2021 Society of Physics Students Zone 11 Regional Meeting
Location
Virtual Meeting, University of Northern Iowa
Start Date
20-2-2021 10:00 AM
End Date
20-2-2021 11:00 AM
Publication Date
2-20-2021
Publication Type
Open Access Presentation
Description
The responsivity of the proposed Net Flux Radiometer (NFR) for the Ice Giants was examined, using a specialty browser tool. This tool takes simulated spectra of Uranus, along with specific parameters of the NFR, and applies Net Flux calculations in order to produce a net flux profile, a simulated view of what the NFR probe would observe as it plunged into Uranus’s atmosphere. The efforts of this project led to a redesign of the NFR to include an increase in the FOV of the radiation-collection windows from 5° to 10°, as well as the selection of spectral bandwidths for observation in the seven available detector windows.
Department
Department of Physics
Copyright
©2021 Meredith Wieber, Shahid Aslam, Maarten Roos, Patrick Irwin, and Geronimo Villanueva
File Format
application/pdf
Recommended Citation
Wieber, Meredith; Aslam, Shahid; Roos, Maarten; Irwin, Patrick; and Villanueva, Geronimo, "Poster Session: Predicted Net Flux Versus Pressure Profiles During a Probe Descent into Uranus’s Atmosphere" (2021). Society of Physics Students Regional Meeting. 6.
https://scholarworks.uni.edu/sps/2021/all/6
Poster Session: Predicted Net Flux Versus Pressure Profiles During a Probe Descent into Uranus’s Atmosphere
Virtual Meeting, University of Northern Iowa
The responsivity of the proposed Net Flux Radiometer (NFR) for the Ice Giants was examined, using a specialty browser tool. This tool takes simulated spectra of Uranus, along with specific parameters of the NFR, and applies Net Flux calculations in order to produce a net flux profile, a simulated view of what the NFR probe would observe as it plunged into Uranus’s atmosphere. The efforts of this project led to a redesign of the NFR to include an increase in the FOV of the radiation-collection windows from 5° to 10°, as well as the selection of spectral bandwidths for observation in the seven available detector windows.
Comments
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