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- W2022065044 abstract "[1] The propagation of a fast coronal mass ejection through the interplanetary medium results in compression and draping of existing heliospheric magnetic fields, forming an upstream sheath. Such sheaths are a common context for planar magnetic structures, where the magnetic field is ordered into laminar sheets. A technique is presented to estimate the location of spacecraft with respect to the large-scale structure of ejecta which they encounter. The technique employs the characteristics of sheath planar magnetic structures, assuming that they are formed by field-line draping. The technique's results for four magnetic clouds encountered by the Ulysses spacecraft are compared to those of a flux rope model. Very good agreement is found, suggesting that this is a promising technique for estimating an ejection's location from single-spacecraft data." @default.
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- W2022065044 date "2002-01-01" @default.
- W2022065044 modified "2023-10-18" @default.
- W2022065044 title "The draping of heliospheric magnetic fields upstream of coronal mass ejecta" @default.
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- W2022065044 doi "https://doi.org/10.1029/2001gl014110" @default.
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