GGR100H1 Study Guide - Final Guide: Thermosphere, Density Of Air, Sustainable Agriculture
Document Summary
Stefan-boltzmann law: q proportionate to t^(4) (t=temperature, q=radiation) K*=k(down) x (1-a) a= outgoing radiation/incoming radiation unit: watts/m^2. P= q + e + change in s (q=runoff, p=precipitation, e=evapotranspiration, s=storage) Rh=actual water vapour in the air/ maximum water vapor possible x100. Soil water balance= evapotranspiration + surplus+ change in soil-moisture storage evapotranspiration=transpiration+evaporation. Radiation= the radiation intensity emitted depends on temperature of the object. Earth"s layers thermopause: outer boundary of earth"s energy system top of atmosphere. Solar constant=1372 wm^2 = incoming sw radiation at top of atmosphere. Global net radiation= higher latitudes, net radiation is negative which means we are losing more energy to space than we gain from the sun. Uneven receipt of solar insolation at earth"s surface (2. 5x more concentrated at equator than poles) Insolation is latitude dependent, due to curve of earth. Further diffused at higher latitudes because the path through the atmostphere is longer-more scattering, absorption, and reflection. Lw energy is eventually radiated back to space, keeping equillibrium.