Storm-time distortion of the inner magnetosphere

Standard

Storm-time distortion of the inner magnetosphere : How severe can it get? / Tsyganenko, NA; Singer, HJ; Kasper, JC.

In: JOURNAL OF GEOPHYSICAL RESEARCH-EARTH SURFACE, Vol. 108, No. A5, 1209, 23.05.2003.

Research output: Contribution to journal › Article › peer-review

Author

Tsyganenko, NA ; Singer, HJ ; Kasper, JC. / Storm-time distortion of the inner magnetosphere : How severe can it get?. In: JOURNAL OF GEOPHYSICAL RESEARCH-EARTH SURFACE. 2003 ; Vol. 108, No. A5.

BibTeX

@article{40d7295473b34302905bd7228d6c2418,

title = "Storm-time distortion of the inner magnetosphere: How severe can it get?",

abstract = "First results are presented of an effort to model the storm-time distortion of the magnetic field in the inner magnetosphere using space magnetometer data. Strong geomagnetic storms are relatively rare events, represented by only a small fraction of the data used in the derivation of existing empirical geomagnetic field models. Hence using those models for the mapping of the storm-time magnetosphere is at most an extrapolation based on trends, obtained from quiet and moderately disturbed data. To overcome that limitation, a set of data was created, containing only clear-cut events with Dst less than or equal to -65 nT, with the goal to derive models of the inner and near geomagnetic field (R",

keywords = "inner magnetosphere, space storms, geomagnetic field, empirical modeling, partial ring current, field line deformation, DAWN-DUSK ASYMMETRY, MAGNETOPAUSE, MODEL",

author = "NA Tsyganenko and HJ Singer and JC Kasper",

year = "2003",

month = may,

day = "23",

doi = "10.1029/2002JA009808",

language = "English",

volume = "108",

journal = "Journal of Geophysical Research: Biogeosciences",

issn = "0148-0227",

publisher = "American Geophysical Union",

number = "A5",

}

RIS

TY - JOUR

T1 - Storm-time distortion of the inner magnetosphere

T2 - How severe can it get?

AU - Tsyganenko, NA

AU - Singer, HJ

AU - Kasper, JC

PY - 2003/5/23

Y1 - 2003/5/23

N2 - First results are presented of an effort to model the storm-time distortion of the magnetic field in the inner magnetosphere using space magnetometer data. Strong geomagnetic storms are relatively rare events, represented by only a small fraction of the data used in the derivation of existing empirical geomagnetic field models. Hence using those models for the mapping of the storm-time magnetosphere is at most an extrapolation based on trends, obtained from quiet and moderately disturbed data. To overcome that limitation, a set of data was created, containing only clear-cut events with Dst less than or equal to -65 nT, with the goal to derive models of the inner and near geomagnetic field (R

AB - First results are presented of an effort to model the storm-time distortion of the magnetic field in the inner magnetosphere using space magnetometer data. Strong geomagnetic storms are relatively rare events, represented by only a small fraction of the data used in the derivation of existing empirical geomagnetic field models. Hence using those models for the mapping of the storm-time magnetosphere is at most an extrapolation based on trends, obtained from quiet and moderately disturbed data. To overcome that limitation, a set of data was created, containing only clear-cut events with Dst less than or equal to -65 nT, with the goal to derive models of the inner and near geomagnetic field (R

KW - inner magnetosphere

KW - space storms

KW - geomagnetic field

KW - empirical modeling

KW - partial ring current

KW - field line deformation

KW - DAWN-DUSK ASYMMETRY

KW - MAGNETOPAUSE

KW - MODEL

U2 - 10.1029/2002JA009808

DO - 10.1029/2002JA009808

M3 - Article

VL - 108

JO - Journal of Geophysical Research: Biogeosciences

JF - Journal of Geophysical Research: Biogeosciences

SN - 0148-0227

IS - A5

M1 - 1209

ER -

ID: 28044167