1,721,006 research outputs found
INFLUENCE OF NEOTECTONICS IN THE VENTENA RIVER BASIN, NORTHERN APPENNINES (CENTRAL ITALY)
No full textRelationship between Intensity of erosive processes and orientation of the slope in the Romagna-Marche area (northern Apennine, Italy).
No full textEGU2010-6853-
Drainage basin asymmetry and erosion processes relationship through a new representation of two geomorphic indices in the Conca river (northern Apennines)
No full textPossible karst landforms in two unnamed craters in Tyrrhena Terra, Mars
No full textTyrrhena Terra, an area in the cratered highlands South of the Martian equator, contains two unnamed craters.The mineralogical composition of light-toned deposits (LTDs) within these craters is unknown. We performed morphologic and morphometric analyses of the surfaces of these LTDs through an integrated study of images available through the Reconnaissance Mars OrbiterHigh-Resolution Imaging Science Experiment. Our analysis revealed that the Martian landforms contain dolines of polygenetic origin. These dolines are similar to karst landforms observed indifferent karst terrains on Earth and other regions on Mars.The observed karst landforms might highlight the possible evaporiticorigin of these materials, suggesting a climatic change and the presence of liquid water caused by ice melting during the Amazonian age
Analisi dell’energia del rilievo quale indice geomorfico per lo studio e identificazione dell’attività tettonica sottomarina: studio campione eseguito sul bacino della Sardegna (Mar Tirreno).
No full textIce-related Landfoms in Danielson Crater, Arabia Terra region, Mars
Full text linkThis paper describe the ice-related landforms investigated within Danielson crater, a Martian deep crater which is centered at about 7°W and 8°N, in the region of southwestern Arabia Terra about 775 km south of Becquerel crater. A morphological and morphometric survey of the study area through an integrated analysis of the available Mars images was carried out. The morphological features of the landforms were analyzed through an integrated analysis of Reconnaissance Orbiter (MRO) High Resolution Imaging Science Experiment (HiRISE) and Context Camera (CTX) data. In addition, a DTM of the study area within the Danielson crater was built using two stereo pair HiRISE images. Different landforms interpreted as due to ice-related processes was observed in the study area. The landforms investigated resemble similarly ice-related landforms that can be observed both in the cold region on the Earth, and in other region of Mars. The analysis carried out seem to indicate the presence of landforms attributed to the presence of ground ice and ice-melting processes which can reflect significantly climatic changes and different climatic conditions than those existing now. Moreover, they appear to display young erosional age, suggesting that are quite young, probably of middle-late Amazonian age
- …
