Results 111 to 120 of about 1,105,860 (262)
We determine magnetic fields from the photosphere to the upper chromosphere combining data from the Hinode satellite and the CLASP2.1 sounding rocket experiment.
Ryohko Ishikawa +19 more
doaj +1 more source
Collisional dissipation of Alfvén waves in a partially ionised solar chromosphere [PDF]
J. E. Leake +2 more
openalex +1 more source
PROPAGATION OF ALFVÉNIC WAVES FROM CORONA TO CHROMOSPHERE AND CONSEQUENCES FOR SOLAR FLARES [PDF]
A. J. B. Russell, L. Fletcher
openalex +1 more source
Zero-Field Dichroism in the Solar Chromosphere
We explain the linear polarization of the Ca II infrared triplet observed close to the edge of the solar disk. In particular, we demonstrate that the physical origin of the enigmatic polarizations of the 866.2 nm and 854.2 nm lines lies in the existence of atomic polarization in their metastable lower levels, which produces differential absorption of ...
Sainz, R. Manso, Bueno, J. Trujillo
openaire +3 more sources
High-frequency Wave Power Observed in the Solar Chromosphere with IBIS and ALMA [PDF]
Momchil Molnar +5 more
openalex +1 more source
THE INFLUENCE OF THE MAGNETIC FIELD ON RUNNING PENUMBRAL WAVES IN THE SOLAR CHROMOSPHERE [PDF]
D. B. Jess +4 more
openalex +1 more source
Height and dynamics of the quiet solar chromosphere at the limb [PDF]
K. Muglach, W. Schmidt
openalex +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Effects of Ion Magnetization on the Farley–Buneman Instability in the Solar Chromosphere [PDF]
Alex Fletcher +3 more
openalex +1 more source
Solar Flare Ribbon Fronts. II. Evolution of Heating Rates in Individual Flare Footpoints
Solar flare ribbon fronts appear ahead of the bright structures that normally characterize solar flares, and can persist for an extended period of time in spatially localized patches before transitioning to “regular” bright ribbons. They likely represent
Graham S. Kerr +3 more
doaj +1 more source

