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River ice cover influence on sediment transportation at present and under projected hydroclimatic conditions 
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下载免费PDF全文 Maria Kämäri Petteri Alho Noora Veijalainen Juha Aaltonen Mikko Huokuna Eliisa Lotsari 《水文研究》2015,29(22):4738-4755
A large number of rivers are frozen annually, and the river ice cover has an influence on the geomorphological processes. These processes in cohesive sediment rivers are not fully understood. Therefore, this paper demonstrates the impact of river ice cover on sediment transport, i.e. turbidity, suspended sediment loads and erosion potential, compared with a river with ice‐free flow conditions. The present sediment transportation conditions during the annual cycle are analysed, and the implications of climate change on wintertime geomorphological processes are estimated. A one‐dimensional hydrodynamic model has been applied to the Kokemäenjoki River in Southwest Finland. The shear stress forces directed to the river bed are simulated with present and projected hydroclimatic conditions. The results of shear stress simulations indicate that a thermally formed smooth ice cover diminishes river bed erosion, compared with an ice‐free river with similar discharges. Based on long‐term field data, the river ice cover reduces turbidity statistically significantly. Furthermore, suspended sediment concentrations measured in ice‐free and ice‐covered river water reveal a diminishing effect of ice cover on riverine sediment load. The hydrodynamic simulations suggest that the influence of rippled ice cover on shear stress is varying. Climate change is projected to increase the winter discharges by 27–77% on average by 2070–2099. Thus, the increasing winter discharges and possible diminishing ice cover periods both increase the erosion potential of the river bed. Hence, the wintertime sediment load of the river is expected to become larger in the future. Copyright © 2015 John Wiley & Sons, Ltd. 相似文献
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Paer Weihed Pasi Eilu Rune B. Larsen Henrik Stendal Mikko Tontti 《《幕》》2008,31(1):125-132
The Nordic countries, including Greenland, have a long tradition in mining. Documented mining dates back to the 8th century AD. Today this region is the most important metallic mining district of the European Union. Metals are produced from active mines in all countries except Iceland and related industries are thriving in all countries.
Important ore deposit types include： volcanogenic massive sulphide deposits （Cu, Zn, Pb, Au, Ag）, orogenic gold deposits （Au）, layered intrusions （Ni, PGE, Ti±V）, intrusive hosted Cu-Au, apatite-Fe deposits, Cr- and anorthosite hosted Ti deposits. Besides these well- documented deposits, new kinds of deposits are being explored, e.g., iron oxide-copper-gold （IOCG）, shale-hosted Ni-Zn-Cu and different types of uranium deposits. 相似文献
Important ore deposit types include： volcanogenic massive sulphide deposits （Cu, Zn, Pb, Au, Ag）, orogenic gold deposits （Au）, layered intrusions （Ni, PGE, Ti±V）, intrusive hosted Cu-Au, apatite-Fe deposits, Cr- and anorthosite hosted Ti deposits. Besides these well- documented deposits, new kinds of deposits are being explored, e.g., iron oxide-copper-gold （IOCG）, shale-hosted Ni-Zn-Cu and different types of uranium deposits. 相似文献
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Josef ?urech Mikko Kaasalainen David Dunham Josef Hanuš John Talbot Brian D. Warner Adrián Galád 《Icarus》2011,214(2):652-670
Asteroid sizes can be directly measured by observing occultations of stars by asteroids. When there are enough observations across the path of the shadow, the asteroid’s projected silhouette can be reconstructed. Asteroid shape models derived from photometry by the lightcurve inversion method enable us to predict the orientation of an asteroid for the time of occultation. By scaling the shape model to fit the occultation chords, we can determine the asteroid size with a relative accuracy of typically ∼10%. We combine shape and spin state models of 44 asteroids (14 of them are new or updated models) with the available occultation data to derive asteroid effective diameters. In many cases, occultations allow us to reject one of two possible pole solutions that were derived from photometry. We show that by combining results obtained from lightcurve inversion with occultation timings, we can obtain unique physical models of asteroids. 相似文献
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Many sites in Fennoscandia contain pre-Late Weichselian beds of organic matter, located mostly in the flanks of eskers. It is a matter of debate whether these fragmentary beds were deposited in situ, or whether they were deposited elsewhere and then picked up and moved by glacial ice. The till-mantled esker of Harrinkangas includes a shallow depression filled with sand and silt containing, for example, several tightly packed laminar sheets of brown moss (Bryales) remains. It is argued that these thin peat sheets were transported at the base of the ice sheet, or englacially, and were deposited together with the silt and sand on the side of a subglacial meltwater tunnel. Subglacial meltout till subsequently covered the flanks of the esker near the receding ice margin. Information about the depositional and climatic environments was obtained from biostratigraphic analysis of the organic matter. Pollen spectra for the peat represent an open birch forest close to the tundra zone. A thin diamicton beneath the peat contains charred pine wood, recording the former presence of pine forests in western Finland. The unhumified, extremely well-preserved peat evidently originated during the final phase of an ice-free period, most probably the end of the Eemian Interglaciation. It was redeposited in the esker by the last ice sheet. Reconstructions of the Pleistocene chronology and stratigraphy of central Fennoscandia that rely on such redeposited organic matter should be viewed with caution. 相似文献
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Stephen M. Slivan Richard P. Binzel Mikko Kaasalainen Andrew N. Hock Alison J. Klesman Laura J. Eckelman Robert D. Stephens 《Icarus》2009,200(2):514-530
We recorded 101 new rotation lightcurves of five Koronis family members, and then combined the new observations with previous data to determine the objects' sidereal rotation periods, spin vector orientations, and model shape solutions. The observing program was tailored specifically for spin vector analyses by determining single-apparition Lumme–Bowell solar phase coefficients, and by measuring synodic rotation periods precisely enough to unambiguously count the rotations between two consecutive oppositions, which is a prerequisite for identifying the correct sidereal period. The new data make possible first pole and shape determinations for (263) Dresda, (462) Eriphyla, and (1289) Kutaïssi, and they improve the models for (277) Elvira and (534) Nassovia, two objects previously studied by Slivan et al. [Slivan, S.M., Binzel, R.P., Crespo da Silva, L.D., Kaasalainen, M., Lyndaker, M.M., Kr?o, M., 2003. Icarus 162, 285–307]. Our results increase the number of Koronis family spin vectors reported in the literature to fourteen, a sample which now includes the seven largest family members. The spin properties of Eriphyla (rotation period , spin vector obliquity ε=51°) and Kutaïssi (P=3.62 h, ε=165°) are consistent with the markedly nonrandom distribution reported by Slivan [Slivan, S.M., 2002. Nature 419, 49–51], and explained by Vokrouhlický et al. [Vokrouhlický, D., Nesvorný, D., Bottke, W.F., 2003. Nature 425, 147–151] as the result of the effects of thermal “YORP” torques combined with solar and planetary gravitational torques. Dresda (P=16.81 h, ε=16°) is the first prograde Koronis member whose spin obliquity and spin rate significantly differ from the clustered spin properties previously found for other prograde Koronis members; nevertheless, its spin vector is consistent with several of the spin evolution possibilities that were identified in the YORP modeling. 相似文献
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The accretion of magmatic arcs gives rise to elongate, linear orogens and is a key process in forming new continental crust. Many Precambrian continents are, however, presently equidimensional or have large areas without any clear linearity, such as the central part of the Palaeoproterozoic Svecofennian Orogen (1.92–1.77 Ga). One way of forming an equidimensional continental domain is by buckling of a linear orogen about vertical axes of rotation into one or more coupled oroclines. Here, we reinterpret existing data and demonstrate the occurrence of coupled Bothnian oroclines in the Svecofennian Orogen. Palinspastic restoration of the southern and northern Bothnian oroclines brings a 1000‐km‐long segment of the Svecofennian Orogen into an originally linear, NW‐striking geometry that restores the lithological belts, metamorphic zones and structural vergences to a common direction, and which indicates that the orogen consists of a SW‐facing arc, which has been shortened along NE‐verging folds and thrust faults. 相似文献
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The Hernemäki and Sydänmaa granitoid plutons in southern Finland lie within the Svecokarelian metagreywackes, with an approximate age of 1.9 Ga. The Hernemäki porphyritic granite was emplaced and deformed early in the regional D2 deformation, and acquired a rectilinear foliation. The Sydänmaa pluton has a mainly concentric foliation, and its intrusion spanned D2. It was probably emplaced as a ballooning pluton. The magmas of the two plutons were possibly derived from a similar source, but evolved independently. Both plutons show plagioclasebiotite-hornblende fractionation. The Sydänmaa pluton is reversely zoned, with a granodiorite rim and a diorite core.Crystal-residual liquid segregation in a deep magma chamber produced a normal geochemical stratification. This fractionated magma was drained from the top down, and injected into a higher, final chamber. Hence, the granodiorite was emplaced before the diorite. There is a component of normal zonation, which suggests that early hornblende crystals were incorporated in the most fractionated granodiorite.
Zusammenfassung Die Hernemäki- und Sydänmaa-Granite in Südfinnland liegen innerhalb der svecokarelischen Metagrauwacken und haben ein ungefähres Alter von 1,9 Ga. Der porphyrische Hernemäki-Granit intrudierte frühzeitig während der regionalen D, Deformation. Er wurde zur gleichen Zeit deformiert, woraus eine geradlinige Schieferung resultierte. Der Sydänmaa-Granit, dessen Intrusoin die D,-Phase überdauerte, zeigt dagegen eine überwiegend konzentrische Schieferung. Sehr wahrscheinlich stieg er als ballonförmiger Granit auf.Die Magmen der zwei Plutone entstammen eventuell derselben Quelle, entwickelten sich aber unabhängig voneinander. Beide zeigen Plagioklas-Biotit-Hornblende Fraktionierung. Der Sydänmaa-Granit ist umgekehrt zoniert, er hat einen Granodiorit-Rand und einen Diorit-Kern. Residuale Flüssigkeitsdifferenzierung in einer tiefgelegenen Magmenkammer erzeugte eine normale geochemische Abfolge. Dieses fraktionierte Magma floß vom Top des Plutons nach unten ab und wurde in eine höher gelegene Kammer injiziert. Also intrudierte der Granodiorit vor dem Diorit. Es existiert eine Komponente normaler Zonierung, was für eine Aufnahme früh gebildeter Hornblendekristalle in den am stärksten fraktionierten Granodiorit spricht.
Résumé Les plutons granitoïdes de Hernemäki et Sydänmaa (Finlande méridionale) sont inclus dans les métagrauwackes svecocaréliennes, avec un âge approximatif de 1,9 Ga. Lors du début de la déformation régionale D2, le granite prophyrique de Hernemäki s'est mis en place et a été déformé, acquérant ainsi une structure linéaire. Le pluton de Sydänmaa, dont l'intrusion a dépassé la phase D2, possède une schistosité essentiellement concentrique. Il a été probablement mis en place par »ballooning«. Il est possible que les magmas des deux plutons dérivent d'une source similaire, mais ils ont évolué de manière indépendante. Les deux plutons montrent un fractionnement par cristallisation du plagioclase, de la biotite et de la hornblende. Celui de Sydänmaa présente une zonation inverse: bordure granodioritique et coeur dioritique. La séparation des cristaux et du liquide résiduel dans une chambre magmatique profonde a engendré une stratification géochimique normale. La partie supérieure de cet ensemble fractionné a ensuite été injectée dans une chambre définitive plus élevée, suivie des parties plus profondes: de la sorte, la granodiorite s'est mise en place avant la diorite. Il existe une composante de zonation normale, qui laisse supposer que de la hornblende, cristallisée lors des premiers stades, a été incorporée à la fraction granodioritique ultime.
Hernemki Sydnmaa ; 1,9 Ga. Hernemaki , D2, , . Sydnmaa, D2, . . - , , . - . Sydnmaa , , - . . . , , — . , .相似文献
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Josef Ďurech Tommy Grav Robert Jedicke Larry Denneau Mikko Kaasalainen 《Earth, Moon, and Planets》2005,97(3-4):179-187
We present simulations on the asteroid photometric data that will be provided by the Pan-STARRS (Panoramic Survey Telescope and Rapid Response System). The simulations were performed using realistic shape and light-scattering models, random orientation of spin axes, and rotation periods in the range 2–24 h. We show that physical models of asteroids can be reconstructed from this data with some limitations (possible multiple pole solutions). We emphasize the potential of sparse photometric data to produce models of a large number of asteroids within the next decade and we outline further tests with fast and slow rotators, tumblers, and binary asteroids. 相似文献