The NEAR X-ray Spectrometer detectors are three gas proportional counters collimated to 5 degrees field of view to determine X-ray line emissions from the asteroid. Balanced filters on two detectors (Al on one and Mg on the other) are used to separate Mg, Al, and Si lines and the Fe, S, Ti, and Ca lines can be resolved. The detectors have a 25 square cm active aperture area and a 25 micrometer beryllium window with a beryllium liner and window support. The detector energy range is 1 to 10 keV with rise-time discrimination to reduce background contamination. The energy resolution is better than 1 keV FWHM at 5.95 keV.
urn:nasa:pds:context:instrument:xrs.near
1.1
The data sets listed in the table below are PDS3 legacy data sets. Once these data sets have been migrated to PDS4 they will be listed in the section above.
| Data Processing Level | Data set ID | Mission phase | Browse | Download |
| Raw data (level 1b): | ||||
| NEAR-A-XRS-2-EDR-CRUISE2-V1.0 | Cruise 2 | 432 Mb | 87 M | |
| NEAR-A-XRS-2-EDR-EARTH-V1.0 | Earth Flyby | 254 Mb | 33 Mb | |
| NEAR-A-XRS-2-EDR-CRUISE3-V1.0 | Cruise 3 | 400 Mb | 77 Mb | |
| NEAR-A-XRS-2-EDR-CRUISE4-V1.0 | Cruise 4 | 409 Mb | 81 Mb | |
| NEAR-A-XRS-2-EDR-EROS/ORBIT-V1.0 | Eros Orbit | 1.5 Gb | 404 Mb | |
| Calibrated data (levels 2 and 3): | ||||
| NEAR-A-XRS-3-EDR-EROS/ORBIT-V1.0 | Eros Orbit | 2.0 Gb | 596 Mb |
Note that each Level 3 product is simply a subset of one Level 2 product where XRS recorded very high fluorescence during a solar flare. The data are generally from low orbital distances, usually less than 50 km from the surface of Eros.
Days of major fluorescence coverage are:
yyyy-mm-dd (doy)
2000-05-04 (125)
2000-06-02 (154)
2000-06-15 (167)
2000-06-17 (169)
2000-07-19 (201)
2000-12-27 (362)
2000-12-28 (363)
2001-01-02 (002)