Steratmosfeer (Dutch Wikipedia)

Analysis of information sources in references of the Wikipedia article "Steratmosfeer" in Dutch language version.

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archive.org

Lang, K.R. (September 2006). Sun, earth, and sky, 2nd. Springer, "5.1 MAGNETIC FIELDS IN THE VISIBLE PHOTOSPHERE", 81. ISBN 978-0-387-30456-4 "this opaque layer is the photosphere, the level of the Sun from which we get our light and heat"
Lewis, J.S. (23 februari 2004). Physics and chemistry of the solar system, Second. Elsevier Academic Press, 87. ISBN 978-0-12-446744-6 "The dominant color is influenced by the Balmer radiation of atomic hydrogen"

R.C. Altrock (2004). The Temperature of the Low Corona During Solar Cycles 21–23. Solar Physics 224. DOI: 10.1007/s11207-005-6502-4.
Griffin, R.E. (27 augustus 2007). Only Binary Stars Can Help Us Actually SEE a Stellar Chromosphere, 1. Cambridge University Press. DOI:10.1017/S1743921307006163, p. 460. ISBN 978-0-521-86348-3. Geraadpleegd op 21 mei 2010.

The Sun's Corona – Introduction. NASA. Geraadpleegd op 21 mei 2010. “Now most scientists believe that the heating of the corona is linked to the interaction of the magnetic field lines.”

"Beyond the Blue Horizon" – A Total Solar Eclipse Chase (5 augustus 1999). Geraadpleegd op 21 mei 2010. “On ordinary days, the corona is hidden by the blue sky, since it is about a million times fainter than the layer of the sun we see shining every day, the photosphere.”