2016
DOI: 10.3986/ac.v29i2.450
|View full text |Cite
|
Sign up to set email alerts
|

Large Collapse Dolines in Puglia (Southern Italy): The Cases of “Dolina Pozzatina” in the Gargano Plateau and of “Puli” in the Murge

Abstract: Prispevek opisuje največjo udornico na planoti Gargano in druge velike udornice (puli) v pokrajini Puglia v južni Italiji. Avtorja predlagata razlago nastanka in razvoja teh vrtač: sovpadanje tektonskih dogodkov, kraških korozijskih procesov ter transgresijskih in regresijskih ciklov.The paper deals with the description of the largest doline of Gargano and of other large dolines (puli) of Puglia in southern Italy aiming to suggest an interpretation of their origin and development, in relationship with tectonic… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
5
0

Year Published

2016
2016
2022
2022

Publication Types

Select...
6
1
1

Relationship

0
8

Authors

Journals

citations
Cited by 8 publications
(5 citation statements)
references
References 0 publications
0
5
0
Order By: Relevance
“…Morphology of the Gargano Promontory is mostly controlled by E-W and NW-SE-trending faults (Funiciello et al, 1991;Gambini and Tozzi, 1996;Brankman and Aydin, 2004). Karst is well-developed over the entire area, as well as in the rest of the region: the main karst features are represented by a multitude of sinkholes, reaching a maximum density of up to 100 per square kilometer in the Chiancate area (Castiglioni and Sauro, 2000;Simone and Fiore, 2014). Due to widespread outcroppings of soluble rocks (Bosellini et al, 1999), surface hydrography is limited to a few, short, ephemeral drainages along slopes that bound the elevated central plateau (reaching 1000 m a.s.l.)…”
Section: Resultsmentioning
confidence: 99%
“…Morphology of the Gargano Promontory is mostly controlled by E-W and NW-SE-trending faults (Funiciello et al, 1991;Gambini and Tozzi, 1996;Brankman and Aydin, 2004). Karst is well-developed over the entire area, as well as in the rest of the region: the main karst features are represented by a multitude of sinkholes, reaching a maximum density of up to 100 per square kilometer in the Chiancate area (Castiglioni and Sauro, 2000;Simone and Fiore, 2014). Due to widespread outcroppings of soluble rocks (Bosellini et al, 1999), surface hydrography is limited to a few, short, ephemeral drainages along slopes that bound the elevated central plateau (reaching 1000 m a.s.l.)…”
Section: Resultsmentioning
confidence: 99%
“…(npr. Mihevc 1998;Castiglioni in Sauro 2000;Sauro 2000;Šebela in Čar 2000;Šušteršič 2000;Stepišnik 2004;Zhu in Waltham 2005;Stepišnik 2008;Gabrovšek in Stepišnik 2011;Hiller idr. 2014;Stepišnik 2014;Kaufmann in Romanov 2016;Stepišnik 2017;Stepišnik in Grlj 2018;Lipar, Stepišnik in Ferk 2019;Stepišnik in Gostinčar 2020).…”
Section: Pregled Ciljev Raziskovanja Vrtačmentioning
confidence: 99%
“…The name derives from the pre-Latin term grava, meaning pit or hole, and is locally used to indicate deep entrance to cave systems [104]. This type of feature, generally produced through collapse or cover-collapse sinkhole processes, is very common in the Apulian karst [74,75,[105][106][107]. At Castellana, given the relevance of the Grave (the most iconic symbol of the Castellana Caves, with the typical picture showing the solar ray entering the sinkhole at middle morning), its location above parts of the tourist path, and the need to evaluate the stability conditions, this site was surveyed by means of the laser scanner RIEGL VZ400 (Figure 1).…”
Section: Castellana Cavesmentioning
confidence: 99%