Wide-angle image of solar corona

Totally 117 images taken with two cameras were used for creation of this breathtaking wide-angle image of solar corona. The 24th solar activity cycle was probably very near to its peak during 2013 eclipse therefore a lot of interesting features including two CMEs are visible in the solar corona. The full resolution version of this image you may download here.
Click on the image or on the following reference to display the higher resolution image version (1.3 MB, PNG format).

Date3. 11. 2013
Time2nd contact 13:52:40 UT, total eclipse duration 65 s
Place50 km far from Lambarene, Gabon
CoordinateS 0° 22' 47",   E 10° 20' 43",  Alt. 78 m
ConditionsClear sky in the vicinity of the Sun (solar altitude above the horizon: 45°)
Optics(1) Takahashi FSQ106N
(2) Takahashi FS60C
Camera(1) Nikon D7100
(2) Canon 350D modif.
Exposure(1) 1/2000 s - 2 s (ISO 100) - computer control Solar Eclipse Maestro
(2) 1/2000 s - 2 s (ISO 100) - computer control Solar Eclipse Maestro
ProcessingComposition of totally 117 eclipse images, (1) 66 images, (2) 51 images. Eclipse images were calibrated by means of large number of dark frames and flat-fields, aligned by means of phase correlation, composed by means of LDIC 5.0 software, processed using Corona 4.1 in order to visualize coronal structures. Final processing was done using ACC 6.1 software.
Image processing by Miloslav Druckmüller
SoftwareAstro D3F 2.0, PhaseCorr 6.0, LDIC 6.0, Corona 4.1, Sofo ACC 6.1
Copyright© 2013 Constantinos Emmanoulidis, © 2014 Miloslav Druckmüller

Miloslav Druckmüller
Institute of Mathematics, Faculty of Mechanical Engineering
Brno University of Technology, Czech Republic
Page last update: 27.11.2019