The integrated sun as a (magnetic) variable star

Ronald L. Gilliland

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

Although the source of the solar magnetic cycle is not yet fully understood, it is clear that observed solar variations result primarily from surface manifestations of magnetic field associated active regions. Globally, and at depth in the solar interior, variations of convective efficiency following from magnetic field variations may cause luminosity and diameter changes. The waxing and waning of sunspots and faculae in the photosphere lead to luminosity variations on time scales of days to months, or longer. In the chromosphere magnetically controlled plage leads to a variation of UV flux and line emission such as Ca II H and K. The coronal structure is dominated by background magnetic fields and experiences factor of 2 variations of total mass over the solar cycle. Relative modulation characteristics are remarkably similar from the different atmospheric levels with their unique activity types.

Original languageEnglish (US)
Pages (from-to)53-63
Number of pages11
JournalAdvances in Space Research
Volume6
Issue number8
DOIs
StatePublished - 1986

Fingerprint

magnetic stars
variable stars
Sun
Stars
sun
Magnetic fields
magnetic field
Luminance
faculae
sunspot
solar cycle
luminosity
magnetic fields
Modulation
Fluxes
solar interior
timescale
chromosphere
photosphere
sunspots

All Science Journal Classification (ASJC) codes

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

Cite this

Gilliland, Ronald L. / The integrated sun as a (magnetic) variable star. In: Advances in Space Research. 1986 ; Vol. 6, No. 8. pp. 53-63.
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The integrated sun as a (magnetic) variable star. / Gilliland, Ronald L.

In: Advances in Space Research, Vol. 6, No. 8, 1986, p. 53-63.

Research output: Contribution to journalArticle

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