Climatic fluctuations of glaciers of the Little Ice Age (LIA)-rank used to show comparable magnitudes
during the Holocene. That is why the extent of maximal LIA moraines in the Alps attains similar
position as those of the previous LIA-type Holocene advances. Consequently, the LIA moraines represent
a massive and frequently multi-ridge depositional system. Certain differences in reaction to climatic
changes and in moraine development result from the glacier size, percentage of debris-covered ice surfaces,
and topography of alimentary areas. Such differences are particularly spectacular regarding "pure
ice" and debris-covered glaciers. Another system represent rock glaciers which, however, frequently
accompany regular glaciers. Some rock glaciers originated due to one-time transformation of a "glacial"
glacier during its recession, while others formed owing to long-term accumulation of rock debris within
glacial cirques during successive oscillations of small cirque glaciers in the Holocene, given suitable topographic
and topoclimatic conditions. The relationship between the ELA and altitude of cirque bottom
and/or debris supply from surrounding walls is of key importance in this case