SIMPLE = T / Standard FITS format BITPIX = 8 / Character information NAXIS = 0 / No image data array present EXTEND = T / Standard extensions OBJECT = 'P/HALLEY' / Object of investigation FILE-NUM= 089007 / File number DATE-OBS= '13/03/86' / Date of mid-observation TIME-OBS= '.98 ' / Mid-time of observation LONG-OBS= '999/99/99' / Longitude of observatory LAT-OBS = '+99/99/99' / Latitude of observatory DATE-REL= '01/07/90' / Date of release DISCIPLN= 'GIOTTO/DID' / Giotto DIDSY experiment data SYSTEM = '05009983' / Observation system OBSERVER= 'MCDONNELL,J.A.M/ET AL.' / Giotto DIDSY team (as A&A, 1987) SUBMITTR= 'GREEN,S.F/PANKIEWICZ,G.S' / Submitters to IHW SPEC-EVT= F / No special events inserted or deleted DAT-FORM= 'ASCII ' / Data in tabular ASCII form ORIGIN = 'UNIV.KENT,U.K' / Site at which tape was written DATE = '08/05/90' / Date tape was written COMMENT GIOTTO DUST IMPACT DETECTION SYSTEM (DIDSY) DATA COMMENT UNIT FOR SPACE SCIENCES, UNIVERSITY OF KENT, COMMENT CANTERBURY, KENT, CT2 7NR. COMMENT FILE 089007 COMMENT CUMULATIVE FLUXES FROM DISCRETE DATA FOR 10 TIME PE COMMENT COMMENT COMMENT ADD. OBS. ALEXANDER,W.M/BURTON,W.M/BUSSOLETTI,E/EVANS,G.C/ COMMENT ADD. OBS. EVANS,S.T/FIRTH,J.G/GRARD,R.J.L/GREEN,S.F/GRUN,E/ COMMENT ADD. OBS. HANNER,M.S/HUGHES,D.W/IGENBERGS,E/KISSEL,J/ COMMENT ADD. OBS. KUCZERA,H/LINDBLAD,B.A/LANGEVIN,Y/MANDEVILLE,J.C/ COMMENT ADD. OBS. NAPPO,S/PANKIEWICZ,G.S/PERRY,C.H/SCHWEHM,G.H/ COMMENT ADD. OBS. SEKANINA,Z/STEVENSON,T.J/TURNER,R.F/WEISHAUPT,U/ COMMENT ADD. OBS. WALLIS,M.K/ZARNECKI,J.C END XTENSION= 'TABLE ' / Table extension BITPIX = 8 / Character NAXIS = 2 / 2-D matrix NAXIS1 = 45 / Number of characters per row NAXIS2 = 167 / Number of rows PCOUNT = 0 / No random parameters GCOUNT = 1 / Only one group TFIELDS = 8 / Number of fields per row EXTNAME = 7 DIDSY DISCRETE / Name of file EXTVER = 4 / Extension version number TTYPE1 = 'MEAN HR ' / Mean ground received time (hr) TBCOL1 = 1 / Start in column 1 TFORM1 = 'I2 ' / Integer nn TUNIT1 = 'HOUR ' / Hours TTYPE2 = 'MIN ' / Mean ground received time (min) TBCOL2 = 4 / Start in column 4 TFORM2 = 'I2 ' / Integer nn TUNIT2 = 'MIN ' / Minutes TTYPE3 = 'SEC ' / Mean ground received time (sec) TBCOL3 = 7 / Start in column 7 TFORM3 = 'F4.1 ' / Real xx.x TUNIT3 = 'SEC ' / Seconds TTYPE4 = 'MEAN DISTANCE' / Cometocentric distance TBCOL4 = 12 / Start in column 12 TFORM4 = 'I6 ' / Integer nnnnnn TUNIT4 = 'KM ' / Kilometres TTYPE5 = 'COUNTS ' / Discrete counts > mass TBCOL5 = 20 / START IN COLUMN 20 TFORM5 = 'I2 ' / Integer nn TTYPE6 = 'MASS ' / Mass threshold TBCOL6 = 23 / Start in column 23 TFORM6 = 'E9.3 ' / Real x.xxxE+xx TUNIT6 = 'KG ' / Kilogrammes TTYPE7 = 'FLUX ' / Derived particle flux TBCOL7 = 33 / Start in column 33 TFORM7 = 'E9.3 ' / Real x.xxxE+xx TUNIT7 = 'M-2.SEC-1' / PER SQUARE METRE PER SECOND TTYPE8 = 'ERROR ' / Statistical error from counts TBCOL8 = 43 / Start in column 43 TFORM8 = 'I3 ' / Integer nnn TUNIT8 = '% ' / Percentage COMMENT DIDSY DISCRETE DATA ARE A SUBSET OF THE LARGE MASS PARTICLES DETECTED. COMMENT THEY CONSIST OF UP TO FOUR IMPACTS PER DATA GATHERING INTERVAL (1.13S) COMMENT FOR WHICH SIGNALS FROM 2 OR MORE SENSORS ARE AVAILABLE. THIS ALLOWS ANCOMMENT ACTUAL MASS TO BE DERIVED. THE UNCERTAINTY IN MASS FOR AN INDIVIDUAL COMMENT PARTICLE MAY BE HIGH, BUT FOR >10 IMPACTS THE DISTRIBUTION OF MASSES ISCOMMENT REPRESENTATIVE OF THE TRUE POPULATION (C.PERRY PHD). DATA ARE PRESENTEDCOMMENT IN 10 TIME PERIODS (~50% OVERLAP) AS GIVEN IN TABLE: COMMENT PERIOD START TIME END TIME NO OF IMPACTS COMMENT 1 22:59:50 (-4272S) 00:08:52 (-130S) 20 COMMENT 2 00:04:32 (-390S) 00:09:52 (-70S) 20 COMMENT 3 00:08:53 (-129S) 00:10:19 (-43S) 21 COMMENT 4 00:09:53 (-69S) 00:10:36 (-26S) 20 * COMMENT 5 00:10:20 (-42S) 00:10:47 (-18S) 19 * COMMENT 6 00:10:37 (-25S) 00:10:47 (-15S) 18 * COMMENT 7 00:11:18 (+16S) 00:11:41 (+39S) 15 * COMMENT 8 00:11:28 (+26S) 00:12:42 (+100S) 14 * COMMENT 9 00:11:42 (+40S) 00:13:02 (+120S) 12 COMMENT 10 00:12:43 (+100S) 01:01:02 (+3000S) 8 COMMENT PERIODS MARKED * HAVE LARGER UNCERTAINTIES IN MASS DUE TO THE HIGH FLUXCOMMENT OF SMALLER PARTICLES WHICH CAN CAUSE FALSE COINCIDENCE. HISTORY MASSES FOR EACH DISCRETE IMPACT WERE CALCULATED WITH MOMENTUM ENHANCEM-HISTORY ENT OF E=11 FOR NON-PENETRATING PARTICLES: P(MEASURED)=E*P(TRUE). HISTORY FOR PARTICLES WHICH PENETRATE THE FRONT SHIELD THE MEASURED MOMENTUM ISHISTORY DERATED: P(MEASURED)=E*P(TRUE)*(MPEN/M)**G HISTORY WHERE MPEN=PENETRATION MASS (3E-9KG) AND G=MOMENTUM DERATING EXPONENT. HISTORY A VALUE OF G=0.4 WAS USED HERE. MEAN TIME AND DISTANCE QUOTED ARE MEANSHISTORY IN LOG(DISTANCE) SPACE. FLUXES FOR TIMES WITHIN 60 SECONDS OF ENCOUNTERHISTORY ARE CORRECTED FOR INCOMPLETE SAMPLING BY COMPARISON WITH BINNED DATA. END