Model predictions of magnetic perturbations observed by MAGSAT in dawn-dusk orbit
One use to which Magsat data can be put is to test the various models of auroral current flow which have been generated in the past. To do this, predictions of the perturbation magnetic field can be calculated from a current model, and these can be critically examined in light of the Magsat data. In...
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Veröffentlicht in: | Geophysical research letters 1982-04, Vol.9 (4), p.357-360 |
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creator | Hughes, Terence J. Wallis, D. D. Burrows, J. R. Wilson, Margaret D. |
description | One use to which Magsat data can be put is to test the various models of auroral current flow which have been generated in the past. To do this, predictions of the perturbation magnetic field can be calculated from a current model, and these can be critically examined in light of the Magsat data. In this progress report, current models derived from the electric field models of Heppner (1977) and the conductivity models of Wallis and Budzinski (1981) are used to predict the field at Magsat orbit. Some features of the predictions are compared with Magsat data. |
doi_str_mv | 10.1029/GL009i004p00357 |
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D. ; Burrows, J. R. ; Wilson, Margaret D.</creator><creatorcontrib>Hughes, Terence J. ; Wallis, D. D. ; Burrows, J. R. ; Wilson, Margaret D.</creatorcontrib><description>One use to which Magsat data can be put is to test the various models of auroral current flow which have been generated in the past. To do this, predictions of the perturbation magnetic field can be calculated from a current model, and these can be critically examined in light of the Magsat data. In this progress report, current models derived from the electric field models of Heppner (1977) and the conductivity models of Wallis and Budzinski (1981) are used to predict the field at Magsat orbit. 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D.</creatorcontrib><creatorcontrib>Burrows, J. R.</creatorcontrib><creatorcontrib>Wilson, Margaret D.</creatorcontrib><title>Model predictions of magnetic perturbations observed by MAGSAT in dawn-dusk orbit</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>One use to which Magsat data can be put is to test the various models of auroral current flow which have been generated in the past. To do this, predictions of the perturbation magnetic field can be calculated from a current model, and these can be critically examined in light of the Magsat data. In this progress report, current models derived from the electric field models of Heppner (1977) and the conductivity models of Wallis and Budzinski (1981) are used to predict the field at Magsat orbit. Some features of the predictions are compared with Magsat data.</description><subject>Electric fields</subject><subject>Geophysics</subject><subject>Magnetic fields</subject><subject>Mathematical models</subject><subject>Orbits</subject><subject>Perturbation methods</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1982</creationdate><recordtype>article</recordtype><recordid>eNqFkM1P20AQxVeoSE2h5173VPViMvthr_cY0WIQCR8NiONq7R2jLY5tdh1C_nuMEvXAob3MjOb93mj0CPnG4IQB19NiDqA9gOwBRKoOyIRpKZMcQH0ik1EbZ66yz-RLjH9gZECwCblddA4b2gd0vhp810ba1XRlH1scfEV7DMM6lHavlBHDCzpabuliVixnd9S31NlNm7h1fKJdKP1wTA5r20T8uu9H5P7s193peTK_Li5OZ_OkEnmWJ6LmGjnTKGoU5Vg0z0G7cVVVElNAybFyeZpm0jlbS8FzhboGrsCWSllxRL7v7vahe15jHMzKxwqbxrbYraPhQkrFeT6CP_4JslQyKVTG9IhOd2gVuhgD1qYPfmXD1jAw7ymbDymPDrlzbHyD2__hpvg9Z5q9_5TsbD4O-PrXZsOTyZRQqXm4Kgy_vPx5s1gsjRBv3miOTA</recordid><startdate>198204</startdate><enddate>198204</enddate><creator>Hughes, Terence J.</creator><creator>Wallis, D. D.</creator><creator>Burrows, J. R.</creator><creator>Wilson, Margaret D.</creator><general>Blackwell Publishing Ltd</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>198204</creationdate><title>Model predictions of magnetic perturbations observed by MAGSAT in dawn-dusk orbit</title><author>Hughes, Terence J. ; Wallis, D. D. ; Burrows, J. R. ; Wilson, Margaret D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3868-3f29e219e3fe3b3fe92809de21cc4e50e42ecd85564ddaf43287e9f0270ab77a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1982</creationdate><topic>Electric fields</topic><topic>Geophysics</topic><topic>Magnetic fields</topic><topic>Mathematical models</topic><topic>Orbits</topic><topic>Perturbation methods</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hughes, Terence J.</creatorcontrib><creatorcontrib>Wallis, D. D.</creatorcontrib><creatorcontrib>Burrows, J. R.</creatorcontrib><creatorcontrib>Wilson, Margaret D.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hughes, Terence J.</au><au>Wallis, D. D.</au><au>Burrows, J. R.</au><au>Wilson, Margaret D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Model predictions of magnetic perturbations observed by MAGSAT in dawn-dusk orbit</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>1982-04</date><risdate>1982</risdate><volume>9</volume><issue>4</issue><spage>357</spage><epage>360</epage><pages>357-360</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>One use to which Magsat data can be put is to test the various models of auroral current flow which have been generated in the past. To do this, predictions of the perturbation magnetic field can be calculated from a current model, and these can be critically examined in light of the Magsat data. In this progress report, current models derived from the electric field models of Heppner (1977) and the conductivity models of Wallis and Budzinski (1981) are used to predict the field at Magsat orbit. Some features of the predictions are compared with Magsat data.</abstract><pub>Blackwell Publishing Ltd</pub><doi>10.1029/GL009i004p00357</doi><tpages>4</tpages></addata></record> |
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source | Wiley Online Library Journals Frontfile Complete |
subjects | Electric fields Geophysics Magnetic fields Mathematical models Orbits Perturbation methods |
title | Model predictions of magnetic perturbations observed by MAGSAT in dawn-dusk orbit |
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