An Atlas of Past and Present Pollen Maps for Europe: 0-13000 Years Ago, and The Overlay Maps.

[1] Comets, planetary rings, exposed dusty surfaces, and the zodiacal dust cloud are all examples of environments where dusty plasma effects establish the size and spatial distributions of small grains. Simultaneously, dust often influences the composition, density, and temperature of the plasma surrounding it. The dynamics of charged dust particles can be surprisingly complex and fundamentally different from the well-understood limits of gravitationally dominated motions of neutral particles or the adiabatic motion of electrons and ions in electromagnetic fields that dominate gravity. In this review we focus on observations that are best explained by theories concerning dusty plasma effects at Saturn. In addition to presenting our current models we also discuss our expectations for new discoveries based on existing observations at Jupiter or on purely theoretical considerations. Our intent is to give an up-to-date overview of dusty plasma effects in Saturn's magnetosphere and to draw attention to several outstanding problems that could be resolved by the Cassini mission.

Dusty plasma effects in Saturn's magnetosphere

Applied Discriminant Analysis

/pdf/modelling-outburst-floods-from-moraine-dammed-glacial-lakes-1c5qr1h3yb.pdf

Modelling outburst floods from moraine-dammed glacial lakes

https://repositorio.ul.pt/bitstream/10451/36205/1/Oliva%20Marc_2017%283%29.pdf

Recent regional climate cooling on the Antarctic Peninsula and associated impacts on the cryosphere.

This chapter brings a review of current evidences of continental and mountain glaciation in Czechia and provides a closer look at the mid Pleistocene (Elsterian and Saalian) continental glaciation limits and chronology from northern part of the country, as well as late Pleistocene mountain glaciations in the Krkonose and Sumava Mountains.

Pleistocene Glaciations of Czechia

Sedimentary evidence of landscape and climate history since the end of MIS 3 in the Krkonoše Mountains, Czech Republic

Geomorphological evidence and 10Be exposure ages for the Last Glacial Maximum and deglaciation of the Velká and Malá Studená dolina valleys in the High Tatra Mountains, central Europe

The response of active-layer thickness and the ground thermal
regime to climatic conditions on the Ulu Peninsula (James Ross
Island, northeastern Antarctic Peninsula) in 2011 – 13 is
presented. The mean air temperature over this period was –
8.0°C and ground temperature at 5 cm depth varied from – 6.4°C
(2011 – 12) to – 6.7°C (2012 – 13). The active-layer thickness
ranged between 58 cm (January 2012) and 52 cm (February 2013).
Correlation analyses indi- cate that air temperature affects
ground temperature more signi fi cantly on snow-free days (R 2
=0.82) than on snow cover days (R 2 = 0.53). Although the
effect of snow cover on the daily amplitude of ground
temperature was observ- able to 20 cm depth, the overall in fl
uence of snow depth on ground temperature was negligible
(freezing n -factor of 0.95 – 0.97)

Zbyněk Engel

Papers

Pleistocene Glaciations of Czechia

Sedimentary evidence of landscape and climate history since the end of MIS 3 in the Krkonoše Mountains, Czech Republic

Geomorphological evidence and 10Be exposure ages for the Last Glacial Maximum and deglaciation of the Velká and Malá Studená dolina valleys in the High Tatra Mountains, central Europe

Effect of Snow Cover on the Active‐Layer Thermal Regime – A Case Study from James Ross Island, Antarctic Peninsula

Outburst flood hazard: Case studies from the Tien-Shan Mountains, Kyrgyzstan