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  • 2020-2024  (2)
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  • 1
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-07-25
    Description: Development of 2.05 um Fiber Lasers for CO2 DIAL lidar Measuring Martian CO2 and Pressure A new concept of Martian differential absorption lidar (DIAL) operating in the 2050 nm CO2 absorption band for atmospheric CO2 and pressure observations has been proposed recently. Based on the concept, we are awarded to develop 2.05 um fiber lasers by the NASA Planetary Instrument Concepts for the Advancement of Solar System Observations (PICASSO) Program. The laser is designed to be an all-fiber master oscillator and power amplifier (MOPA) system with laser output of ~3 mJ at a repetition frequency of 2 kHz. The primary master oscillator (PMO) is locked to the center of the selected CO2 absorption line (2050.428 nm). The frequency of a second MO (SMO) is locked to that of PMO. This SMO frequency is adjustable and switched between the online (2050.44156 nm) and offline (2050.50812 nm) wavelengths for demonstration. The online wavelength is optimally selected so that the CO2 absorption optical depth (AOD) is ~1.1 at 3 km and the measurement in the low Martian atmosphere has largest signal-to-noise ratio. The online wavelength can also be adjusted to a line slope location where AOD is larger to observe atmospheric pressure at higher altitudes. We will present more detail about this project and instrument development at the conference.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 2
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-07-18
    Description: In order to facilitate human exploration on Mars, a need exists to study weather patterns and atmospheric conditions on Mars. Mars has colder weather than Earth, is known for its dust storms, and has a very thin atmosphere, yet its atmosphere and climate are more like Earth's than any other planet in our solar system. Despite these challenges, NASA scientists believe that Mars is the most promising planet for exploration and habitation. We are developing a new measurement concept that uses differential absorption Lidar system in the 2-μm CO2 absorption band to measure atmospheric CO2 and pressure on Mars. By selecting two or more closely spaced wavelengths, one can eliminate the effects of other gases and surface reflections, allowing us to accurately measure CO2 absorption and determine CO2 levels and air pressure on Mars. Our simulations show that this system will be able to measure air pressure with 1 Pa precision up to 5 km away, even in the presence of moderate dust, and measure CO2 and pressure profiles from the surface up to 13 km with a horizontal resolution of 100 km and a vertical resolution of 100 m (400 m during the day). These measurements will improve weather and climate modeling and prediction on Mars.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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