File:Jan2010 solar halo.jpg: Difference between revisions
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(Solar halos seen at the CSU-CHILL site on Jan 4, 2010. The 22 degree arc is most prominent, with parhelia (sun dogs) on either side. An upper tangent arc is visible above the sun. Also faintly visible is the parhelic circle running parallel to the horizon) |
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Solar halos seen at the CSU-CHILL site on Jan 4, 2010. The 22 degree arc is most prominent, with parhelia (sun dogs) on either side. An upper tangent arc is visible above the sun. Also faintly visible is the parhelic circle running parallel to the horizon. Also visible (but not pictured here) are [[ | Solar halos seen at the CSU-CHILL site on Jan 4, 2010. The 22 degree arc is most prominent, with parhelia (sun dogs) on either side. An upper tangent arc is visible above the sun. Also faintly visible is the parhelic circle running parallel to the horizon. Also visible (but not pictured here) are [[:Image:Jan2010 solar halo2.jpg|46 degree arcs]]. |
Latest revision as of 22:38, 27 January 2010
Solar halos seen at the CSU-CHILL site on Jan 4, 2010. The 22 degree arc is most prominent, with parhelia (sun dogs) on either side. An upper tangent arc is visible above the sun. Also faintly visible is the parhelic circle running parallel to the horizon. Also visible (but not pictured here) are 46 degree arcs.
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current | 22:32, 27 January 2010 | 2,816 × 2,112 (1,001 KB) | Jgeorge (talk | contribs) | Solar halos seen at the CSU-CHILL site on Jan 4, 2010. The 22 degree arc is most prominent, with parhelia (sun dogs) on either side. An upper tangent arc is visible above the sun. Also faintly visible is the parhelic circle running parallel to the horizon |
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