Results 141 to 146 of about 1,089,572 (146)
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Numerical simulations of trapped slow magnetosonic waves in solar coronal plumes

Advances in Space Research, 2000
Abstract Recent observations of polar plumes in the southern solar coronal hole by the Extreme ultraviolet Imaging Telescope (EIT) on board the SOHO spacecraft show signatures of quasi-periodic compressional waves. Here, we present the results of a nonlinear, 2D MHD simulation of the slow magnetosonic waves in plumes for typical coronal conditions ...
L. Ofman, C.E. DeForest
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Modelling the formation and  evolution of solar wind microstreams:from coronal plumes to propagating Alfvénic velocity spikes.

Our research delves into solar wind's mesoscale features known as microstreams—periods of heightened speed and temperature lasting hours. Initially observed in Helios and Ulysses data, they're now prevalent in the 'young' solar wind by Parker Solar Probe and Solar Orbiter.
Bahaeddine Gannouni   +2 more
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Plume and interplume regions and solar wind acceleration in polar coronal holes between 1.5 and 3.5 solar radii

1997
S. Giordano   +8 more
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Plume and interplume regions and solar wind acceleration in polar coronal holes between 1.5 and 3.5 R

1997
S. Giordano   +8 more
openaire   +1 more source

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