Laboratory Modelling of Solar Wind Interaction with Lunar Magnetic Anomalies
The paper presents the results of laboratory experiment modeling the interaction between Lunar magnetic anomalies and Solar wind. To model the LMA we use quadrupole magnetic field. The main dimensionless parameter of the problem, the ion inertia length relative to the mini-magnetosphere size, well c...
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| Veröffentlicht in: | Astronomy reports 2023, Vol.67 (1), p.78-85 |
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| creator | Rumenskikh, M. C. Chibranov, A. A. Efimov, M. A. Berezutsky, A. G. Posukh, V. G. Zakharov, Yu. P. Boyarintsev, E. L. Miroshnichenko, I. B. Trushin, P. A. Divin, A. V. Shaikhislamov, I. F. |
| description | The paper presents the results of laboratory experiment modeling the interaction between Lunar magnetic anomalies and Solar wind. To model the LMA we use quadrupole magnetic field. The main dimensionless parameter of the problem, the ion inertia length relative to the mini-magnetosphere size, well corresponds between experiment and LMA conditions. The main result is measurement of the magnetically reflected proton fluxes, which show qualitative agreement to available satellite data. |
| doi_str_mv | 10.1134/S1063772923010079 |
| format | Article |
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C. ; Chibranov, A. A. ; Efimov, M. A. ; Berezutsky, A. G. ; Posukh, V. G. ; Zakharov, Yu. P. ; Boyarintsev, E. L. ; Miroshnichenko, I. B. ; Trushin, P. A. ; Divin, A. V. ; Shaikhislamov, I. F.</creator><creatorcontrib>Rumenskikh, M. C. ; Chibranov, A. A. ; Efimov, M. A. ; Berezutsky, A. G. ; Posukh, V. G. ; Zakharov, Yu. P. ; Boyarintsev, E. L. ; Miroshnichenko, I. B. ; Trushin, P. A. ; Divin, A. V. ; Shaikhislamov, I. F.</creatorcontrib><description>The paper presents the results of laboratory experiment modeling the interaction between Lunar magnetic anomalies and Solar wind. To model the LMA we use quadrupole magnetic field. The main dimensionless parameter of the problem, the ion inertia length relative to the mini-magnetosphere size, well corresponds between experiment and LMA conditions. The main result is measurement of the magnetically reflected proton fluxes, which show qualitative agreement to available satellite data.</description><identifier>ISSN: 1063-7729</identifier><identifier>EISSN: 1562-6881</identifier><identifier>DOI: 10.1134/S1063772923010079</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Magnetic anomalies ; Magnetic fields ; Magnetospheres ; Observations and Techniques ; Physics ; Physics and Astronomy ; Quadrupoles ; Qualitative analysis ; Satellite data ; Solar wind</subject><ispartof>Astronomy reports, 2023, Vol.67 (1), p.78-85</ispartof><rights>Pleiades Publishing, Ltd. 2023. ISSN 1063-7729, Astronomy Reports, 2023, Vol. 67, No. 1, pp. 78–85. © Pleiades Publishing, Ltd., 2023. 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G.</creatorcontrib><creatorcontrib>Zakharov, Yu. P.</creatorcontrib><creatorcontrib>Boyarintsev, E. L.</creatorcontrib><creatorcontrib>Miroshnichenko, I. B.</creatorcontrib><creatorcontrib>Trushin, P. A.</creatorcontrib><creatorcontrib>Divin, A. V.</creatorcontrib><creatorcontrib>Shaikhislamov, I. F.</creatorcontrib><title>Laboratory Modelling of Solar Wind Interaction with Lunar Magnetic Anomalies</title><title>Astronomy reports</title><addtitle>Astron. Rep</addtitle><description>The paper presents the results of laboratory experiment modeling the interaction between Lunar magnetic anomalies and Solar wind. To model the LMA we use quadrupole magnetic field. The main dimensionless parameter of the problem, the ion inertia length relative to the mini-magnetosphere size, well corresponds between experiment and LMA conditions. 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A.</au><au>Divin, A. V.</au><au>Shaikhislamov, I. F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Laboratory Modelling of Solar Wind Interaction with Lunar Magnetic Anomalies</atitle><jtitle>Astronomy reports</jtitle><stitle>Astron. Rep</stitle><date>2023</date><risdate>2023</risdate><volume>67</volume><issue>1</issue><spage>78</spage><epage>85</epage><pages>78-85</pages><issn>1063-7729</issn><eissn>1562-6881</eissn><abstract>The paper presents the results of laboratory experiment modeling the interaction between Lunar magnetic anomalies and Solar wind. To model the LMA we use quadrupole magnetic field. The main dimensionless parameter of the problem, the ion inertia length relative to the mini-magnetosphere size, well corresponds between experiment and LMA conditions. 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| subjects | Astronomy Magnetic anomalies Magnetic fields Magnetospheres Observations and Techniques Physics Physics and Astronomy Quadrupoles Qualitative analysis Satellite data Solar wind |
| title | Laboratory Modelling of Solar Wind Interaction with Lunar Magnetic Anomalies |
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