Number of the records: 1  

MESSENGER Observations of Extreme Loading and Unloading of Mercury's Magnetic Tail

  1. 1.
    SYSNO ASEP0356503
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleMESSENGER Observations of Extreme Loading and Unloading of Mercury's Magnetic Tail
    Author(s) Slavin, J.A. (US)
    Andreson, B.J. (US)
    Baker, D. N. (US)
    Benna, M. (US)
    Boardsen, S.A. (US)
    Gloeckler, G. (US)
    Gold, R.E. (US)
    Ho, G.C. (US)
    Korth, H. (US)
    Krimigis, S.M. (US)
    McNutt, Jr., R.L. (US)
    Nittler, L.R. (US)
    Raines, J.M. (US)
    Sarantos, M. (US)
    Schriver, D. (US)
    Solomon, S.C. (US)
    Starr, R.D. (US)
    Trávníček, Pavel M. (ASU-R) RID, ORCID
    Zurbuchen, T.H. (US)
    Source TitleScience. - : American Association for the Advancement of Science - ISSN 0036-8075
    Roč. 329, č. 5992 (2010), s. 665-668
    Number of pages4 s.
    Languageeng - English
    CountryUS - United States
    Keywordssolar-wind ; magnetosphere ; substorms
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000280602700034
    DOI10.1126/science.1188067
    AnnotationDuring MESSENGER's third flyby of Mercury, the magnetic field in the planet's magnetic tail increased by factors of 2 to 3.5 over intervals of 2 to 3 minutes. Magnetospheric substorms at Earth are powered by similar tail loading, but the amplitude is lower by a factor of similar to 10 and typical durations are similar to 1 hour. The extreme tail loading observed at Mercury implies that the relative intensity of substorms must be much larger than at Earth. The correspondence between the duration of tail field enhancements and the characteristic time for the Dungey cycle, which describes plasma circulation through Mercury's magnetosphere, suggests that such circulation determines the substorm time scale. A key aspect of tail unloading during terrestrial substorms is the acceleration of energetic charged particles, but no acceleration signatures were seen during the MESSENGER flyby
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2011
Number of the records: 1  

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