Animation, 13 min difference
This animation shows a huge CME propagating through the solar corona. The images for the animation were
taken from two observing places in Argentina with time difference approximately 13 minutes.
Click on the image or on the following reference to display the
higher resolution image version (432 KB, GIF format).
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| Image | TSE_2020_anim_dmh.gif |
| Date | 14. 12. 2020 |
| Time | (1) 2nd contact 16:07:59 UT, 3rd contact 16:10:04 UT
(2) 2nd contact 16:21:11 UT, 3rd contact 16:23:20 UT |
| Place | (1) Fortin Nogueira, Neuquen, Argentina
(2) Bahia Creek, Rio Negro, Argentina |
| Coordinate | (1) S 39° 57.680', W 69° 59.576', Alt. 485 m
(2) S 41°04.93033', W 63° 56.18783', Alt. 28 m |
| Conditions | (1) Clear sky for 85 s of totality otherwise thin clouds
Solar altitude at mid-eclipse 72.4° above horizon
(2) Clear sky
Solar altitude at mid-eclipse 72° above horizon |
| Optics | (1) Nikkor 80-400mm 1:4.5-5.6G ED VR (set to FL 400 mm, F5.6)
(2) Nikkor 105 mm, F 2.5 |
| Camera | (1) Nikon Z6
(2) Nikon D7200 |
| Exposure | (1) 1/640 s - 3 s, ISO 100
(2) 1/500 s - 1/30 s, ISO 400 |
| Processing | Image processing by Miloslav Druckmüller
Images acquired by Andreas Möller and Dario Harari |
| Orientation | This animation has exact solar North on top orientation |
| Copyright | © 2020 Miloslav Druckmüller, Andreas Möller, Dario Harari |
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Miloslav Druckmüller
Institute of Mathematics, Faculty of Mechanical Engineering
Brno University of Technology, Czech Republic
druckmuller@fme.vutbr.cz
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Page last update: 30.1.2021
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