## Abstract The details of the processes by which heat is transported through the lower atmosphere are, for the most part, still obscure although our knowledge of typical temperature distributions near the ground is now well founded, thanks chiefly to the researches of Johnson (1929), Best (1935),
The ionisation of the atmosphere near the ground in fair weather
β Scribed by J. Law
- Publisher
- John Wiley and Sons
- Year
- 1963
- Tongue
- English
- Weight
- 979 KB
- Volume
- 89
- Category
- Article
- ISSN
- 0035-9009
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β¦ Synopsis
Abstract
In Part 1 observations of the positive and negative small ions in the lowest 2 m of the atmosphere near Cambridge are described, showing that the conductivity decreases with height in this region under most conditions. Simultaneous observations of the spaceβcharge density are incompatible with the theory that the convection current is small compared with the conduction current, and are supported by observations of the vertical electric field. Estimates of the size of the convection current and the vertical distribution of space charge have been made.
Observations at the time of the βsunrise effectβ show that the increase in the field is associated with an increase in the positive spaceβcharge density and the breakdown of the nocturnal inversion, while the conductivity shows no reduction.
In Part 2 the equation relating the concentration of atmospheric small ions to their rate of production and lifetime, the electric field and the atmospheric diffusivity has been solved on a computer. The solutions obtained for various sets of conditions are compared with experimental results. Good agreement is found with observations of the space charge, and moderate agreement with those of the field and the diffusivity, but the theoretical prediction that the nucleus concentration is the most important factor influencing the smallion concentration is not supported by the observations. Some possible reasons for this are discussed.
π SIMILAR VOLUMES
## Abstract There is evidence for quite a sharp transition between the regimes of fully forced and of dominantly free convection in the atmosphere near the ground. The two appear to overlap significantly only over a narrow range of Richardson numbers, which may be less than twofold.
## Abstract The result of Hogg (1939) that the positive and negative conductivities in the air vary with height in the lowest regions of the atmosphere, and the fact of a field strength almost unaltered with height can be reconciled by assuming the rate of ionisation to depend upon the height.