Formation of hazes at microbar pressures has been explored by theoretical models of exoplanet atmo- spheres to explain Rayleigh scattering and/or featureless transmission spectra, however observationa
Aerosol transmission spectra for a variety of proposed cloud and haze species computed assuming monodisperse 0.1 micron particles distributed with a constant mass mixing ratio profile in the atmospher
Aerosol transmission spectra for a variety of proposed cloud and haze species computed assuming monodisperse 0.1 micron particles distributed with a constant mass mixing ratio profile in the atmospher
Aerosol transmission spectra for a variety of proposed cloud and haze species computed assuming monodisperse 0.1 micron particles distributed with a constant mass mixing ratio profile in the atmospher