The effect of moist layer location on the stability of trapped gravity waves in an almost saturated atmosphere

Summary The stability characteristics of trapped gravity waves, generated by an isothermal bounded tanh (z) velocity profile in the presence of a saturated finite layer, are studied. The saturated layer is introduced at different levels above the inlection point and the variations of moisture content, layer thickness and distance from the origin are examined. The growthyrates and phase speeds of the unstable modes are obtained by solving numerically the equations of motion in the linear, inviscid, Boussinesq limit, via the technique of Lalas and Einaudi (1976).It is shown that the presence of the saturated layer can significantly affect the stability characteristics of the waves. inereases in moisture, layer thickness and distance of the layer from the inflection point are found to amplify the wave response because the saturated layer behaves as a top boundtry to the shear flow. The presence of such effective boundaries is found to stabilize short wavelengths and destabilize longer wavelengths. Finally, an application of the results to a rainband case produces values of the wave parameters in good agreement with the observed ones.With II Figures     

Water type variation during pumping test —Al Jaww plain southeast of Al-Ain in the United Arab Emirates

The waterquality of ten selected wells was investigated during the pumping test where possible future irrigation projects and land reclamation are concentrated. The investigation of the groundwater modification during the pumping test is combined with a change of water type. A hydrogeochemical model is presented for the water quality modification during pumping tests. This model indicates the presence of calcium-bicarbonate, calcium-sulphate, sodium-sulphate and sodium-chloride water families from top to bottom within the water-bearing formations. The existence of these different families is due to the time of pumping test.     

Geochronology of the Spessart Crystalline Complex,Mid-German Crystalline Rise

Summary New Rb-Sr and K-Ar datings help to clarify the geologic history of the Spessart Crystalline Complex, Mid-German Crystalline Rise. The oldest dates, refined by new measurements, are recorded by whole-rock Rb-Sr analyses of the orthogneisses of the Rotgneiss Complex. These confirm a late Ordovician to Silurian age which is interpreted as the time of intrusion of the granitic precursors.Hornblendes, muscovites. and biotites from different lithostratigraphic units and rock types of the Spessart Crystalline Complex yielded K-Ar dates mainly in the range 324 to 318 Ma, an interval which conforms to the analytical precision. Two hornblendes and one muscovite show slightly older dates up to 328 Ma. On the other hand, there is a tail of younger hornblende dates towards 311 Ma, and two hornblendes gave dates as low as 293 and 274 Ma for no immediately obvious reason.The concordant dates around 324 Ma on the three different minerals may be interpreted as marking the time of a rapid uplift and cooling at about the boundary between Early and Late Carboniferous, presumably soon after culmination of the Variscan deformation and amphibolite facies metamorphism.

---

Geochronologie des Spessart-Kristallins, mitteldeutsche Kristallinschwelle

Zusammenfassung Neue Rb-Sr- und K-Ar-Datierungen liefern einen Beitrag zum Verständnis der geologischen Geschichte des Spessart-Kristallins. Die älteste radiometrische Datierung, die bislang im Spessart-Kristallin zur Verfügung steht, leitet sich aus Rb-Sr-Gesamtgesteinsanalysen von Orthogneisen des Rotgneis-Komplexes ab. Die bereits von früheren Bearbeitern gefundenen spät-ordovizischen bis silurischen Daten wurden durch neuere Messungen bestätigt. Sie werden als Intrusionsalter des granitischen Ausgangsmaterials der Rotgneise interpretiert.Hornblenden, Muscovite und Biotite aus unterschiedlichen lithostratigraphischen Einheiten und Gesteinstypen des Spessartkristallins erbrachten K-Ar-Daten vorwiegend zwischen 324 und 318 Ma, d. h. einen Streubereich, der etwa der analytischen Genauig keit entspricht. Zwei Hornblenden und ein Muscovit ergaben etwas ältere Daten bis 328 Ma. Auf der anderen Seite beobachtet man eine Reihe von jüngereren Hornblendedaten bis 311 Ma, und zwei Hornblenden von nur 293 und 274 Ma, die sich nicht ohne weiteres erklären lassen.Die konkordanten Alterswerte um 320 Ma, die für die drei Mineralarten gewonnen wurden, können als die Zeit einer raschen Hebung und Abkühlung etwa an der Grenze Unter-/Oberkarbon interpretiert werden, die vermutlich bald nach dem Höhepunkt der variscischen Deformation und amphibolit-faziellen Metamorphose erfolgte.

---

---

Dedicated to Borwin Grauert on the occasion of his 60th birthday.

---

With 6 Figures