PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT INTERCHANGE_FORMAT = ASCII PUBLICATION_DATE = 2001-09-01 NOTE = "N/A" END_OBJECT = TEXT END RESINFO.TXT Written as part of the NEAR XGRS submission to the Planetary Data System (PDS). The data presented in this directory are specific to the NEAR X-ray Spectrometer Level 3 submission. The following files comprise Figure 2 from Nittler, 2001 MAPS n000504.lbl n000504.tab n000615.lbl n000615.tab n000710.lbl n000710.tab n001227.lbl n001227.tab n010102.lbl n010102.tab Description: Observed and best fit model Soft X-ray spectra (0 to 10 KeV) obtained from NEAR XGRS solar monitor and three asteroid pointing detectors (bare, Mg filter, and Al filter) during five solar flares (a through e) which occurred during the NEAR mision orbital phase. Two theoretical spectra for the solar monitor correspond to best solar two temperature and one temperature above 4 KeV fit to observed spectra. Theoretical spectra for asteroid pointing detectors are best fit using Levenberg-Marquardt least squares minimization. All spectra have had background removed. A typical background during that time was removed from the solar monitor spectrum, and a background removed using the method from the asteroid pointing detectors. The following files comprise Figure 3 from Nittler, 2001 MAPS quietsummer.lbl quietsummer.tab quietwinter.lbl quietwinter.tab Description: Observed and best fit model soft X-ray spectra (0.5 to 3 KeV obtained from NEAR XGRS three asteroid pointing detectors (bare, Mg filter, and Al filter) during solar quiescence in summer (a) and winter (b) halves of the mission, respectively. Lower energy lines (for Mg and Si at 1.25 and 1.75 respectively) are clearly observable during quiescent times. Theoretical spectra for asteroid pointing detectors are best fit using Levenberg-Marquardt least squares minimization. All spectra have had background removed. A typical background during that time was removed from the solar monitor spectrum, and a background removed using the method from the asteroid pointing detectors. The following files comprise Figure 4 from Nittler, 2001 MAPS nfig4.lbl nfig4.tab Description: Theoretical models of continuum plus lines for single average temperature solar corona at 4, 8, and 16 million degrees, from models by Mewe. The following files comprise Figure 6 from Nittler, 2001 MAPS nfig6.lbl nfig6.tab Description: For Mg/Si (a) and Fe/Si (b), photon (X-ray intensity) ratios versus weight ratios for typical meteorite compositions generated using solar output at 4, 8, and 16 million degrees. Tables 1-3 from the Nittler, MAPS 2001 paper are elaborated in XRSMAPS_FLOURESCENCE.TXT in this directory. Table 4 is addendum to XRSMAPS_FLOURESCENCE.TXT.