Thematische Bibliographien / Osservatorio astronomico di Roma

Auswahl der wissenschaftlichen Literatur zum Thema „Osservatorio astronomico di Roma“

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Veröffentlicht am 25. Juli 2024

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Zeitschriftenartikel zum Thema "Osservatorio astronomico di Roma"

Foreword, Editorial,. „Workshop on The Golden Age of Cataclysmic Variables and Related Objects - II .“ Acta Polytechnica CTU Proceedings 2, Nr. 1 (23.02.2015): ii—xvii. http://dx.doi.org/10.14311/app.2015.02.9001.

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Organizing Institutions: INAF – Istituto di Astrofisica e Planetologia Spaziali, Roma – INAF-IAPS, Roma, Italy INTA – Dpt. de Cargas Utiles y Ciencias del Espacio, INTA-DCUCE, Madrid, Spain Czech Republic Academy of Sciences – Astronomical Institute, ASCR-AI, Ondřejov, Czech Republic Czech Technical University, CTU in Prague, Czech Republic Department of Physics, Technion, Haifa, Israel Russian Academy of Sciences – Institute of Astronomy, RAS-IA, Moscow, Russia INAF - Osservatorio Astronomico di Capodimonte, INAF-OAC, Napoli, Italy Department of Astronomy, University of Washington, Seattle, WA, USA

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MINIATI, MARA. „MARINELLA CALISI, Storia e strumenti del Museo Astronomico e Copernicano di Roma. Guida alle collezioni, Roma, Osservatorio Astronomico di Roma, 2000, 167 pp., ill.“ Nuncius 15, Nr. 2 (2000): 798. http://dx.doi.org/10.1163/182539100x00308.

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MINIATI, MARA. „MARINELLA CALISI, Guida alla visita del Museo Astronomico e Copernicano di Roma, Roma, Osservatorio Astronomico e Museo Astronomico e Copernicano, 1991, 145 pp., fig.“ Nuncius 7, Nr. 2 (1992): 333. http://dx.doi.org/10.1163/182539192x01234.

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MINIATI, MARA. „MARINELLA CALISI, Storia e strumenti del Museo Astronomico e Copernicano di Roma. Guida alle collezioni, Roma, Osservatorio Astronomico di Roma, 2000, 167 pp., ill.“ Nuncius 15, Nr. 2 (01.01.2000): 798. http://dx.doi.org/10.1163/221058700x00302.

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Ermolli, I., T. Chatzistergos, F. Giorgi, V. M. S. Carrasco, A. J. P. Aparicio und I. Chinnici. „Solar Observations by Angelo Secchi. I. Digitization of Original Documents and Analysis of Group Numbers over the Period of 1853–1878“. Astrophysical Journal Supplement Series 269, Nr. 2 (01.12.2023): 53. http://dx.doi.org/10.3847/1538-4365/ad0886.

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Abstract Angelo Secchi, an Italian Jesuit and prominent scientist of the 19th century, and one of the founders of modern astrophysics, observed the Sun regularly at the Collegio Romano in Rome, Italy, for more than 25 yr. Results from his observations are reported in articles published in the scientific journals of the time, as well as in drawings and personal notebooks that are stored in the historical archive of the Istituto Nazionale di Astrofisica Osservatorio Astronomico di Roma. The latter material, which reports solar observations performed from 1853–1878, includes original documents from Secchi and from a few of his close collaborators. The above unique material has recently been digitized for preservation purposes and for allowing the scientific exploitation of data not easily accessible so far. A total of more than 5400 digital images have been produced. Here we present the archival material and the new digital data derived from it. We also present results obtained from our primary analysis of the new digital data. In particular, we produced new measurements of the group number from 1853–1878, which will be available for future recalibration of the group number series.

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Ermolli, I., K. Matthes, T. Dudok de Wit, N. A. Krivova, K. Tourpali, M. Weber, Y. C. Unruh et al. „Recent variability of the solar spectral irradiance and its impact on climate modelling“. Atmospheric Chemistry and Physics 13, Nr. 8 (17.04.2013): 3945–77. http://dx.doi.org/10.5194/acp-13-3945-2013.

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Abstract. The lack of long and reliable time series of solar spectral irradiance (SSI) measurements makes an accurate quantification of solar contributions to recent climate change difficult. Whereas earlier SSI observations and models provided a qualitatively consistent picture of the SSI variability, recent measurements by the SORCE (SOlar Radiation and Climate Experiment) satellite suggest a significantly stronger variability in the ultraviolet (UV) spectral range and changes in the visible and near-infrared (NIR) bands in anti-phase with the solar cycle. A number of recent chemistry-climate model (CCM) simulations have shown that this might have significant implications on the Earth's atmosphere. Motivated by these results, we summarize here our current knowledge of SSI variability and its impact on Earth's climate. We present a detailed overview of existing SSI measurements and provide thorough comparison of models available to date. SSI changes influence the Earth's atmosphere, both directly, through changes in shortwave (SW) heating and therefore, temperature and ozone distributions in the stratosphere, and indirectly, through dynamical feedbacks. We investigate these direct and indirect effects using several state-of-the art CCM simulations forced with measured and modelled SSI changes. A unique asset of this study is the use of a common comprehensive approach for an issue that is usually addressed separately by different communities. We show that the SORCE measurements are difficult to reconcile with earlier observations and with SSI models. Of the five SSI models discussed here, specifically NRLSSI (Naval Research Laboratory Solar Spectral Irradiance), SATIRE-S (Spectral And Total Irradiance REconstructions for the Satellite era), COSI (COde for Solar Irradiance), SRPM (Solar Radiation Physical Modelling), and OAR (Osservatorio Astronomico di Roma), only one shows a behaviour of the UV and visible irradiance qualitatively resembling that of the recent SORCE measurements. However, the integral of the SSI computed with this model over the entire spectral range does not reproduce the measured cyclical changes of the total solar irradiance, which is an essential requisite for realistic evaluations of solar effects on the Earth's climate in CCMs. We show that within the range provided by the recent SSI observations and semi-empirical models discussed here, the NRLSSI model and SORCE observations represent the lower and upper limits in the magnitude of the SSI solar cycle variation. The results of the CCM simulations, forced with the SSI solar cycle variations estimated from the NRLSSI model and from SORCE measurements, show that the direct solar response in the stratosphere is larger for the SORCE than for the NRLSSI data. Correspondingly, larger UV forcing also leads to a larger surface response. Finally, we discuss the reliability of the available data and we propose additional coordinated work, first to build composite SSI data sets out of scattered observations and to refine current SSI models, and second, to run coordinated CCM experiments.

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Maggio, A., F. Reale, G. Peres und A. Ciaravella. „The analysis system for astrophysical plasmas (ASAP) of the Osservatorio Astronomico di Palermo“. Computer Physics Communications 81, Nr. 1-2 (Juni 1994): 105–19. http://dx.doi.org/10.1016/0010-4655(94)90114-7.

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BRENNI, PAOLO. „IL METEOROGRAFO DI PADRE ANGELO SECCHI“. Nuncius 8, Nr. 1 (1993): 197–247. http://dx.doi.org/10.1163/182539183x00082.

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Abstract<title> SUMMARY </title>During the 19th Century the systematic collecting of meteorological data became a general practice. Several scientists and instrument makers invented new meteorological instruments and improved the existing ones. Probably the most impressive and sophisticated recording apparatus was the meteorograph devised between 1855 and 1865 by the Italian astronomer Padre Angelo Secchi (1818-1878). This huge and complicated machine was presented to the 1867 Paris Universal Exhibition where it was considered the technological masterpiece. The instrument worked in Rome for several years and then, partially dismanteled, was finally stored in the Osservatorio Astronomico di Monte Porzio (Rome). Recently carried to Florence, the meteorograph is now beeing restored in the laboratories of the Opificio delle Pietre Dure under the supervision of the Istituto e Museo di Storia della Scienza. My paper will trace the history of this ingeniuos instrument which represented a technological achievement but an economic failure.

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Crisci, Massimiliano. „I commercianti e l'immigrazione straniera: accoglienza e diffidenza“. ARGOMENTI, Nr. 28 (Juni 2010): 83–101. http://dx.doi.org/10.3280/arg2010-028005.

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Il lavoro analizza gli atteggiamenti e le opinioni dei commercianti romani sui cittadini stranieri, esponendo alcuni risultati di un'indagine svolta da un gruppo di lavoro del CISR - Centro di Ricerca su Roma della Sapienza Universitŕ di Roma. La categoria dei commercianti rappresenta un osservatorio privilegiato del fenomeno immigrazione, perché esprime una domanda di manodopera che incontra facilmente l'offerta proveniente da lavoratori stranieri, spesso poco qualificata e a basso costo, e si trova ad avere molteplici occasioni di interazione con gli immigrati.. L'obiettivo principale dell'articolo č comprendere come le dimensioni economica, sociale e individuale del piccolo imprenditore entrano in gioco nell'orientare l'opinione sull'inclusione degli stranieri nella societŕ italiana. Le articolate posizioni dei commercianti sono sintetizzate attraverso due profili speculari di atteggiamento: quello dell'accoglienza e della diffidenza.

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Leiber, Th, und K. Reif. „First Observations by the Bonn Wide-Field Photometer and Polarimeter (WWFPP): Surface Polarimetry of the Crab Nebula“. Symposium - International Astronomical Union 161 (1994): 481–83. http://dx.doi.org/10.1017/s0074180900047926.

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To test the performance of the WWFPP in polarimetric mode, we performed surface polarimetry of the Crab nebula in February 1993 using the Asiago 1.82 m telescope of the ‘Osservatorio Astronomico di Padova’. The polarimeter is a new design and enables us to do simultaneous wide-field polarimetry (15 × 15 arcmin field with 0.43 arcsec/pixel) of four polarization angles using a twin Wollaston prism or simultaneous polarimetry of two angles using a double wedge plate with orthogonal sheet polarizers in combination with an achromatic half wave plate. For the observations described here we used the twin Wollaston. The advantages of this design are independency of fluctuations of atmospheric transmission and identical seeing for one set of Stokes parameters. The results of the observations are in agreement with results of other investigators who performed surface polarimetry of the Crab Nebula.

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Dissertationen zum Thema "Osservatorio astronomico di Roma"

Pieretti, Davide. „Sviluppo di un sistema informatico per il controllo remoto di un osservatorio astronomico“. Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/10559/.

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L'obiettivo di questo elaborato è quello di indicare una via verso una nuova modalità di utilizzo degli osservatori astronomici disseminati lungo la penisola italiana. Utilizzando le tecnologie disponibili e integrandole fra loro il sistema che si andrà a progettare permetterà di controllare da remoto un osservatorio astronomico. Questa nuova modalità di interazione con strumenti scientifici quali i telescopi potrà rendere possibile nuove modalità di divulgazione astronomica, sia in ambito educativo fornendo nuovi strumenti alle scuole che in ambito culturale potendo avvicinare tutti i curiosi all'osservazione dei corpi celesti che circondano il pianeta Terra. Utilizzare la tecnologia per avvicinare le persone alla scienza è una grande sfida per il futuro: le nuove scoperte e le nuove invenzioni non sono ormai piu frutto di singole menti brillanti ma frutto di collaborazioni e figlie della "sapienza collettiva" che Internet sta fortificando e rendendo sempre piu fruibile.

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Bücher zum Thema "Osservatorio astronomico di Roma"

Miotto, E. La strumentazione nella storia dell'Osservatorio astronomico di Brera. Milano: Università degli Studi di Milano, 1989.

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Elio, De Rosa, Hrsg. La Collina di Urania: Il Museo storico dell'Osservatorio astronomico di Capodimonte. Napoli: EdR, 1992.

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Serio, Giorgia Foderà. L' Osservatorio astronomico di Palermo: La storia e gli strumenti. Palermo: Flaccovio, 1997.

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Böhm, Conrad A. 250 anni di astronomia a Trieste. Trieste: MGS Press, 1998.

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Brera, Osservatorio astronomico di. Catalogo della corrispondenza degli astronomi di Brera. Milano: Università degli studi di Milano, 1986.

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Curir, Anna. Osservar le stelle: 250 anni di astronomia a Torino : la storia e gli strumenti dell'Osservatorio astronomico di Torino. Cinisello Balsamo (Milano): Silvana, 2009.

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Pigatto, Luisa, und Valeria Zanini. La Specola di Padova: Da torre medievale a museo. Padova: Signum Padova editrice, 2007.

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Calisi, Marinella. Storia e strumenti del Museo astronomico e copernicano di Roma: Guida alle collezioni. Roma: Osservatorio astronomico, 2000.

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copernicano, Museo astronomico e. Storia e strumenti del Museo astronomico e copernicano di Roma: Guida alle collezioni. Roma: Osservatorio astronomico, 2000.

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Osservatorio sul moderno a Roma (Università degli studi di Roma "La Sapienza") und Università degli studi di Roma "La Sapienza." Dipartimento di architettura e analisi della città., Hrsg. Il moderno e Roma: Tre giornate di fondazione dell'Osservatorio sul moderno a Roma. Roma: F.lli Palombi, 1997.

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Konferenzberichte zum Thema "Osservatorio astronomico di Roma"

Collura, Alfonso, Marco Barbera, Giuseppe Inzerillo, Filippo Mirabello, Salvatore Sciortino und Salvatore Serio. „X-ray Astronomy Calibration and Testing Facility (XACT) at Osservatorio Astronomico di Palermo G.S. Vaiana“. In SPIE's 1994 International Symposium on Optics, Imaging, and Instrumentation, herausgegeben von Oswald H. W. Siegmund und John V. Vallerga. SPIE, 1994. http://dx.doi.org/10.1117/12.186814.

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Collura, Alfonso, Marco Barbera, Alessandro Dara, Giuseppe Inzerillo, Filippo Mirabello, Salvatore Sciortino und Salvatore Serio. „Calibration of the AXAF-HRC UV/ion shields at Osservatorio Astronomico di Palermo G.S. Vaiana: I -instrumental setup“. In SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, herausgegeben von Oswald H. W. Siegmund und Mark A. Gummin. SPIE, 1996. http://dx.doi.org/10.1117/12.255990.

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Barbera, Marco, Alfonso Collura, Alessandro Dara, Salvatore Serio und Martin V. Zombeck. „Calibration of the AXAF-HRC UV/ion shields at the Osservatorio Astronomico di Palermo G.S. Vaiana: IV - UV rejection measurements“. In SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, herausgegeben von Oswald H. W. Siegmund und Mark A. Gummin. SPIE, 1996. http://dx.doi.org/10.1117/12.255987.

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Collura, Alfonso, Marco Barbera, Alessandro Dara, Salvatore Serio und Martin V. Zombeck. „Calibration of the AXAF-HRC UV/ion shields at Osservatorio Astronomico di Palermo G.S. Vaiana: II - x-ray transmission measurements“. In SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, herausgegeben von Oswald H. W. Siegmund und Mark A. Gummin. SPIE, 1996. http://dx.doi.org/10.1117/12.255989.

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Barbera, Marco, Alfonso Collura und Alessandro Dara. „Calibration of the AXAF-HRC UV/ion shields at Osservatorio Astronomico di Palermo G.S. Vaiana: III - synchrotron measurements of XANES in aluminum-coated Lexan film samples“. In SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, herausgegeben von Oswald H. W. Siegmund und Mark A. Gummin. SPIE, 1996. http://dx.doi.org/10.1117/12.255988.

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