Source processes for the alkali metals in the atmosphere of Mercury

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

17

Alkali Metals, Atmospheric Composition, Mercury Atmosphere, Potassium, Solar Flux, Statistical Analysis

Scientific paper

A large (fivefold) increase in Mercury's potassium (K) column abundance on October 14, 1987, has been reported by Sprague et al. (1990), who attributed the enhancement to diffusion through the surface in the Caloris Basin, from depths of order 10 km. The postulated source rate is much larger than any previously estimated diffusion rate, and, if true, certainly affects consideration of the origin of other atmospheric species. However, Killen et al. (1991) have pointed out that the claim is not supported by the published observations of K or sodium as a whole. Sprague et al. (1991) have responded by further hypothesizing the existence of several other sources of gas diffusing out of the regolith, all of which are time variable. In any case, the Sprague et al. data indicate large variations in abundance, and it is important to understand the cause. With this issue in mind, the available abundance estimates for correlation with possible controlling physical parameters has ben examined. A significant correlation between the average zenith K column abundance and indices of solar activity has been found.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Source processes for the alkali metals in the atmosphere of Mercury does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Source processes for the alkali metals in the atmosphere of Mercury, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Source processes for the alkali metals in the atmosphere of Mercury will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1339686

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.