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dc.contributor.authorLakhina, G.S.
dc.contributor.authorTsurutani, Bruce T.
dc.date.accessioned2018-06-25T05:21:19Z
dc.date.accessioned2021-02-12T10:12:53Z-
dc.date.available2018-06-25T05:21:19Z
dc.date.available2021-02-12T10:12:53Z-
dc.date.issued2017
dc.identifier.citationNonlinear Processes Geophysics, 24, 745–750, doi: 10.5194/npg-24-745-2017en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1189-
dc.description.abstractDuring 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.isoen_USen_US
dc.subjectMagnetic stormsen_US
dc.subjectDayside super-fountain effecten_US
dc.titleSatellite drag effects due to uplifted oxygen neutrals during super magnetic stormsen_US
dc.typeArticleen_US
dc.identifier.accession091726
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