Results 181 to 190 of about 306,228 (194)
Some of the next articles are maybe not open access.
Response of earth and venus ionospheres to corotating solar wind stream of 3 July 1979
Earth, Moon and Planets, 1985Corotating solar wind stream interactions are examined for the earth and Venus in light of data from the plasma detectors aboard ISEE-3, the Pioneer Venus Orbiter (PVO), and Helios-A, as well as in situ ion composition measurements taken by the mass spectrometers aboard the PVO and Atmosphere Explorer-E spacecraft.
S T Suess, P A Cloutier, H A Taylor
exaly +2 more sources
Structure and Dynamics of Corotating and Transient Streams in Three Dimensions
1986This paper reviews current ideas concerning the sources of interplanetary flows and their dynamical revolution, with emphasis on results that are relevant to measurements which will be made by Ulysses.
openaire +1 more source
2023
Generally, a corotating high-speed stream is formed when a high-speed stream (HSS) overtakes the slow wind, originating a corotating interaction region (CIR) upstream and a rarefaction region (RR) downstream. Mainly within CIRs and HSSs, the interplanetary magnetic field (IMF) presents wide fluctuations that can lead to the enhancement of geomagnetic ...
Carnevale, G. +4 more
openaire +2 more sources
Generally, a corotating high-speed stream is formed when a high-speed stream (HSS) overtakes the slow wind, originating a corotating interaction region (CIR) upstream and a rarefaction region (RR) downstream. Mainly within CIRs and HSSs, the interplanetary magnetic field (IMF) presents wide fluctuations that can lead to the enhancement of geomagnetic ...
Carnevale, G. +4 more
openaire +2 more sources
AIP Conference Proceedings, 1996
Ulysses measurements of energetic solar wind ions (5-23 MeV) associated with the trailing reverse shock found to be consistent with an earlier result obtained by Pioneers. The observations cover the middle latitude region 20-30 deg.of south heliosphere.
Devrie S. Intriligator +4 more
openaire +1 more source
Ulysses measurements of energetic solar wind ions (5-23 MeV) associated with the trailing reverse shock found to be consistent with an earlier result obtained by Pioneers. The observations cover the middle latitude region 20-30 deg.of south heliosphere.
Devrie S. Intriligator +4 more
openaire +1 more source
Solar wind turbulence and shear: A superposed-epoch analysis of corotating interaction regions at 1 AU [PDF]
Journal of Geophysical Research: Space Physics, 2010 Michael H Denton, Joseph E Borovsky
exaly +1 more source
AIP Conference Proceedings, 2013
From late 2007 to early 2008, a pair of coronal holes lasted for many solar rotations while Earth and Mars were radially aligned. The wind emanating from coronal holes is fast (typically 500-850 km/s) and forms Corotating Interaction Regions (CIRs) as the fast wind runs into slower wind emitted at an earlier time.
Heather A. Elliott +8 more
openaire +1 more source
From late 2007 to early 2008, a pair of coronal holes lasted for many solar rotations while Earth and Mars were radially aligned. The wind emanating from coronal holes is fast (typically 500-850 km/s) and forms Corotating Interaction Regions (CIRs) as the fast wind runs into slower wind emitted at an earlier time.
Heather A. Elliott +8 more
openaire +1 more source
Astronomy Reports, 2019
Solar and geomagnetic data demonstrate that, at the decay phase of solar activity in 2016, the dominating role in strong geomagnetic perturations was played by long-lived corotating regions of interaction between solar-wind streams with different velocities.
I. V. Chashei +3 more
openaire +1 more source
Solar and geomagnetic data demonstrate that, at the decay phase of solar activity in 2016, the dominating role in strong geomagnetic perturations was played by long-lived corotating regions of interaction between solar-wind streams with different velocities.
I. V. Chashei +3 more
openaire +1 more source
Journal of Geophysical Research: Space Physics, 1978
An opportunity to test an MHD one‐dimensional time‐dependent model of corotating solar wind streams presented itself during the period from September 30 to November 25, 1973, when Pioneer 11 and Pioneer 10 were near radial alignment with the sun. This observational period was characterized by five or six corotating interaction regions which streamed ...
M. Dryer +6 more
openaire +1 more source
An opportunity to test an MHD one‐dimensional time‐dependent model of corotating solar wind streams presented itself during the period from September 30 to November 25, 1973, when Pioneer 11 and Pioneer 10 were near radial alignment with the sun. This observational period was characterized by five or six corotating interaction regions which streamed ...
M. Dryer +6 more
openaire +1 more source
Geoeffectiveness of corotating interaction regions as measured by Dst index
Journal of Geophysical Research: Space Physics, 2006Walter Gonzalez +2 more
exaly