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Hard X-ray and gamma-ray spectrometer of high resolution and sensitivity on board the international space station (ISS)
The project of a spectrometer of hard X ( X h -rays and gamma-rays (approximate energy range 0.05 – 50 MeV) was proposed to a competition of scientific instruments to be accommodated onboard the international space station ( ISS). The objectives of this experiment are as follows: detailed study of a...
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| Published in: | Advances in space research 2000, Vol.25 (3), p.901-904 |
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| Main Authors: | , , , , , |
| Format: | Article |
| Language: | English |
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| cites | cdi_FETCH-LOGICAL-c201t-ec250790d38b0b97889cb322b29b1bc4389c05c0ad9da99247abbc258fdc05973 |
| container_end_page | 904 |
| container_issue | 3 |
| container_start_page | 901 |
| container_title | Advances in space research |
| container_volume | 25 |
| creator | Svertilov, S.I. Stolpovskii, V.G. Bogomolov, V.V. Kudryavtsev, M.I. Mitrofanov, I.G. Klapdor-Kleingrothaus, H.V. |
| description | The project of a spectrometer of hard
X (
X
h
-rays and gamma-rays (approximate energy range 0.05 – 50 MeV) was proposed to a competition of scientific instruments to be accommodated onboard the international space station (
ISS). The objectives of this experiment are as follows: detailed study of astrophysical phenomena including cosmic gamma-ray bursts (
GRB), lines in Galactic diffuse background,
e
+e
−
annihilation line from the Galactic Centre and high resolution observation of solar
X
h
-rays and gamma-radiation in lines and continuum. The spectrometer detector system includes three enriched
Ge crystals (each of ∼200 cm
3 volume) cooled to |
| doi_str_mv | 10.1016/S0273-1177(99)00864-9 |
| format | article |
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X (
X
h
-rays and gamma-rays (approximate energy range 0.05 – 50 MeV) was proposed to a competition of scientific instruments to be accommodated onboard the international space station (
ISS). The objectives of this experiment are as follows: detailed study of astrophysical phenomena including cosmic gamma-ray bursts (
GRB), lines in Galactic diffuse background,
e
+e
−
annihilation line from the Galactic Centre and high resolution observation of solar
X
h
-rays and gamma-radiation in lines and continuum. The spectrometer detector system includes three enriched
Ge crystals (each of ∼200 cm
3 volume) cooled to <100K and six NaI/CsI phoswich detectors (each of ∼10
4 cm
3 volume) with crossed axes. The effective instrument field of view is about π sr. The expected energy resolution at 1 MeV for
Ge and
NaI are ∼2 keV and ∼50 keV, respectively. The detection of solar flares neutrons is also possible by this instrument owing to the separation of different components of light flashes in
CsI. The program of
ISS provides a long exposure time for the detectors of the proposed spectrometer. Using results of the “
Grif-1” experiment onboard the “
Mir” station we obtain that it will be possible to accomplish precise
X
h
and gamma-measurements under background conditions onboard
ISS.</description><identifier>ISSN: 0273-1177</identifier><identifier>EISSN: 1879-1948</identifier><identifier>DOI: 10.1016/S0273-1177(99)00864-9</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><ispartof>Advances in space research, 2000, Vol.25 (3), p.901-904</ispartof><rights>2000 COSPAR</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c201t-ec250790d38b0b97889cb322b29b1bc4389c05c0ad9da99247abbc258fdc05973</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,4024,27923,27924,27925</link.rule.ids></links><search><creatorcontrib>Svertilov, S.I.</creatorcontrib><creatorcontrib>Stolpovskii, V.G.</creatorcontrib><creatorcontrib>Bogomolov, V.V.</creatorcontrib><creatorcontrib>Kudryavtsev, M.I.</creatorcontrib><creatorcontrib>Mitrofanov, I.G.</creatorcontrib><creatorcontrib>Klapdor-Kleingrothaus, H.V.</creatorcontrib><title>Hard X-ray and gamma-ray spectrometer of high resolution and sensitivity on board the international space station (ISS)</title><title>Advances in space research</title><description>The project of a spectrometer of hard
X (
X
h
-rays and gamma-rays (approximate energy range 0.05 – 50 MeV) was proposed to a competition of scientific instruments to be accommodated onboard the international space station (
ISS). The objectives of this experiment are as follows: detailed study of astrophysical phenomena including cosmic gamma-ray bursts (
GRB), lines in Galactic diffuse background,
e
+e
−
annihilation line from the Galactic Centre and high resolution observation of solar
X
h
-rays and gamma-radiation in lines and continuum. The spectrometer detector system includes three enriched
Ge crystals (each of ∼200 cm
3 volume) cooled to <100K and six NaI/CsI phoswich detectors (each of ∼10
4 cm
3 volume) with crossed axes. The effective instrument field of view is about π sr. The expected energy resolution at 1 MeV for
Ge and
NaI are ∼2 keV and ∼50 keV, respectively. The detection of solar flares neutrons is also possible by this instrument owing to the separation of different components of light flashes in
CsI. The program of
ISS provides a long exposure time for the detectors of the proposed spectrometer. Using results of the “
Grif-1” experiment onboard the “
Mir” station we obtain that it will be possible to accomplish precise
X
h
and gamma-measurements under background conditions onboard
ISS.</description><issn>0273-1177</issn><issn>1879-1948</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><recordid>eNqFkE1LAzEURYMoWD9-gpCV6GI0yUybeSsRUSsILqrgLiSZ1zYyM6lJqvTfm07FratwH-deyCHkjLMrzvjkesaELAvOpbwAuGSsnlQF7JERryUUHKp6n4z-kENyFOMHY1xIyUbke6pDQ9-LoDdU9w1d6K7TQ4ortCn4DhMG6ud06RZLGjD6dp2c7wc6Yh9dcl8ubWg-Gb8dS0ukrs-tXm9B3eYpbZHGNGR68TSbXZ6Qg7luI57-vsfk7eH-9W5aPL88Pt3dPhdWMJ4KtGLMJLCmrA0zIOsarCmFMAIMN7Yqc2Zjy3QDjQYQldTG5E49b_IdZHlMzne7q-A_1xiT6ly02La6R7-OSshxORFQZXC8A23wMQacq1VwnQ4bxZnaalaDZrV1qADUoFlB7t3seph_8eUwqGgd9hYbF7JA1Xj3z8IPsq-GDg</recordid><startdate>2000</startdate><enddate>2000</enddate><creator>Svertilov, S.I.</creator><creator>Stolpovskii, V.G.</creator><creator>Bogomolov, V.V.</creator><creator>Kudryavtsev, M.I.</creator><creator>Mitrofanov, I.G.</creator><creator>Klapdor-Kleingrothaus, H.V.</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TB</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>2000</creationdate><title>Hard X-ray and gamma-ray spectrometer of high resolution and sensitivity on board the international space station (ISS)</title><author>Svertilov, S.I. ; Stolpovskii, V.G. ; Bogomolov, V.V. ; Kudryavtsev, M.I. ; Mitrofanov, I.G. ; Klapdor-Kleingrothaus, H.V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c201t-ec250790d38b0b97889cb322b29b1bc4389c05c0ad9da99247abbc258fdc05973</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Svertilov, S.I.</creatorcontrib><creatorcontrib>Stolpovskii, V.G.</creatorcontrib><creatorcontrib>Bogomolov, V.V.</creatorcontrib><creatorcontrib>Kudryavtsev, M.I.</creatorcontrib><creatorcontrib>Mitrofanov, I.G.</creatorcontrib><creatorcontrib>Klapdor-Kleingrothaus, H.V.</creatorcontrib><collection>CrossRef</collection><collection>Mechanical & Transportation Engineering Abstracts</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Advances in space research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Svertilov, S.I.</au><au>Stolpovskii, V.G.</au><au>Bogomolov, V.V.</au><au>Kudryavtsev, M.I.</au><au>Mitrofanov, I.G.</au><au>Klapdor-Kleingrothaus, H.V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Hard X-ray and gamma-ray spectrometer of high resolution and sensitivity on board the international space station (ISS)</atitle><jtitle>Advances in space research</jtitle><date>2000</date><risdate>2000</risdate><volume>25</volume><issue>3</issue><spage>901</spage><epage>904</epage><pages>901-904</pages><issn>0273-1177</issn><eissn>1879-1948</eissn><abstract>The project of a spectrometer of hard
X (
X
h
-rays and gamma-rays (approximate energy range 0.05 – 50 MeV) was proposed to a competition of scientific instruments to be accommodated onboard the international space station (
ISS). The objectives of this experiment are as follows: detailed study of astrophysical phenomena including cosmic gamma-ray bursts (
GRB), lines in Galactic diffuse background,
e
+e
−
annihilation line from the Galactic Centre and high resolution observation of solar
X
h
-rays and gamma-radiation in lines and continuum. The spectrometer detector system includes three enriched
Ge crystals (each of ∼200 cm
3 volume) cooled to <100K and six NaI/CsI phoswich detectors (each of ∼10
4 cm
3 volume) with crossed axes. The effective instrument field of view is about π sr. The expected energy resolution at 1 MeV for
Ge and
NaI are ∼2 keV and ∼50 keV, respectively. The detection of solar flares neutrons is also possible by this instrument owing to the separation of different components of light flashes in
CsI. The program of
ISS provides a long exposure time for the detectors of the proposed spectrometer. Using results of the “
Grif-1” experiment onboard the “
Mir” station we obtain that it will be possible to accomplish precise
X
h
and gamma-measurements under background conditions onboard
ISS.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/S0273-1177(99)00864-9</doi><tpages>4</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0273-1177 |
| ispartof | Advances in space research, 2000, Vol.25 (3), p.901-904 |
| issn | 0273-1177 1879-1948 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_27536294 |
| source | ScienceDirect Freedom Collection 2022-2024 |
| title | Hard X-ray and gamma-ray spectrometer of high resolution and sensitivity on board the international space station (ISS) |
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