Credit & Copyright: Miloslav DruckmEller
(Brno U. of Tech.),
Martin Dietzel, Peter Aniol, Vojtech Ruin
Explanation:
Only in the fleeting darkness of a total solar eclipse is the
light of the solar corona easily visible.
Normally overwhelmed by the bright solar disk, the
expansive corona, the
sun's outer atmosphere,
is an alluring sight.
But the subtle details and
extreme ranges in the corona's brightness, although discernible
to the eye, are notoriously difficult to photograph.
Pictured
here,
however, using multiple images and digital processing, is a detailed image of the
Sun's corona taken during the
2008 August total
solar eclipse from
Mongolia.
Clearly visible are
intricate layers and glowing caustics of an ever
changing mixture of hot gas and
magnetic fields.
Bright looping prominences
appear pink just above the Sun's
limb.
A similar solar corona might be
visible through clear
skies in a
thin swath across the USA during a
total solar eclipse that occurs
just one week from tomorrow.
Citizen Science:
How to participate during the Aug. 21 eclipse.
1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 |
Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr' |
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Publikacii s klyuchevymi slovami:
total solar eclipse - polnoe solnechnoe zatmenie - Protuberanec - Solnechnaya korona
Publikacii so slovami: total solar eclipse - polnoe solnechnoe zatmenie - Protuberanec - Solnechnaya korona | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
