Explore: Solar Lines
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AI-Generated Overview About “solar-lines”:
Books Results
Source: The Open Library
The Open Library Search Results
Search results from The Open Library
1The Astrophysical journal
By No name

“The Astrophysical journal” Metadata:
- Title: The Astrophysical journal
- Author: No name
- Publish Date: 1902
“The Astrophysical journal” Subjects and Themes:
- Subjects: ➤ lines - spectrum - solar - spectra - arc - grating - spark - velocity - intensity - slit - minor contributions - bruce spectrograph - solar spectrum - subordinate series - radial velocity - bright lines - angular momentum - solar lines - iron lines - arc spectrum
Edition Identifiers:
- The Open Library ID: OL20555686M
Author's Alternative Names:
"Sine Nomine"Access and General Info:
- First Year Published: 1902
- Is Full Text Available: Yes
- Is The Book Public: Yes
- Access Status: Public
Online Access
Online Borrowing:
- Borrowing from Open Library: Borrowing link
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Wiki
Source: Wikipedia
Wikipedia Results
Search Results from Wikipedia
Fraunhofer lines
and are formed when atoms in the solar atmosphere absorb light being emitted by the solar photosphere. The lines are named after German physicist Joseph
Solar prominence
time. During the solar eclipse of August 18, 1868, spectroscopes were for the first time able to detect the presence of emission lines from prominences
Solar power
Solar power, also known as solar electricity, is the conversion of energy from sunlight into electricity, either directly using photovoltaics (PV) or indirectly
Solar wind
The solar wind is a stream of charged particles released from the Sun's outermost atmospheric layer, the corona. This plasma mostly consists of electrons
Sun
The Sun is the star at the centre of the Solar System. It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion
Solar term
of Solar Terms" (simplified Chinese: 节气歌; traditional Chinese: 節氣歌; pinyin: jiéqìgē) is used to ease the memorization of jieqi: The first four lines provides
Solar flare
ejections, solar particle events, and other eruptive solar phenomena. The occurrence of solar flares varies with the 11-year solar cycle. Solar flares are
Aurora
derived from the solar wind, the electrons themselves do not travel directly from the solar wind into Earth's auroral zone; magnetic field lines from these
Solar symbol
A solar symbol is a symbol representing the Sun. Common solar symbols include circles (with or without rays), crosses, and spirals. In religious iconography
Geomagnetic storm
often originate from solar active regions, while the latter originate at the boundary between high- and low-speed streams of solar wind. The frequency