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Mass Spectrometer Telescope (MAST)

ResourceID
spase://SMWG/Instrument/SAMPEX/MAST

Description

MAST was an 11 layer array of detectors, each of area >20 cm2, stacked one below the other. The first four of these, M1, M2, M3, and M4, were surface-barrier, one-dimensional, position sensitive detectors, each having 92 coplanar, parallel electrode strips with 0.5 mm pitch. The combination of these four layers enabled determination of the X-Y coordinates at two positions, and hence the exact trajectories of penetrating nuclei. Following these were two more surface-barrier detectors, D1 and D2. Further downstream were lithium-drifted solid state detectors, D3 through D7. The areas and thicknesses of the detectors were as follows: M1--M4:20 cm2, 115 micrometer; D1:20 cm2, 175 micrometer; D2:20 cm2, 500 micrometer; D3 through D7 had area of 30 cm**2, with thicknesses, respectively, of 1.8 mm, 3.0 mm, 6.0 mm (compound stack of 2 3.0 mm detectors), 9.0 mm (compound stack of 3 3.0 mm detectors), and 3.0 mm. The signal from the last-penetrated detector measured the residual energy E', and the upstream detectors provided dE/dx with abundant redundancy. The trajectory system, together with preflight calibrations at the Bevalac particle accelerator, enabled considerably more precision in isotopic mass determination, i.e., 0.2 amu, than would otherwise have been possible for the energy range of 10 MeV/nucleon to several hundred MeV/nucleon, and charge ranges of 3 <= Z <= 28. The on-board DPU enabled down-linking of data from Z > 3 events on a priority basis. For more information, see IEEE Transactions on Geoscience and Remote Sensing, vol 31, May 93, pp 557-564. The instrument functioned normally as of 15 July 1996; the next update will be only when any significant status change occured.

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Details

Version:2.0.0

Instrument

ResourceID
spase://SMWG/Instrument/SAMPEX/MAST
ResourceHeader
ResourceName
Mass Spectrometer Telescope (MAST)
AlternateName
MAST
ReleaseDate
2019-05-05 12:34:56Z
Description

MAST was an 11 layer array of detectors, each of area >20 cm2, stacked one below the other. The first four of these, M1, M2, M3, and M4, were surface-barrier, one-dimensional, position sensitive detectors, each having 92 coplanar, parallel electrode strips with 0.5 mm pitch. The combination of these four layers enabled determination of the X-Y coordinates at two positions, and hence the exact trajectories of penetrating nuclei. Following these were two more surface-barrier detectors, D1 and D2. Further downstream were lithium-drifted solid state detectors, D3 through D7. The areas and thicknesses of the detectors were as follows: M1--M4:20 cm2, 115 micrometer; D1:20 cm2, 175 micrometer; D2:20 cm2, 500 micrometer; D3 through D7 had area of 30 cm**2, with thicknesses, respectively, of 1.8 mm, 3.0 mm, 6.0 mm (compound stack of 2 3.0 mm detectors), 9.0 mm (compound stack of 3 3.0 mm detectors), and 3.0 mm. The signal from the last-penetrated detector measured the residual energy E', and the upstream detectors provided dE/dx with abundant redundancy. The trajectory system, together with preflight calibrations at the Bevalac particle accelerator, enabled considerably more precision in isotopic mass determination, i.e., 0.2 amu, than would otherwise have been possible for the energy range of 10 MeV/nucleon to several hundred MeV/nucleon, and charge ranges of 3 <= Z <= 28. The on-board DPU enabled down-linking of data from Z > 3 events on a priority basis. For more information, see IEEE Transactions on Geoscience and Remote Sensing, vol 31, May 93, pp 557-564. The instrument functioned normally as of 15 July 1996; the next update will be only when any significant status change occured.

Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://SMWG/Person/Glenn.M.Mason
InformationURL
Name
NSSDC's Master Catalog
URL
Description

Information about the Mass Spectrometer Telescope (MAST) experiment on the SAMPEX mission.

InstrumentType
EnergeticParticleInstrument
InvestigationName
Mass Spectrometer Telescope (MAST) on SAMPEX
ObservatoryID