Results 121 to 130 of about 5,952,631 (141)
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The influence of Corotating Interaction Region (CIR) driven geomagnetic storms on the development of equatorial plasma bubbles (EPBs) over wide range of longitudes

Advances in Space Research, 2015
Abstract Recurrent high speed solar wind streams from coronal holes on the Sun are more frequent and Geoeffective during the declining phase of solar cycle which interact with the ambient solar wind leading the formation of Corotating Interaction Regions (CIRs) in the interplanetary medium.
S. Tulasi Ram   +4 more
openaire   +3 more sources

The Acceleration of Charged Particles in Corotating Interaction Regions (Cir) – a Review with Particular Emphasis on the Ulysses Mission

Surveys in Geophysics, 1998
Observations on the acceleration of charged particles to higher energies in corotating interaction regions in interplanetary space are reviewed. Particular emphasis is given to the Ulysses observations which at the moment provide the latest extensive set.
openaire   +5 more sources

Voyager 2 Observations of Corotating Interaction Regions (CIRs) in the Outer Heliosphere

Space Science Reviews, 1999
We review observations from Voyager 2 of CIRs and merged CIRs in the outer heliosphere. The rather simple characteristics of the CIR-associated changes in plasma, magnetic field, and particles become more complex as observations are made at greater and greater distances.
A. J. Lazarus   +3 more
openaire   +1 more source

Interaction of ICMEs with Corotating Interaction Region (CIR)

2023
The research in the scope of the ICOHOSS project is expected to significantly impact the understanding of the propagation and evolution of CMEs, which is one of the fundamental problems of Heliospheric Physics An an important factor in this endeavor is comprehending the evolution of CMEs in interplanetary space (studying different interactions it ...
Remeshan, Akshay Kumar   +1 more
openaire  

“Corotating Interaction Regions (CIRs)”, “Interaction Regions (IRs)” and “Stream Interaction Regions (SIRs)”, which term should be used?

We discuss the early history of quasiperiodic ~27-day recurrent geomagnetic activity starting with Maunder (1904, 1905), Chree (1913) and Bartels (1932, 1934), and the Bartels term “M-regions”. We show the iconic “interaction region (IR)” schematic of Belcher and Davis (1971) and the further development of Smith and Wolfe (1976)
Tsurutani, Bruce T.   +2 more
openaire   +1 more source

Solar wind flow angle and geoeffectiveness of corotating interaction regions: First results

Geophysical Research Letters, 2017
Diptiranjan Rout   +2 more
exaly  

Statistical analysis of corotating interaction regions and their geoeffectiveness during solar cycle 23

Journal of Geophysical Research: Space Physics, 2008
C D Fry, C S Deehr, X S Feng
exaly  

Solar wind turbulence and shear: A superposed-epoch analysis of corotating interaction regions at 1 AU

Journal of Geophysical Research: Space Physics, 2010
Michael H Denton, Joseph E Borovsky
exaly  

Solar wind interaction with comet 67P: Impacts of corotating interaction regions

Journal of Geophysical Research: Space Physics, 2016
Jasper S. Halekas   +2 more
exaly  

STEREO observations of the energetic ions in tilted corotating interaction regions

Journal of Geophysical Research: Space Physics, 2011
Radoslav Bučík, Glenn M Mason, U Mall
exaly  

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