Abstract
In Part I of this review, the concepts of solar vacuum-ultraviolet (VUV) observations were outlined together with a discussion of the space instrumentation used for the investigations. A section on spectroradiometry provided some quantitative results on the solar VUV radiation without considering any details of the solar phenomena leading to the radiation. Here, in Part II, we present solar VUV observations over the last decades and their interpretations in terms of the plasma processes and the parameters of the solar atmosphere, with emphasis on the spatial and thermal structures of the chromosphere, transition region and corona of the quiet Sun. In addition, observations of active regions, solar flares and prominences are included as well as of small-scale events. Special sections are devoted to the elemental composition of the solar atmosphere and theoretical considerations on the heating of the corona and the generation of the solar wind.
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Abbreviations
- ACE:
-
Advanced Composition Explorer
- BCS:
-
Bragg Crystal Spectrometer
- CDS:
-
Coronal Diagnostic Spectrometer
- CI:
-
Carbonaceous Ivuna
- CHASE:
-
Coronal Helium Abundance Spacelab Experiment
- CME:
-
Coronal Mass Ejection
- DEM:
-
Differential Emission Measure
- EIT:
-
Extreme-ultraviolet Imaging Telescope
- EUV:
-
Extreme Ultraviolet
- FIP:
-
First Ionization Potential
- FUSE:
-
Far-Ultraviolet Spectroscopic Explorer
- GIS:
-
Grazing-Incidence Spectrometer
- HCO:
-
Harvard College Observatory
- HRTS:
-
High-Resolution Telescope and Spectrograph
- ISSI:
-
International Space Science Institute
- IUE:
-
International Ultraviolet Explorer
- JOP:
-
Joint Observing Programme
- KPNSO:
-
Kitt Peak National Solar Observatory
- LASCO:
-
Large Angle Spectroscopic Coronagraph
- LASP:
-
Laboratory for Atmospheric and Space Physics
- LOS:
-
Line of Sight
- MDI:
-
Michelson Doppler Imager
- MHD:
-
Magneto-Hydrodynamics
- MICA:
-
Mirror Coronagraph for Argentina
- MPS:
-
Max-Planck-Institut für Sonnensystemforschung
- MSDP:
-
Multichannel Subtractive Double Pass
- MSSTA:
-
Multi-Spectral Solar Telescope Array
- NRL:
-
Naval Research Laboratory
- NIXT:
-
Normal-Incidence X-ray Telescope
- OSO:
-
Orbiting Solar Observatory
- QLT:
-
Quasi-Linear Theory
- RESIK:
-
Rentgenovsky Spektrometr s Izognutymi Kristalami
- SEM:
-
Solar Extreme-ultraviolet Monitor
- SERTS:
-
Solar Extreme-ultraviolet Research Telescope and Spectrograph
- SMM:
-
Solar Maximum Mission
- SOHO:
-
Solar and Heliospheric Observatory
- SOLFLEX:
-
Solar Flare X-rays
- SOLSTICE:
-
Solar-Stellar Irradiance Comparison Experiment
- STEREO:
-
Solar Terrestrial Relations Observatory
- SUMER:
-
Solar Ultraviolet Measurements of Emitted Radiation
- SWICS:
-
Solar Wind Ion Composition Spectrometer
- SXT:
-
Soft X-ray Telescope
- THEMIS:
-
Telescopio Heliografico para el Estudio del Magnetismo y de las Inestabilidades Solares
- TRACE:
-
Transition Region and Coronal Explorer
- TRC:
-
Transition Region Camera
- UCS:
-
Ultraviolet Coronal Spectrometer
- UVCS:
-
Ultraviolet Coronagraph Spectrometer
- UVSP:
-
Ultraviolet Spectrometer and Polarimeter
- VAULT:
-
Very high Angular-resolution Ultraviolet Telescope
- VDF:
-
Velocity Distribution Function
- VLA:
-
Very Large Array
- VUV:
-
Vacuum Ultraviolet
- WKB:
-
Wentzel–Kramers–Brillouin (method)
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Wilhelm, K., Marsch, E., Dwivedi, B.N. et al. Observations of the Sun at Vacuum-Ultraviolet Wavelengths from Space. Part II: Results and Interpretations. Space Sci Rev 133, 103–179 (2007). https://doi.org/10.1007/s11214-007-9285-0
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DOI: https://doi.org/10.1007/s11214-007-9285-0