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The Phoenix TECP Relative Humidity Sensor: Revised ResultsThe original calibration function of the RH sensor on the Phoenix mission's Thermal and Electrical Conductivity Sensor (TECP), has been revised to correct the erroneously-published original calibration equation, to demonstrate the value of this unique data set, and to improve characterization of H2O exchange between the martian regolith and atmosphere. TECP returned two data streams, the temperature of the electronics analog board (Tb) and the digital 12-bit output of the RH sensor (DN), both of which are required to uniquely specify the H2O abundance. Because the original flight instrument calibration was performed against a pair of hygrometers that measured frost point (Tf), the revised calibration equation is also cast in terms of frost point. The choice of functional form for the calibration function is minimally constrained. A series of profiles across the calibration data cloud at constant DN and Tb does not reveal any evidence of a complex functional form. Therefore, a series of polynomials in both DN and Tb was investigated, along with several non-linear functions of DN and Tb.
Document ID
20140011327
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Zent, Aaron
(NASA Ames Research Center Moffett Field, CA United States)
Date Acquired
September 3, 2014
Publication Date
July 14, 2014
Subject Category
Astronomy
Report/Patent Number
ARC-E-DAA-TN15703
Report Number: ARC-E-DAA-TN15703
Meeting Information
Meeting: International Conference on Mars
Location: Pasadena, CA
Country: United States
Start Date: July 14, 2014
End Date: July 18, 2014
Sponsors: Lunar and Planetary Inst.
Funding Number(s)
WBS: WBS 203959.02.03.18.88
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Keywords
Phoenix mission
H2O exchange between the martian regolith and atmosphere
calibration data
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