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Solar Wind And Milky Way
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Solar Wind And Milky Way
Credit & Copyright: LASCO, SOHO Consortium, NRL, ESA, NASA
Explanation: The Sun is bright, so bright that it overwhelms the light from other stars even for most satellite-borne telescopes. But LASCO, a coronograph onboard the space-based SOHO Observatory, uses occulting disks to block the intense solar light and examine the tenuous, hot gases millions of miles above the Sun's surface. In this LASCO image from December 24, 1996, an occulting disk (center) and mechanical support (extending from the lower left) are visible along with the billowing Solar Wind. Appearing in the background are faint stars and obscuring dust clouds toward the center of our Milky Way Galaxy! The field of view covers about 16 degrees, corresponding to 28 million miles at the distance of the Sun - just under half the diameter of Mercury's orbit. A prominent dark interstellar dust cloud cuts through the Milky Way starfield running approximately south (lower right) to north. Blemishes on the image are camera streaks caused by charged particles.

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Pn Vt Sr Cht Pt Sb Vs
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31            
1995   1996   1997
1998   1999   2000
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2004   2005   2006
2007   2008   2009
2010   2011   2012
2013   2014   2015
2016   2017   2018
2019   2020   2021
Yanvar'
Fevral'
Mart
Aprel'
Mai
Iyun'
Iyul'
Avgust
Sentyabr'
Oktyabr'
Noyabr'
Dekabr'
Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Russkii tekst
Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: solar wind - Milky Way - Solnechnyi veter - Mlechnyi Put' - Solnechnaya korona - solnechnaya observatoriya - koronograf - kosmicheskie observatorii
Publikacii so slovami: solar wind - Milky Way - Solnechnyi veter - Mlechnyi Put' - Solnechnaya korona - solnechnaya observatoriya - koronograf - kosmicheskie observatorii
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