This is the first of two guest posts from Tim Cullen on the fascinating subject of photon production in planetary atmospheres:
The concept of a “fluorescing atmosphere” is generally dismissed as cranky [or just plain crazy] by most pundits and commentators.
Therefore, I am extremely grateful to Professor Mark A. Smith and Hiroshi Imanaka for publishing a truly remarkable paper on the Geochemical Society website that clearly illustrates that photons are produced in the atmosphere.
The blue emissions are indicative of atomic hydrogen [but there are other atmospheric atomic gases that emit blue photon – such as helium] and are produced in many ways [including]:
a) Electrons colliding with atomic gas particles.
b) Solar photon colliding with atomic gas particles.
c) Atomic gas particles recombining to form molecules.
Though less is directly known regarding the haze layers, lying predominantly below the direct reach of Cassini, much is now known regarding the atmosphere above the haze.Using the Ion-Neutral Mass Spectrometer (INMS) on Cassini, we now know that even in the ionosphere, there is a rich and complex organic chemistry unparalleled in any known atmosphere (Waite, 2005; Waite, 2009).














