Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere

Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Yau, A. W. [verfasserIn] Garbe, G. P. [verfasserIn] Greffen, M. J. [verfasserIn] Miyake, W. [verfasserIn] Sagawa, E. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	1998

Schlagwörter:	Solar Wind Topside Ionosphere Plasma Drift Solar Wind Interaction Martian Ionosphere

Anmerkung:	© The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998

Übergeordnetes Werk:	Enthalten in: Earth, planets and space - Springer Berlin Heidelberg, 1998, 50(1998), 3 vom: März, Seite 195-198
Übergeordnetes Werk:	volume:50 ; year:1998 ; number:3 ; month:03 ; pages:195-198

Links:	Volltext

DOI / URN:	10.1186/BF03352103

Katalog-ID:	SPR036894141

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allfields	10.1186/BF03352103 doi (DE-627)SPR036894141 (SPR)BF03352103-e DE-627 ger DE-627 rakwb eng 550 VZ 38.70 bkl 39.22 bkl Yau, A. W. verfasserin aut Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere 1998 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998 Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. Solar Wind (dpeaa)DE-He213 Topside Ionosphere (dpeaa)DE-He213 Plasma Drift (dpeaa)DE-He213 Solar Wind Interaction (dpeaa)DE-He213 Martian Ionosphere (dpeaa)DE-He213 Garbe, G. P. verfasserin aut Greffen, M. J. verfasserin aut Miyake, W. verfasserin aut Sagawa, E. verfasserin aut Enthalten in Earth, planets and space Springer Berlin Heidelberg, 1998 50(1998), 3 vom: März, Seite 195-198 (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:50 year:1998 number:3 month:03 pages:195-198 https://dx.doi.org/10.1186/BF03352103 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 38.70 VZ 39.22 VZ AR 50 1998 3 03 195-198
spelling	10.1186/BF03352103 doi (DE-627)SPR036894141 (SPR)BF03352103-e DE-627 ger DE-627 rakwb eng 550 VZ 38.70 bkl 39.22 bkl Yau, A. W. verfasserin aut Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere 1998 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998 Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. Solar Wind (dpeaa)DE-He213 Topside Ionosphere (dpeaa)DE-He213 Plasma Drift (dpeaa)DE-He213 Solar Wind Interaction (dpeaa)DE-He213 Martian Ionosphere (dpeaa)DE-He213 Garbe, G. P. verfasserin aut Greffen, M. J. verfasserin aut Miyake, W. verfasserin aut Sagawa, E. verfasserin aut Enthalten in Earth, planets and space Springer Berlin Heidelberg, 1998 50(1998), 3 vom: März, Seite 195-198 (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:50 year:1998 number:3 month:03 pages:195-198 https://dx.doi.org/10.1186/BF03352103 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 38.70 VZ 39.22 VZ AR 50 1998 3 03 195-198
allfields_unstemmed	10.1186/BF03352103 doi (DE-627)SPR036894141 (SPR)BF03352103-e DE-627 ger DE-627 rakwb eng 550 VZ 38.70 bkl 39.22 bkl Yau, A. W. verfasserin aut Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere 1998 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998 Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. Solar Wind (dpeaa)DE-He213 Topside Ionosphere (dpeaa)DE-He213 Plasma Drift (dpeaa)DE-He213 Solar Wind Interaction (dpeaa)DE-He213 Martian Ionosphere (dpeaa)DE-He213 Garbe, G. P. verfasserin aut Greffen, M. J. verfasserin aut Miyake, W. verfasserin aut Sagawa, E. verfasserin aut Enthalten in Earth, planets and space Springer Berlin Heidelberg, 1998 50(1998), 3 vom: März, Seite 195-198 (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:50 year:1998 number:3 month:03 pages:195-198 https://dx.doi.org/10.1186/BF03352103 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 38.70 VZ 39.22 VZ AR 50 1998 3 03 195-198
allfieldsGer	10.1186/BF03352103 doi (DE-627)SPR036894141 (SPR)BF03352103-e DE-627 ger DE-627 rakwb eng 550 VZ 38.70 bkl 39.22 bkl Yau, A. W. verfasserin aut Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere 1998 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998 Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. Solar Wind (dpeaa)DE-He213 Topside Ionosphere (dpeaa)DE-He213 Plasma Drift (dpeaa)DE-He213 Solar Wind Interaction (dpeaa)DE-He213 Martian Ionosphere (dpeaa)DE-He213 Garbe, G. P. verfasserin aut Greffen, M. J. verfasserin aut Miyake, W. verfasserin aut Sagawa, E. verfasserin aut Enthalten in Earth, planets and space Springer Berlin Heidelberg, 1998 50(1998), 3 vom: März, Seite 195-198 (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:50 year:1998 number:3 month:03 pages:195-198 https://dx.doi.org/10.1186/BF03352103 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 38.70 VZ 39.22 VZ AR 50 1998 3 03 195-198
allfieldsSound	10.1186/BF03352103 doi (DE-627)SPR036894141 (SPR)BF03352103-e DE-627 ger DE-627 rakwb eng 550 VZ 38.70 bkl 39.22 bkl Yau, A. W. verfasserin aut Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere 1998 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998 Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. Solar Wind (dpeaa)DE-He213 Topside Ionosphere (dpeaa)DE-He213 Plasma Drift (dpeaa)DE-He213 Solar Wind Interaction (dpeaa)DE-He213 Martian Ionosphere (dpeaa)DE-He213 Garbe, G. P. verfasserin aut Greffen, M. J. verfasserin aut Miyake, W. verfasserin aut Sagawa, E. verfasserin aut Enthalten in Earth, planets and space Springer Berlin Heidelberg, 1998 50(1998), 3 vom: März, Seite 195-198 (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:50 year:1998 number:3 month:03 pages:195-198 https://dx.doi.org/10.1186/BF03352103 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 38.70 VZ 39.22 VZ AR 50 1998 3 03 195-198
language	English
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topic_facet	Solar Wind Topside Ionosphere Plasma Drift Solar Wind Interaction Martian Ionosphere
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authorswithroles_txt_mv	Yau, A. W. @@aut@@ Garbe, G. P. @@aut@@ Greffen, M. J. @@aut@@ Miyake, W. @@aut@@ Sagawa, E. @@aut@@
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author	Yau, A. W.
spellingShingle	Yau, A. W. ddc 550 bkl 38.70 bkl 39.22 misc Solar Wind misc Topside Ionosphere misc Plasma Drift misc Solar Wind Interaction misc Martian Ionosphere Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere
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topic_title	550 VZ 38.70 bkl 39.22 bkl Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere Solar Wind (dpeaa)DE-He213 Topside Ionosphere (dpeaa)DE-He213 Plasma Drift (dpeaa)DE-He213 Solar Wind Interaction (dpeaa)DE-He213 Martian Ionosphere (dpeaa)DE-He213
topic	ddc 550 bkl 38.70 bkl 39.22 misc Solar Wind misc Topside Ionosphere misc Plasma Drift misc Solar Wind Interaction misc Martian Ionosphere
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title	Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere
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title_full	Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere
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title_sort	planned observations of thermal plasma drifts and solar wind interactions in the martian ionosphere
title_auth	Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere
abstract	Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998
abstractGer	Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998
abstract_unstemmed	Abstract The structure and dynamics of the Martian ionosphere are believed to be strongly dependent on the nature, magnitude, and topology of its magnetic field, and whether or not Mars has an intrinsic magnetic field. Due to the weak magnetic field on Mars, the Martian ionosphere interacts directly with the solar wind, resulting in significant outflows of keV ion beams and lower-energy “pick-up” ions. We discuss the planned study of ion drifts and solar wind interactions in the Martian ionosphere using the Planet-B Thermal Plasma Analyzer. © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998
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title_short	Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere
url	https://dx.doi.org/10.1186/BF03352103
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Planned observations of thermal plasma drifts and solar wind interactions in the Martian ionosphere

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