Interplanetary Gas. XIX. Observational Evidence for a Meridional Solar-Wind Flow Diverging from the Plane of the Solar Equator

1973 ◽  
Vol 184 ◽  
pp. 27 ◽  
Author(s):  
John C. Brandt ◽  
S. Robert Harrington ◽  
Robert G. Roosen
Keyword(s):  
Solar Wind ◽  
Observational Evidence ◽  
Wind Flow ◽  
Solar Wind Flow

Solar wind flow past Venus and its implications for the occurrence of the Kelvin–Helmholtz instability

2007 ◽  
Vol 55 (12) ◽  
pp. 1793-1803 ◽  
Author(s):  
H.K. Biernat ◽  
N.V. Erkaev ◽  
U.V. Amerstorfer ◽  
T. Penz ◽  
H.I.M. Lichtenegger
Keyword(s):  
Solar Wind ◽  
Wind Flow ◽  
Helmholtz Instability ◽  
Flow Past ◽  
Solar Wind Flow

Effects on the Jovian magnetosheath arising from solar wind flow around nonaxisymmetric bodies

1996 ◽  
Vol 101 (A5) ◽  
pp. 10665-10672 ◽  
Author(s):  
N. V. Erkaev ◽  
C. J. Farrugia ◽  
H. K. Biernat
Keyword(s):  
Solar Wind ◽  
Wind Flow ◽  
Solar Wind Flow

Estimation of the entropy of the solar wind flow

2000 ◽  
Vol 62 (5) ◽  
pp. 6496-6504 ◽  
Author(s):  
Wiesław M. Macek ◽  
Stefano Redaelli
Keyword(s):  
Solar Wind ◽  
Wind Flow ◽  
Solar Wind Flow

Genesis On-board Determination of the Solar Wind Flow Regime

2003 ◽  
pp. 153-171 ◽  
Author(s):  
M. Neugebauer ◽  
J. T. Steinberg ◽  
R. L. Tokar ◽  
B. L. Barraclough ◽  
E. E. Dors ◽  
...  
Keyword(s):  
Solar Wind ◽  
Flow Regime ◽  
Wind Flow ◽  
Solar Wind Flow

scholarly journals Interplanetary Response to Solar Long Time-Scale Phenomena

1980 ◽  
Vol 91 ◽  
pp. 105-125
Author(s):  
C. D'Uston ◽  
J. M. Bosqued
Keyword(s):  
Solar Wind ◽  
Time Scale ◽  
High Speed ◽  
Coronal Holes ◽  
Observational Evidence ◽  
Solar Wind Flow ◽  
Speed Solar Wind ◽  
Long Time ◽  
Outer Corona ◽  
High Speed Solar Wind

In this paper, we briefly review the experimental knowledge gained in the recent years on the interplanetary response to solar long-time scale phenomena such as the coronal magnetic structure and its evolution. Observational evidence that solar wind flow in the outer corona comes from the unipolar diverging magnetic regions of the photosphere is discussed along with relations to coronal holes. High-speed solar wind streams observed within the boundary of interplanetary magnetic sectors are associated with these structures. Their boundaries appear as very narrow velocity shears.

Strong influence of lunar crustal fields on the solar wind flow

2011 ◽  
Vol 38 (3) ◽  
pp. n/a-n/a ◽  
Author(s):  
Charles Lue ◽  
Yoshifumi Futaana ◽  
Stas Barabash ◽  
Martin Wieser ◽  
Mats Holmström ◽  
...  
Keyword(s):  
Solar Wind ◽  
Strong Influence ◽  
Wind Flow ◽  
Solar Wind Flow

Solar-wind flow behind the Moon

1968 ◽  
Vol 73 (13) ◽  
pp. 4281-4289 ◽  
Author(s):  
R. A. Wolf
Keyword(s):  
Solar Wind ◽  
Wind Flow ◽  
The Moon ◽  
Solar Wind Flow
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