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J/A+A/531/A173     Spectroscopy of CaII-H line at solar limb   (Beck+, 2011)

Spectroscopy at the solar limb. I. Average off-limb profiles and Doppler shifts of Ca II H. Beck C., Rezaei R. <Astron. Astrophys. 531, A173 (2011)> =2011A&A...531A.173B
ADC_Keywords: Sun ; Spectroscopy Keywords: Sun: chromosphere - techniques: spectroscopic - methods: data analysis Abstract: We present constraints on the thermodynamical structure of the chromosphere from ground-based observations of the CaII H line profile near and off the solar limb. Description: The data used in the publication consist of a set of CaII H spectra taken near and beyond the solar limb on 25/08/2009 at UT 08:43-09:15. The data were obtained with the POLIS instrument at the German VTT. The wavelength range covers the core and the blue wing of the CaII H line from 396.332nm to 396.969nm in 326 steps of 1.96pm. The observations were done by moving the solar image across the slit of the spectrograph with a step width of 0.3-arcsec, yielding in total 134 slit spectra of 326 wavelength points on 244 CCD rows along the slit. The spatial sampling along the slit was 0.3-arcsec. The center of the field-of-view was located at (x,y)=(+37",+920") relative to the center of the solar disk. The data have been corrected for stray-light with the methods described in the article and are normalized to the continuum intensity on disc center. The corresponding data file data.fit is organized as floating array (x,y,wavelength)=(134x244x326) pixels. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file data.fit 2880 14806 Reduced spectra in fits format (stored as a data cube of 134x244x326; steps of 0.3arcsec along X and X, of 1.96pm along Z in range 396.332-396.969nm)
See also: J/A+A/508/1403 : Oxygen lines in solar granulation. II. (Pereira+, 2009) J/A+A/423/1109 : Center-to-limb variation of quiet Sun (Allende+, 2004) Acknowledgements: Christian Beck, cbeck(at)iac.es
(End) Patricia Vannier [CDS] 07-Jun-2011
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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