SIMPLE = T /CONFORMS TO FITS FORMAT? BITPIX = 16 /NUMBER OF BITS PER PIXEL NAXIS = 1 /NUMBER OF AXES IN ARRAY NAXIS1 = 1284 /DIMENSION OF FASTEST VARYING AXIS EXTEND = T OBJECT = 'VB106 G5V SOLAR ANALOG 'FILE-NUM= 700007 /NUMBER OF FILE SENT FROM SPECTRSCPY TO JPL DATE-OBS= '20/02/84 ' /DATE OF MIDDLE OF DATA ACQUISITION TIME-OBS= 0.09090 /FRACTION OF DATE DATE-REL= '01/04/85 ' /RELEASE DATE DISCIPLN= 'SPECTROSCOPY ' /IHW DISCIPLIN LONG-OBS= '248/27/51 ' /LONGITUDE OF STATION LAT--OBS= '+35/05/49 ' /LATITUDE OF STATION SYSTEM = '76880101 ' /STATION SYSTEM CODE OBSERVER= 'LUTZ,B/WAGNER,M 'SUBMITTR= 'WAGNER,M 'SPEC-EVT= F /SPECIAL EVENT FLAG DAT-FORM= 'STANDARD' /DATA FORM DAT-TYPE= 'REDUCED DIGITAL ' /DATA TYPE DIS-CODE= '010206052 ' /DISCIPLIN CODE OBSVTORY= 'LOWELL OBSERVATORY 'TELESCOP= '1.8-M 'INSTRUME= 'Y SPECT/IDS/600GPM 'ELEV-OBS= 2130 /STATION ELEVATON (METERS) RESOL-SP= '9 ' /APPROX. SPECTRAL RESOLUTION (ANG.) RANGE-SP= '3828-6394 ' /APPROX. SPECTRAL RANGE (ANG.) EXPOSURE= 1920.00000 /EXPOSURE-INTEGRATION TIME (SECONDS) APERSIZE= '7.46 ' /APER SIZE OR SLIT WIDTH & LEN.(ARCSECS) QUALITY = 'VERY GOOD ' /QUALITY FLAG (0-5) CTYPE1 = 'LAMBDA ' /UNITS OF INDEPENDENT VARIABLE BUNIT = 'FLAMBDA ' /UNITS OF DEPENDENT VARIABLE CRVAL1 = 0.382800E+04 /REFERENCE POINT VALUE FOR CTYPE1 CRPIX1 = 0.100000E+01 /REFERENCE PIXEL FOR CTYPE1 CDELT1 = 0.200000E+01 /INCREMENT IN CTYPE1 PER PIXEL HISTORY DATE-CMP 16/06/85 COMMENT HARDORP SOLAR ANALOG BSCALE = 0.358480E-16 /SCALE FACTOR FOR PIXEL TO TRUE VALUES BZERO = 0.194892E-11 /OFFSET APPLIED TO TRUE PIXEL VALUES DEP-MAX = 0.312355E-11 /MAXIMUM OF DEPENDENT VARIABLE DEP-MIN = 0.774253E-12 /MINIMUM OF DEPENDENT VARIABLE END ╣Mù«Ö áü░φ░n⌐f▓┐½╬d╔{▓∙│f¿i╖°á%ú"ñû¬¿}¼9¢ ₧êÑcæ╛ò%£F¥lò;òⁿáûº2▒$╢ì╜(║>½í╜#╛*├φ╟j╙?π:╦â╬$╘╙┐δ¬└▓qª╣₧¼ÖQâíÇ Ç?Ä¿êós¬â▒ⁿ┴K╘â▐g╤╥ ═Ç╬Ö┐■¬*ÿ├ö≤Ö(Å¿Ö1╖g╦Σ╩Γ┐°O°≈»αæÆñ≤ √ÿf░«·╧
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