On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements
| ISSN: |
1572-946X
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|---|---|
| Source: |
Springer Online Journal Archives 1860-2000
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| Topics: |
Physics
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| Notes: |
Abstract The diffuse X-ray background from 20 to 200 keV has been measured many times by rocket-, satellite-, and balloon-borne detectors. As has been noted by a number of authors, the balloon measurements do not agree with those outside the atmosphere. This suggests some systematic difference in the derivation of the diffuse flux. In the present article we propose a method for the analysis of balloon data in which the source function (atmospherically produced and scattered primary) is derived from the experimental data and is then used to calculate the residual counting rate due only to the transmitted primary photons.
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798296454042746880 |
|---|---|
| autor | Horstman-Moretti, E. Horstman, H. |
| autorsonst | Horstman-Moretti, E. Horstman, H. |
| book_url | http://dx.doi.org/10.1007/BF01093869 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLM193099349 |
| issn | 1572-946X |
| journal_name | Astrophysics and space science |
| materialart | 1 |
| notes | Abstract The diffuse X-ray background from 20 to 200 keV has been measured many times by rocket-, satellite-, and balloon-borne detectors. As has been noted by a number of authors, the balloon measurements do not agree with those outside the atmosphere. This suggests some systematic difference in the derivation of the diffuse flux. In the present article we propose a method for the analysis of balloon data in which the source function (atmospherically produced and scattered primary) is derived from the experimental data and is then used to calculate the residual counting rate due only to the transmitted primary photons. |
| package_name | Springer |
| publikationsjahr_anzeige | 1977 |
| publikationsjahr_facette | 1977 |
| publikationsjahr_intervall | 8024:1975-1979 |
| publikationsjahr_sort | 1977 |
| publisher | Springer |
| reference | 52 (1977), S. 307-311 |
| search_space | articles |
| shingle_author_1 | Horstman-Moretti, E. Horstman, H. |
| shingle_author_2 | Horstman-Moretti, E. Horstman, H. |
| shingle_author_3 | Horstman-Moretti, E. Horstman, H. |
| shingle_author_4 | Horstman-Moretti, E. Horstman, H. |
| shingle_catch_all_1 | Horstman-Moretti, E. Horstman, H. On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements Abstract The diffuse X-ray background from 20 to 200 keV has been measured many times by rocket-, satellite-, and balloon-borne detectors. As has been noted by a number of authors, the balloon measurements do not agree with those outside the atmosphere. This suggests some systematic difference in the derivation of the diffuse flux. In the present article we propose a method for the analysis of balloon data in which the source function (atmospherically produced and scattered primary) is derived from the experimental data and is then used to calculate the residual counting rate due only to the transmitted primary photons. 1572-946X 1572946X Springer |
| shingle_catch_all_2 | Horstman-Moretti, E. Horstman, H. On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements Abstract The diffuse X-ray background from 20 to 200 keV has been measured many times by rocket-, satellite-, and balloon-borne detectors. As has been noted by a number of authors, the balloon measurements do not agree with those outside the atmosphere. This suggests some systematic difference in the derivation of the diffuse flux. In the present article we propose a method for the analysis of balloon data in which the source function (atmospherically produced and scattered primary) is derived from the experimental data and is then used to calculate the residual counting rate due only to the transmitted primary photons. 1572-946X 1572946X Springer |
| shingle_catch_all_3 | Horstman-Moretti, E. Horstman, H. On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements Abstract The diffuse X-ray background from 20 to 200 keV has been measured many times by rocket-, satellite-, and balloon-borne detectors. As has been noted by a number of authors, the balloon measurements do not agree with those outside the atmosphere. This suggests some systematic difference in the derivation of the diffuse flux. In the present article we propose a method for the analysis of balloon data in which the source function (atmospherically produced and scattered primary) is derived from the experimental data and is then used to calculate the residual counting rate due only to the transmitted primary photons. 1572-946X 1572946X Springer |
| shingle_catch_all_4 | Horstman-Moretti, E. Horstman, H. On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements Abstract The diffuse X-ray background from 20 to 200 keV has been measured many times by rocket-, satellite-, and balloon-borne detectors. As has been noted by a number of authors, the balloon measurements do not agree with those outside the atmosphere. This suggests some systematic difference in the derivation of the diffuse flux. In the present article we propose a method for the analysis of balloon data in which the source function (atmospherically produced and scattered primary) is derived from the experimental data and is then used to calculate the residual counting rate due only to the transmitted primary photons. 1572-946X 1572946X Springer |
| shingle_title_1 | On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements |
| shingle_title_2 | On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements |
| shingle_title_3 | On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements |
| shingle_title_4 | On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Springer Online Journal Archives 1860-2000 |
| timestamp | 2024-05-06T09:52:21.317Z |
| titel | On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements |
| titel_suche | On a new method of separating the diffuse cosmic X-ray component in balloon-borne measurements |
| topic | U |
| uid | nat_lic_papers_NLM193099349 |