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5 papers · 2 filters
Windsock memory conditioned RAM (Co-Ram) pressure effect: forced reconnection in the Earth's magnetotail
Z. Vörös, G. Facskó, M. Khodachenko +3
Magnetic reconnection (MR) is a key physical concept explaining the addition of magnetic flux to the magnetotail and closed flux lines back-motion to the dayside magnetosphere. Thi…
Reconnection outflow generated turbulence in the solar wind
Z. Vörös, Y. L. Sasunov, V. S. Semenov +3
Petschek-type time-dependent reconnection (TDR) and quasi-stationary reconnection (QSR) models are considered to understand reconnection outflow structures and the features of the…
Magnetic moment and plasma environment of HD 209458b as determined from Ly observations
K. G. Kislyakova, M. Holmström, H. Lammer +2
Transit observations of HD 209458b in the stellar Lyman- (Ly) line revealed strong absorption in both blue and red wings of the line interpreted as hydrogen atoms escaping fr…
What frequencies of standing surface waves can the subsolar magnetopause support?
Martin Archer, Ferdinand Plaschke
It is has been proposed that the subsolar magnetopause may support its own eigenmode, consisting of propagating surface waves which reflect at the northern/southern ionospheres for…
Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
Ying D. Liu, Janet G. Luhmann, Primož Kajdič +8
Space weather refers to dynamic conditions on the Sun and in the space environment of the Earth, which are often driven by solar eruptions and their subsequent interplanetary distu…