Results 141 to 150 of about 205 (182)
Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24. [PDF]
J Adv Res, 2013 Luhmann JG, Petrie G, Riley P.
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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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Large-scale Globally Propagating Coronal Waves. [PDF]
Living Rev Sol Phys, 2015 Warmuth A.
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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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Coronal streamers in the solar wind at 1 AU
Journal of Geophysical Research: Space Physics, 1981Examination of solar wind plasma data obtained by the Los Alamos experiments on Imp 6, 7, and 8 during the 1971–1978 interval has revealed a frequent association between minimums in helium abundance and maximums in proton density. These events occur at low flow speeds and are strongly correlated with polarity reversals in the interplanetary magnetic ...
J. T. Gosling +5 more
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