Results 131 to 140 of about 10,729 (219)
Interaction of minor ions with fast and slow shocks [PDF]
The coronal slow shock was predicted to exist embedded in large coronal holes at 4 to 10 solar radii. A three-fluid model was used to study the jumps in minor ions propertes across the coronal slow shock.
Whang, Y. C.
core +1 more source
The solar minima between solar cycles 22–23, 23–24, and 24–25 are the best observed minima on record. In situ solar wind and interplanetary magnetic field measurements by the Wind and ACE spacecraft at L1 with 1 hr cadence are explored using wavelet ...
P. J. Steyn +3 more
doaj +1 more source
The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models
In this review, our present day understanding of the Sun’s global photospheric and coronal magnetic fields is discussed from both observational and theoretical viewpoints. Firstly, the large-scale properties of photospheric magnetic fields are described,
Duncan Mackay, Anthony Yeates
doaj
The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images. [PDF]
Seaton DB +7 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
Coronal Streamer Brightness Profiles Investigated with BriLo Using Parker Solar Probe White-Light Data. [PDF]
Cappello GM +10 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
Simulating high-speed solar wind streams from coronal holes using an L5-L1 configuration of lagrangian points. [PDF]
Podladchikova T +3 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

