlands
Y. Tanaka
Affiliation:
Dept. of Physics, Nagoya University, Nagoya, Japan

Extract

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A cosmic ray detector, sensitive to γ-Rays with energies greater than 500 MeV is being flown on board the OGO-5 satellite. The spacecraft was launched into a highly eccentric orbit, apogee 145000 km, on March 4, 1968. γ-Ray observations are restricted to altitudes higher than 80000 km, thereby excluding interference from the radiation belts and reducing the influence from the earth albedo flux. A description of the instrument is published in the literature (Rogowski et al., 1969).

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 297 - 299
Copyright
Copyright © Reidel 1970 

References

Clark, G. W., Garmire, G. P., and Kraushaar, W. L.: 1968, Astrophys. J. Letters 153, L203.CrossRefGoogle Scholar
Rogowski, L. K., Hicks, D. B., Gilland, J. R., and Swanenburg, B. N.: 1969, IEEE Trans. Nucl. Science NS—16, 325.CrossRefGoogle Scholar