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Earth's collision with a solar filament on 21 January 2005: Overview
dc.contributor.authorKozyra, J. U.en_US
dc.contributor.authorManchester, W. B.en_US
dc.contributor.authorEscoubet, C. P.en_US
dc.contributor.authorLepri, S. T.en_US
dc.contributor.authorLiemohn, M. W.en_US
dc.contributor.authorGonzalez, W. D.en_US
dc.contributor.authorThomsen, M. W.en_US
dc.contributor.authorTsurutani, B. T.en_US
dc.date.accessioned2013-12-04T18:58:05Z
dc.date.available2014-12-01T17:22:25Zen_US
dc.date.issued2013-10en_US
dc.identifier.citationKozyra, J. U.; Manchester, W. B.; Escoubet, C. P.; Lepri, S. T.; Liemohn, M. W.; Gonzalez, W. D.; Thomsen, M. W.; Tsurutani, B. T. (2013). "Earth's collision with a solar filament on 21 January 2005: Overview." Journal of Geophysical Research: Space Physics 118(10): 5967-5978.en_US
dc.identifier.issn2169-9380en_US
dc.identifier.issn2169-9402en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/101865
dc.description.abstractOn 21 January 2005, one of the fastest interplanetary coronal mass ejections (ICME) of solar cycle 23, containing exceptionally dense plasma directly behind the sheath, hit the magnetosphere. We show from charge‐state analysis that this material was a piece of the erupting solar filament and further, based on comparisons to the simulation of a fast CME, that the unusual location of the filament material was a consequence of three processes. As the ICME decelerated, the momentum of the dense filament material caused it to push through the flux rope toward the nose. Diverging nonradial flows in front of the filament moved magnetic flux to the sides of the ICME. At the same time, reconnection between the leading edge of the ICME and the sheath magnetic fields worked to peel away the outer layers of the flux rope creating a remnant flux rope and a trailing region of newly opened magnetic field lines. These processes combined to move the filament material into direct contact with the ICME sheath region. Within 1 h after impact and under northward interplanetary magnetic field (IMF) conditions, a cold dense plasma sheet formed within the magnetosphere from the filament material. Dense plasma sheet material continued to move through the magnetosphere for more than 6 h as the filament passed by the Earth. Densities were high enough to produce strong diamagnetic stretching of the magnetotail despite the northward IMF conditions and low levels of magnetic activity. The disruptions from the filament collision are linked to an array of unusual features throughout the magnetosphere, ionosphere, and atmosphere. These results raise questions about whether rare collisions with solar filaments may, under the right conditions, be a factor in producing even more extreme events. Key Points Study of unusual solar filament evolution and collision with geospace As CME decelerated, filament pushed through flux rope reaching sheath Within 1 h after arrival, cold dense plasma sheet formed from solar filamenten_US
dc.publisherWiley Periodicals, Inc.en_US
dc.publisherCambridge Univ. Pressen_US
dc.subject.otherMagnetic Reconnectionen_US
dc.subject.otherMagnetotailen_US
dc.subject.otherPlasma Sheeten_US
dc.subject.otherSolar Filamenten_US
dc.subject.otherCoronal Mass Ejectionen_US
dc.titleEarth's collision with a solar filament on 21 January 2005: Overviewen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomy and Astrophysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/101865/1/jgra50567.pdf
dc.identifier.doi10.1002/jgra.50567en_US
dc.identifier.sourceJournal of Geophysical Research: Space Physicsen_US
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