Počet záznamů: 1  

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

  1. 1.
    SYSNO ASEP0356503
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevMESSENGER Observations of Extreme Loading and Unloading of Mercury's Magnetic Tail
    Tvůrce(i) 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)
    Zdroj.dok.Science. - : American Association for the Advancement of Science - ISSN 0036-8075
    Roč. 329, č. 5992 (2010), s. 665-668
    Poč.str.4 s.
    Jazyk dok.eng - angličtina
    Země vyd.US - Spojené státy americké
    Klíč. slovasolar-wind ; magnetosphere ; substorms
    Vědní obor RIVBN - Astronomie a nebeská mechanika, astrofyzika
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000280602700034
    DOI10.1126/science.1188067
    AnotaceDuring 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
    PracovištěAstronomický ústav
    KontaktRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Rok sběru2011
Počet záznamů: 1  

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