Results 81 to 90 of about 10,692 (216)
Coronal and Chromospheric Dynamics of a Coronal Hole Bright Point
The Astrophysical JournalData from the Atmospheric Imaging Assembly (AIA) and the Helioseismic Magnetic Imager on board the Solar Dynamics Observatory and from the Interface Region Imaging Spectograph, are used to study the evolution at different atmospheric layers of a bright ...
Ana Cristina Cadavid, Mari Paz Miralles
doaj +1 more source
LUCI onboard Lagrange, the next generation of EUV space weather monitoring
Journal of Space Weather and Space Climate, 2020 Lagrange eUv Coronal Imager (LUCI) is a solar imager in the Extreme UltraViolet (EUV) that is being developed as part of the Lagrange mission, a mission designed to be positioned at the L5 Lagrangian point to monitor space weather from its source on the ...
West Matthew J. +9 more
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Coronal Pseudo-Streamer and Bipolar Streamer Observed by SOHO/UVCS in March 2008
, 2015 The last solar minimum is characterized by several peculiar aspects and by the presence of a complex magnetic topology with two different kinds of coronal streamers: pseudo-streamers and bipolar streamers.
Abbo, Lucia +3 more
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Low-latitude coronal holes, decaying active regions and global coronal magnetic structure [PDF]
, 2013 We study the relationship between decaying active region magnetic fields, coronal holes and the global coronal magnetic structure using Global Oscillations Network Group (GONG) synoptic magnetograms, Solar Terrestrial RElations Observatory (STEREO ...
Haislmaier, Karl, Petrie, Gordon
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Journal of Geophysical Research: Space Physics, Volume 131, Issue 1, January 2026.Abstract A number of mechanisms have been suggested to operate within the terrestrial bow shock to redistribute energy contained in the incoming solar wind flow. The majority of mechanisms involve the generation of turbulence while some are based on particle motion alone.
Simon N. Walker +2 more
wiley +1 more source
Geomagnetic storms and their sources on the sun:the rising phase of the sunspot cycle
Antarctic Record, 2013 Solar phenomena, including solar flares and coronal holes, are considered in the context of a NEWS coordinate system, obtained by application of the heliographic and heliomagnetic coordinate systems to the solar latitude and longitude, respectively.
Takao Saito +4 more
doaj +1 more source
Out-of-ecliptic studies of coronal holes and their relation to the solar wind [PDF]
The advantages of observing coronal holes of the sun above the solar ecliptic plane by a solar probe are discussed. Also discussed are the size of coronal holes, their temperature, and magnetic fields associated with the holes.
Noyes, R. W.
core +1 more source
Recent Observations of Plasma and Alfvenic Wave Energy Injection at the Base of the Fast Solar Wind
, 2012 We take stock of recent observations that identify the episodic plasma heating and injection of Alfvenic energy at the base of fast solar wind (in coronal holes).
McIntosh, Scott W.
core +1 more source
A turbulence-driven model for heating and acceleration of the fast wind in coronal holes [PDF]
, 2009 A model is presented for generation of fast solar wind in coronal holes, relying on heating that is dominated by turbulent dissipation of MHD fluctuations transported upwards in the solar atmosphere.
A. Verdini +24 more
core +8 more sources
Solar Wind Acceleration in Coronal Holes
, 2002 This paper reviews the current state of our understanding of high-speed solar wind acceleration in coronal holes. Observations by SOHO, coupled with interplanetary particle measurements going back several decades, have put strong constraints on possible explanations for how the protons, electrons, and minor ions receive their extreme kinetic properties.
openaire +2 more sources