ࡱ> *,)q`0bjbjqPqP.2:: <<<<<<<P8 8 8 8 4l PH2 p       $zh!Q<     <<  000 < < 0 00h<< o8 #w0H3v" pv" v"<  0        H    PPPd PPP PPP<<<<<< Comments to SEP events composition database. This database is connected from SEP fluences, measured from 1998 to 2006 with the instruments on the satellites GOES and ACE. In this period we selected 56 SEP events and determined the p, He (instruments DOME and GOES), C, N, O, Ne, Mg, Si, S and Fe (instrument SIS, spacecraft ACE) fluences. The event selection The SEP events were selected by GOES-8 4th channel (15-40 MeV) data (see Fig.1). By given data was determined the 24 hour time period with a maximum proton flux. The fluxes of another particles were determined in the same time period. For the particle fluence determination the 24 1-hour fluxes from Internet databases were summarized.  Fig. 1. The proton fluxes measured by GOES-8 instrument in energy channel 15-40 MeV from 8 to 11 Nov. 2000. The 24 hour maximum particle flux interval selected, is shown. The energy spectra, determined from experimental data. The all energy spectra are given as power function of the particle momentum (per nucleon):  EMBED Equation.3  where  EMBED Equation.3  and  EMBED Equation.3  EMBED Equation.3  E  ion s kinetic energy in MeV/nucl; Moc2 =938 MeV  nucleon rest energy; =v/c  particle s relative velocity. Value p=239 MeV/nucleon corresponds to the particle s energy E=30 MeV/nucl and proton s rigidity R=239 MV. In case of Ee"30 MeV/nucleon (z)=o(z) and if E<30 MeV/nucl -  EMBED Equation.3  (3) So, every spectrum is determined by 3 parameters: C(z) - spectral coefficient, o(z)  spectral index and (z) - droop index. On the Fig. 2 the Oxygen fluences and the corresponding energy spectra for the SEP event from 8 Nov. 2000 are demonstrated. At Ee"30 MeV/nucleon the spectrum is power law from particle momentum (per nucleon) with the spectral index o(O)=8.0. At the E<30 MeV/nucleon the spectrum droops according to the droop index (O)=0.30 value. At the E=30 MeV/nucleon the particle fluence is F(30)=C(O)/, where C=28.6 and =0.25.  Fig.2. Measured by SIS ACE oxygen fluences for Nov. 26 2000 SEP event (the stepped line) and corresponding energy spectrum (green line). The spectrum without the droop effect (blue dashed line) is also shown. The database content The database contents data of 56 SEP events. The data are systematized by the 6 numbers code: 000000. First 2 numbers are the 2 last number of the year. Examples: 00 is 2000, 06 is 2006, 99 is 1999. Second 2 numbers are the month number, third 2 numbers are day, when the 15-40 MeV proton flux started grow from the flux background or fr,-He 9 F I R S U h i m   g ȼpg\ThD mH sH hD hD mH sH hfh5mH sH  jhvC3hvC35UmH sH hShfhmH sH hu~mH sH hShSH*mH sH hSmH sH hShSmH sH hF5mH sH haha5mH sH hamH sH h'YmH sH hX mH sH hFmH sH ha1mH sH ha`mH sH h#)mH sH  -.T U i h i j * >>$  !h`ha$gdu~  !h`hgdu~  !gdSh^hgdSh^hgdu~$a$gdD $a$gdfh`gdS0g h j " $ & ( 6 8 ^ ` b d n p ҿxgXG8jK hSCJUVaJ!j hhSEHUmH sH jK hSCJUVaJ!jh-#hSEHUmH sH jK hSCJUVaJhSmH sH jhSUmH sH h;(hS5\mH sH +h,hSCJOJQJ\^JaJmH sH %hSCJOJQJ\^JaJmH sH .hu~hu~5CJOJQJ\^JaJmH sH hD hD mH sH hD hND:mH sH     .024>J˺ڱڨڨڱڙڨڱڨڀxof^hmmH sH hmH*mH sH hu~H*mH sH hD mH sH hu~mH sH !j?(h v$(((J)):*****D+ $^a$gdU $ & Fa$gdU $h^ha$gdU $ & Fa$gdI$a$gdD $a$gdfh$a$gdu~("($(((((()I)J)))))* *,*-*.*/*1*8*9*:*Q*X*Y*p***********+˷˯{jhUUmH sH hUH*mH sH h1mH sH hUhUH*mH sH hUhUmH sH hUmH sH hUH*mH sH hIhImH sH hImH sH hS pmH sH Uh^kmH sH h^kh^kmH sH hG.mH sH hB4mH sH ,om the flux of previous SEP event. Each event box contents the data of 10 particle fluences (p, He, C, N, O, Ne, Mg, Si, S, Fe). These data are distributed between 3 files. Every file begins with the particles name first or second letters (p, H, C, N, O, Ne, M, Si, S, F) and finishes with one of three indexes a, or f, or p. a-file contents the measured particle fluences (energy interval and fluences are presented as stepwise data, convenient to graphic representation. f-file contents the differential (part/(cm2 MeV/nucl)) and the integral (part/cm2) spectra. p-file contents the parameters of the event particles the differential spectrum. These are: number of the event mean square declination S the differential spectrum Ft from experimental data Fe.  EMBED Equation.3  where n is the number of measurement channels. Spectral coefficient C Spectral index ++++C+D+,000000ǿǽǴǩh1h1mH sH h1H*mH sH UhUmH sH h1mH sH jhUUmH sH !jC?hUh1EHUmH sH %jM h1CJUVaJnHtH D+[+0"00$ & F`a$gd1o Droop index  F(Ee"30 MeV)  integral fluence of event  conventional it is the event size. ,1h. 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