SCORE Data Display and Analysis Software
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1 SCORE Data Display and Analysis Software S. Giordano Rapporto nr /01/2009
2 SCORE DATA DISPLAY and ANALYSIS SOFTWARE SCORE Project prepared by S. Giordano authors S. Giordano reference issue 1.0 revision date of issue 22 January 2009 CHANGE LOG Date issue Revision released by comments 06 Jun S. Giordano Preliminary release sent to team members 06 Sep S. Giordano First Software release for Eclipse data analysis 06 Nov S. Giordano Software release with shutter-less correction 22 Jan S. Giordano Improved software description Table of Contents UVCI FITS Keywords...2 Data processing pipeline...3 Data Display/Analysis software...3 1
3 UVCI FITS Keywords KEYWORD TYPE VALUES DESCRIPTION SIMPLE S*1 T Conforms to FITS standard BITPIX I*2 16 Number of bits per pixel AXIS I*2 2 Number of axes in the image NAXIS1 I*2 512 Length of the first axis (columns) NAXIS2 I*2 512 Length of the second axis (rows) FILENAME S*30 ' fts' Name of the FITS file ONUM I Observation Number TLM_FILE1 S*30 '960501_ img' Name of the raw telemetry file TLM_FILE2 S*30 '960501_ img' Name of the raw telemetry file DATE S*23 '1996/06/06 14:16:50.193' Date of file generation DATE-OBS S*10 '1996/05/01' Date of the start of the exposure TIME-OBS S*12 '03:29:43.489' Time of the start of the exposure EXPTIME S Number of seconds of the exposure time TELESCOP S*8 'HERSCHEL' Name of the satellite INSTRUME S*8 'SCORE' Name of the instrument DETECTOR S*8 'VLD' Name of the telescope TEMP R*4 WLCR Temperature VOLT R*4 WLCR Voltage P1COL I*2 276 CCD column number of start of image P1ROW I*2 257 CCD row number of start of image P2COL I*2 787 CCD column number at end of image P2ROW I*2 768 CCD row number at end of image SUMROW I*2 Number of rows being summed on the CCD SUMCOL I*2 Number of columns being summed on the CCD LAMP I*2 Calibration lamp was/was not commanded FILTER S*8 Position of the filter wheel POLAR S*8 '+60 deg' Position of the polarizer OS_NUM I*2 Observing Sequence Number WAVELENG R* Central observed wavelength PLATESCL R* Number of arc seconds per pixel OFFSET I*2 320 Electronic offset in DN OBT_TIME R* e+09 Value of the On-Board Time DATAMIN R*4 Minimum value of the image, including the bias DATAMAX R*4 Maximum value of the image DATAZER I*4 Number of zero pixels in the image DATAAVG R*4 Average value of the image DATASIG R*4 Standard deviation in computing the average CRPIX1 R*4 Column number of the reference pixel CRPIX2 R*4 Row number of the reference pixel CRVAL1 R*4 Number of arc seconds of the center of the sun from the reference position in the azimuthal direction (E-W). Positive is to the solar west CRVAL2 R*4 Number of arc seconds of the center of the sun from the reference position in the elevation direction (N-S). Positive is to solar north CROTA1 R*4 Rotation of axis 1 with respect to solar north Positive is westward (clockwise) CROTA2 R*4 Rotation of axis 2 with respect to solar north Positive is westward (clockwise) CTYPE1 S*8 SOLAR-X Type of units of axis #1 CTYPE2 S*8 SOLAR-Y Type of units of axis #2 CUNIT1 S*8 ARCSEC Units along axis #1 CUNIT2 S*8 ARCSEC Units along axis #1 CDELT1 R*8 7.0 Increment along axis #1 (Number of arcseconds per pixel) CDELT2 R*8 7.0 Increment along axis #2 (Number of arcseconds per pixel) HISTORY S*80 History of processing. Can be repeated COMMENT S*80 Comments. Can be repeated END 2
4 Data processing pipeline Level 0 - Telemetry Level 0.5 FITS Raw data o o file format file keywords Level 1 from raw into physical units Calibration Processing Steps Subtract bias Multiply by flat field Replace missing blocks or spikes Multiply by (inverse) vignetting function/array Multiply by calibration factor (radiometric sensitivity) Subtract stray light Distortion correction Multiply by (distortion corrected) mask of occulter/pylon/outer edge Level 2 image processing image restoration (PSF deconvolution) image filtering image enhancement sharpening/smoothing/region stretching difference images An open issue is the final data calibration flow, which must be discussed and described in order to develop the data processing code. Data Display/Analysis software A preliminary Graphical User Interface (GUI) of the SCORE Data Display and Analysis Software, Version 0.0, has been developed in Interactive Data Language (IDL) and released to the team on Jun for the analysis of March 2006 eclipse images and comparison with SOHO imagers (LASCO and EIT) and UVCS observations. The code is Operating Systems (OS) independent, that is, it has been tested on Mac OSX, Linux and MS Windows OS. Some features of the developed program requires to run the code into SolarSoft environment, in particular for what concerns the analysis of LASCO and EIT images. An updated version has been released on Nov 6, 2008 with improvements mainly related to instrumental effects correction (shuttler-less correection) Software features requirements Read raw data (level 0.5) Display data display images zoom images plot x and y profiles Calibrate data (to level 1) TBD Save level 1 data Image processing Print images and plots 3
5 The main features implemented are: File menu o Read FITS Read a generic FITS file o FI FITS Read FITS files generated by Firenze group (calibration files) o Read LASCO Read LASCO C2 and C3 FITS files o Read EIT Read EIT FITS files o Write o Keywords Calibration menu o remove dark count o apply flat field o correct distorsion o shutterless correction o define coordinates o LASCO C2 Background o Undo Edit menu o filters unsharp radial sobel o rotate o reverse o modify data range o cut edges o despike o zoom o cut region o composite o UVCS slit o Undo Composite images from different uploaded files Overlap UVCS slit positions Save menu o Image array o image o plot x y radial polar The following procedure allows the user to install the package from distributed compressed file pro.zip and run the code: 1. Unpack the pro.zip file 2. The following directory is created i. PRO 3. Run IDL, compile the code and run the GUI i. ssw ; run the SolarSoft environment ii. idl iii. Working directory PRO/ v. SCORE_DDAS_MW 4
6 The following figure shows the main window of SCORE Data Display and Analysis Software. Figure 1: main window of SCORE Data Display and Analysis Software(V0.0) Figure 2: Example of shutterless correction (Software V0.1) 5
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