The terrestrial potassium layer (75-110 km) between 71 degrees S and 54 degrees N: Observations and modeling

Observations of the nighttime atmospheric potassium layer were performed on the German research vessel Polarstern from March to June 1996. K density p rofiles were obtained between 71 degrees S and 45 degrees N. The nightly me an peak densities ranged from 140 cm(-3) in the equatorial region to 10 cm( -3) in the Antarctic, and the column abundances decreased from 1.2 x 10(8) to 1.3 x 10(7) cm(-2) going from low to high latitudes. High peak densities and column abundances were also commonly observed together with sporadic K layers. The global mean peak height of the normal (background) K layer was found to be 88.3 km. After the Polarstern campaign, observations were cont inued at Kuhlungsborn (54 degrees N). The summer and winter K layers, obser ved during July 1996 and January 1997, were quite different in shape but ha d similar peak densities and column abundances. A one-dimensional model of the K layer was developed which includes meteoric deposition, vertical tran sport through eddy diffusion, and a full chemical scheme. This model was ab le to reproduce very satisfactorily the seasonal behavior of the K layer at 54 degrees N if the wintertime deposition flux of the metal was reduced by 30% compared to the summer. The midlatitude ratio of K to Na was about 1%, much less than either the chondritic or cosmic ratios of the two metals (a pproximate to 8 or 6%, respectively). The most likely reason is that potass ium vaporizes less efficiently from meteoroids than sodium, in agreement wi th a thermodynamic model of a nonideal chondritic magma and observations in the exosphere of Mercury. Finally, the model was generally very successful in reproducing the latitudinal variations in the K layer.