Results 151 to 160 of about 306,228 (194)

<i>Solar Terrestrial Relations Observatory</i> (STEREO) Observations of Stream Interaction Regions in 2007 - 2016: Relationship with Heliospheric Current Sheets, Solar Cycle Variations, and Dual Observations. [PDF]

Sol Phys, 2019
Jian LK, Luhmann JG, Russell CT, Galvin AB.   +3 more
europepmc   +1 more source

Ionospheric response to solar and interplanetary disturbances: a Swarm perspective. [PDF]

Philos Trans A Math Phys Eng Sci, 2019
Balasis G, Papadimitriou C, Boutsi AZ.
europepmc   +1 more source

Simultaneous Occurrence of Magnetospheric Fluctuations at Different Discrete Frequencies ( f ≈ 1 - 5 mHz): A Review. [PDF]

Space Sci Rev
Di Matteo S, Villante U.
europepmc   +1 more source

TWO EVENTS SHOWING THE INTERACTION OF INTENSE MAGNETIC CLOUD WITH COROTATING HIGH SPEED STREAMS

Chinese Journal of Space Science, 1989
openaire   +1 more source

The composition of corotating energetic particle streams [PDF]

Astrophysical Journal, 1978
The relative abundances of 1.5 to 23 MeV/nucleon ions in corotating nucleon streams were compared with ion abundances in particle events associated with solar flares and with solar and solar wind abundances.
T T von Rosenvinge, R E McGuire, Frank B McDonald   +2 more
exaly   +4 more sources

AE index variability during corotating fast solar wind streams [PDF]

Journal of Geophysical Research: Space Physics, 2005
[ 1] We examine the AE index variability while 12 corotating fast solar wind streams pass the Earth during the ascending phase of the ongoing solar activity cycle. We apply the Discrete Fourier Transform analysis to the associated interplanetary magnetic
Piero Diego, M Storini, M Parisi
exaly   +4 more sources

Corotating solar wind streams and recurrent geomagnetic activity: A review

Journal of Geophysical Research: Space Physics, 2006
Solar wind fast streams emanating from solar coronal holes cause recurrent, moderate intensity geomagnetic activity at Earth. Intense magnetic field regions called Corotating Interaction Regions or CIRs are created by the interaction of fast streams with upstream slow streams.
Nat Gopalswamy, Bruce T. Tsurutani, Manuel Grande   +2 more
exaly   +4 more sources

Some of the next articles are maybe not open access.

Related searches:

Magnetic Storms Caused by Corotating Solar Wind Streams

Geophysical Monograph Series, 2006
Geomagnetic activity at Earth due to corotating high speed solar wind streams are reviewed. High density plasma regions in the vicinity of the heliospheric current sheet in the slow solar wind impinge upon the magnetosphere and create magnetic storm intial phases.
Nat Gopalswamy, Bruce T. Tsurutani, Walter Gonzalez   +2 more
exaly   +2 more sources

Evolution of corotating stream structures in the heliospheric equatorial plane

Journal of Geophysical Research: Space Physics, 1993
This paper develops a numerical method and applies it to the study of corotating high‐speed streams in the equatorial plane of the heliosphere from 0.3 AU up to 10 AU, where corotating shocks undergo processes of formation, development and interaction.
Y Q Hu
exaly   +2 more sources

Corotating pressure waves without fast streams in the solar wind

Journal of Geophysical Research: Space Physics, 1983
Voyager 1 and 2 magnetic field and plasma data are presented which demonstrate the existence of large scale, corotating, nonlinear pressure waves between 2 AU and 4 AU that are not accompanied by fast streams. The pressure waves are presumed to be generated by the interaction between fast corotating streams and slower flows near the sun. For two of the
Leonard F. Burlaga
exaly   +2 more sources