Pioneer Venus Sounder Probe Neutral Gas Mass Spectrometer
| Autor: | K. D. Duerksen, J. H. Hoffman, L. D. Brooks, W. W. Wright, R. R. Hodges, V. A. Blevins |
|---|---|
| Rok vydání: | 1980 |
| Předmět: |
Atmospheric pressure
biology business.industry Venus biology.organism_classification Mass spectrometry Ion source Atmosphere Atmosphere of Venus Optics Atmosphere of Earth Mass spectrum General Earth and Planetary Sciences Environmental science Electrical and Electronic Engineering business Remote sensing |
| Zdroj: | IEEE Transactions on Geoscience and Remote Sensing. :80-84 |
| ISSN: | 0196-2892 |
| DOI: | 10.1109/tgrs.1980.350286 |
| Popis: | A neutral gas mass spectrometer was flown to Venus as part of the Pioneer Venus Multiprobe to measure the composition of its lower atmosphere. Encounter occurred on December 9, 1978. The instrument, mounted in the Sounder Probe, was activated after the probe entered the top of the atmosphere, and it obtained data during the descent from 62 km to the surface. Atmospheric gases were sampled through a pair of microleaks, the effluent from which was pumped by a combination of ion and getter pumping. A pneumatically operated valve, controlled by the ambient atmospheric pressure, maintained the ion source pressure at a nearly constant value during descent while the atmospheric pressure varied by 3 orders of magnitude. This action preserved the more than 6-decade dynamic range of the instrument throughout the descent. A single focusing magnetic sector field mass spectrometer with mass resolution sufficient to reasonably separate argon from C3H4 at 40 amu provided the mass analysis and relative abundance measurements. A microprocessor controlled the operation of the mass spectrometer through a highly efficient peak-top stepping routine and data compression algorithm that effected a scan of the mass spectrum from 1 to 208 amu in 64 s while requiring an information rate of only 40 b/s to return the data to earth. A subscale height altitude resolution was thus obtained. Weight, size, and power requirements were minimized to be consistent with interplanetary flight constraints. |
| Databáze: | OpenAIRE |
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