SIMPLE = T BITPIX = 32 NAXIS = 2 NAXIS1 = 2048 NAXIS2 = 2048 BUNIT = 'PERCENT ' BSCALE = 0.0100000 BZERO = 0.00000 DATAMIN = -25.9900 DATAMAX = 39.6100 CTYPE1 = 'SOLAR_X ' CTYPE2 = 'SOLAR_Y ' CUNIT1 = 'arcsec ' CUNIT2 = 'arcsec ' CRPIX1 = 1024.50 / [pix] CRPIX2 = 1024.50 / [pix] CRVAL1 = -0.0112710 CRVAL2 = -0.390978 CDELT1 = 1.02591 / [arcsec/pix] CDELT2 = 1.02591 / [arcsec/pix] DATE_OBS= '2022-02-12T07:36:02Z' DATE-OBS= '2022-02-12T07:36:02' CENTER_X= 1024.51 / [pix] CENTER_Y= 1024.88 / [pix] SOLAR_R = 952.190 / [pix] ANGLE = -17.1952 / [deg] CROTA1 = 17.1952 / [deg] SOLAR_P0= -16.4408 / [deg] SOLAR_B0= -6.69554 / [deg] OBJECT = 'SUN ' OBS_TYPE= 'HALPH ' OBS_MODE= 'FULL DISK' OBS_PROG= 'HALPHA PATROL' TYPE-DP = 'RESIDUAL' / Data Processing Type TELESCOP= 'KHPI ' INSTRUME= 'HA2 ' DETECTOR= 'TM4200-6' WAVELNTH= 6563 / [ANG], FWHM=0.7 [ANG] EXPTIME = 0.00234900 / [sec] ORIGIN = 'KANZELHOEHE OBSERVATORY, A-9521 TREFFEN, AUSTRIA' DATE = '2022-02-12' / Date of FITS Creation COMMENT Orientation: N up, W right, first pix is left bottom HISTORY Large scale asymmetries corrected by fitting HISTORY polynomials into rings of the Solar disk HISTORY residuals (IMAGE - CLV) normalized to disk center END