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chromosphere

American  
[kroh-muh-sfeer] / ˈkroʊ məˌsfɪər /

noun

Astronomy.
  1. a scarlet, gaseous envelope surrounding the sun outside the photosphere, from which enormous quantities of hydrogen and other gases are erupted.

  2. a gaseous envelope surrounding a star.


chromosphere British  
/ ˈkrəʊməˌsfɪə, ˌkrəʊməˈsfɛrɪk /

noun

  1. a gaseous layer of the sun's atmosphere extending from the photosphere to the corona and visible during a total eclipse of the sun

"Collins English Dictionary — Complete & Unabridged" 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

chromosphere Scientific  
/ krōmə-sfîr′ /
  1. A glowing, transparent layer of gas surrounding the photosphere of a star. The Sun's chromosphere is several thousand kilometers thick, is composed mainly of hydrogen at temperatures of 6,000° to 20,000°K, and gives off reddish light.


Other Word Forms

  • chromospheric adjective

Etymology

Origin of chromosphere

First recorded in 1865–70; chromo- + -sphere

Example Sentences

Examples are provided to illustrate real-world usage of words in context. Any opinions expressed do not reflect the views of Dictionary.com.

And last month the agency released the first-ever full-disk images of the Sun in wavelengths ranging from 200 to 400 nanometres, saying they provided "insights into the intricate details of the Sun's photosphere and chromosphere".

From BBC • Jan. 5, 2024

The spacecraft is equipped with seven payloads to study the sun’s corona, chromosphere, photosphere and solar wind, the Indian Space Research Organization said.

From Seattle Times • Sep. 1, 2023

The hot, outer layers of its atmosphere known as the chromosphere appeared to be missing.

From Scientific American • Dec. 23, 2019

Unlike the chromosphere, the corona has been known for many centuries: it was referred to by the Roman historian Plutarch and was discussed in some detail by Kepler.

From Textbooks • Oct. 13, 2016

Slender columns can ordinarily be seen to connect the surface of the chromosphere with its outlying portions.

From A Popular History of Astronomy During the Nineteenth Century Fourth Edition by Clerke, Agnes M. (Agnes Mary)