The Magnetosphere 1972
DOI: 10.1007/978-94-010-3130-1_1
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The Configuration of the Geomagnetic Field

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“…The dawn‐dusk, i.e., the B y component of the interplanetary magnetic field (IMF), may affect the large‐scale structure and topology of the Earth's magnetotail causing a twisting of the tail [e.g., Fairfield , ; Cowley , ; Kaymaz et al , ; Owen et al , ; Kullen and Janhunen , , ; Tsyganenko et al , ]. For nonzero IMF B y the plasma sheet and cross‐tail current/neutral sheet can get rotated along the Earth‐Sun axis, and an additional IMF B y component appears in tail lobes and the plasma sheet that has the same sign as IMF B y .…”
Section: Introductionmentioning
confidence: 99%
“…The dawn‐dusk, i.e., the B y component of the interplanetary magnetic field (IMF), may affect the large‐scale structure and topology of the Earth's magnetotail causing a twisting of the tail [e.g., Fairfield , ; Cowley , ; Kaymaz et al , ; Owen et al , ; Kullen and Janhunen , , ; Tsyganenko et al , ]. For nonzero IMF B y the plasma sheet and cross‐tail current/neutral sheet can get rotated along the Earth‐Sun axis, and an additional IMF B y component appears in tail lobes and the plasma sheet that has the same sign as IMF B y .…”
Section: Introductionmentioning
confidence: 99%