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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] We develop generalized mathematical expressions for time and space variations of peak electron densities of the ionospheric D, E, F1 and F2 layers as well as corresponding variations in the altitudes of the electron density peaks in each of these layers. On the basis of the Chapman characteristics of the E and F1 layers and other techniques, a generalized expression is developed for the electron density height profile of each of the four ionospheric layers. Consequently a generalized mathematical expression is developed for the entire electron density height profile of the whole ionosphere as a function of time, latitude and longitude. The latter mathematical expression may be used to compute or predict ionospheric parameters associated with ratio and satellite communications. Finally we show that some well documented equations on ionospheric parameters are simplified (or approximated) versions of some of our mathematical expressions. (author). 29 refs
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Dec 1990; 12 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] Directional microwave repeater systems are still in significant use for radio-telephone communications as well as terrestrial TV transmissions. In these systems, the optimally maximum distance D0 between one transmitter and the next repeater-receiver partly depends on meteorological conditions since the refractive index n for microwaves is considerably influenced by these conditions. We show that, under dry atmospheric conditions, certain zonally travelling heat/temperature waves which are normally in the weather/climate system significantly vary n and hence inevitably impose specific conditions on the evaluation of D0. Finally we use some Tanzanian meteorological records to arrive at an expression for D0 that is suitable for regions whose meteorological conditions are comparable to those in Tanzania. (author). 11 refs, 3 figs
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Dec 1990; 10 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] The theory of solar-terrestrial relationships developed earlier by the author is extended to incorporate expressions that represent the non-linear responses of the earth-atmosphere system to incoming solar radiation in a more detailed manner. Application of the extended theory to equatorial locations leads to new and interesting features that are consistent with past observations. It also predicts the existence of new oscillations in the equatorial atmosphere whose causative physical processes are given and explained. Non-equatorial locations are treated along similar lines in Part 2 of the series. (author). 44 refs
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Jul 1988; 14 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] A new theory is developed for explaining the processes that give rise to desertification. This theory is arrived at through analyses of possible influences of Earth's surface albedo modifications upon the general atmospheric circulation patterns with the aid of a recent theory of Sun-Climate/Weather links (Njau, 1985a; 1985b; 1986; 1987a; 1987b). It is shown that surface-albedo modification in a given region will not induce significant changes in the general atmospheric circulation patterns unless the region's size is at least equal to a certain minimum value. Finally, a new desertification indicator is suggested. (author). 27 refs, 3 figs
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Dec 1987; 18 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] We derive from first principles, an equation which expresses global radiation as a function of specific humidity and air temperature at screen height. The practical validity of this equation is tested by using humidity, air temperature and global radiation data from Tanzania. It is shown that global radiation values calculated on the basis of the derived equation agree with measured radiation values to within ± 8% as long as the prevalent (horizontal) winds are either calm or light. It is noted that the equation is equally valid at times of strong horizontal winds provided that the temperature and humidity measuring site is sufficiently shielded from the winds. This implies that meteorological stations that are (for some unavoidable reasons) unable to stock pyranometers can still procure reasonable estimates of local global radiation as long as they can, at least, stock the relatively cheaper barometers and wet- and dry-bulb psychrometers. (author). 12 refs, 1 fig., 4 tabs
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Jun 1988; 16 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] We show, on the basis of meteorological records, that certain spatial and time-dependent cycles exist in the earth-atmosphere system (EAS). These cycles seem to be associated with sunspot cycles and hence have been referred to in the text as ''data-derived solar cycles''. Our analysis establishes three important characteristics of the data-derived solar cycles (DSC's). Firstly the crests and troughs of these data-derived solar cycles are mostly latitudinally aligned and have (zonal) spatial wavelengths greater than about 7 degrees of longitude. Secondly the DSC's have periods mostly lying between 6 years and 12 years. In certain stations, some DSC's coincide quite well with corresponding sunspot cycles. Thirdly the crests and troughs of the DSC's drift eastwards at speeds exceeding about 1.5 longitude degrees per year. Furthermore, these DSC's display peak-to-peak amplitudes of about 2 deg. C along East Africa. On the basis of earlier work and bearing in mind the considerable temperature-dependence of the stratospheric ozone layer, we predict existence of latitudinally aligned enhancement and depletion structures (corresponding to the DSC's) in the stratospheric ozone layer within cloudless midnight-to-predawn sectors. (author). 9 refs, 5 figs
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Nov 1990; 15 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] The viable theories already proposed to explain polar ozone holes generally fall into two main categories, namely, chemical theories and dynamical theories. In both of these categories, polar stratospheric clouds (PSCs) are taken as part of the essential basis. Besides, all the dynamical theories are based upon temperature changes. Since formation of the PSCs is highly temperature-dependent, it has been concluded from recent research (e.g. see Kawahira and Hirooka) that temperature changes are a cause, not a result of ozone depletion in polar regions. On this basis, formulations are developed that represent short-term and long-term temperature variations in the polar regions due to natural processes. These variations, which are confined to a limited area around each pole, include specific oscillations with periods ranging from ∼ 2 years up to ∼ 218,597 years. Polar ozone variations are normally expected to be influenced by these temperature oscillations. It is, therefore, apparent that the generally decreasing trend observed in mean October ozone column at Halley Bay (76 deg. S, 27 deg. W) from 1956 up to 1987 is mostly caused by the decreasing phase of a combination of two natural temperature oscillations, one with a period of ∼ 70-80 years and the other with a period of ∼ 160-180 years. Contributions of other natural temperature oscillations are also mentioned and briefly discussed. (author). 35 refs, 4 figs
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Dec 1990; 14 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] We predict the maximum latitudinal shifts of the Inter-Tropical convergence zone (ITCZ) over land masses due to variations in the surface or near-surface temperature fields. We also predict the mean locations of the ITCZ over oceans during northern hemisphere (NH) and southern hemisphere (SH) summers. All our predictions are shown to agree well with observations. Finally, on the basis of the association between the latitudinal location of the eastern pacific portion of the ITCZ and El Nino-Southern Oscillation (ENSO) events as well as some previous related work (Njau, 1985a; 1985b; 1986; 1987; 1988), we suggest possible physical causes of the ENSO events. (author). 39 refs, 1 fig., 2 tabs
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Aug 1988; 15 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] The basic formulations presented in Part 1 of this series (hereinafter simply referred to as ''Paper 1'') are modified in order to mathematically represent the expected solar-terrestrial influences in non-equatorial regions. Analysis and interpretation of these formulations lead to the establishment of several new periodicities as well as other features associated with the non-equatorial atmosphere. Besides, we show through suitable examples that the physical processes that cause and influence some previously observed climatic and upper atmospheric variations in temperate and polar regions are easily deduced from our formulations. (author). 35 refs
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Jul 1988; 15 p
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Njau, E.C.
International Centre for Theoretical Physics, Trieste (Italy)
International Centre for Theoretical Physics, Trieste (Italy)
AbstractAbstract
[en] A climatic model based upon analytical expressions is presented. This model is capable of making long-range predictions of heat energy variations on regional or global scales. These variations can then be transformed into corresponding variations of some other key climatic parameters since weather and climatic changes are basically driven by differential heating and cooling around the earth. On the basis of the mathematical expressions upon which the model is based, it is shown that the global heat energy structure (and hence the associated climatic system) are characterized by zonally as well as latitudinally propagating fluctuations at frequencies downward of 0.5 day-1. We have calculated the propagation speeds for those particular frequencies that are well documented in the literature. The calculated speeds are in excellent agreement with the measured speeds. (author). 13 refs
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Dec 1990; 8 p
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