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 |
|