A chromosphere ("sphere of color") is the second layer of a star's atmosphere, located above the photosphere and below the solar transition region and corona. The term usually refers to the Sun's chromosphere, but not exclusively.
In the Sun's atmosphere, the chromosphere is roughly 3,000 to 5,000 kilometers (1,900 to 3,100 miles) in height, or slightly more than 1% of the Sun's radius at maximum thickness. It possesses a homogeneous layer at the boundary with the photosphere. Narrow jets of plasma, called spicules, rise from this homogeneous region and through the chromosphere, extending up to 10,000 km (6,200 mi) into the corona above.
The chromosphere has a characteristic red color due to electromagnetic emissions in the Hα spectral line. Information about the chromosphere is primarily obtained by analysis of its emitted electromagnetic radiation.[1] The chromosphere is also visible in the light emitted by ionized calcium, Ca II, in the violet part of the solar spectrum at a wavelength of 393.4 nanometers (the Calcium K-line).[2]
Chromospheres have also been observed on stars other than the Sun.[3] On large stars, chromospheres sometimes make up a significant proportion of the entire star. For example, the chromosphere of supergiant star Antares has been found to be about 2.5 times larger in thickness than the star's radius.[4]
- ^ 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.
- ^ [1]
This article incorporates text from this source, which is in the public domain.
- ^ "The Chromosphere". Archived from the original on 2014-04-04. Retrieved 2014-04-28.
- ^ "Supergiant Atmosphere of Antares Revealed by Radio Telescopes". National Radio Astronomy Observatory. Retrieved 9 September 2022.
