Hot flow anomaly remnant in the far geotail?
  • Metaadatok
Tartalom: http://dx.doi.org/10.1016/j.jastp.2015.01.011
Archívum: MTA Könyvtár
Gyűjtemény: Status = Published



Type = Article
Cím:
Hot flow anomaly remnant in the far geotail?
Létrehozó:
Facskó, Gábor István
Opitz, Andrea
Lavraud, B.
J G Luhmann, J. G.
C T Russell, C. T.
Kis, Árpád
Wesztergom, Viktor
Dátum:
2015
Téma:
QB Astronomy, Astrophysics / csillagászat, asztrofizika
QE01 Geophysics / geofizika
QE04 Meteorology / meteorológia
Tartalmi leírás:
A hot flow anomaly (HFA) like event was observed by the Solar TErrestrial RElations Observatory (STEREO) in the night side magnetosheath in the far tail in February-March 2007. The magnetic signature of the tangential discontinuity was visible, but the resolution of the plasma ion data is not sufficient for our analysis, so a method is given to identify HFAs without solar wind velocity measurements. The event observed in the night side magnetosheath in the far tail might be the remnant of an HFA event, a not-so-active current sheet. This observation suggests that the lifetime of the HFAs might be several 10 minutes, much longer than the expected several minutes.
Típus:
Article
PeerReviewed
info:eu-repo/semantics/article
Formátum:
text
Azonosító:
Facskó, Gábor István and Opitz, Andrea and Lavraud, B. and J G Luhmann, J. G. and C T Russell, C. T. and Kis, Árpád and Wesztergom, Viktor (2015) Hot flow anomaly remnant in the far geotail? JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 124. pp. 39-43. ISSN 1364-6826
Kapcsolat:
263325