Image

Fe XIV, 530.3 nm

Fe XIV (coronium) is one of two prominent forbidden lines of Fe ions in the visible part of coronal spectrum. This line is the "easiest" emission line in the solar corona. It is placed near the maximum of both human vision and CCD chips sensitivity. Fe XIV emission was visible even in the viewfinder of Canon EOS 5D camera during taking of slitless spectra.
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ImageTse2010t_Fe_XIV.jpg
Date11. 07. 2010
Time2nd contact 18:45:36 UT, 3rd contact 18:50:05 UT
Total eclipse duration 4 m 29 s
PlaceTatakoto Atoll, French Polynesia
CoordinateS 17° 20' 39.3'',   W 138° 27' 3.1'',  Alt. 6 m
ConditionsPartially clear, partially thin clouds
Optics2× Thorlabs visible achromat 4/200mm equipped with following narrow band filters:
  On-band filter: Andover, center wavelenght: 530.4 nm, bandwidth 50%: 0.5 nm
  Off-band filter: Andover, center wavelenght: 529.2 nm, bandwidth 50%: 0.5 nm
Camera2× Atik 314L+ (chip Sony ICX285AL)
ProcessingImage processing by Miloslav Druckmüller
SoftwarePhaseCorr 6.0, LDIC 5.0, Corona 4.1, Sofo ACC 6.1
NoteSee this ApJ paper for more details.
OrientationSee 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
 


Miloslav Druckmüller
Institute of Mathematics, Faculty of Mechanical Engineering
Brno University of Technology, Czech Republic
druckmuller@fme.vutbr.cz
Page last update: 7.8.2014