A preliminary evaluation of ERTS-1 images on the volcanic areas of Southern Italy

The test site selected for the investigation covers nearly all the regions of active and quiescent volcanism in southern Italy, i.e. the eastern part of the island of Sicily, the Aeolian Islands and the area of Naples. The three active European volcanoes (Etna, Stromboli and Vesuvius) are included. The investigation is in the frame of a program for the surveillance of active volcanoes by geophysical (including remote sensing thermal methods) and geochemical methods. By the multispectral analysis of ERTS-1 data it is intended to study the spectral behavior of the volcanic materials as well as the major geological lineaments with special reference to those associated with the volcanic region. Secondary objectives are also the determination of the hydrographic network seasonal behavior and the relationship between the vegetation cover and the different type of soils and rocks

Results of Skylab investigation over Italy

The author has identified the following significant results. Multispectral high resolution photography of S190A was successfully applied to the detection of paleoriverbeds in flat lands. Results of SL-3 mission were compared to those of LANDSAT for two regional geological surveys (linear structures) on the islands of Sicily and Sardinia. On Sicily, the seasonal conditions were unfavorable for Skylab while LANDSAT played a major role in discovering long, unknown lineaments of great interest for the geodynamics of the area. On Sardinia, owing to the vegetation type and to the geomorphic conditions, the Skylab imagery was successfully employed to describe the network of linears, both regional and local. Results can be used to study the relationship between linears, actual fracturing and the occurrence of mineral deposits

Contribution of Skylab multispectral imagery to the remote sensing studies of Mount Etna volcano

There are no author-identified significant results in this report

Reply to discussion on the article “Remarks on the Permian- Triassic transition in Central and Eastern Lombardy (Southern Alps, Italy)” by G. Cassinis, M. Durand and A. Ronchi

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Heat Capacity Mapping Mission (HCMM) program: Study of geological structure of Sicily and other Italian areas

The usefulness of thermal inertia mapping in discriminating geolithological units was investigated using Sardinia and the Gulf of Orosei as test sites. Software designed for LANDSAT data were modified and improved for HCMM tapes. A first attempt was made to compare the geological cross section, the topography, the IR radiance, and the thermal inertia along selected profiles of the test site. Thermal inertia profiles appear smoothed in comparison with the thermal radiance. The lowest apparent thermal inertia (ATI) was found on granitic and basaltic outcrops where their image is of sufficient extent, while ATI is higher on carbonatic and dolomitic or moist deposits. Almost every fault is marked by a jump of ATI, the interval being sometimes of the order of one pixel. This seems to demonstrate the ability of ATI to detect contacts or tectonically disturbed zones with a good resolution. It seems more difficult to measure the differences in ATI between homogeneous materials having different lithology. Ground surveys conducted and a simulation model of diurnal temperatures of rocks having different thermal inertia are discussed

Remarks on the Permian-Triassic transition in Central and Eastern Lombardy (Southern Alps, Italy)

The main lithological and petrographical characteristics of the Permian-Lower Triassic Orobic and Brescian successions in central and eastern Lombardy are briefl y recorded, especially with regard to the units cropping out below and above the P-T boundary. The lower formation is represented by the Verrucano Lombardo, which consists of continental, fluvial red clastics, barren of fossils, generally Late Permian (Lopingian) in age, whereas the overlying Servino Formation, which is represented by well-bedded clastic and carbonate polychrome sediments, generally rich in fossils, pertains to the Early Triassic (Induan-Olenekian). The sequences of the two above-mentioned areas differ at least in part, as proof of their regional division, probably because of an inherited paleotopography and syntectonic activity. Taking into account the units bracketing the P-T boundary, which represents the real topic of this work, the Verrucano Lombardo of the Orobic Alps is paraconformably covered by the conglomerates and sandstones of the Prato Solaro Member in the lower part of the Servino Formation, cropping out extensively, although discontinuously, from the eastern side of Lake Como to the upper Scalve Valley in the Camonica region. The shape of some quartz rock fragments, derived from the Variscan crystalline basement and its Upper Carboniferous siliciclastic cover, has been interpreted as due to relatively coeval aeolian activity, and testifi es to an arid climatic “event” probably late Dienerian-early Smithian in age. In contrast, in the Brescia province, the onset of the Servino is made up of wave and current rippled, fi ne clastics, 1-2 m thick, and a typical horizon of oolitic dolostones (“Praso Limestone” Auct.), continuous from the lower Camonica Valley to the western Trentino. This unit could laterally correlate towards east, in the eastern South-Alpine segment, with the famous oolitic Tesero Member at the base of the Werfen Formation of the Dolomitic and Carnic Alps. In the Brescian Prealps, the above oolitic deposits crop out below some Claraia beds yielding forms common to those present in the Siusi Member of the Dolomites, generally attributed to late Griesbachian-early Dienerian times. Their age could be ascribed to a slightly older Griesbachian, i.e. to early Induan. Therefore, the P-T boundary in central and eastern Lombardy seems substantially located between the fi nal part of the Permian and the very base of the respective Triassic successions, temporally and spatially ranging in different ways and generally affected by non-depositional and perhaps tectonic processes. In our opinion, however, the duration of the gap, based on correlations with the well-documented stratigraphical studies recently carried out in the nearby Dolomitic area and other European regions, should be considered as slightly longer than previously recognized: the maximum gap could be estimated at about 3-4 Ma. As a consequence, we thus point out that the Servino Formation of the Brescian Alps rests, itself, paraconformably on the Verrucano Lombardo red beds, even if the P-T gap was probably less for correlation with the well-known Dolomites sections. At the end of the paper, for a more comprehensible understanding of the late- to post-Variscan geological scenario, is a tentative synthesis of the regional evolution.Se resumen las principales características litológicas y petrológicas de las sucesiones Oróbica y Bresciana del Pérmico y Triásico Inferior del este de Lombardía, especialmente las referidas a aquellas unidades que afl oran por encima y por debajo del límite P-T. La formación inferior está representada por el “Verrucano Lombardo”, que está constituido de sedimentos continentales clásticos de color rojo, de origen fluvial y sin fósiles y que muestran generalmente una edad Pérmico Superior (Lopingiense), mientras que la unidad inmediatamente superior, Formación Servino, representada por sedimentos bien estratifi cados, clásticos y carbonáticos, con abundantes fósiles y diferentes colores, es de edad Triásico Inferior (Induense-Olenekian). Las sucesiones de las dos áreas arriba mencionadas difieren entre sí, debido, entre otros motivos, a aquellos ligados a las características paleogeográfi cas y tectónicas propias de las zonas en las que afloran. El Verrucano Lombardo, en los afloramientos de los Alpes Oróbicos, que aflora extensivamente aunque de forma discontinua desde la parte este del lago Como hasta la parte alta del valle Scalve, en la región Carmónica, se sitúa, mediante una paraconformidad, bajo los conglomerados y areniscas del Miembro Prato Solaro, pertenecientes a la parte inferior de la Formación Servino. La forma de algunos fragmentos de roca, derivados del basamento cristalino varisco, así como los sedimentos siliciclásticos del Carbonífero Superior que los cubren, han sido relacionadas con una actividad de tipo eólica, testificando un evento climático de tipo árido, probablemente de edad Dieneriense superior-Smithiense inferior. En contraste, en la provincia de Brescia, la Formación Servino está constituida por sedimentos clásticos con ripples de oscilación y corriente, de tamaño de grano fino, constituyendo un espesor de 1-2 m y un nivel típico de dolomías oolíticas (“Praso Limestone” Auct.), que aparece desde la parte inferior del valle de Camonica hasta el oeste Trentino. Hacia el oeste, en el segmento este de los Alpes Meridionales, esta unidad podría correlacionarse lateralmente con el Miembro Tesero, de carácter oolítico, de la base de la Formación Werfen de los Alpes Dolomíticos y Cárnicos. En los Prealpes Brescianos, los depósitos oolíticos anteriormente mencionados afloran por debajo de algunas capas con Claraia, mostrando formas parecidas a las existentes del actual Miembro Siusi de los Dolomitas, generalmente atribuidos a una edad Griesbachiense-Dineriense inferior. Su edad podría ser ligeramente anterior a Griesbachiense, i.e. Induense inferior. Así, el límite P-T en el centro y este de Lombardía, estaría básicamente estar localizado entre la parte final de los sedimentos considerados pérmicos y aquellos de la parte más baja de los considerados Triásico Inferior, aunque con ciertas variaciones temporales y espaciales, variando en función de los procesos no deposicionales y, posiblemente, tectónicos. En nuestra opinión y, basándonos en correlaciones bien documentadas estudios estratigráficos llevados a cabo en los Dolomitas y en otras regiones europeas, prolongación en el tiempo de esta etapa en la que falta registro sedimentario podría ser considerada como ligeramente más larga de lo inicialmente reconocido: esta etapa podría ser considerada en torno a 3-4 Ma. Como consecuencia, consideramos que la Formación Servino de los Alpes Brescianos, como tal, paraconformable sobre las capas rojas del Verrucano Lombardo incluso aunque el vacío sedimentario de la transición P-T en esta zona fuese menor que el de la zona correlacionable y bien conocida de las secciones de los Dolomitas

Study of geological structure of Sicily and other Italian areas

There are no author-identified significant results in this report

Skylab multispectral photography of Italian volcanology, geology, rice fields, and Paleo river beds

There are no author-identified significant results in this report