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The plasma sheet and boundary layers under northward IMF: A multi-point and multi-instrument perspective
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SYSNO ASEP 0322109 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title The plasma sheet and boundary layers under northward IMF: A multi-point and multi-instrument perspective Title Plasma sheet a rozhrani pri severne orientovanem IMF: Author(s) Taylor, M. G. G. T. (NL)
Lavraud, B. (US)
Escoubet, C. P. (NL)
Milan, S.E. (GB)
Nykyri, K. (GB)
Dunlop, M. W. (GB)
Davies, J.A. (GB)
Friedel, R.H.W. (US)
Frey, H. (US)
Bogdanova, Y.V. (GB)
Asnes, A. (NL)
Laakso, H. (NL)
Trávníček, Pavel M. (ASU-R) RID, ORCID
Masson, A. (NL)
Opgenoorth, H. (NL)
Vallat, C. (NL)
Fazakerley, A. N. (GB)
Lahiff, A. (GB)
Owen, C. J. (GB)
Pitout, F. (DE)
Pu, Y. (CN)
Shen, C. (CN)
Zong, Q.-G. (US)
Rème, H. (FR)
Scudder, J. D. (US)
Zhang, T. L. (AT)Source Title Advances in Space Research. - : Elsevier - ISSN 0273-1177
Roč. 41, č. 10 (2008), s. 1619-1629Number of pages 11 s. Language eng - English Country GB - United Kingdom Keywords plasma sheet ; magnetopshere ; cold dense plasma sheet Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000256186300014 DOI 10.1016/j.asr.2007.10.013 Annotation During conditions of northward interplanetary magnetic field (IMF), the near-tail plasma sheet is known to become denser and cooler, and is described as the cold-dense plasma sheet (CDPS). While its source is likely the solar wind, the prominent penetration mechanisms are less clear. The two main candidates are solar wind direct capture via double high-latitude reconnection on the dayside and Kelvin&-Helmholtz/diffusive processes at the flank magnetopause. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2009
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