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| Date & Time: | Oct 25 2014, Times are displayed in image |
| Optical: | CORONADO SolarMax 40, with 1.5× conversion lens (f=600mm, F15.0) |
| Auto-guided with Kenko SKYMEMO Equatorial | |
| Camera: | CELESTRON Skyris445C with IDAS IR-cut filter |
| Location: | Ooizumi, Hokuto city, Yamanashi pref. |
| Camera Settings: | 15 flames/sec.×8sec., Exp....1/60sec |
| 110 flames stacked each & Wavelet process with Registax6 |
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The large-scaled active region of #2192 in Oct 2014 had several solar explosions, the flare.
This set of images shows you the appearance of a largest-scale (X-class) flare and its change chased through the Hα light.
You can see the flare as over-exposed region between two principal sunspots in an image at 8:33, and the light is reducing with time course.
And the images show several thin stripes between the sunspots, it's called "the post-flare-loops", the prominences with its shapes change in short time. |  Full-disk image with Hα light (Oct 25) |
| Warning:
When using a telescope for observing or photographing the sun, lacking knowledge of proper solar filtering methods can pose risks of visual impairment or blindness. I do not assume any responsibility for any accidents that may occur as a result of observing or photographing the sun through this site. |
 Sunspot Group #2192 in Oct 2014: White-light images for 4days |
 SunspotGroup #2192 in Oct 2014: Change of shape with White & Hα light |
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Copyright(c) 2014 by Naoyuki Kurita, All rights reserved. |
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