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1The Astrophysical journal

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“The Astrophysical journal” Metadata:

  • Title: The Astrophysical journal
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  • First Year Published: 1902
  • Is Full Text Available: Yes
  • Is The Book Public: Yes
  • Access Status: Public

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    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