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dc.contributor.authorYousif, ME
dc.date.accessioned2015-06-30T15:17:28Z
dc.date.available2015-06-30T15:17:28Z
dc.date.issued2013-11
dc.identifier.citationYousif, M. E. (2013, December). What was the source of Magnetic Field Measured by Pioneer V In 1960?. In AGU Fall Meeting Abstracts (Vol. 1, p. 1005).en_US
dc.identifier.urihttp://adsabs.harvard.edu/abs/2013AGUFMGC51D1005Y
dc.identifier.urihttp://hdl.handle.net/11295/85760
dc.description.abstractThe engulfment of Pioneer V with solar plasma on March 30, 1960, and the later measurement of high interplanetary magnetic field (IMF) by the probe were interpreted as of solar origin. Studies and analysis of that event showed that the maximum IMF was measured six hours after that engulfment and two hours after been measured by Honolulu earth station. Such IMF is thought to be produced at around 12.5RE within the magnetosheath in form of an external magnetic field (ExMF). A suggestion which can easily be tested by two probes such as NASA THEMIS satellites, as it is crucial for the current human knowledge, which is seeking such mechanism for related energization process. Fig.1. Re-analysis of March 30/31, geomagnetic storms, by combining Fig.2.a&b Coleman et al. [1961], with Fig.2-A Fan et al. [1960]. The figure shows the following sequence: Starts of the solar flare, plasma arriving at Pioneer V (no detection of an embedded solar field), arrival to the earth, registration of Horizontal field at Honolulu, and high magnetic field measured 6 hours later at Pioneer V satellite.en_US
dc.language.isoenen_US
dc.publisherUniversity of Nairobien_US
dc.subject2134 INTERPLANETARY PHYSICS Interplanetary magnetic fields, 1739 HISTORY OF GEOPHYSICS Solar/planetary relationships, 7845 SPACE PLASMA PHYSICS Particle accelerationen_US
dc.titleWhat was the source of magnetic field measured by pioneer V in 1960en_US
dc.typeArticleen_US
dc.type.materialenen_US


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