Results 81 to 90 of about 155,544 (195)

A Comparative Analysis of the Solar Ultraviolet Spectral Irradiance Measured from Earth and Mars: Toward a General Empirical Model for the Study of Planetary Aeronomy

open access: yesThe Astrophysical Journal Supplement Series
Accurate estimation of the solar vacuum ultraviolet irradiance between 0.1 and 200 nm is critical for the study of planetary aeronomy. Previous empirical models have relied on a limited number of reference spectra, or on multiple data sets with various ...
Zhen Xu, Jianqi Qin
doaj   +1 more source

Propagating and Stationary Bright Knots in the Quiet Solar Corona

open access: yesThe Astrophysical Journal
Small-sized localized brightenings are an important candidate for resolving the problem of the solar atmospheric heating. They are spread over the whole solar disk and are suggested to be caused by magnetic reconnection or wave dissipation.
Shaoxuan Tong, Jun Zhang
doaj   +1 more source

Emission of Extreme Ultraviolet Line Radiation from Solar Centers of Activity.

open access: yesThe Astronomical Journal, 1963
Correlation of extreme ultraviolet radiation spectral line emission intensity with active regions on solar disk based on corona electron temperature and ...
openaire   +1 more source

3D Nonequilibrium Ionization and Spectroscopic Modeling of Coronal Mass Ejections. I. Comparison with Hinode/EIS Observations

open access: yesThe Astrophysical Journal
High-resolution EUV spectroscopy provides an informative diagnostic tool for the early evolution of coronal mass ejections (CMEs) since it can directly measure many physical properties of CME plasma close to the Sun that cannot be determined from white ...
E. M. Wraback   +3 more
doaj   +1 more source

Extreme-ultraviolet Polarimetric Diagnostics of the Solar Corona: The Hanle Effect of Ne viii 770 Å

open access: yesThe Astrophysical Journal
Magnetic fields are the primary driver of the plasma thermodynamics in the upper solar atmosphere, especially in the corona. However, magnetic field measurements in the solar corona are sporadic, thereby limiting us from the complete understanding of ...
Raveena Khan   +3 more
doaj   +1 more source

Time-dependent Hinode/EIS Atlas of a Coronal Mass Ejection Containing Cool Material

open access: yesThe Astrophysical Journal
We report the first time-dependent spectral atlas of a coronal mass ejection (CME) observed by the Hinode/Extreme Ultraviolet Imaging Spectrometer (EIS).
E. M. Wraback   +2 more
doaj   +1 more source

Evolution of Flare Ribbon Bead-like Structures in a Solar Flare

open access: yesThe Astrophysical Journal Letters
We present fast-cadence and high-resolution observations of flare ribbons from the Solar Orbiter Extreme Ultraviolet Imager (EUI). Utilizing the short-exposure observations from the EUI High Resolution Imager in the extreme-ultraviolet, we find small ...
Ryan J. French   +8 more
doaj   +1 more source

Extreme-ultraviolet Synthesis of Nanojet-like Ejections due to Coalescing Flux Ropes

open access: yesThe Astrophysical Journal Letters
Detection and characterization of small-scale energetic events such as nanoflares and nanojets remain challenging owing to their short lifetimes, small spatial extent, and relatively low energy release, despite their potential role in coronal heating ...
Samrat Sen   +5 more
doaj   +1 more source

Emission lines in the solar ultraviolet spectrum.

open access: yesThe Astronomical Journal, 1955
F. S. Johnson   +3 more
openaire   +1 more source

Morphological Study of Quiescent Streamers during Solar Minimum by Ultraviolet Emission Lines

open access: yesThe Astrophysical Journal, 2007
We perform, by utilizing spectroscopic measurements made with SOHO/UVCS, a morphological characterization of the quiescent streamer during solar minimum, by means of both a comprehensive survey of daily synoptic observations over 33 weeks from 1996 April to November and detailed analysis of several specialized observations targeting quiescent streamers.
openaire   +1 more source

Home - About - Disclaimer - Privacy