Remnant magnetic fields of Mars and their interaction with the solar wind
This work presents a review of studies of the Martian magnetic fields during the early Soviet missions to Mars in 1971–1974, which never approached Mars by closer than 1000 km before the experiment with the Magnetometer/Electronic Reflectometer (MAG/ER) on board the Mars Global Surveyor spacecraft,...
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| Veröffentlicht in: | Cosmic research 2017-07, Vol.55 (4), p.235-247 |
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| creator | Breus, T. K. Krymskii, A. M. |
| description | This work presents a review of studies of the Martian magnetic fields during the early Soviet missions to Mars in 1971–1974, which never approached Mars by closer than 1000 km before the experiment with the Magnetometer/Electronic Reflectometer (MAG/ER) on board the
Mars Global Surveyor
spacecraft, which could descend to altitudes of 80–100 km. At present, the experiment with the magnetometer (MAG) onboard the American
MAVEN
spacecraft adds new data, but the map of distribution of remnant magnetic fields of Mars and the picture of their interaction with the solar wind are already formed and, at its core, obviously, will not be revised. Thus, it would be very instructive to consider the following in detail: (a) what is already known regarding the features and distribution of remnant magnetic fields on Mars; (b) how they control the interaction of solar wind with a weakly magnetized planet (Mars); and (c) what is its distinction from another nonmagnetized planet (Venus). |
| doi_str_mv | 10.1134/S0010952517040025 |
| format | Article |
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Mars Global Surveyor
spacecraft, which could descend to altitudes of 80–100 km. At present, the experiment with the magnetometer (MAG) onboard the American
MAVEN
spacecraft adds new data, but the map of distribution of remnant magnetic fields of Mars and the picture of their interaction with the solar wind are already formed and, at its core, obviously, will not be revised. Thus, it would be very instructive to consider the following in detail: (a) what is already known regarding the features and distribution of remnant magnetic fields on Mars; (b) how they control the interaction of solar wind with a weakly magnetized planet (Mars); and (c) what is its distinction from another nonmagnetized planet (Venus).</description><identifier>ISSN: 0010-9525</identifier><identifier>EISSN: 1608-3075</identifier><identifier>DOI: 10.1134/S0010952517040025</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Magnetic fields ; Mars ; Mars Global Surveyor ; Mars missions ; Mars spacecraft ; Physics ; Physics and Astronomy ; Planetary magnetic fields ; Solar wind ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Spacecraft ; Venus</subject><ispartof>Cosmic research, 2017-07, Vol.55 (4), p.235-247</ispartof><rights>Pleiades Publishing, Ltd. 2017</rights><rights>Copyright Springer Science & Business Media 2017</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-b0faa1543633075f109da8f8639133c3ba54826b2e5e5c8d134c5b652bde71703</citedby><cites>FETCH-LOGICAL-c316t-b0faa1543633075f109da8f8639133c3ba54826b2e5e5c8d134c5b652bde71703</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0010952517040025$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0010952517040025$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Breus, T. K.</creatorcontrib><creatorcontrib>Krymskii, A. M.</creatorcontrib><title>Remnant magnetic fields of Mars and their interaction with the solar wind</title><title>Cosmic research</title><addtitle>Cosmic Res</addtitle><description>This work presents a review of studies of the Martian magnetic fields during the early Soviet missions to Mars in 1971–1974, which never approached Mars by closer than 1000 km before the experiment with the Magnetometer/Electronic Reflectometer (MAG/ER) on board the
Mars Global Surveyor
spacecraft, which could descend to altitudes of 80–100 km. At present, the experiment with the magnetometer (MAG) onboard the American
MAVEN
spacecraft adds new data, but the map of distribution of remnant magnetic fields of Mars and the picture of their interaction with the solar wind are already formed and, at its core, obviously, will not be revised. Thus, it would be very instructive to consider the following in detail: (a) what is already known regarding the features and distribution of remnant magnetic fields on Mars; (b) how they control the interaction of solar wind with a weakly magnetized planet (Mars); and (c) what is its distinction from another nonmagnetized planet (Venus).</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Magnetic fields</subject><subject>Mars</subject><subject>Mars Global Surveyor</subject><subject>Mars missions</subject><subject>Mars spacecraft</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetary magnetic fields</subject><subject>Solar wind</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Spacecraft</subject><subject>Venus</subject><issn>0010-9525</issn><issn>1608-3075</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp1UEtLxDAQDqJgXf0B3gKeq5OkSdujLD4WVgQf55KmyW6WNl2TLOK_N6WCB_E0zHyPmW8QuiRwTQgrbl4BCNScclJCAUD5EcqIgCpnUPJjlE1wPuGn6CyEHQDUJRMZWr3owUkX8SA3TkersLG67wIeDX6SPmDpOhy32npsXdReqmhHhz9t3E5jHMZe-tS67hydGNkHffFTF-j9_u5t-Zivnx9Wy9t1rhgRMW_BSEl4wQSbTjPp6k5WphKsJowp1kpeVFS0VHPNVdWlcIq3gtO202UKxxboavbd-_HjoENsduPBu7SyoSAKIeq6LhKLzCzlxxC8Ns3e20H6r4ZAM32s-fOxpKGzJiSu22j_6_y_6Bsgimtb</recordid><startdate>20170701</startdate><enddate>20170701</enddate><creator>Breus, T. K.</creator><creator>Krymskii, A. M.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20170701</creationdate><title>Remnant magnetic fields of Mars and their interaction with the solar wind</title><author>Breus, T. K. ; Krymskii, A. M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-b0faa1543633075f109da8f8639133c3ba54826b2e5e5c8d134c5b652bde71703</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Magnetic fields</topic><topic>Mars</topic><topic>Mars Global Surveyor</topic><topic>Mars missions</topic><topic>Mars spacecraft</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Planetary magnetic fields</topic><topic>Solar wind</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Spacecraft</topic><topic>Venus</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Breus, T. K.</creatorcontrib><creatorcontrib>Krymskii, A. M.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Cosmic research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Breus, T. K.</au><au>Krymskii, A. M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Remnant magnetic fields of Mars and their interaction with the solar wind</atitle><jtitle>Cosmic research</jtitle><stitle>Cosmic Res</stitle><date>2017-07-01</date><risdate>2017</risdate><volume>55</volume><issue>4</issue><spage>235</spage><epage>247</epage><pages>235-247</pages><issn>0010-9525</issn><eissn>1608-3075</eissn><abstract>This work presents a review of studies of the Martian magnetic fields during the early Soviet missions to Mars in 1971–1974, which never approached Mars by closer than 1000 km before the experiment with the Magnetometer/Electronic Reflectometer (MAG/ER) on board the
Mars Global Surveyor
spacecraft, which could descend to altitudes of 80–100 km. At present, the experiment with the magnetometer (MAG) onboard the American
MAVEN
spacecraft adds new data, but the map of distribution of remnant magnetic fields of Mars and the picture of their interaction with the solar wind are already formed and, at its core, obviously, will not be revised. Thus, it would be very instructive to consider the following in detail: (a) what is already known regarding the features and distribution of remnant magnetic fields on Mars; (b) how they control the interaction of solar wind with a weakly magnetized planet (Mars); and (c) what is its distinction from another nonmagnetized planet (Venus).</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0010952517040025</doi><tpages>13</tpages></addata></record> |
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| ispartof | Cosmic research, 2017-07, Vol.55 (4), p.235-247 |
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| source | Springer Nature - Complete Springer Journals |
| subjects | Astronomy Astrophysics and Astroparticles Astrophysics and Cosmology Magnetic fields Mars Mars Global Surveyor Mars missions Mars spacecraft Physics Physics and Astronomy Planetary magnetic fields Solar wind Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spacecraft Venus |
| title | Remnant magnetic fields of Mars and their interaction with the solar wind |
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