Temporal Changes in the Rigidity Spectrum of Forbush Decreases Based on Neutron Monitor Data

The Forbush decrease (Fd) of the Galactic cosmic ray (GCR) intensity and disturbances in the Earth’s magnetic field generally take place simultaneously and are caused by the same phenomenon, namely a coronal mass ejection (CME) or a shock wave created after violent processes in the solar atmosphere. The magnetic cut-off rigidity of the Earth’s magnetic field changes because of the disturbances, leading to additional changes in the GCR intensity observed by neutron monitors and muon telescopes. Therefore, one may expect distortion in the temporal changes in the power-law exponent of the rigidity spectrum calculated from neutron monitor data without correcting for the changes in the cut-off rigidity of the Earth’s magnetic field. We compare temporal changes in the rigidity spectrum of Fds calculated from neutron monitor data corrected and uncorrected for the geomagnetic disturbances. We show some differences in the power-law exponent of the rigidity spectrum of Fds, particularly during large disturbances of the cut-off rigidity of the Earth’s magnetic field. However, the general features of the temporal changes in the rigidity spectrum of Fds remain valid as they were found in our previous study. Namely, at the initial phase of the Fd, the rigidity spectrum is relatively soft and it gradually becomes hard up to the time of the minimum level of the GCR intensity. Then during the recovery phase of the Fd, the rigidity spectrum gradually becomes soft. This confirms that the structural changes of the interplanetary magnetic field turbulence in the range of frequencies of 10^?6?–?10^?5 Hz are generally responsible for the time variations in the rigidity spectrum we found during the Fds.     

Paleoproterozoic molassoid complexes of southwestern Ghana

The lithology, sedimentation conditions, tectonic evolution features, and mineralization of molassoid complexes in southwestern Ghana that fill the Tarkwa and Bui basins located within the Birrimian Paleoproterozoic orogenic belt are described on the basis of an analysis of published and our own data. The formation of these sediments in geodynamic conditions of pull-apart basins is described. The deposits of the Tarkwa group are compared with the Archean Timiskaming group of the Superior Province and similar younger complexes. The Tarkwa group is considered as the Paleoproterozoic equivalent of molasse-like complexes that formed at the last stage of accretion orogens of different ages in pull-apart structures.     

REMOTE SENSING RESEARCH IN GEOGRAPHY AT MOSCOW UNIVERSITY

A paper describing activities of the Laboratory of Remote Sensing Methods at Moscow University presents a chronology of the Laboratory's efforts to improve sensor capabilities for acquiring remote sensing data and to develop more effective image processing techniques. Among the accomplishments cited are early advances in sensor system design and photochemical processing in conjunction with “Salyut” orbital station activities, multispectral imaging experiments in conjunction with high-resolution space photography from the Soyuz-12 (1973) and Soyuz-22 (1976) missions, testing of the first high-resolution Soviet (“Fragment”) scanner imagery (1984), and ongoing work in digital and applied image processing. Translated from: Vestnik Moskovsskogo Universiteta, geografiya, 1987, No. 2, pp. 27-31.     

Variations of Trends in Delta Development under the Effect of External Natural and Anthropogenic Factors: Case Study of the Modern Huang He Mouth

The paper considers the major geographic features of the modern Huang He delta, which ranks among the most rapidly varying in the world. The structure of the hydrographic network and the combination of the natural and anthropogenic geosystems of the delta are characterized. The major external riverine and marine, as well as local anthropogenic factors that have affected the development of the Huang He delta in the recent half century are identified. The regularities of the jump-like development of the Huang He delta in the XIX–early XXI centuries are considered. Special attention is paid to the development of the delta after the artificial redistribution of flow in its boundaries in 1996. Satellite images and methods of their interpretation improved by the authors were used. The trends in Huang He delta development are shown to have changed since the last quarter of the XX century under the effect of an abrupt decrease in river sediment load and the growing impact of marine factors. The active progradation of the delta into the sea slowed down significantly, accompanied by erosion and retreat in many segments of its coastline. Huang He delta was used to establish the conditions of changes in the development trends of other deltas under the effect of changes in the climate and economic activity.     

Independent estimate of the interstellar extinction toward FU Ori

Speckle-interferometric observations of FU Ori are performed with the 6-m telescope of the Special Astrophysical Observatory with 600/40 nm and 800/100 nm (central bandwidth/halfwidth) filters. The companion star FU Ori S that was recently discovered at λ >-1.25µm was recorded in observations with the λ/Δλ==800/100 nm filter. The positional parameters and magnitude difference of the companion in the filter considered are found to be θ = (163.9 ± 1.0)°, ρ = (0.493 ± 0.007)″, Δm = 3.96 ± 0.28. An analysis of the spectral energy distribution of the companion implies that for the extinction A _V toward FU Ori to be greater than about 1.6 ^m , i.e., the minimum value required by the available models of the fuor, the spectral type of the companion star must be no later than K3. The reliability of this conclusion and the possible ways for obtaining more accurate estimates of A _V are discussed.     

Fast Apsidal Rotation and Physical Parameters of V1103 Cas

Astronomy Reports - We present the first high accuracy UBV RI(RI)c light curves of poor investigated eclipsing star V1103 Cas = GSC 3682 736 ( $$P{{ = 6.18}^{d}}$$ , $$V = {{11.16}^{m}}$$ , $$e =...     

Surface Typochemistry of Native Gold

Using the methods of electron spectroscopy of the surface and SEM–EDS, it is shown that native gold of the deposit related to the epithermal Au–Ag ore formation contains oxidized gold with an oxidation degree of Au (I) or higher on the surface. A thin layer (~15 nm) with high concentrations of Ag and S and an underlying SiO₂-bearing layer with a thickness of ~30–60 nm play a protective role providing preservation of Ag and Au sulfides in the surface parts of the Au–Ag grains under the oxidizing conditions. S-rich marginal parts of native gold particles may be represented by solid solutions Ag_2–xAu _x S or (with a lack of S) by agglomerates of Ag _n Au _m S clusters. The formation of surface zoning in the nanoscale on the surface of native Au is abundant in nature and may be applied in prospecting.     

Bryolithochemical studies in the search for and evaluation of gold-silver mineralization based on stream sediments (northeastern Russia)

The first bryolithochemical studies have been carried out within the Dukat ore field (Balygychan-Sugoi trough, northeastern Russia), in its northeast (Dukat Au-Ag deposit, Chaika site) and on its eastern flank (Au-Ag ore occurrence, Piritovyi site). Sampling was made along primary water streams draining Au-Ag ore zones, because the headstreams localized in the permafrost zone are poor in alluvial sediments or lack them, whereas the stream banks and beds are overgrown with aquatic and semiaquatic mosses. We examined samples of moss cushions with loose sediments (fine silt suspension and sand-silt material). The study has shown that moss cushions are an effective natural trap extracting finely dispersed, ultradisperse, and colloid-dispersed particles, including ore ones, from water stream suspension. The contents of major elements indicating Au-Ag mineralization (Au, Ag, Hg, Sb, As, Pb, and Zn) in the bryolithochemical and lithochemical samples were compared. The highest contents of these elements have been revealed in the bryolithochemical samples. Scintillation analysis shows a predominance of finely dispersed Au and Ag particles. The chemical composition of lithoparticles and probable species of elements indicating mineralization were studied by energy-dispersive X-ray microanalysis. It has been concluded that the bryolithochemical stream sediments are an integral part of the lithochemical ones and can also be effectively used to reveal geochemical anomalies and identify the corresponding ores. It is shown that the bryolithochemical sediment streams bear important information about the chemical composition of primary ores, as they have the same major indicator elements (Au, Ag, Hg, Sb, As, Pb, and Zn) and nearly the same mineral composition (finely dispersed gold and silver, electrum, silver sulfosalts, and simple sulfides). The proposed bryolithochemical research is promising not only for northeastern Russia but also for other areas with similar landscapes, primarily areas where lithochemical and bryolithochemical stream sediments form in the northern subarctic and arctic environments.     

Distribution and segregation of trace elements during the growth of ore mineral crystals in hydrothermal systems: geochemical and mineralogical implications

The interfacial crystal layer of poorly soluble mineral grown under hydrothermal conditions is modified chemically into a surficial nonautonomous phase (SNAP) and, in this capacity, takes part in growth process, doing several important functions. This paper considers some of them related to geochemistry and mineralogy. The new interpretation is given to the following phenomena: (1) selection of components during crystal growth in multiphase associations; (2) stability of multiphase parageneses having a common chemical component; (3) dual character of the distribution coefficients due to different properties of the crystal volume and SNAP; (4) formation of nano- and microinclusions of unusual composition different from the basic mineral phase; (5) spatial ordering of nano- and microparticles during their directed aggregation at the growing crystal face; (6) accumulation of valuable components (primarily noble metals), incompatible in most of mineral matrixes, in the surficial layer; and (7) effect of “hidden” metal content, associated with the presence of noble metals in the SNAP or of nano- and microinclusions formed during the SNAP evolution.