Some useful solar physics info


+ Electron rest mass: 0.5 MeV

+ Proton rest mass: 1000 MeV

+ 1 eV = 1.6022e-12 erg = 1.160e+4 K

+ Heating requirement: 10e-6 ergs $cm^{-3}$ $s^{-1}$

+ Coronal heating requirement flux: 10e+3 – 10e+8 ergs $sec^{-1}$ $cm^{-2}$ (Uniform loop)

+ Brehumstrallung power P(W/m$^2$) = Z$_i^2$ n$_e$ n$_i$ T$_e^{0.5}$ [eV] / [7.69e18 $m^2$]

+ Assuming Brehumstrallung 1 eV = 10e4 K = 10e3 ergs cm$^{-2}$ $sec^{-1}$ (Flux)

+ Solar Wind mass flux: 2e(-11-- -10) g cm$^{-2}$ s$^{-1}$

Solar Orientation

Solar Coordinates keywords

W.T. Thompson paper

Solar Radio Bursts

GX Simulator

https://hesperia.gsfc.nasa.gov/ssw/packages/gx_simulator/util/Step-by-step%20instructions%20for%20creating%20GX%20Simulator%20models.html