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Yohkoh Galileo meeting J. Sato The Goal of the Flare Catalogue 1: Sufficient information for flare analysis 2: Easy access to the Catalogue Direct and.

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Presentation on theme: "Yohkoh Galileo meeting J. Sato The Goal of the Flare Catalogue 1: Sufficient information for flare analysis 2: Easy access to the Catalogue Direct and."— Presentation transcript:

1 Yohkoh Galileo meeting J. Sato The Goal of the Flare Catalogue 1: Sufficient information for flare analysis 2: Easy access to the Catalogue Direct and indirect usage for scientific paper product ◎

2 Instruments for the Catalogue SXT: Images HXT: Images, Timeprofiles, Spectrum WBS SXS: Timeprofiles and Spectrum(X) HXS: Timeprofiles and Spectrum GRS: Timeprofiles and Spectrum BCS:?? Supplements: Goes and NOAA number.. etc

3 Current Flare Catalogue Yohkoh Flare Image Catalogue (flare list and images) It covers from 1991/10 to 2001/12. We achieved 1: HXT Flare list 2: SXT and HXT images as a PNG File 3: FITS data of the HXT image near the peak time 4: Simplified documentation

4 Current Flare Catalogue

5 Future plan, I think at this point A1: Data correction of HXT 1: Correction of HXT PC and PH data (TBD) 2: flare images in some saturated flares 3 : BGD database (fits format) 4: Re-calibration of the HXT H-band modulation parameters (TBD) A2: Other instrumental data in the catalogue 5: Timeprofile and Spectrum derived from SXS, HXS and GRS 6: Gamma-line flare information from GRS 7: Plasma temperature derived from GOES data

6 Important future plan, I think…. B: Flare images 1: SXT Te, EM map near the peak time 2: HXT Spectral map near the peak time 3: beginning and decay flare images 4: Providing image data as a fits file 5: Flare movies and HXT movies (TBD)

7 HXT FITS FORMAT (common header and Time info) SIMPLE = T / Written by IDL: Thu Oct 11 16:36: BITPIX = -32 / floating data NAXIS = 2 / NAXIS1 = 64 / NAXIS2 = 64 / TELESCOP= 'Yohkoh Hard X-ray Telescope(HXT)' / OBJECT = 'SUN (flare)' / DATE = ' ' / Date of File Creation ORIGIN = 'Montana State University and HXT Group ' / AUTHOR = 'Jun Sato, M. SAWA and MSU' HDRIDENT= 'hxtFITS 0.8' / HXT Fits version ENE_BAND= 0 / 0=L, 1=M1, 2=M2, 3=H band ENE_RANG= 'L : keV' / 0=L, 1=M1, 2=M2, 3=H band DATE-OBS= ' ' / Date of observation (UT) TIME-OBS= '17:52: ' / mid of observing time(UT) STRT-OBS= '17:51: ' / (UT) END-OBS = '17:52: ' / (UT) EXPTIME = ' ' / Integration Time (sec) BGD-DATE= ' ' / (UT) BGD-STAR= '18:27: ' / (UT) BGD-END = '18:32: ' / (UT)

8 HXT FITS FORMAT (HXT Image info) BSCALE = 1.0 / BZERO = 0.0 / BUNIT = 'count/cm2' / Image Brightness Unit HXT_X0 = / HXT X image center position HXT_Y0 = / HXT Y image center position HXT_EXPF= / Expansion factor of FOV HXT_SERR= / Systematic error factor HXT_GAMA= / Gamma HXT_LINC= 1 / Lambda increment HXT_CLIM= / Chi2 Limit HXT_CHI2= / Final Chi2 Value HXT_LAMB= 11 / Final Lambda HXT_ITER= 20 / Final Iteration Number HXT_DELT= / Final delta HXT_BTOT= / Final Total Brightness HXT_MAXB= / Final max brightness HXT_MINB= / Final min brightness DATA_TYP= 'mem_sato image 1.0' / Imaging method and the version

9 HXT FITS FORMAT (Coordinate and other) CDELT1 = 2.47 / Pixel size x (arc sec) CDELT2 = 2.47 / Pixel size x (arc sec) CTYPE1 = 'Solar-West' / CTYPE2 = 'Solar-North' / CRPIX1 = 32.5 / CRPIX2 = 32.5 / CRVAL1 = / arcsec CRVAL2 = / arcsec SOLAR_R = / optical solar radius (arc sec) SOLAR_B0= / optical solar radius (arc sec) FILENAME= 'hda ' / file name used for selecting flare interval ATTTIM = '14-Apr-01 17:52: ' / Input time to read ATT information COMMENT HISTORY ver Jul END

10 Publications 1.WEB at MSU (from 2001) and ISAS 2.Booklet (Yohkoh Flare Image Catalogue (BW & Color?) ー Yohkoh HXT and SXT Image Catalogue (BW) (2002) Similar to that of Yohkoh HXT Catalogue ー Yohkoh Flare Catalogue (Color?) (2003) Including SXT Te, EM analysis and a good ATT data 3. CDROM (Solar physics, 2002 or 2003) Other 1. Documentation of manual and instruments 2. Calibration History

11 Working group for the Catalogue J. Sato (MSU) K. Yoshimura (ISAS, Japan) T. Watanabe (NAOJ) (WBS) Supporting S. Masuda, M.Sawa and T. Kosugi


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