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		Geomorphology  
    Apuan Alps 
		landforms and deposits 
 
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			Relief landforms 
			
	 
	
	The Apuan Alps 
	are characterized by a physical landscape with Alpine features or perhaps 
	features more similar to those of the Lombard Prealps, if the famous 
	comparison by Antonio Stoppani in “Il bel paese” (The beautiful 
	Country) (1876) is to be recalled. The geologist compared the fields of the 
	Po Plain to the Ligurian Sea because of their being flat at the foot of the 
	mountains. The range’s sharp and therefore “Alpine” morphology is more 
	evident on the coastal side. The inland side has similar characteristics but 
	its profile is slightly more gentle. 
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			As a matter of fact, there is “asymmetry” on the main two sides of 
			the range because of different levels of steepness and the overall 
			direction of the mountain range owing to structural more than 
			morphogenetic reasons. 
	Since the Middle-Late Pliocene onwards, the differences between the two 
	sides of the Apuan Alps have greatly increased as the denudation process, 
	depending on tectonic rather than erosional elements, developed within 
	complex uplift and quiet stages of the Apuan range. The axis of the range 
	was oriented by the deformation geometry which was also responsible for the 
	position of carbonate formations along the main alignment of the range 
	itself. 
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			Therefore, the coastal side was 
			characterized by an early exposure of marble and 
			metadolomites as well as a rapid and intense erosion of the valleys 
			not least because of the occurrence of Paleozoic Phyllites in the 
			west, now denudated and therefore more easily erodible.  
			On the other 
			hand, on the inland side the evolution of the physical landscape was 
			characterized by a long period during which the Tuscan Nappe covered 
			the ‘Metamorphic Complex’. The limbs of the folds with “apenninic” vergence have accompanied the slope toward the Serchio graben 
			more gently.  
			Apuan transverse valleys, with “Adriatic flow”, were 
			antecedent to the late upthrust of the horst of the tectonic rift 
			itself. The particular distribution of plastic and rigid structural 
			elements, on which played mainly the fluvial morphogenetic action, 
			has contributed to the “asymmetry” between the two main sides of the 
			Apuan Alps.  
			On the coastal side, the Apuan Alps create a vertical 
			barrier with narrow and deep valleys, whereas on the inland side 
			slopes descend, more regularly and more similarly to the Northern 
			Apennines’ morphology.  
			Yet, the range never lowers in a uniformed 
			fashion as the slope is regularly interrupted by terrains with low 
			inclination. Moreover, the inclination angle is different but 
			constant on the two main sides. Orographic anomalies are 
			concentrated within certain altitudes (500-650; 750-850; 900-1,050; 
			1,200-1,250; 1,500-1,600 m) and bear the marks of past morphological 
			features.   | 
		
		 
		
			  
		 
		
			
			"Alpine" morphology of the Apuan mountains 
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	Supposedly, they are orographic terraces 
	which were ancient basal levels during phases of tectonic quiet, then 
	re-carved by superficial running water during uplift phases. 
	The heritage of a relatively mature morphology is still visible in some 
	embedded meanders which are scattered along the narrow Apuan thalwegs. In 
	fact, these meanders have superposed on higher and wider valleys, cutting 
	the bedrock, during a phase of relif-rejuvenating.  
	The 
	layout of the hydrographic network in the Apuan Alps has been affected by 
	differences in the structural setting and the morphological “asymmetry” of 
	the main mountain sides. On the coastal side, where slopes are steeper, 
	valleys are radially arranged and join together at lower altitudes. On the 
	inland side, which is less steep, each watercourse keeps its initial 
	direction, perpendicular to the main ridge. Parallel valleys prevail on the 
	eastern side, whereas the western side is characterized by more or less 
	complex systems of converging valleys with dendritic or subdendritic 
	hydrographic networks. Apuan watercourses belong to three different 
	categories, depending on whether they flow into the Ligurian Sea or they are 
	tributaries of the Rivers Serchio or Magra. The western side is 
	characterized by rivers with steep upper courses reaching the sea after 
	crossing the short coastal plain largely originated by their deposits. 
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			Zucchi di Cardeto: 
			cuèstas landscape 
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			The whole coastal 
			surface, amounting to 315 km2, 
			is divided into hydrographic basins of different dimensions, of 
			which that of River Versilia accounts for 1/3 and is twice as large 
			as the surface covered by the Carriona and Frigido watercourses.  
			Most of the inland side of the range, amounting to 545 km2, 
			belongs to the hydrographic basin of the River Serchio as parallel 
			valleys are crossed by its right tributaries.  
			All tributaries have a length comprised between 9 and 14 km. The 
			longest is Serchio di Minucciano, followed in order by Tùrrite Secca, 
			Tùrrite di Gallicano, Èdron and Tùrrite Cava. 
			
	In the northern area of the inland side, totalling almost 220 km2, 
	watercourses, starting from streams Lucido and Bàrdine descending from the 
	Apuan mountains, join River Magra through the stream Aulella. 
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	The presence of 
			highly permeable carbonate rocks across the main ridge contributes 
			to the existence of intermittent watercourses with semi-permanent or 
			temporary regimes, especially in their upper courses. A well-know 
			case is the karst 
	circulation of River Tùrrite Secca, which is characterized by a 4 km-long 
	underflow when flowing along the Mt. Sumbra southern side 
	
			 
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			Karst landforms and deposits 
	 
	Despite heavy rains, the central part of the main range is arid and bare on 
	the surface, as rainwater is immediately absorbed by the carbonate bedrock 
	and released in large, complex hypogean karst Systems. Water flows down into 
	the mountains and, upon reaching the impermeable Paleozoic basement, it 
	emerges from karst springs located between 200 and 500 m of altitude. The 
	phenomenon is evident on the coastal side and it is often the reason for the 
	extension of the hydrogeological basin, larger than their hydrographic 
	basin. Water is captured from the eastern to the western side of the ridge 
	through underground paths in karst aquifers. This creates larger catchment 
	areas for Rivers Frigido, Versilia and Carriona compared to those created on 
	the surface by the watersheds.  
	Despite large areas of carbonate rocks outcrop, the epigean karst forms in 
	the Apuan Alps are not well developed in medium and large scale. In these 
	formations harsh and steep orographic features contributed to other 
	morphogenetic processes, which is why epigean phenomena are mainly 
	represented by small karst landforms. They are particularly common on pure 
	calcareous rocks (Marble and “massiccio” Limestone) characterized by intense 
	fracturation, high infiltration and scarce vegetation cover. 
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			Hell's Valley (Mt. Pania): epigean 
			karst landforms 
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			The most common microforms, the karren, are solution pits, grooves and 
	runnels. Karren fields are widespread at high altitudes, where the snow is 
	more persistent and rocks are more fractured forming a karst landscape with 
	clints and grikes. Dolines and shallow wells are less frequent and amount to 
	180 units in the whole mountain range.  
			They are morphoscultpures of various 
	dimensions, from metres to decametres long, often quite deep and therefore 
	with a bowl or funnel-like shape or even snow dolines.  
			Dolines are usually 
	either isolated or gathered in small groups (Campocecina, Spallone, Pian 
	della Fioba, Passo Sella, Vetricia, etc.) in areas with little inclination 
	and facing north-eastern quadrants.  
			The north-eastern side of Mt.Tambura in 
	Carcaia and, to a lesser extent, the northern side of Mt. Pisanino are 
	characterized by an unusual karst landscape with numerous concave 
	dissolution forms.  | 
	
	
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			Epigean forms have seen a reduced development, whereas hypogean karst 
	phenomena in the Apuan Alps acquire paramount importance and extreme value. 
	The Apuan Alps boast 19 out of the 50 deepest caves and 8 out of the 50 
	longest karst cavities in Italy. The Geopark is also home to 
	Italian all-time records: Abisso Paolo Roversi (Paolo Roversi Abyss), the 
	cave with the largest difference in heights (1358 m) and Antro del Corchia, 
	the longest karst Complex (~ 60 km). 
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			So far speleological research has found more than a thousand karst caves 
	formed by gravitative hypogean circulation, both in vadose and phreatic 
	conditions, from high-altitude infiltration areas to low-altitude emergence 
	areas. The Apuan caves are mainly characterized by wells, sometimes in a 
	sequence, which have developed in the vertical transfer zone of infiltration 
	water. They were originated from small superficial absorption fractures 
	which then expanded and deepened by corrosion until they reached huge 
	differences in heights, sometimes exceeding a kilometre. Caves originated by 
	horizontal water transfer are less frequent but not unusual. They are 
	characterized by sub-horizontal tunnels and labyrinths on gentle slopes 
	originated near the saturated zone during phases of tectonic quiet of the 
	Apuan Alps. There are tipically phreatic morphologies (pressure conduits) or 
	morphologies conducting rainwater (canyons). 
	Karst Complexes with a spatial mix of wells and tunnels as a result of 
	polyphasic evolution are rarer. They derive from the superposition of 
	different generations of caves with horizontal features associated to phases 
	of tectonic inactivity and vertical features which formed after the 
	relief-rejuvenations. The largest cavities of the Apuan Alps belong to this 
	special category and Antro del Corchia is its main example. As a matter of 
	fact, the Apuan Alps still preserve traces of “ancient” karst phenomena, 
	probably dating back to the first phases of denudation/erosion of carbonate 
	rocks of the “Metamorphic Complex”. Witness the numerous “relict” tunnels 
	along the higher ridges of the mountain chain, which are characterized by 
	cavities with large section and reduced linear development. Therefore, they 
	are truncated segments of once larger karst Systems formed by the 
	progressive erosion of mountain sides and the general deepening of the 
	valleys.  | 
		
			 
			
			  
			 
			Wind Cave (Mt. Pania): pendant room 
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			Glacial landforms and deposits 
	 
	In the Apuan Alps, the Quaternary Glaciation left clear and remarkable 
	traces of diffuse erosion and deposit landforms despite the moderate height 
	of mountain peaks and their vicinity to the sea. The mountain range provides 
	an obstacle to Atlantic humid currents and nowadays causes heavy orographic 
	rain. It is likely that during cold phases in the Pleistocene it was 
	responsible for heavy solid precipitation leading to the formation of 
	perpetual snowfields. The glacial phenomenon mainly developed on the inland 
	side of the mountain range, yet recognizable and remarkable traces are also 
	found on the coastal side. Since glaciers were exposed to the north-east and 
	located on a more gentle slope, they could build up more and survive longer, 
	compared to the opposite side which was hampered by the relief-energy and 
	its exposure to southern quadrants. 
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			The Apuan Glaciers during the Wurm Maximum (reconstruction) 
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			Attempts 
			to piece together the glacial extension of the Apuan Alps led to the 
			identification of twelve large valley glaciers on the inland side of 
			the range. The main glacier (Orto di Donna-Val Serenaia-La Mandria) 
			is likely to have extended over more than 12 km2 with a 
			length of 6 km. The side exposed to the sea saw the formation of few 
			perpetual snowfields in the shape of cirque, slope, niche, mountain, 
			valley glaciers. The terminal part of the tongue of the Pizzo 
			d’Uccello glacier reached Solco d’Equi Terme at a lower altitude of 
			475 m a.s.l. Whereas, the ice tongue of Arnetola basin, along Edron 
			valley, is thought to have descended to 550 m a.s.l. The formation 
			of terminal moraines at a low altitude shows the exceptional nature 
			of the glaciation in the Apuan Alps. As a matter of fact, it is 
			different from what happened in the whole Apennines and the western 
			Alps at similar altitudes. 
			
	Apuan 
			glaciers descended to very low altitudes and this was accompanied by 
			the exceptional low level of the snow line. 
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			More recent calculation methods 
	estimate that the ideal line of balance between the accumulation and fusion 
	of snow was to be found at around 1250-1300 m a.s.l., at least on the 
	northern side of the range.  
	The formation of glaciers in the Apuan Alps is unanimously linked to the 
	Würm on the basis of deductive reasoning, even though a Pre-Würm (Riss?) 
	glaciation has been also suggested by the occurrence of cemented glacial 
	deposits covered by more recent melted moraine deposits (Passo del Vestito, 
	Val Terreno, Solco d’Equi). The glacial growth kinematics is unknown, 
	whereas the retreat was quick and not uniform, considering the small number 
	of documented late glacial phases.  
	The Apuan glaciation has preserved the main erosion forms. The glacial 
	cirque is the most widespread morphosculpture in the whole range but it is 
	rarely found in its typical form with semicircular vertical cliffs, a flat 
	bottom and a reverse slope threshold (Grotta Giuncona, Cervaiole and Catino 
	del Sagro are among the best preserved). A number of crests (Mt. Sumbra, 
	Corchia and the south-east side of Mt. Altissimo) are characterized by close 
	or coalescent small cirques perfectly carved on southward-looking carbonate 
	walls. Saddles, which lower Apuan crests, especially along the main 
	watershed, enabled glaciers to cross mountain sides. 
	 
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			Transfluence saddles are more common (Foce Giovo, Focolaccia, Passo 
			Sella, Foce di Mosceta), whereas diffluence saddles are rarer (Foce 
			Pianza, Passo del Vestito).  
			
			The inland side (Pianizza, 
			Fatonero, Orto di Donna) houses typical U-shaped glacial valleys 
			with a parabolic cross-section and overdeepened glacial basins which 
			have often been characterized by peat bogs and wetlands (Mosceta, 
			Fociomboli, Campocatino, Pianellaccio, etc.). Valley steps, perhaps 
			linked to a stop of the glacier retreat are more often found in the 
			furthest northern area of the Apuan Alps (Orto di Donna, Acqua 
			Bianca, Pisanino), whereas “Marmitte dei Giganti” (Giant’s 
			pot-holes) along the ditches Fatonero and Angullaja (southern side 
			of Mt. Fiocca and Mt. Sumbra) are likely to have a fluvioglacial 
			origin. Finally, roches moutonnées are not widespread. The only few 
			examples can be found in Val Serenaia and Arnetola. 
			Depositional landforms predominantly comprise glacial ridges mainly 
			showing terminal moraines and to a lesser extent lateral and stadial 
			moraines. Terminal arches are well recognizable in various inland 
			Apuan valleys (i.e. Canale del Libardo in Gramolazzo), whereas 
			Campocatino depression boasts the best preserved morainic 
			amphitheatre characterized by concentric circles of ridges. Huge 
			glacial erratics are found in the valleys of Rivers Edron and 
			Serchio di Gramolazzo. In particular, marble erratics have been 
			subject to quarrying activity in Vagli di Sopra and Campocatino. 
			As it is well known, nowadays there are no active glaciers in the 
			Apuan Alps. Perpetual snowfields have been preserved at the bottom 
			of high-altitude karst wells (“snow holes”), especially in the group 
			of Pania della Croce, even at a few metres depth. On the surface 
			there are places maintaining their snow cover until the hot season 
			and even late summer. A case in point is the place at the bottom of 
			the northern wall of Mt Pizzo d’Uccello which is indicated with the 
			name “Corners of old snow” on the maps of the Italian Military 
			Geographical Institute (IGMI). 
			
			Vinca: glacial 
			morphology 
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			from right to left: Cresta Botto; Punta Carina, Punta Graziosa, 
			Sicilia, Ferro; Coda del Cavallo 
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