Radiative Effect of Dust on the Climate of Early Mars
Project, School of Engineering and Applied Sciences, Harvard University, Cambridge, MA, US
- Calculated key radiative parameters for early Mars dust analogs by applying Mie scattering theory, generating look-up tables for radiative transfer models
- Integrated custom Mie scattering outputs into the PCM_LBL 1D radiative-convective model to simulate the climatic impact of dust on early Mars
- Using the theory of reflectance spectroscopy to determine the reflectance spectra of regolith