Session
2022 poster session
Location
Space Dynamics Laboratory, Auditorium Rooms D & E
Start Date
5-9-2022 9:55 AM
End Date
5-9-2022 10:45 AM
Description
Using three inputs, metallicity, effective temperature, and surface gravity, we can model a BD to simulate traits like pressure, temperature, density, spectra, etc.
By comparing the modeled spectra with observed spectra, we can make changes to our models to make them more accurate.
Modeling Brown Dwarf Atmospheres in Preparation for JWST Observations
Space Dynamics Laboratory, Auditorium Rooms D & E
Using three inputs, metallicity, effective temperature, and surface gravity, we can model a BD to simulate traits like pressure, temperature, density, spectra, etc.
By comparing the modeled spectra with observed spectra, we can make changes to our models to make them more accurate.