Tablas de logaritmos para los números y los senos : con las explicaciones y principales usos para la Astronomía, la Gnomónica, la Geometría, la Navegacion, la Geografía, la Fisica, Arte Militar, Arquitectura, Agrimensura, Estadística y Rentas /

Mode of access: Internet.

Omaggi alle Maestà di Carlo Lodovico Re d'Etrubia e Maria Luisa Infanta di Spagna Regina Reggente per l'appertura del Regio Licèo eretto nel Museo Reale di Fisica e di Storia Naturale di Firenze : con motupropio del di 20 febraio 1807.

Mode of access: Internet.

[¿Cuál es la educacion fisica y moral de la mujer, mas conforme á los grandes destinos la ha confiado la providencia?] : Discurso leido en la Universidad Central por el Licenciado don Juan Perez y Garcia, del Cuerpo de Sanidad de la Armada, en el ejercicio del grado de doctor en Medicina, y en el acto de recibir la investidura del mismo el dia 24 de octubre de 1859.

Tesis Universidad Central, 1859.

Giornale di fisica, chimica, storia naturale, medicina ed arti ...

Title varies slightly.

Historia fisica y politica de Chile segun documentos adquiridos en esta republica durante doce años de residencia en ella y publicada bajo los auspicios del supremo gobierno.

Title following prologue: Flora Chilena.

Dizionario etimologico-scientifico delle voci italiane di greca origine usate in letteratura, metafisica, fisica ...

Mode of access: Internet.

Prodromo della corografia e della topografia fisica della Toscana,

Mode of access: Internet.

Elementi di fisica,

"Il Melzi ... dice che l' analisi dei Problemi di Diofanto è del Crivelli, e la traduzione è del p. Jacopo Paitoni."--Riccardi, Bibl. math. ital.

Ensayo sobre la perfeccion del hombre en la estension de su ser; ó sea, La armonia de la naturaleza y la civilizacion en la formacion fisica, moral é intelectual del mismo desde su individual origen hasta la juventud.

Mode of access: Internet.

Conferencias sobre fisica matematica por Jose Echegaray.

Mode of access: Internet.

Jeografia fisica i politica del estado de Bolivar,

Mode of access: Internet.

Estudio de los instrumentos y aparatos de fisica de aplicacion a la farmacia. Curso de fisica practica

Mode of access: Internet.

Stratigrafia fisica ed analisi di facies dei depositi torbiditici della Formazione delle Arenarie del Monte Cervarola tra la Val Secchia e la Val Scoltenna (Aquitaniano-Burdigaliano, Appennino Settentrionale)

The Cervarola Sandstones Formation (CSF), Aquitanian-Burdigalian in age, was deposited in an elongate, NW-stretched foredeep basin formed in front of the growing Northern Apennines orogenic wedge. The stratigraphic succession of the CSF, in the same way of other Apennine foredeep deposits, records the progressive closure of the basin due to the propagation of thrust fronts toward north-east, i.e. toward the outer and shallower foreland ramp. This process produce a complex foredeep characterized by synsedimentary structural highs and depocenters that can strongly influence the lateral and vertical turbidite facies distribution. Of consequence the main aim of this work is to describe and discuss this influence on the basis of a new high-resolution stratigraphic framework performed by measuring ten stratigraphic logs, for a total thickness of about 2000m, between the Secchia and Scoltenna Valleys (30km apart). In particular, the relationship between the turbidite sedimentation and the ongoing tectonic activity during the foredeep evolution has been describe through various stratigraphic cross sections oriented parallel and perpendicular to the main tectonic structures. On the basis of the high resolution physical stratigraphy of the studied succession, we propose a facies tract and an evolutionary model for the Cervarola Sandstones in the studied area. Thanks to these results and the analogies with others foredeep deposits of the northern Apennines, such as the Marnoso-arenacea Formation, the Cervarola basin has been interpreted as a highly confined foredeep controlled by an intense synsedimentary tectonic activity. The most important evidences supporting this hypothesis are: 1) the upward increase, in the studied stratigraphic succession (about 1000m thick), of sandstone/mudstone ratio, grain sizes and Ophiomorpha-type trace fossils testifying the high degree of flow deceleration related to the progressive closure and uplift of the foredeep. 2) the occurrence in the upper part of the stratigraphic succession of coarse-grained massive sandstones overlain by tractive structures such as megaripples and traction carpets passing downcurrent into fine-grained laminated contained-reflected beds. This facies tract is interpreted as related to deceleration and decoupling of bipartite flows with the deposition of the basal dense flows and bypass of the upper turbulent flows. 3) the widespread occurrence of contained reflected beds related to morphological obstacles created by tectonic structures parallel and perpendicular to the basin axis (see for example the Pievepelago line). 4) occurrence of intra-formational slumps, constituted by highly deformed portion of fine-grained succession, indicating a syn-sedimentary tectonic activity of the tectonic structures able to destabilize the margins of the basin. These types of deposits increase towards the upper part of the stratigraphic succession (see points 1 and 2) 5) the impressive lateral facies changes between intrabasinal topographic highs characterized by fine-grained and thin sandstone beds and marlstones and depocenters characterized by thick to very thick coarse-grained massive sandstones. 6) the common occurrence of amalgamation surfaces, flow impact structures and mud-draped scours related to sudden deceleration of the turbidite flows induced by the structurally-controlled confinement and morphological irregularities. In conclusion, the CSF has many analogies with the facies associations occurring in other tectonically-controlled foredeeps such as those of Marnoso-arenacea Formation (northern Italy) and Annot Sandstones (southern France) showing how thrust fronts and transversal structures moving towards the foreland, were able to produce a segmented foredeep that can strongly influence the turbidity current deposition.

Fisica dell'accrescimento

Questo elaborato presenta una descrizione del fenomeno dell’accrescimento di materia su oggetti compatti, esponendo i principali modelli fisici a riguardo. Dopo un’introduzione, in cui viene mostrato come l’accrescimento rappresenti la più importante fonte di energia in astrofisica, si discute nel capitolo 1 il più semplice modello di accresci- mento, dovuto ad Hermann Bondi (1952). Tale modello, proprio per la sua semplicità, risulta molto importante, nonostante trascuri importanti aspetti fisici. Nel capitolo 2 si studia la fisica dei dischi di accrescimento, analizzando sia il caso generale che alcuni casi particolari, come quello stazionario o a viscosità costante. L’elaborato si conclude con una breve analisi dell’emissione termica da parte del disco di accrescimento.