Hydromagnetic shock waves and their infrared emission in H I regions.
Shock wave structure in H I taking into account magnetic fields and radiative losses to evaluate IR intensities due to various cooling transitions
Engineering topics
Publications and source records attributed to Field, G. B..
Shock wave structure in H I taking into account magnetic fields and radiative losses to evaluate IR intensities due to various cooling transitions
OH molecule production in interstellar shock waves, discussing rapid hydrogen production on grains
Anisotropic soft X ray background flux detection, discussing extragalactic and possible galactic corona components
Molecular hydrogen structure, considering planetary and stellar atmospheres and interstellar space
Stability of dilute gas in mechanical and thermal equilibrium with application to nongravitational condensation phenomena in astronomy, particularly solar corona
Oort model of stars and interstellar cloud formation and destruction mathematically formulated, obtaining time-dependent cloud-mass spectrum equations
Free-free emission by intergalactic hydrogen calculated for steady state and closed evolving models