Solar wind backmapping is a critical technique for analyzing the origin of the solar wind and space weather events by correlating in situ measurements with solar remote-sensing observations.
Xinyi Ma +9 more
doaj +1 more source
Solar Force-free Magnetic Fields
The structure and dynamics of the solar corona is dominated by the magnetic field. In most areas in the corona magnetic forces are so dominant that all non-magnetic forces like plasma pressure gradient and gravity can be neglected in the lowest order ...
Thomas Wiegelmann, Takashi Sakurai
doaj
Day-to-Day Boundary Fluctuations in Coronal Holes: Causes and Consequences. [PDF]
Ugarte-Urra I +3 more
europepmc +1 more source
Spectroscopic Analysis and RHD Modeling of the First Ca II H and H ϵ Flare Spectra from DKIST/ViSP. [PDF]
Tamburri C +9 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
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code. [PDF]
Liakh V, Jenkins J.
europepmc +1 more source
Spatial variation of energy transport mechanisms within solar flare ribbons. [PDF]
Kerr GS +12 more
europepmc +1 more source
Evidence for small-scale torsional Alfvén waves in the solar corona. [PDF]
Morton RJ +5 more
europepmc +1 more source
Martian ionospheric response during the may 2024 solar superstorm. [PDF]
Parrott J +7 more
europepmc +1 more source
Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information. [PDF]
Heinemann SG +7 more
europepmc +1 more source

