Atmospheric Infrared Radiation Over the Antarctic

Atmospheric Infrared Radiation Over the Antarctic
Author: Peter M. Kuhn
Publisher:
Total Pages: 0
Release: 1967
Genre: Atmospheric radiation
ISBN:

The total thermal radiative power exchange at the atmosphere-earth interface and within the atmosphere is a direct measure of energy (power) available to drive the "heat engine" that circulates the atmosphere. In view of this, its implication in meteorological analysis is vital for the approach to a full solution of atmospheric circulation. The lack of a sufficient number of surface and upper air thermal radiation soundings prompted the development of the radiometersonde, a low-cost balloon-borne radiometer. This instrument, flown as part of a standard radiosonde ascent, separately measure upward, downward, and net thermal radiation. A summary and analysis of 400 out of 2,000 Antarctic radiometersonde ascents gives 40,000 individual measurements of net, upward, and downward thermal radiation. The average stratospheric net outward radiation for Pole Station in the dark season is 0.145 ly/min, and that for Byrd Station is 0.210 ly/min. The standard deviation about the average for Pole Station is 0.039, and for Byrd Station is 0.005 ly/min

Radiation in a Cloudy Atmosphere

Radiation in a Cloudy Atmosphere
Author: E.M. Feigelson
Publisher: Springer Science & Business Media
Total Pages: 303
Release: 2013-06-29
Genre: Science
ISBN: 9400964439

Radiative heat transfer is a fundamental factor in the energetics of the terrestrial atmosphere: the system consisting of the atmosphere and the underlying layer is heated by the Sun, and this heating is compensated, on the average, by thermal radia tion. Only over a period of 1-3 days from some specified initial moment can the dynamic processes in the atmosphere be considered to be adiabatic. Global dynamic processes of long duration are regulated by the actual influxes of heat, one of the main ones being the radiative influx. Radiation must be taken into account in long-term, weather forecasting and when considering the global circulation of the atmosphere, the theory of climate, etc. Thus it is necessary to know the albedo of the system, the amount of solar radiation transmitted by the atmosphere, the absorptivity of the atmosphere vis-a-vis solar radiation, and also the effective radiation flux, the divergence of which represents the radiative cooling or heating. All these quantities have to be integrated over the wavelength spectrum of the solar or thermal radiation, and they must be ascertained as functions of the determining factors. The relation ships between the indicated radiation characteristics, the optical quantities directly determining them, the optically active compo nents of the atmosphere, and the meteorological fields will be discussed in this book.

Cloud Radiative Effects and Associated Changes in Tropospheric Temperature and Winds at the South Pole During Austral Winter

Cloud Radiative Effects and Associated Changes in Tropospheric Temperature and Winds at the South Pole During Austral Winter
Author: Robert S. Stone
Publisher:
Total Pages: 6
Release: 1992
Genre:
ISBN:

Both the increasing concentrations of greenhouse gases and potential changes in cloud distributions are likely to affect the surface energy budget of the polar regions. Changes in the polar atmosphere are, linked to dynamical processes that control the transport of mass, heat, and moisture from lower latitudes and in turn, feed back into the global circulation. An assimilation of radiation and meteorological data collected at the South Pole during the 1986 austral winter is analyzed to gain a better understanding of the relationships between cloud radiative effects, transport processes and the vertical distribution of temperature and wind. An algorithm is developed to characterize the quasi-permanent surface-based temperature inversion and the warm radiatively active layer above it. Mean winter temperature and wind profiles for clear and overcast conditions are, combined with surface radiation measurements to study the mechanisms that cause periodic weakening of the inversion. Results support previous studies that ascribe this weakening to (1) warm air advection, (2) downward vertical mixing of sensible and latent heat, and (3) longwave cloud radiative heating. The integrity of the inversion depends on the combined effects of all three mechanisms. Parameters representing the intensity of the inversion and the bulk wind shear through the lower troposphere are suggested as appropriate indices for the detection of climate change in the region of the Antarctic Plateau.

Ozone in the Troposphere and Stratosphere

Ozone in the Troposphere and Stratosphere
Author: Robert D. Hudson
Publisher:
Total Pages: 498
Release: 1994
Genre: Atmospheric ozone
ISBN:

Abstract: The papers presented at the 1992 Quadrennial Ozone Symposium held in Charlottesville, Virginia, cover topics in both tropospheric and stratospheric research. These topics include ozone trends and climatology, ground based, aircraft, balloon, rocket and satellite measurements, artic and antarctic research, global and regional modeling, and volcanic effects.