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OSO-G satellite instrumentation for measurements of cosmic X-rays in the energy range from 25 to 190 keV

Оборудование спутника OSO-G для измерений космических гамма-лучей в области знергий от 25 до 190 кэВ

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Il Nuovo Cimento B (1971-1996)

Summary

An experiment for the detection of solar and celestial X-rays in the energy range from about 20 keV to about 200 keV has been prepared for operation aboard the NASA satellite OSO-G. This paper presents details of design and assembly to meet flight specifications and scientific objectives. The instrument is presently in orbital operation.

Riassunto

Un esperimento per la rivelazione dei raggi X solari e celesti nel campo di energia da circa 20 keV a circa 200 keV è stato preparato per funzionare a bordo del satellite NASA OSO-G. Questo lavoro descrive dettagliatamente il progetto e la sua realizzazione capace di soddisfare le esigenze di volo e gli obiettivi scientifici. Lo strumento è attualmente operante in orbita.

Резюме

Был подготовлен эксперимент для проведения на борту спутника HACA OSO-G по детектированию солнечных и небесных гамма-лучей в области энергий приблизительно от 20 кэВ до 200 кэВ. В этой статье подробно описывается схема и сборка с учетом технических условий полета и научных целей. В настоящее время с помощью этого оборудования проводятся орбитальные исследования.

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References

  1. D. Brini, U. Ciriegi andF. Fuligni:Ric. Sci.,6, 565 (1964).

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  2. D. Brini, F. Fuligni andE. Moretti-Horstman:Nonsolar X- and γ-ray astronomy, inI.A.U. Rome Symposium, 1969, edited byL. Gratton.

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Authors and Affiliations

  1. Laboratory TE.S.R.E. of C.N.R., Space Research Group, Istituto di Fisica dell’Università, Bologna

    D. Brini, F. Evangelisti, F. Fuligni & G. Vespignani

Authors
  1. D. Brini
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  2. F. Evangelisti
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  3. F. Fuligni
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  4. G. Vespignani
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Brini, D., Evangelisti, F., Fuligni, F. et al. OSO-G satellite instrumentation for measurements of cosmic X-rays in the energy range from 25 to 190 keV. Nuov Cim B 2, 193–207 (1971). https://doi.org/10.1007/BF02723083

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  • DOI: https://doi.org/10.1007/BF02723083

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