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Sciences and Exploration Directorate

Shahid Aslam

(RESEARCH AST, PLANETARY STUDIES)

Shahid Aslam's Contact Card & Information.
Email: shahid.aslam-1@nasa.gov
Phone: 301.614.6961
Org Code: 693
Address:
NASA/GSFC
Mail Code 693
Greenbelt, MD 20771
Employer:
NASA

Brief Bio


Many years of space instrument hardware development and remote sensing experience with direct contributions to the following NASA flight programs: Pressure Modulated Infra-Red Radiometer (PMIRR) on Mars Observer; Composite Infra-Red Spectrometer (CIRS) on Cassini; Gas and Aerosol Monitoring Sensor-craft (GAMS); Stratospheric Aerosol and Gas Experiment III (SAGE III) and James Web Space Telescope (JWST). Currently is the principal lead for the Compact Ultraviolet to Visible Spectrometer (CUVIS) on the DAVINCI Mission to Venus, to be launched in 2030 timeframe.

For h-index and complete publication list see:

https://scholar.google.com/citations?user=6erZJw0AAAAJ&hl=en

Research Interests


Infra-Red Radiometry and Spectroscopy

Solar System: Remote Sensing

Development of infra-red radiometers and Fourier transform spectrometers for remote sensing of planetary atmospheres.


Net Flux Energy in Planetary Atmospheres

Solar System: Uranus

Development of advanced net flux radiometers for studying the atmospheric (thermal) structure of planetary atmospheres, in particular to, (i) determine the planet’s atmospheric heat balance and (ii) determine the planet’s tropospheric 3-D flow.


Time Resolved Raman and Photoluminescence Spectroscopy

Solar System: Planetary surfaces

Development of instrumentation to carry out in-situ time-resolved Raman and photoluminescence (PL) spectroscopy, of samples collected from planetary regoliths, to discover, if present, the types and distribution of biotic and abiotic organic compounds, measure CHNOPS containing organics and minerals and correlate them to radiolysis processed and textural features. 


Non-Dispersive Infra-Red Gas Analyzer

Solar System: Comets

We are designing and building a Non Dispersive Infra-Red Gas Analyzer (NDIRGA) for the New Fontiers CAESAR project (Pre-Phase A), that uses a measurement scheme based on the Beer-Lambert Law. The NDIRGA is used to measure H2O and CO2 partial pressures between the SCS and GCS and uses two redundant 4-channel (quad) thermopile detectors with 2.7-μm and 6.6-μm H2O absorption band, 4.0-μm reference filter and 4.2 µm CO2 absorption band, each paired with redundant IR sources. Knowledge of the water vapor partial pressure will ensure that we avoid reaching the triple point of water (within the P-T range 3 Torr @ 268 K and 16 mTorr @ 218 K). The measurement uses a collimated pulsed IR light source focused onto the quad thermopile detectors with IR bandpass filters in front of them. The absorbed IR light on the thermopiles generate small thermoelectric voltages that are amplified and digitized by a multi-channel digitizer (MCD) ASIC. The 20 bit digitized signals from the MCD ASIC are communicated to the FPGA board in the MEB for further data processing.

Education


D.Phil., Planetary Physics, University of Oxford, Oxford, UK