Satellite drag effects due to uplifted oxygen neutrals during super magnetic storms

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dc.contributor.author Lakhina, G.S.
dc.contributor.author Tsurutani, Bruce T.
dc.date.accessioned 2018-06-25T05:21:19Z
dc.date.accessioned 2021-02-12T10:12:53Z
dc.date.available 2018-06-25T05:21:19Z
dc.date.available 2021-02-12T10:12:53Z
dc.date.issued 2017
dc.identifier.citation Nonlinear Processes Geophysics, 24, 745–750, doi: 10.5194/npg-24-745-2017 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/1189
dc.description.abstract During intense magnetic storms, prompt penetration electric fields (PPEFs) through E × B forces near the magnetic equator uplift the dayside ionosphere. This effect has been called the “dayside super-fountain effect”. Ionneutral drag forces between the upward moving O+ (oxygen ions) and oxygen neutrals will elevate the oxygen atoms to higher altitudes. This paper gives a linear calculation indicating how serious the effect may be during an 1859-type (Carrington) superstorm. It is concluded that the oxygen neutral densities produced at low-Earth-orbiting (LEO) satellite altitudes may be sufficiently high to present severe satellite drag. It is estimated that with a prompt penetrating electric field of ∼ 20 mV m−1 turned on for 20 min, the O atoms and O + ions are uplifted to 850 km where they produce about 40-times-greater satellite drag per unit mass than normal. Stronger electric fields will presumably lead to greater uplifted mass. en_US
dc.language.iso en_US en_US
dc.subject Magnetic storms en_US
dc.subject Dayside super-fountain effect en_US
dc.title Satellite drag effects due to uplifted oxygen neutrals during super magnetic storms en_US
dc.type Article en_US
dc.identifier.accession 091726


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