Fig. 11.From: Variability of solar/stellar activity and magnetic field and its influence on planetary atmosphere evolutionThermospheric temperature profiles according to Tian (2009) for “super-Earths” with ~6 Earth masses and CO2-type atmospheres within orbits of M-star habitable zones between 100 km and the corresponding exobase levels when their thermospheres exposed to a 80, 200 and 800 times higher EUV flux.Back to article page