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Numerical simulations of trapped slow magnetosonic waves in solar coronal plumes
Advances in Space Research, 2000Abstract 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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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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Bahaeddine Gannouni +2 more
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Properties of solar polar coronal plumes constrained by UVCS data
2007Raouafi, N., Harvey, J., Solanki, S.
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