Results 81 to 90 of about 1,347 (224)
Magnetic tornadoes, characterized as impulsive Alfvén waves initiated by photospheric vortices in intergranular lanes, are considered efficient energy channels to the corona.
Hidetaka Kuniyoshi +2 more
doaj +1 more source
remendous progress has been made in the field of observational coronal magnetometry in the first decade of the 21st century. With the successful construction of the Coronal Multichannel Magnetometer (CoMP) instrument, observations of the linear ...
Haosheng eLin
doaj +1 more source
We investigated the role of vision in host‐seeking behaviour by Philaenus spumarius, the main European vector of Xylella fastidiosa, through an integrated anatomical, optical, physiological, and behavioural study. Our data highlight that the spittlebug uses visual cues, including polarized light, which may aid in detecting the polarized reflections ...
Domen Lazar +4 more
wiley +1 more source
Near-Sun Characteristics of a CME Inferred from Observations in the 5303 Å Coronal Emission Line
Using observations of the solar corona in the 5303 Å (Fe XIV ) emission line with the Visible Emission Line Coronagraph (VELC) on board Aditya-L1, we estimated the electron density ( N _e ), thermal energy ( E _CME ), and mass ( M _CME ) of a coronal ...
V. Muthu Priyal +4 more
doaj +1 more source
The Effect of Solar Wind Expansion and Nonequilibrium Ionization on the Broadening of Coronal Emission Lines [PDF]
Chris R. Gilly, Steven R. Cranmer
openalex +1 more source
PERIODIC SPECTRAL LINE ASYMMETRIES IN SOLAR CORONAL STRUCTURES FROM SLOW MAGNETOACOUSTIC WAVES
Recent spectral observations of upward moving quasi-periodic intensity perturbations in solar coronal structures have shown evidence of periodic line asymmetries near their footpoints. These observations challenge the established interpretation of the intensity perturbations in terms of propagating slow magnetoacoustic waves.
Verwichte, E. +6 more
openaire +2 more sources
SERTS‐95 Measurements of Wavelength Shifts in Coronal Emission Lines Across a Solar Active Region [PDF]
J. W. Brosius +2 more
openalex +2 more sources
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
Erratum An Assessment of Magnetic Conditions for Strong Coronal Heating in Solar Active Regions by Comparing Observed Loops with Computed Potential Field Lines [PDF]
D. A. Falconer +3 more
openalex +1 more source

