Showing papers on "Solar constant published in 1972"

Solar radiation and productivity in tropical ecosystems

Abstract: In thermodynamic terms, ecosystems are machines supplied with energy from an external source, usually the sun. When the input of energy to an ecosystem is exactly equal to its total output of energy, the state of equilibrium which exists is a special case of the First Law of Thermodynamics. The Second Law is relevant too. It implies that in every spontaneous process, physical or chemical, the production of 'useful' energy, which could be harnessed in a form such as mechanical work, must be accompanied by a simultaneous 'waste' of heat. No biological system can break or evade this law. The heat produced by a respiring cell is an inescapable component of cellular metabolism, the cost which Nature has to pay for creating biological order out of physical chaos in the environment of plants and animals. Dividing the useful energy of a thermodynamic process by the total energy involved gives a figure for the efficiency of the process, and this procedure has been widely used to analyse the flow of energy in ecosystems. For example, the efficiency with which a stand of plants produces dry matter by photosynthesis can be defined as the ratio of chemical energy stored in the assimilates to radiant energy absorbed by foliage during the period of assimilation. The choice of absorbed energy as a base for calculating efficiency is convenient but arbitrary. To derive an efficiency depending on the environment of a particular site as well as oil the nature of the vegetation, dry matter production can be related to the receipt of solar energy at the top of the earth's atmosphere. This exercise was attempted by Professor William Thomson, later Lord Kelvin, in 1852. 'The author estimates the mechanical value of the solar heat which, were none of it absorbed by the atmosphere, would fall annually on each square foot of land, at 530 000 000 foot pounds; and infers that probably a good deal more, 1/1000 of the solar heat, which actually falls on growing plants, is converted into mechanical effect.' Outside the earth's atmosphere, a surface kept at right angles to the sun's rays receives energy at a mean rate of 1360 W m-2 or 1f36 kJ m-2 s-1, a figure known as the solar constant. As the energy stored by plants is about 17 kJ per gram of dry matter, the solar constant is equivalent to the production of dry matter at a rate of about 1 g m-2 every 12 s, 7 kg m-2 per day, or 2 6 t m-2 year-'. The annual yield of agricultural crops ranges from a maximum of 30-60 t ha-' in field experiments to less than I t ha-' in some forms of subsistence farming. When these rates are expressed as a fraction of the integrated solar constant, the efficiencies of agricultural systems lie between 0-2 and 0 004%, a range including Kelvin's estimate of 0-1%. Conventional estimates of efficiency in terms of the amount of solar radiation incident at the earth's surface provide ecologists and agronomists with a method for comparing plant productivity under different systems of land use and management and in different * Opening paper read at IBP/UNESCO Meeting on Productivity of Tropical Ecosystems, Makerere University, Uganda, September 1970.

Long-Period Global Variations of Incoming Solar Radiation

Abstract: Milankovitch’s results on radiation chronology are recomputed with the following refinements: 1) The variations in the earth’s orbital elements are computed from the solutions of the differential equations for secular inequalities which include the second-order effect caused by the great inequality in the motions of Jupiter and Saturn, and are accurate to the second degree of eccentricity of the earth’s orbit. 2) The incoming solar radiation is computed for every 5° of latitude from pole to pole. 3) The radiation chronology is extended to two million years before and one hundred thousand years after 1950 A.D. 4) The value of the solar constant used is based on the most recent observations.

Evaluating the light from the Sun

Abstract: Recent measurements from high altitude observing platforms have produced evidence that the values regarding the energy from the sun and its spectral distribution need significant revisions. In all ground-based measurements, the dust, haze, and smoke of the atmosphere, the permanent gases and, above all, the highly variable and absorbent water vapor are a source of uncertainty. With the advent of the space age the need for a more reliable set of values of the solar constant and the solar spectrum began to be realized. Measurements for the derivation of the solar constant were conducted with aircraft, balloons, and spacecraft. Values for solar spectral irradiance were also obtained.

Solar constant and the energy distribution in the solar spectrum

Abstract: Available data on the solar energy flux and its spectral components are reviewed and critically analyzed. On the basis of extensive measurement data obtained by various methods, it is shown that the most reliable value of the solar constant is 195 cal/sq cm-sec (or 136 mWt/sq cm). Weighted-mean data on the energy distribution in the solar spectrum from 1400 A to 0.3 mm are presented. Among the topics studied are: the attenuation of radiation in the Earth's atmosphere, instrument probiems in absolute spectrophotometry, the influence of limb darkening of the soiar disk on the energy distribution in the solar spectrum, and the energy distribution in the spectrum of the solar photosphere. (IAA)

Analytical and experimental studies of an all specular thermal control louver system in a solar vacuum environment.

Abstract: Thermal control louvers are used on the ATS-F&G spacecraft to regulate temperature by varying the effective radiating area. Since solar energy on louvers has a detrimental effect on their ability to radiate energy, an analytical and experimental program was developed to evaluate the performance of an all specular louver system as a function of sun angle and blade angle. Solar simulation tests and analyses show a maximum effective absorptance of .25 for the full open condition. The application of white paint to the blades resulted in lowering the blade temperatures by 130 C without significantly affecting the system performance.

Measurements of the energy exchange between earth and space from satellites during the 1960's

Abstract: The net radiation budget of the earth-atmosphere system can be obtained from satellite measurements of the infrared radiant emittance and reflected and scattered solar radiation along with a knowledge of the solar constant. During the 1960's experimental and operational meteorological satellites carrying thermistor bolometer sensors were in orbit for about 60 months. Results from these measurements are given including: a global planetary albedo of 30%, long-term global radiation balance within measurement accuracy (2-3%), the net equator-to-pole radiation gradients that drive our atmospheric and oceanic circulations, as well as selected measurements of radiation budget terms over particular geographical areas.

Environmental simulation from 0.01 to 100 solar constants

Abstract: The design and development of two solar radiation simulators with an intensity variation ranging from 0.01 to greater than 100 solar constants under vacuum conditions are discussed. The characteristics of the simulators are presented in terms of spectral content, beam uniformity, and stability. Preliminary thermal radiative property data obtained at high temperatures are reported. The general operating characteristics of the simulator are automatic starting, control of both positive and negative electrodes, and uninterrupted operation for periods in excess of 24 hours.