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Coronal holes are areas where the Sun's corona is darker, and colder, and has lower-density plasma than average. These were found when X-ray telescopes in the Skylab mission were flown above the Earth's atmosphere to reveal the structure of the corona. Coronal holes are linked to unipolar concentrations of open magnetic field lines. During solar minimum, coronal holes are mainly found at the Sun's polar regions, but they can be located anywhere on the sun during solar maximum. The fast-moving component of the solar wind is known to travel along open magnetic field lines that pass through coronal holes.
Originally posted by TauCetixeta
Sorry, but SOHO offered me no Composite Image of our sun in 1996.
I guess it can be stated that i see relationships that others cannot. Hmmm.....
Originally posted by TauCetixeta
reply to post by eriktheawful
Space Weather.com appears to keep an eye on all coronal holes everyday.
Lower Left Side of their webpage.
They also let us know when the coronal hole solar wind will hit the Earth.
Coronal Holes: Wikipedia
Gazing at sun spots has been downright boring.
We can't find any. When we do, they are tiny.edit on 29-4-2013 by TauCetixeta because: (no reason given)edit on 29-4-2013 by TauCetixeta because: (no reason given)
Originally posted by Vasa Croe
Very cool pic. Nice band of activity around the center and very smooth on the top and bottom. Whats up with that?
Originally posted by ngchunter
That's a basic feature of the sunspot cycle. Sunspots (which will correlate with areas of activity like this) start out at higher latitudes early in the sunspot cycle and migrate towards the equator later in the cycle near the maximum.
. As the cycle progresses the number of spots increases and they tend to be formed at lower latitudes toward the equator.
www.enotes.com...