Results 81 to 90 of about 1,774 (127)

The helium chromosphere, coronal holes, and stellar X-rays

open access: yesThe Astrophysical Journal, 1975
The solar chromosphere at the limb seen in D3 is an irregular bright band 1000 km thick with a dark band 1000 km thick beneath. The D3 chromosphere disappears in coronal holes. It is shown that the D3 emission, as well as the other He I and He II lines, can be explained quantitatively by photoionization by coronal back-radiation. A Chapman layer with N(
openaire   +1 more source

Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]

open access: yesNat Commun
Cang T   +13 more
europepmc   +2 more sources

Combined ultraviolet studies of astronomical sources [PDF]

open access: yes
Ultraviolet studies of astronomical sources are discussed. Some studies utilized IVE data. Non-radiative shock at the edge of the Cygnses Loop, stellar flares, local interestellar medium, hot galaxies, stellar mass ejection, contact binaries, double ...
Dupree, A. K.   +5 more
core   +1 more source

Stellar activity and coronal heating: an overview of recent results. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci, 2015
Testa P, Saar SH, Drake JJ.
europepmc   +1 more source

Further observations of the lambda 10830 He line in stars and their significance as a measure of stellar activity [PDF]

open access: yes
Measurements of the lambda 1030 He line in 198 stars are given along with data on other features in that spectral range. Nearly 80% of all G and K stars show some lambda 10830; of these, half are variable and 1/4 show emission.
Zirin, H.
core   +1 more source

Potential biosignatures in super-Earth atmospheres II. Photochemical responses. [PDF]

open access: yesAstrobiology, 2013
Grenfell JL   +8 more
europepmc   +1 more source

Asymmetry in zeta Auriage chromospheres [PDF]

open access: yes
Asymmetry in the ultraviolet spectra of zeta-Aur, similar to that reported in optical observations, was studied using IUE data. A plot of the integrated flux of zeta Aurigae from 1625 to 1675 A as a function of absolute phase shows no significant ...
Ahmad, I. A.
core   +1 more source

Beam electrons as a source of Hα flare ribbons. [PDF]

open access: yesNat Commun, 2017
Druett M   +5 more
europepmc   +1 more source

Home - About - Disclaimer - Privacy