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Creating Calibrated Images with SECCHI_PREP

Creating Calibrated Images with SECCHI_PREP. 5 th SECCHI Consortium Meeting March 6, 2007 Robin Colaninno Naval Research Laboratory George Mason University. What is SECCHI_PREP?. SECCHI_PREP. Level 1.0 Data.

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Creating Calibrated Images with SECCHI_PREP

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  1. Creating Calibrated Images • with • SECCHI_PREP 5th SECCHI Consortium Meeting March 6, 2007 Robin Colaninno Naval Research Laboratory George Mason University 5th SECCHI Consortium Meeting Orsay, France

  2. 5th SECCHI Consortium Meeting Orsay, France What is SECCHI_PREP? SECCHI_PREP Level 1.0 Data • IDL software routine to read in and perform the latest calibration and image correction procedures for all SECCHI instruments. • SECCHI_PREP is intended to be the single routine that the user would interact with to process level 0.5 data. Level 0.5 Data Level 2.0 Data

  3. 5th SECCHI Consortium Meeting Orsay, France The SECCHI_PREP Way • Fast, Efficient, Flexible and Friendly • All Procedures Are Modular • Calibration is Easily Updatable • Optional XSECCHI_PREP GUI • Intended Users • Instrument Teams • Solar Physicists and Researchers • Other SSW Applications (Festival and SWB)

  4. 5th SECCHI Consortium Meeting Orsay, France SECCHI_PREP • General Procedures • Reads Image and Header • Trims Image • Buffers Subfield Images • Calibrates Images • Updates Header • Returns to Memory and/or Writes Image Files • FITS, PNG, and JPG

  5. 5th SECCHI Consortium Meeting Orsay, France Using SECCHI_PREP with EUVI • Correction • SEB Image Processing Correction • SEB IP - divide by 2, 3, 4 and square root • Normalize to 'Clear Filter' • Subtract the Bias • Normalize Exposure Time • Apply a Calibration Image • DN to Detected Photons Correction

  6. 5th SECCHI Consortium Meeting Orsay, France Using SECCHI_PREP with COR1 & COR2 • Calibration • SEB Image Processing Correction • SEB IP - divide by 2, 3, 4 and square root • Subtract the Bias • Normalize Exposure Time • Apply a Calibration Image • vignetting and flat fielding • DN to MSB Calibration Factor

  7. 5th SECCHI Consortium Meeting Orsay, France Creating Level 2 Images • Polarization Image • Total Brightness • Polarized Brightness • Percent Polarized • Polarization Angle • Restrictions • Input files must be sorted into triples • Only one type of image can be returned

  8. 5th SECCHI Consortium Meeting Orsay, France Using SECCHI_PREP with HI1 & HI2 • Correction • Corrects for Shutterless Mode • Steve Crothers • Apply a Calibration Image

  9. Default call: IDL> secchi_prep, files, image, header To limit the memory usage: IDL> secchi_prep, files, image ,header, outsize = 512 To save FITS file and return to memory: IDL> secchi_prep, files, image, header, /write_fts To only save FITS file : IDL> secchi_prep, files, /write_fts Example Calls 5th SECCHI Consortium Meeting Orsay, France

  10. SECCHI_PREP, filenames, images, headers [,SAVEPATH=path] [,OUTSIZE=value] [,/WRITE_FTS] [,/WRITE_PNG] [,/WRITE_JPG] [,/TRIM_OFF] [,/ROTATE_ON] [,/CALIBRATE_OFF] [,/CALFAC_OFF] [,/NORMAL_OFF] [,/DN2P_OFF] [,/BIAS_OFF] [,/EXPTIME_OFF] [,/CALIMG_OFF] [,/SEBIP_OFF] [,/NEW_CALIMG] [,CALIMG_FILENAME=filename] [,/SHUTTERLESS_OFF] [/SMASK_ON] [/IMASK_ON] [,/BMASK_OFF] [,/FILL_MEAN] [,/FILL_VALUE=value] [/POLARIZ_ON] [,/pB] [,/MU] [,/PERCENT] [,/COLOR_ON] [,/DATE_ON] [/LOGO_ON] SECCHI_PREP Keywords 5th SECCHI Consortium Meeting Orsay, France

  11. 5th SECCHI Consortium Meeting Orsay, France XSECCHI_PREP

  12. 5th SECCHI Consortium Meeting Orsay, France Future Improvements • ICER Missing Sector Masking • Background Subtraction • Cosmic Ray and Star Removal • Expanding COR_POLARIZ • And?

  13. 5th SECCHI Consortium Meeting Orsay, France Websites • SECCHI_PREP User Guide http://secchi.nrl.navy.mil/wiki/pmwiki.php?n=Main.SecchiPrep • Feedback • SECCHI Bugzilla http://secchi.nrl.navy.mil/bugzilla/ • SECCHI_PREP Feature Request Wiki Page http://secchi.nrl.navy.mil/wiki/pmwiki.php?n=Main.SecchiPrep

  14. SECCHI Prepped 5th SECCHI Consortium Meeting Orsay, France

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