Breakfast and dinner are usually associated with overnight accommodation. Lunches are planned in the nice outcrops in the field and trip organizers will prepare all necessary lunch materials. Weather: Kola Peninsula is situated at the latitude of 68 degrees N behind the polar circle. Besides, Khibina and Lovozero massifs occupy mountainous area up to 1200 m above sea level. Because of these two factors temperature during excursion may vary dramatically from +25 o C near the Apatity town down to +10 o C at the top of the mountains. Weather in the middle of August on White Sea shore is usually mild and cloudy. Rains are quite often. 4
General introduction Kola Peninsula is a key area for understanding of the glaciations evolution, especially at their final stages, of the development of glacioisostatic, eustatic and tectonic events during the Late Glacial and Interglacial time, and the character of interaction between the Ice Sheet and local mountain glaciations in high latitudes conditions. During the field trip we will examine: well preserved push and damp marginal moraines, subglacial interlobate ridge, and their geological structures (western part of the Kola Peninsula); landforms resulted from the glacial activity and displaying long-term glacialerosion features and smaller scale landforms which in great detail record the process of the deglaciation of the area, as the glacial cirques, marginal moraines, end moraines, hummocky moraines, De Geer moraines, lateral meltwater channels, spillways, troughs, delta formations, ice-dammed lake shoreline, tor-formations (Khibiny and Lovosero Mountains); features of the glaciotectonic rising of the Kola Peninsula in the form of the isostatically raised beach ridges (coast of the White sea) and the seismodislocations caused by the neotectonic activity of the Baltic Shield (area of the Imandra Lake); the well known in region interglacial section of marine sediments, which bear the evidences of the glacio-eustatic marine transgression (valley of the Varzuga River). Quaternary stratigraphic records of Kola Region Geological chronicle of the formation of unconsolidated cover on the Kola region begins with the Moscowian (Saalian) glacial horizon. It is overlaid by the Mikulinian (Eemian) Interglacial horizon and the Valdaian (Weichselian) glacial superhorizon. Moscowian (Saalian) glacial horizon (QBIIBms, MIS 6) Moscowian tills and melt-water deposits (gIIms, fIIms, lgIIms, gmIIms) overlie the basement rocks and eluvium and are located in the deepest depressions of the pre-glaciation relief and river valleys. They are found by same researchers in various times (Armand et al., 1969; Yevzerov, Koshechkin, 1980; Semjonova, 1998; Korsakova et al., 2004; and another) on western and central parts of Kola region (on the northeastern slopes of the Pechenga Tundra, in the area of the Kovdor alkaline-ultrabasic massif and Umbozero Lake), on the South and Northeast Kola Peninsula within the Terskii Coast of White Sea (at the lower parts of the Kamenka, Strel'na, Chapoma, Ust-Pyalka, Ponoi rivers, and at the valley of the Iokanga river and at the head part of the Svyatoj Nos Bay). There is an opinion (Armand et al., 1969), that in these cases the formation of the Moscowian (Saalian) Glaciation’ till came to the end in marine basin under the Dryas-like conditions (according to paleontological data). Judging from petrographic composition of the detrital material from the till horizon of the Moscowian (Saalian) Glaciation, ice flows moved towards the north-east in the north-western part of the region, and towards the south-east in the area of Kovdor massif and southern coast of the Kola Peninsula (Geology ..., 1995). Moskowian (Saalian) Glacial Horizon is overlaied by the Mikulinian (Eemian) or the Valdaian (Weichselian) Horizons in the all known sections. 5