At present we lose perhaps a kilogram of oxygen and 10 kilograms of nitrogen per year to outer space due to the Sun's radiation (includes average CMEs = coronal mass ejection, solar wind, neutrinos etc) If the radiation doubles we will lose about 2 kilograms of oxygen and about 20 kilograms of nitrogen per year due to solar radiation = still negligible, but only the poles of Earth and very high elevations will cool enough for humans to go outside at noon. A doubling of the solar radiation is likely to be billions of years in our future. Hydrogen, helium, and water vapor will, however, be lost at several times the rate of solar radiation increase, as they are likely non linear. Neil