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Sol

by chipdatajeffb

Our Sun, at h-alpha and Ca-K wavelengths.

Telescope and mount used to make these images, and the computer used to process them, are supplied by 3RF, the Three Rivers Foundation for the Arts & Sciences (www.3rf.org).

45 photos and 3 videos · 478 views
balrog-20060430
AE_Antler_prominence
Solar seagulls
AR875-250frs-20060429
Balrog-comparo.jpg
Sun-20060529
Sunspots 885, 889, and 890 (with loop prominence)
Sunspot group 887 and "curly fries" prominence
20060704-Sunspot898
AR917-early
AR917-10192006-MAP8
Solar Prominence 2-18-2008-B
Processing comparison
Solar Prominence-02-17-2008-a
Prominences
Sunspots 988 and 987. 03-24-2008
Sunspot 988, 03-24-2008
Sunspots, March 24, 2008
Kestrel-frame1
Sunspots, March 25, 2008
First contact
45 minutes into transit
06-Mercury_and_AR923
60 minutes into transit
15 minutes into transit
30 minutes into transit
flare-3-color
flare-2-color
Sunspot 923 Actively flaring during Mercury transit 2006
flare-1-color
Sunspot / Active Region with filaments
Active region (processed), Sept. 8, 2011
Active region processed 0003 negative
Flaring in another active region Sept. 8, 2011
Chromospheric spicule detail, Sept. 8, 2011
Solar image processing note Sept. 8 2011
A solar "filaprom"
The Sun, November 10, 2011
"Negative" image treatment
Active Region 1402, The Sun, Jan. 23, 2012
Prominence over AR 1402 CME site
SolarHalo, January 28, 2012
Solar Prominences, Jan. 27, 2012--Video
Prominence, March 20, 2012
Sunspot group (AR1476 12-05-13), run 7
Sunspot group (AR1476, 12-05-13), run 9
Sunspot group (AR1476, 12-05-13), run 9b
Satellite crossing the Sun?