Results 171 to 180 of about 2,470 (205)
Solar Radio Bursts of Type V Interpreted as Type III's in Superheated Coronal Streamers
The Astrophysical Journal, 1967 openaire +1 more source
Solar prominences: theory and models: Fleshing out the magnetic skeleton. [PDF]
Living Rev Sol Phys, 2018 Gibson SE.
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Cyclic Evolution of Coronal Fields from a Coupled Dynamo Potential-Field Source-Surface Model. [PDF]
Sol Phys, 2016 Dikpati M, Suresh A, Burkepile J.
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Solar wind stream interaction regions throughout the heliosphere. [PDF]
Living Rev Sol Phys, 2018 Richardson IG.
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Understanding the Physical Nature of Coronal "EIT Waves". [PDF]
Sol Phys, 2017 Long DM +11 more
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Influence of projection effects on the observed differential rotation rate in the UV corona. [PDF]
J Adv Res, 2013 Mancuso S, Giordano S.
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The solar origins of solar wind interstream flows: Near‐equatorial coronal streamers
Journal of Geophysical Research: Space Physics, 1981Vela heavy ion and IMP solar wind data are used to identify the coronal origins of the interstream, low‐speed solar wind as well as to understand the causes of the long‐term trends in solar wind densities and electron temperatures observed at 1 AU. Several lines of evidence suggest a strong association between interstream flows and the extensions of ...
W. C. Feldman +4 more
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The origin of the slow solar wind in coronal streamers
Advances in Space Research, 2004Abstract The highly variable slow solar wind has been associated with low-latitude regions of the heliosphere most clearly by the Ulysses spacecraft. Although, it is evident today that the slow solar wind originates in coronal helmet streamers, the mechanism of the slow solar wind acceleration, and the origin of the variability are still being ...
Leon Ofman
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Solar Physics, 1970
A unique combination of photographic and K-coronameter data were used to study the structure and evolution of two known coronal streamers. In addition, two other K-coronameter enhancements were studied as representing ideal second examples of the known streamers.
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A unique combination of photographic and K-coronameter data were used to study the structure and evolution of two known coronal streamers. In addition, two other K-coronameter enhancements were studied as representing ideal second examples of the known streamers.
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Formation of the slow solar wind in a coronal streamer
Journal of Geophysical Research: Space Physics, 1999We have investigated a magnetohydrodynamic mechanism that accounts for several fundamental properties of the slow solar wind, in particular its variability, latitudinal extent, and bulk acceleration. In view of the well‐established association between the streamer belt and the slow wind, our model begins with a simplified representation of a streamer ...
EINAUDI, GIORGIO +3 more
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