Solar magnetic fields are closely related to various physical phenomena on the Sun, which can be extrapolated with different models from photospheric magnetograms.
Guanglu Shi +4 more
doaj +1 more source
Observation and modelling of solar jets. [PDF]
Shen Y.
europepmc +1 more source
Connecting the Low to High Corona: Propagating Disturbances as Tracers of the Near-Sun Solar Wind
We revisit a quiet 14 day period of solar minimum during 2008 January and track substreamer propagating disturbances (PDs) from low heights in STEREO/EUVI to the extended corona through STEREO/COR1 and into STEREO/COR2 along nonradial paths that trace ...
Nathalia Alzate +4 more
doaj +1 more source
The Structure of the Large-Scale Heliosphere as Seen by Current Models. [PDF]
Kleimann J +8 more
europepmc +1 more source
The Lyman α and Lyman β lines in solar coronal streamers [PDF]
No abstract available.
Labrosse, N., Li, X., Li, B.
openaire
Investigation of the Middle Corona with SWAP and a Data-Driven Non-Potential Coronal Magnetic Field Model. [PDF]
Meyer KA +4 more
europepmc +1 more source
<i>Solar Terrestrial Relations Observatory</i> (STEREO) Observations of Stream Interaction Regions in 2007 - 2016: Relationship with Heliospheric Current Sheets, Solar Cycle Variations, and Dual Observations. [PDF]
Jian LK +3 more
europepmc +1 more source
Coronal Streamer Brightness Profiles Investigated with BriLo Using Parker Solar Probe White-Light Data. [PDF]
Cappello GM +10 more
europepmc +1 more source
Day-to-Day Boundary Fluctuations in Coronal Holes: Causes and Consequences. [PDF]
Ugarte-Urra I +3 more
europepmc +1 more source
Introduction to the physics of solar eruptions and their space weather impact. [PDF]
Archontis V, Vlahos L.
europepmc +1 more source

