Fe X, forbidden line 637.4 nm
Fe X is one of two prominent forbidden lines of Fe
ions in the visible part of coronal spectrum. The image shows all solar corona which was progressively
visible from our observing place. That is why the black part of the image, which is the area
without any information about solar corona, is not round. It is an intersection of two circles
representing the position of the Moon in the beginning and at the end of the total solar eclipse.
Click on the following reference to display the same
image in the maximum quality (564 KB, PNG format).
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| Image | Tse2010t_Fe_X.jpg |
| Date | 11. 07. 2010 |
| Time | 2nd contact 18:45:36 UT, 3rd contact 18:50:05 UT
Total eclipse duration 4 m 29 s |
| Place | Tatakoto Atoll, French Polynesia |
| Coordinate | S 17° 20' 39.3'', W 138° 27' 3.1'', Alt. 6 m |
| Conditions | Partially clear, partially thin clouds |
| Optics | 2× Thorlabs near IR achromat 4/200mm equipped with following narrow band filters:
On-band filter: Andover, center wavelenght: 637.5 nm, bandwidth 50%: 0.5 nm
Off-band filter: Andover, center wavelenght: 636.4 nm, bandwidth 50%: 0.5 nm |
| Camera | 2× Atik 314L+ (chip Sony ICX285AL) |
| Processing | Image processing by Miloslav Druckmüller |
| Software | PhaseCorr 6.0, LDIC 5.0, Corona 4.1, Sofo ACC 6.1 |
| Note | See this ApJ paper for more details. |
| Orientation | See this image. The white circle represents the position of photosphere. |
| Copyright | © 2010 Shadia Habbal, Huw Morgan, Judd Johnson, Martina Arndt, Adrian Daw
© 2011 Miloslav Druckmüller |
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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: 27.11.2019
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