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Chromosphere

From Simple English Wikipedia, the free encyclopedia

Achromosphere ("sphere of color") is the second layer of astar's atmosphere. It is located above thephotosphere and below thesolar transition region andcorona. The term usually refers to theSun's chromosphere, but not only.

The chromosphere gives off electromagnetic radiation in theHα spectral line, allowing for it to be viewed using special filters.

In theSun's atmosphere, the chromosphere is about 3,000 to 5,000 kilometers (1,900 to 3,100 miles) in height, or a little more than 1% of the Sun's radius at maximum thickness. It possesses a homogeneous layer at the border with the photosphere. Hair-like jets ofplasma, calledspicules, rise from this homogeneous area and through the chromosphere, extending up to 10,000 km (6,200 mi) into the corona above.

The chromosphere has a usual and expected red color due toelectromagnetic emissions in theHαspectral line. Information about the chromosphere is mostly received by analysis of its given-off electromagnetic radiation.[1]

Chromospheres have also been followed onstars other than the Sun.[2] On large stars, chromospheres sometimes make up a significant proportion of the whole star. For example, the chromosphere ofsupergiant starAntares has been found to be about 2.5 times larger in thickness than the star's radius.[3]

References

[change |change source]
  1. Jess, D.B; Morton, RJ; Verth, G; Fedun, V; Grant, S.T.D; Gigiozis, I. (July 2015). "Multiwavelength Studies of MHD Waves in the Solar Chromosphere".Space Science Reviews.190 (1–4):103–161.arXiv:1503.01769.Bibcode:2015SSRv..190..103J.doi:10.1007/s11214-015-0141-3.S2CID 55909887.
  2. "The Chromosphere". Archived fromthe original on 2014-04-04. Retrieved2014-04-28.
  3. "Supergiant Atmosphere of Antares Revealed by Radio Telescopes".National Radio Astronomy Observatory. Retrieved9 September 2022.
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