Data of the stratospheric balloon launched on 5/21/1998
For HEXIS (High Energy X-ray Imaging Spectrometer)
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Data of the stratospheric balloon launched on 5/21/1998For HEXIS (High Energy X-ray Imaging Spectrometer)
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Details of the balloon and launch operations
Launch site:Fort Sumner Municipal Airport, New Mexico, US Launch team: National Scientific Balloon Facility (NSBF) Balloon: Open balloon (zero pressure) Volume: 4.000.000 cuft Serial number: - Flight identification number: - Campaign: No Data Payload weight: - Gondola weight: - Overall weight: - Normal launch. Normal Flight |
ImagesClick to enlarge.     © Hexis Group |
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Description of the payload or experimentHEXIS (High Energy X-ray Imaging Spectrometer) Responsable institution: University of California-San Diego Principal Investigator: Dr. James L. Matteson The High Energy X-ray Imaging Spectrometer (HEXIS) program is developing position sensitive Cadmium Zinc Telluride (CZT) X-Ray detectors for use in X-ray astronomy and mission concepts for both balloon and satellite based telescopes. In a balloon based version of HEXIS, the scientific objectives are to study hot plasmas, non-thermal and accelerated particles, and nuclear and electromagnetic processes in the hard X-ray regime (20-200keV). These processes occur in astrophysical source regions characterized by compact objects, high magnetic fields, high gravitational potentials and general relativistic phenomena. Such sources are known to occur in X-ray pulsars, black hole candidates, active galactic nuclei (AGN) and regions emitting nucleosynthetic gamma rays. CZT detectors are capable of very fine position resolution, to detect this sources. | ||||||||||||||||||||
Performance in flight and data obtainedAs part of the program development, this was the second balloon flight and the first with a long duration flight at float. The primary goal was to test various active and passive shielding configurations. The same cross strip and planar CZT detectors used on the October flight were flown on this flight. The readout electronics were also the same with the exception of a more distant location of the preamps relative to the CZT detectors, about 50 cm. The shielding, however, was different. This time the pressure vessel was surrounded by an annulus of CsI and had a second CsI crystal under it as a rear active shield. A NaI collimator over the detectors provided a 20° field of view to the two detectors. This flight also had a calibration source of 241Am that could be commanded in or out of the field of view of the two CZT detectors, occurring nine times throughout the flight. This series of balloon flights had significantly improved the understanding of the background properties of CZT, including background rejection techniques based on the physics of CZT detectors. Shielding effects are being extensively studied with this unique data set comprising seven different shielding configurations using the same two detectors and readout systems. These data will contribute great insight into optimal shielding for the next generation hard X-ray instruments. |
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External references and bibliographical sources
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| If you detected mistakes in the information presented here, please tell me (Updated on 17-Aug-2007 - 03:27:11pm) | ||||||||||||||||||||
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