Uplift at thermo-mechanically coupled ocean–continent transforms: Modeled at the Senja Fracture Zone, southwestern Barents Sea

 Estimates of uplift at ocean–continent transform margins vary significantly between models incorporating both thermal conduction and viscous coupling across the transform and models taking only one of these processes into account. More heat is predicted to be conducted and advected into the continental lithosphere in combined models than in conductive models. Nevertheless, tectonic uplift predicted by the combined models is only half that predicted conductive models. This is because viscous coupling implies crustal thinning close to the transform. The form and amplitude of uplift in the combined models agree well with erosion estimates along a seismic transect across the Senja shear margin, in the southwestern Barents Sea. Received: 31 January 1995 / Revision received: 20 July 1995     

Fan-shaped coma,orientation of rotation axis,and surface structure of a cometary nucleus I. Test of a model on four comets

Conspicuous anisotropy in the outgassing from comets, especially from short-period ones, appears to be the factor responsible for a frequent occurrence of a fan-shaped coma, extending in the general direction of the Sun. It is proposed that the pattern of deviations from the sunward direction contains information on the orientation of the spin axis and on the time lag in the sublimation process, which in turn provides insight into the nature of the nuclear surface. A simple model of a spherical rotating nucleus is formulated and a trial-and-error technique devised to determine the axis-orientation constants and a lage angle, a meaasure of the time lag in units of the rotation period. The results of application of this method to periodic comets Encke, Tempel 2, Borrelly, and Schwassmann-Wachmann 3 are presented. It is shown that the sense of rotation determined in this fashion is consistent with the results established for three of the four comets from the transverse component of the nongravitational force affecting their orbital motions. It is found that in general the time lag is strongly time dependent and that lag angles approaching 90° are rather common near perihelion, suggesting a complex surface structure that involves an insulting crust of dust of variable thickness and strength. These results are compared with the observed lightcurves of the four comets and with the calculated distributions of integrated insolation at the nuclear surface as functions of the cometocentric latitude and time. Noticed is a tendency of the comets to turn their spin axes to the Sun near perihelion and to replace, on the outbound leg of orbit, the established fan-orientation pattern by a “late”-tail pattern indicative of old, slowly accelerated particles. It is suggested that the motion of P/Schwassmann-Wachmann 3, which is due for a favorable return in 1979, was affected by a secular deceleration in 1930.     

Radioactive and trace element distribution in basaltic rocks of Lower Silesia

Summary The distribution of radioactive(Th, U, K) and selected trace(Rb, Sr, Ba, Y, Zr, V, Cr, Ni) elements in volcanic rocks from the Opole and Jawor regions of the Lower Silesia has been studied. The behaviour of these elements in the studied rocks indicates that the Lower Silesian volcanic rocks are characterized by less differentiated type than other volcanic rocks of the Bohemian Massif, the Opole rock types probably having a less differentiated character than the Jawor rock types.

---

¶rt;a an¶rt;u a¶rt;uamu(Th, U, K) u m ¶rt;u(Rb, Sr, Ba, Y, Zr, V, Cr, Ni) m auu n¶rt;a am n u u uuu. a n mam n¶rt;num, m aum u uuu n¶rt;mam ¶rt; aamuu n¶rt; u ¶rt;uuau, aum u ana¶rt; uu. au a n¶rt;num, m auu n¶rt; amu n ¶rt;uuau ma ua n¶rt; u amu .

     

Palaeocurrents in Mesopotamian geosyncline

Terrigenous sandstone formations of Mesopotamian geosyncline were investigated in order to reconstruct the palaeocurrents in the basin and to compare ancient and recent drainage systems. Direct and indirect methods were used; direct ones, as investigation of the dipping of cross bedding revealing directly the axis or direction of the currents, and indirect ones, as heavy mineral analyses, revealing the possible source areas.All the formations distributed in the southwestern flank of the geosyncline exhibit the palaeocurrents flowing from the southwest towards the northeast, i. e. towards the axis of the geosyncline. By contrast, all the formations distributed in the opposite flank of the geosyncline, exhibit also opposite current directions, i. e. from the northeast towards the southwest. This ancient current system resembles the recent situation; transversal basin filling from both sides towards the geosynclinal axis. In recent times oblong basin filling, executed by Twin rivers, Euphrates and Tigris, also takes place. They transport the material along the geosynclinal axis towards the remaining marine parts of the Mesopotamian geosyncline, represented by Persian Gulf.

---

Zusammenfassung Terrigene sandige Ablagerungen der mesopotamischen Geosynklinale wurden untersucht, um die Paläoströmungen in den Sedimentationsbecken zu rekonstruieren. Es wurden direkte (Untersuchung der Strömungsschichtung) und indirekte Methoden (Schwermineral- und Geröllanalysen) angewendet.Alle Formationen, welche am südwestlichen Rand der Geosynklinale liegen, zeigen Paläoströmungsrichtungen von Südwesten nach Nordosten. Dagegen zeigen die nordöstlichen Formationen umgekehrte Richtungen von Nordosten nach Südwesten, senkrecht zur Geosynklinalachse. Beide Paläoströmungen sind sehr ähnlich dem heutigen Bild. So können wir auch heute eine Querfüllung des Geosynklinalbeckens beobachten. Außerdem tritt heute auch eine Längsfüllung der Geosynklinale durch Euphrat und Tigris auf. Diese Flüsse transportieren das Material entlang der Geosynklinalachse zur rezenten marinen Restgeosynklinale, die heute den Persischen Golf bildet.

---

Résumé Les formations détritiques du géosynclinal Mésopotamique ont été étudiées en vue d'une réconstruction des paléocourants et d'une comparaison de la situation présente et ancienne. Des méthodes directes (études de la stratification croisée) et indirectes (études de minéraux lourds) ont été employées.Toutes les formations situées au bord sud-ouest du géosynclinal montrent des paléocourants dirigés du sud-ouest au nord-est. Au contraire, les formations du bord nord-est présentent la direction inverse. Les paléocourants ont toujours été dirigés perpendiculairement à l'axe du géosynclinal. Le système des paléocourants anciens ressemble au système contemporain. Le remplissage du bassin a toujours été transversal. Mais aujourd'hui le remplissage longitudinal existe aussi. Ce remplissage est effectué par les fleuves Euphrate et Tigre, qui transportent des matériaux détritiques dans le reste marin du géosynclinal Mésopotamique.

---

, . . — , - - - . , - -, . . . . , .

     

Statistical model of meteor streams. IV. A study of radio streams from the synoptic year

With the use of the most powerful stream-search technique in existence, we have detected 275 streams in the synoptic-year (December 2, 1968–December 14, 1969) sample of 19 698 radio meteors, most of which were not reported before. About 16% of all meteors in the sample belong to these streams. We have confirmed the existence of two-thirds of the 83 streams detected by us previously in the 1961–65 sample of radio meteors. Some of the new streams have most uncommon orbits. A new, rich stream with a revolution period of about 30yr has been discovered. Streams of low inclination are often detected at both nodes. A computer technique, developed for determining the two parameters of the D-distribution of meteor orbits in a stream, has been applied to the 275 streams. A number of known comet-meteor associations have been confirmed, and a few new possible associations established. The previously detected orbital similarity between the minor planet Adonis and a few radio streams (including a major, broad stream) has been reinforced, but we have so far failed to prove the evolutionary relationship more quantitatively. Several possible associations with other Earth-crossing asteroids, with the meteorite P?íbram, and with a few fireballs are suggested. The mean space density in streams is shown to be much below the sporadic density, but the central density may significantly exceed the sporadic density. The derived absolute stream-density values are in an order-of-magnitude agreement with space densities estimated from the cometary production rates of solid material of a comparable particle size. Plots on a height-velocity diagram of both the individual radio meteors and the radio streams fail to exhibit the discrete-level structure known to exist for photographic meteors.     

La sénégalite,Al2 (PO4) (OH)3 · H2O,un nouveau minéral

Senegalite is orthorhombic, mm2, a:b:c:=1.296:1:1.007; $\text{a}{}_0\text{=9.673,}\text{b}{}_0\text{=7.596,}\text{c}{}_0\text{=7.668}\text{A}\text{?}$, Z=4, G_calc=2551; space group Pna2. The strongest lines in the powder pattern are: 5.41(7); 4.089(9); 3.834(10); 3.610(8); 2.990(9); 2.348(8); 2.070(7) 1.929(7); 1.505(7) Å. The chemical analysis: Al₂O₃ ? 46.23; Fe₂O₃ ? 0.28; P₂O₅ ? 31.85 H₂O ? 21.00; sum 99.34, gives a formula Al₂(PO₄)(OH)₃ · H₂O. Colourless optically biaxial positive, n_S: α=1.562, β=1.566, γ=1.587, plane of optical axies (001), Z=a, Y=c; 2V=53°, weak dispersion r > v. Measured density 2.552. The DTA curve shows endothermic reactions at 250, 370 and 440°C corresponding to the dehydration of mineral. Infrared spectrum indicates the presence of OH and H₂O groups. Found in oxidation zone of Kouroudiako iron deposit, Senegal, associated with turquoise, augelite, wavellite and crandallite.     

Traces of structural H2O molecules in baryte

The infrared (IR) spectra of gem-quality baryte crystals from different occurrences are characterized by relatively weak but strongly pleochroic absorption bands at 3,280, 3,220, 3,155, and 3,115 cm⁻¹. These bands are assigned to anti-symmetric and symmetric OH stretching vibrations of two types of H₂O molecules localized on vacant Ba sites. The H–H axis of the H₂O I molecule is slightly tilted from the a-axis direction, its twofold axis being nearly parallel to the b-axis, thus defining the plane of the H₂O molecule practically parallel to (001). The H₂O II molecule has its H–H axis parallel to the b-axis direction, with its plane lying approximately parallel to (101). The values of the total water contents of the baryte crystals, calculated on the basis of IR spectroscopic data, are ranging from about 1.7–3.8 wt.ppm. The possible presence of H₃O⁺ ions is also discussed.     

Ccd Photometry of the Neglected Contact Binaries V344 Lac and V1191 Cyg

New photoelectric and CCD observations of the eclipsing contact binary systems V344 Lac and V1191 Cyg are presented and analyzed. All available times of minimum light were used to study period changes of the systems and determine up-to-date ephemerides. The orbital period of V1191 Cyg is found to be increasing at a very fast rate. The photometric elements were determined using the new light curve, radial-velocity curve and broadening function fitting code ROCHE.