Outer corona
This image shows the whole corona in a way very similar to the view in a small telescope. To the contrary to
other images on this page, this image has the approximate orientation of original images and must be
rotated 230.7° clockwise to achieve standard orientation. The small dot on the top of the image
is authentic and it is a star.
Click on the following reference to display the same
image in the maximum quality (630 KB, PNG format).
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| Image | Ecl2005_de_out1.jpg |
| Date | 08. 04. 2005 |
| Time | 2nd contact 21:15:05 UT, 3rd contact 21:15:37 UT
Total eclipse duration 32 s |
| Place | Pacific ocean aboard the MV Galapagos Legend (about 2100 km west from the Galapagos) |
| Coordinate | 1° 19.554' S, 109° 30.190' W |
| Conditions | Clear sky, altitude of the Sun above the horizon 60° |
| Optics | Canon 500 mm f/4 IS lens |
| Camera | Canon EOS 1Ds Mark II digital camera |
| Exposure | 1/2000 s - 1/15 s |
| Processing | Composition of 7 images. Images were aligned by means of phase correlation, calibrated and composed using a new, for this purpose newly developed, software LDIC 1.0, processed using Corona 3.0 in order to visualize coronal structures. Final processing was done using ACC 6.0 software.
Image processing by Miloslav Druckmüller |
| Software | PhaseCorr 3.0, LDIC 1.0, Corona 3.0, Sofo ACC 6.0 |
| Orientation | The image has the orientation of original images and it must be rotated 230.7° clockwise to achieve standard orientation (i.e. North at the top) |
| More info | Original set of images |
| Copyright | © 2005 Miloslav Druckmüller, Fred Espenak |
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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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