Results 111 to 120 of about 39,482 (251)
Solar Cycle Indices from the Photosphere to the Corona: Measurements and Underlying Physics [PDF]
Ilaria Ermolli +3 more
openalex +1 more source
The anatomy of a long gamma-ray burst: a simple classification scheme for the emission mechanism(s)
Ultra-relativistic motion and efficient conversion of kinetic energy to radiation are required by gamma-ray burst (GRB) observations, yet they are difficult to simultaneously achieve.
Burgess, J. Michael, Bégué, Damien
core +1 more source
Magnetic flux ropes are fundamental magnetic structures in solar eruptions, whose formation is generally attributed to: (1) the emergence of subsurface flux tubes; or (2) flux cancellation driven by photospheric horizontal flows and magnetic reconnection.
Can Wang +5 more
doaj +1 more source
Meteoritics &Planetary Science, Volume 60, Issue 12, Page 2757-2758, December 2025.
wiley +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
Hot Mantles, Moderate Photospheres for Wolf-Rayet Stars [PDF]
Anne B. Underhill
openalex +1 more source
Study on the relation of the solar coronal rotation with magnetic field structures. [PDF]
Xiang NB +4 more
europepmc +1 more source
Temporal evolution of small-scale internetwork magnetic fields in the solar photosphere [PDF]
R. J. Campbell +7 more
openalex +1 more source
Statistical Investigation of Wave Propagation in the Quiet-Sun Using IRIS Spectroscopic Observations
In this analysis, we use spectroscopic observations of the quiet Sun made by the IRIS instrument and investigate wave propagation. We analyze various spectral lines formed in different atmospheric layers, such as the photosphere, chromosphere, and ...
Kartika Sangal +4 more
doaj +1 more source
Space weather models endeavoring to connect remote observations to in-situ measurements at various locations in the heliosphere invariably require a coronal model to connect the photosphere magnetically to the inner heliosphere.
Kalman J. Knizhnik
doaj +1 more source

