Design and construction of a ground-based plasma device for Martian boundary layer investigation
Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma di...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Jin, Rong [verfasserIn] Liu, Yu [verfasserIn] Lei, Jiuhou [verfasserIn] Yu, Pengcheng [verfasserIn] Li, Minchi [verfasserIn] Huang, Kexin [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Vacuum - Amsterdam [u.a.] : Elsevier Science, 1951, 216 |
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| Übergeordnetes Werk: |
volume:216 |
| DOI / URN: |
10.1016/j.vacuum.2023.112453 |
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| Katalog-ID: |
ELV062016679 |
|---|
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| 245 | 1 | 0 | |a Design and construction of a ground-based plasma device for Martian boundary layer investigation |
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| 520 | |a Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. | ||
| 650 | 4 | |a Martian ionosphere | |
| 650 | 4 | |a Boundary layer | |
| 650 | 4 | |a Laboratory experiment | |
| 700 | 1 | |a Liu, Yu |e verfasserin |0 (orcid)0000-0002-6085-9365 |4 aut | |
| 700 | 1 | |a Lei, Jiuhou |e verfasserin |4 aut | |
| 700 | 1 | |a Yu, Pengcheng |e verfasserin |4 aut | |
| 700 | 1 | |a Li, Minchi |e verfasserin |4 aut | |
| 700 | 1 | |a Huang, Kexin |e verfasserin |4 aut | |
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10.1016/j.vacuum.2023.112453 doi (DE-627)ELV062016679 (ELSEVIER)S0042-207X(23)00650-4 DE-627 ger DE-627 rda eng 530 VZ 58.19 bkl 33.09 bkl 52.78 bkl Jin, Rong verfasserin (orcid)0009-0001-8242-1663 aut Design and construction of a ground-based plasma device for Martian boundary layer investigation 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. Martian ionosphere Boundary layer Laboratory experiment Liu, Yu verfasserin (orcid)0000-0002-6085-9365 aut Lei, Jiuhou verfasserin aut Yu, Pengcheng verfasserin aut Li, Minchi verfasserin aut Huang, Kexin verfasserin aut Enthalten in Vacuum Amsterdam [u.a.] : Elsevier Science, 1951 216 Online-Ressource (DE-627)271176393 (DE-600)1479044-0 (DE-576)114088187 0042-207X nnns volume:216 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 58.19 Verfahrenstechnik: Sonstiges VZ 33.09 Physik unter besonderen Bedingungen VZ 52.78 Oberflächentechnik Wärmebehandlung VZ AR 216 |
| spelling |
10.1016/j.vacuum.2023.112453 doi (DE-627)ELV062016679 (ELSEVIER)S0042-207X(23)00650-4 DE-627 ger DE-627 rda eng 530 VZ 58.19 bkl 33.09 bkl 52.78 bkl Jin, Rong verfasserin (orcid)0009-0001-8242-1663 aut Design and construction of a ground-based plasma device for Martian boundary layer investigation 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. Martian ionosphere Boundary layer Laboratory experiment Liu, Yu verfasserin (orcid)0000-0002-6085-9365 aut Lei, Jiuhou verfasserin aut Yu, Pengcheng verfasserin aut Li, Minchi verfasserin aut Huang, Kexin verfasserin aut Enthalten in Vacuum Amsterdam [u.a.] : Elsevier Science, 1951 216 Online-Ressource (DE-627)271176393 (DE-600)1479044-0 (DE-576)114088187 0042-207X nnns volume:216 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 58.19 Verfahrenstechnik: Sonstiges VZ 33.09 Physik unter besonderen Bedingungen VZ 52.78 Oberflächentechnik Wärmebehandlung VZ AR 216 |
| allfields_unstemmed |
10.1016/j.vacuum.2023.112453 doi (DE-627)ELV062016679 (ELSEVIER)S0042-207X(23)00650-4 DE-627 ger DE-627 rda eng 530 VZ 58.19 bkl 33.09 bkl 52.78 bkl Jin, Rong verfasserin (orcid)0009-0001-8242-1663 aut Design and construction of a ground-based plasma device for Martian boundary layer investigation 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. Martian ionosphere Boundary layer Laboratory experiment Liu, Yu verfasserin (orcid)0000-0002-6085-9365 aut Lei, Jiuhou verfasserin aut Yu, Pengcheng verfasserin aut Li, Minchi verfasserin aut Huang, Kexin verfasserin aut Enthalten in Vacuum Amsterdam [u.a.] : Elsevier Science, 1951 216 Online-Ressource (DE-627)271176393 (DE-600)1479044-0 (DE-576)114088187 0042-207X nnns volume:216 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 58.19 Verfahrenstechnik: Sonstiges VZ 33.09 Physik unter besonderen Bedingungen VZ 52.78 Oberflächentechnik Wärmebehandlung VZ AR 216 |
| allfieldsGer |
10.1016/j.vacuum.2023.112453 doi (DE-627)ELV062016679 (ELSEVIER)S0042-207X(23)00650-4 DE-627 ger DE-627 rda eng 530 VZ 58.19 bkl 33.09 bkl 52.78 bkl Jin, Rong verfasserin (orcid)0009-0001-8242-1663 aut Design and construction of a ground-based plasma device for Martian boundary layer investigation 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. Martian ionosphere Boundary layer Laboratory experiment Liu, Yu verfasserin (orcid)0000-0002-6085-9365 aut Lei, Jiuhou verfasserin aut Yu, Pengcheng verfasserin aut Li, Minchi verfasserin aut Huang, Kexin verfasserin aut Enthalten in Vacuum Amsterdam [u.a.] : Elsevier Science, 1951 216 Online-Ressource (DE-627)271176393 (DE-600)1479044-0 (DE-576)114088187 0042-207X nnns volume:216 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 58.19 Verfahrenstechnik: Sonstiges VZ 33.09 Physik unter besonderen Bedingungen VZ 52.78 Oberflächentechnik Wärmebehandlung VZ AR 216 |
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530 VZ 58.19 bkl 33.09 bkl 52.78 bkl Design and construction of a ground-based plasma device for Martian boundary layer investigation Martian ionosphere Boundary layer Laboratory experiment |
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design and construction of a ground-based plasma device for martian boundary layer investigation |
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Design and construction of a ground-based plasma device for Martian boundary layer investigation |
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Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. |
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Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. |
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Laboratory experiments have contributed significantly to the exploration of the fundamental physics of Earth’s and planetary space plasma. In this work, a ground-based plasma device was designed and constructed to study the plasma physics in the Martian boundary layer, where the solar wind plasma directly interacts with the Martian ionospheric plasma, and the underlying physical mechanisms and processes are not fully understood. The solar wind plasma and the Martian ionospheric plasma were simulated using two independent plasma sources. A Kaufman source was used to simulate the low-density, high-velocity solar wind plasma, and a lanthanum hexaboride source was utilized to simulate the high-density, low-velocity Martian ionospheric plasma. Additionally, the crustal magnetic field of Mars was modeled using a rotatable electromagnet. The initial results suggest that the interaction in the Martian boundary layer can be simulated based on the device, and the boundary layer’s structure, location, and physical processes can be experimentally studied in the future. |
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