After discussion/suggestions on the dev_zephyrus channel, here is a few propositions for Rxuv/Pxuv computation to implement for the escape :
Some of the formulation are valid fro hydrogen envelope (sub-Neptunes) but maybe we could use it for MO atmospheres ?
After discussion/suggestions on the dev_zephyrus channel, here is a few propositions for Rxuv/Pxuv computation to implement for the escape :
Some of the formulation are valid fro hydrogen envelope (sub-Neptunes) but maybe we could use it for MO atmospheres ?