Radiation belts in the region of the South-Atlantic magnetic anomaly
Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere....
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Vernov, S. N. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1967 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1967 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Kluwer Academic Publishers, 1962, 7(1967), 4 vom: Nov., Seite 490-533 |
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| Übergeordnetes Werk: |
volume:7 ; year:1967 ; number:4 ; month:11 ; pages:490-533 |
| Links: |
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| DOI / URN: |
10.1007/BF00182684 |
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| Katalog-ID: |
OLC2033659569 |
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| 520 | |a Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. | ||
| 650 | 4 | |a Magnetic Anomaly | |
| 650 | 4 | |a Particle Intensity | |
| 650 | 4 | |a Radiation Belt | |
| 650 | 4 | |a Trap Particle | |
| 650 | 4 | |a Radiation Study | |
| 700 | 1 | |a Gorchakov, E. V. |4 aut | |
| 700 | 1 | |a Shavrin, P. I. |4 aut | |
| 700 | 1 | |a Sharvina, K. N. |4 aut | |
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10.1007/BF00182684 doi (DE-627)OLC2033659569 (DE-He213)BF00182684-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vernov, S. N. verfasserin aut Radiation belts in the region of the South-Atlantic magnetic anomaly 1967 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1967 Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. Magnetic Anomaly Particle Intensity Radiation Belt Trap Particle Radiation Study Gorchakov, E. V. aut Shavrin, P. I. aut Sharvina, K. N. aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 7(1967), 4 vom: Nov., Seite 490-533 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:7 year:1967 number:4 month:11 pages:490-533 https://doi.org/10.1007/BF00182684 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2015 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4314 AR 7 1967 4 11 490-533 |
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10.1007/BF00182684 doi (DE-627)OLC2033659569 (DE-He213)BF00182684-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vernov, S. N. verfasserin aut Radiation belts in the region of the South-Atlantic magnetic anomaly 1967 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1967 Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. Magnetic Anomaly Particle Intensity Radiation Belt Trap Particle Radiation Study Gorchakov, E. V. aut Shavrin, P. I. aut Sharvina, K. N. aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 7(1967), 4 vom: Nov., Seite 490-533 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:7 year:1967 number:4 month:11 pages:490-533 https://doi.org/10.1007/BF00182684 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2015 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4314 AR 7 1967 4 11 490-533 |
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10.1007/BF00182684 doi (DE-627)OLC2033659569 (DE-He213)BF00182684-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vernov, S. N. verfasserin aut Radiation belts in the region of the South-Atlantic magnetic anomaly 1967 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1967 Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. Magnetic Anomaly Particle Intensity Radiation Belt Trap Particle Radiation Study Gorchakov, E. V. aut Shavrin, P. I. aut Sharvina, K. N. aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 7(1967), 4 vom: Nov., Seite 490-533 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:7 year:1967 number:4 month:11 pages:490-533 https://doi.org/10.1007/BF00182684 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2015 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4314 AR 7 1967 4 11 490-533 |
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10.1007/BF00182684 doi (DE-627)OLC2033659569 (DE-He213)BF00182684-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vernov, S. N. verfasserin aut Radiation belts in the region of the South-Atlantic magnetic anomaly 1967 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1967 Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. Magnetic Anomaly Particle Intensity Radiation Belt Trap Particle Radiation Study Gorchakov, E. V. aut Shavrin, P. I. aut Sharvina, K. N. aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 7(1967), 4 vom: Nov., Seite 490-533 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:7 year:1967 number:4 month:11 pages:490-533 https://doi.org/10.1007/BF00182684 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2015 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4314 AR 7 1967 4 11 490-533 |
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10.1007/BF00182684 doi (DE-627)OLC2033659569 (DE-He213)BF00182684-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vernov, S. N. verfasserin aut Radiation belts in the region of the South-Atlantic magnetic anomaly 1967 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1967 Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. Magnetic Anomaly Particle Intensity Radiation Belt Trap Particle Radiation Study Gorchakov, E. V. aut Shavrin, P. I. aut Sharvina, K. N. aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 7(1967), 4 vom: Nov., Seite 490-533 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:7 year:1967 number:4 month:11 pages:490-533 https://doi.org/10.1007/BF00182684 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2015 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4314 AR 7 1967 4 11 490-533 |
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radiation belts in the region of the south-atlantic magnetic anomaly |
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Radiation belts in the region of the South-Atlantic magnetic anomaly |
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Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. © D. Reidel Publishing Company 1967 |
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Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. © D. Reidel Publishing Company 1967 |
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Conclusion The difference of the geomagnetic field from the field of the idealized dipole not only creates certain difficulties for studying the geomagnetically trapped radiation but also presents new possibilities for studying the processes which control the particle movement in the magnetosphere. It will be remembered that the fact that the geomagnetic field is not a dipole played a decisive role in the very beginning of the formation of our ideas about the nature of the intense fluxes of the penetrating radiation detected during the satellite flights. In fact, the longitude dependence of the lower boundary of the penetrating radiation in the region of low latitudes according to the properties of the geomagnetic field made it possible to conclude immediately that the detected radiation was caused by the geomagnetically trapped particles. As to the difficulties in the trapped radiation study caused by the existence of the anomalies, they, first of all, result in the original and, at the first glance, incomprehensible form of the particle intensity contours drawn in geographical coordinates for low altitudes. However, when turning to the McIlwain coordinate system, which is naturally connected with the real magnetic field, the seeming chaos in the radiation distribution disappears being unexpectedly replaced by harmony and order. But even in this coordinate system some ambiguities are observed connected with the distortion of the adiabatic invariants during the time comparable with the period of the particle drift around the earth. The thorough analysis of these effects in combination with the observations of the radiation at high altitudes may answer such a principle question as the question about the velocity of the movements of the mirror points. It should be noted that some information has been obtained to date on the movement of the electron-mirror points only and similar information about protons is absent. It is possible that new aspects of the use of the magnetic anomalies for studying the geomagnetosphere will appear in due time. © D. Reidel Publishing Company 1967 |
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