Results 101 to 110 of about 41,536 (207)
X-ray imaging of flare loops and coronal arches [PDF]
HXIS (Hard X-ray Imaging Spectrometer) results related to preflare, flare-decay, and post-flare phases in the solar corona are summarized. Particularly discussed are miniflares, long-lived X-ray enhancements along filament channels, flare precursors ...
Svestka, Z.
core +1 more source
Recent coronal loop modeling has emphasized the importance of combining both Coulomb collisions and turbulent scattering to characterize field-aligned thermal conduction, which invokes a hybrid loop model.
Y. Dai, J. J. Xiang, M. D. Ding
doaj +1 more source
Solar activity cycle variation of the K corona
R. Fisher, D. G. Sime
openaire +1 more source
During the 22nd perihelion of Parker Solar Probe at 9.86 solar radii on 2024 December 24, the WISPR telescope captured a detailed sequence of events marking the return of open magnetic flux back to the Sun via the heliospheric current sheet (HCS ...
Angelos Vourlidas +8 more
doaj +1 more source
We present an analysis of Wide-field Imager for Solar PRobe (WISPR) images of the near-Sun heliospheric current sheet (HCS) region from the Parker Solar Probe (PSP) in 2020 January and June.
Paulett C. Liewer +5 more
doaj +1 more source
Exploring the Origin of Solar Energetic Electrons. II. Investigating Turbulent Coronal Acceleration
Nonthermal particle acceleration in the solar corona is evident from both remote hard X-ray sources in the chromosphere and direct in situ detection in the heliosphere.
Ross Pallister +2 more
doaj +1 more source
The Role of Farside Magnetic Structures in Modeling the 2024 Solar Eclipse
The corona is a crucial region that connects the solar surface to the solar wind and serves as the primary site of solar activity. The 2024 total solar eclipse (TSE) provides a unique opportunity to investigate the large-scale coronal structure. Combined
Guanglu Shi +4 more
doaj +1 more source
Analysis of the solar corona structure during the periods of minimum solar activity from 1867 till 2006 has been carried out. A new flattening index for the large coronal streamers has been proposed. It has been shown that the index has been smoothly changing during the last 140 years.
openaire +2 more sources
Transverse oscillations of coronal loops not only influence coronal dynamics, but also provide a new perspective for coronal detection. To enhance their exploitation and utilization, accurately estimating the oscillation parameters is crucial.
Hongbo Li +5 more
doaj +1 more source
Coronal and chromospheric physics [PDF]
Achievements and completed results are discussed for investigations covering solar activity during the solar maximum mission and the solar maximum year; other studies of solar activity and variability; infrared and submillimeter photometry; solar-related
Jefferies, J. T. +2 more
core +1 more source

