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Field guide - IUGS

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Fig. 2.8. Lateral meltwater channels crossing the southern part of moraine ridge on N-W<br />

Lovozero Mountains.<br />

Excursion 2: Late Glacial ice-marginal formations in Lovozero area<br />

Degradation of the Late Valdai ice sheet in the Kola region occurred in conditions of arctic<br />

climate with alternating phases of stadial falls of temperature and interstadial warming.<br />

External heat was not enough for the active ice margin to retreat (Yevzerov, 1996). In these<br />

environments, three belts of marginal ridges formed in the region (Fig. 2.9).<br />

The degradation stages of the ice sheet in the Kola region have been correlated to climatic<br />

cycles - Oldest, Older and Younger Dryas, and to the previous interstadial warmings. Note,<br />

each marginal belt was formed during the interstadial-stadial cycle of the glacier activity and<br />

was made up of two bands of marginal ridges: the inner band - dump moraine (marginal<br />

esker), and the outer band - a push moraine. The formation of three outer bands of marginal<br />

ridges corresponds to the three final stages (Oldest, Older and Younger Dryas) of the glacier<br />

activity in the Kola region: Terskaya (13,5 ka), Revdozerskaya (12,5 ka), Kandalakshskaya<br />

(10 - 11 ka).<br />

The inner band - dump moraine formed under interstadial conditions and the outer band -<br />

push moraine formed during followed stadial cooling. The all the belts of marginal ridges are<br />

named after stadial cooling - Terskii, Revdozerskii, Kandalakshskii. Most investigated of<br />

them are the recessive formations related to the Revdozerskaya stage of Scandinavian icesheet<br />

development. In one case (Ekman, Iljin, 1991), the marginal ridges north of Lovozero<br />

Mountains are related to the Younger Dryas (Salpausselka) stage, and south of Lovozero<br />

Mountains - to the Older Dryas (Neva stage). In next case (Yevzerov, 1996), the all the<br />

marginal ridge complexes consist of two bands of the marginal formations and are correlated<br />

to the Older Dryas (Neva) stage.<br />

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