User:Dmcandre/sandbox

The Maxwell-Boltzmann distribution corresponding to the solar atmosphere. Particle masses are one proton mass, $m=1{\text{ amu}}=1.67\times 10^{-24}{\text{ g }}$, and the temperature is the effective temperature of the sun's photosphere, $T=5800{\text{ K }}$. ${\tilde {V}},{\bar {V}},{\text{ and }}V_{\text{rms}}$ mark the most probable, mean, and root mean square velocities, respectively. Their values are ${\tilde {V}}\approx 9.79{\text{ km/s, }}$ ${\bar {V}}\approx 11.05{\text{ km/s, }}$ and $V_{\text{rms}}\approx 12.00{\text{ km/s }}$.