Low-energy charged particle ring around equator in the altitude range 400–1100 km
Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Kaul, R. K. [verfasserIn] |
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| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1977 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1977 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 46(1977), 1 vom: Jan., Seite 215-223 |
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| Übergeordnetes Werk: |
volume:46 ; year:1977 ; number:1 ; month:01 ; pages:215-223 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00643766 |
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| Katalog-ID: |
OLC2066128929 |
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| 520 | |a Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. | ||
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10.1007/BF00643766 doi (DE-627)OLC2066128929 (DE-He213)BF00643766-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kaul, R. K. verfasserin aut Low-energy charged particle ring around equator in the altitude range 400–1100 km 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. Detector System Energy Spectrum Charged Particle Energy Particle Geometrical Factor Razdan, H. aut Lockwood, J. A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 46(1977), 1 vom: Jan., Seite 215-223 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:46 year:1977 number:1 month:01 pages:215-223 https://doi.org/10.1007/BF00643766 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 46 1977 1 01 215-223 |
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10.1007/BF00643766 doi (DE-627)OLC2066128929 (DE-He213)BF00643766-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kaul, R. K. verfasserin aut Low-energy charged particle ring around equator in the altitude range 400–1100 km 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. Detector System Energy Spectrum Charged Particle Energy Particle Geometrical Factor Razdan, H. aut Lockwood, J. A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 46(1977), 1 vom: Jan., Seite 215-223 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:46 year:1977 number:1 month:01 pages:215-223 https://doi.org/10.1007/BF00643766 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 46 1977 1 01 215-223 |
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10.1007/BF00643766 doi (DE-627)OLC2066128929 (DE-He213)BF00643766-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kaul, R. K. verfasserin aut Low-energy charged particle ring around equator in the altitude range 400–1100 km 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. Detector System Energy Spectrum Charged Particle Energy Particle Geometrical Factor Razdan, H. aut Lockwood, J. A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 46(1977), 1 vom: Jan., Seite 215-223 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:46 year:1977 number:1 month:01 pages:215-223 https://doi.org/10.1007/BF00643766 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 46 1977 1 01 215-223 |
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10.1007/BF00643766 doi (DE-627)OLC2066128929 (DE-He213)BF00643766-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kaul, R. K. verfasserin aut Low-energy charged particle ring around equator in the altitude range 400–1100 km 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. Detector System Energy Spectrum Charged Particle Energy Particle Geometrical Factor Razdan, H. aut Lockwood, J. A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 46(1977), 1 vom: Jan., Seite 215-223 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:46 year:1977 number:1 month:01 pages:215-223 https://doi.org/10.1007/BF00643766 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 46 1977 1 01 215-223 |
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10.1007/BF00643766 doi (DE-627)OLC2066128929 (DE-He213)BF00643766-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kaul, R. K. verfasserin aut Low-energy charged particle ring around equator in the altitude range 400–1100 km 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. Detector System Energy Spectrum Charged Particle Energy Particle Geometrical Factor Razdan, H. aut Lockwood, J. A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 46(1977), 1 vom: Jan., Seite 215-223 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:46 year:1977 number:1 month:01 pages:215-223 https://doi.org/10.1007/BF00643766 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 46 1977 1 01 215-223 |
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Enthalten in Astrophysics and space science 46(1977), 1 vom: Jan., Seite 215-223 volume:46 year:1977 number:1 month:01 pages:215-223 |
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Kaul, R. K. |
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520 530 620 VZ 16,12 ssgn Low-energy charged particle ring around equator in the altitude range 400–1100 km Detector System Energy Spectrum Charged Particle Energy Particle Geometrical Factor |
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Low-energy charged particle ring around equator in the altitude range 400–1100 km |
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Low-energy charged particle ring around equator in the altitude range 400–1100 km |
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Kaul, R. K. |
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Astrophysics and space science |
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1977 |
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Kaul, R. K. Razdan, H. Lockwood, J. A. |
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10.1007/BF00643766 |
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low-energy charged particle ring around equator in the altitude range 400–1100 km |
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Low-energy charged particle ring around equator in the altitude range 400–1100 km |
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Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. © D. Reidel Publishing Company 1977 |
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Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. © D. Reidel Publishing Company 1977 |
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Abstract Measurements of charged particle fluxes at energies >-13 MeV (if protons), by means of a detector system of high geometrical factor (950 $ cm^{2} $ sr), flown on OGO-6 satellite, reveals a ring of low energy charged particles around equator with fluxes of the order of 50–70 particles ($ m^{−2} $ $ s^{−1} $ $ sr^{−1} $), in the altitude range of 400–1100 km. The ring of charged particles exists below the inner radiation belt and is restricted to ±4° of the geomagnetic equator. Distribution of the maximum flux with geomagnetic latitude andL is presented. Comparison of the observed fluxes with earlier measurements of low energy particles, reveals a differential energy spectrum of the type $ KE^{−γ} $ with the exponent nearly equal to 2.4 to 3. © D. Reidel Publishing Company 1977 |
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Low-energy charged particle ring around equator in the altitude range 400–1100 km |
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