Analysis of narrow spikes in two cosmic gamma-ray bursts
Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on...
Ausführliche Beschreibung
Autor*in: |
Imhof, W. L. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1976 |
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Schlagwörter: |
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Anmerkung: |
© D. Reidel Publishing Company 1976 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 42(1976), 1 vom: Juni, Seite 43-47 |
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Übergeordnetes Werk: |
volume:42 ; year:1976 ; number:1 ; month:06 ; pages:43-47 |
Links: |
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DOI / URN: |
10.1007/BF00645522 |
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Katalog-ID: |
OLC2066127434 |
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10.1007/BF00645522 doi (DE-627)OLC2066127434 (DE-He213)BF00645522-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Imhof, W. L. verfasserin aut Analysis of narrow spikes in two cosmic gamma-ray bursts 1976 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1976 Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. Germanium Time Resolution Satellite System Fast Time Time Structure Nakano, G. H. aut Reagan, J. B. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 42(1976), 1 vom: Juni, Seite 43-47 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:42 year:1976 number:1 month:06 pages:43-47 https://doi.org/10.1007/BF00645522 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 42 1976 1 06 43-47 |
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10.1007/BF00645522 doi (DE-627)OLC2066127434 (DE-He213)BF00645522-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Imhof, W. L. verfasserin aut Analysis of narrow spikes in two cosmic gamma-ray bursts 1976 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1976 Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. Germanium Time Resolution Satellite System Fast Time Time Structure Nakano, G. H. aut Reagan, J. B. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 42(1976), 1 vom: Juni, Seite 43-47 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:42 year:1976 number:1 month:06 pages:43-47 https://doi.org/10.1007/BF00645522 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 42 1976 1 06 43-47 |
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10.1007/BF00645522 doi (DE-627)OLC2066127434 (DE-He213)BF00645522-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Imhof, W. L. verfasserin aut Analysis of narrow spikes in two cosmic gamma-ray bursts 1976 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1976 Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. Germanium Time Resolution Satellite System Fast Time Time Structure Nakano, G. H. aut Reagan, J. B. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 42(1976), 1 vom: Juni, Seite 43-47 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:42 year:1976 number:1 month:06 pages:43-47 https://doi.org/10.1007/BF00645522 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 42 1976 1 06 43-47 |
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10.1007/BF00645522 doi (DE-627)OLC2066127434 (DE-He213)BF00645522-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Imhof, W. L. verfasserin aut Analysis of narrow spikes in two cosmic gamma-ray bursts 1976 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1976 Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. Germanium Time Resolution Satellite System Fast Time Time Structure Nakano, G. H. aut Reagan, J. B. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 42(1976), 1 vom: Juni, Seite 43-47 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:42 year:1976 number:1 month:06 pages:43-47 https://doi.org/10.1007/BF00645522 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 42 1976 1 06 43-47 |
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10.1007/BF00645522 doi (DE-627)OLC2066127434 (DE-He213)BF00645522-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Imhof, W. L. verfasserin aut Analysis of narrow spikes in two cosmic gamma-ray bursts 1976 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1976 Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. Germanium Time Resolution Satellite System Fast Time Time Structure Nakano, G. H. aut Reagan, J. B. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 42(1976), 1 vom: Juni, Seite 43-47 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:42 year:1976 number:1 month:06 pages:43-47 https://doi.org/10.1007/BF00645522 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 42 1976 1 06 43-47 |
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Imhof, W. L. |
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Analysis of narrow spikes in two cosmic gamma-ray bursts |
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Analysis of narrow spikes in two cosmic gamma-ray bursts |
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Imhof, W. L. |
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Imhof, W. L. Nakano, G. H. Reagan, J. B. |
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title_sort |
analysis of narrow spikes in two cosmic gamma-ray bursts |
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Analysis of narrow spikes in two cosmic gamma-ray bursts |
abstract |
Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. © D. Reidel Publishing Company 1976 |
abstractGer |
Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. © D. Reidel Publishing Company 1976 |
abstract_unstemmed |
Abstract An analysis has been made of the narrow intensity spikes occurring in two cosmic gammaray bursts which were observed with a fast time resolution germanium spectrometer on board the low altitude polar orbiting satellite 1972-076B (Imhofet al., 1974a, 1975; Nakanoet al., 1974a). The bursts on 18 December, 1972 and 21 July, 1973, were also recorded on the Vela satellite system. The durations of three spikes were observed to be ∼0.06 s with the limits being 0.03 to 0.10 s. Four other narrow spikes were measured to have time width limits between 0.001 and 0.10 s. An additional eight spikes had widths less than 0.9 s. During the spikes, the gamma-ray intensities increased by factors of ∼2 to ∼10, with a median value of ∼3. These and other characteristics of the fast time structure are presented. © D. Reidel Publishing Company 1976 |
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Analysis of narrow spikes in two cosmic gamma-ray bursts |
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