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    <title>DSpace Collection: 01.01.05. Radiation</title>
    <link>http://hdl.handle.net/2122/90</link>
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      <title>Spectrally resolved observations of atmospheric emitted radiance in the H2O rotation band</title>
      <link>http://hdl.handle.net/2122/3680</link>
      <description>Title: Spectrally resolved observations of atmospheric emitted radiance in the H2O rotation band
&lt;br/&gt;
&lt;br/&gt;Authors: Bhawar, R.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Bianchini, G.; Istituto di Fisica Applicata Nello Carrara, CNR, Sesto Fiorentino, Italy; Bozzo, A.; Dipartimento di Fisica, Universita` di Bologna, Bologna, Italy; Cacciani, M.; Dipartimento di Fisica, Universita di Roma La Sapienza, Roma, Italy; Calvello, M. R.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Carlotti, M.; Dipartimento di Chimica Fisica ed Inorganica, Universita` di Bologna, Bologna, Italy; Castagnoli, F.; Istituto di Fisica Applicata Nello Carrara, CNR, Sesto Fiorentino, Italy; Cuomo, V.; Istituto di Metodologie per l’Analisi Ambientale, CNR, Tito Scalo, Italy; Di Girolamo, P.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Di Iorio, T.; Dipartimento di Fisica, Universita di Roma La Sapienza, Roma, Italy; Di Liberto, L.; Dipartimento di Fisica, Universita di Roma La Sapienza, Roma, Italy; di Sarra, A.; Dipartimento di Fisica, Universita di Roma La Sapienza, Roma, Italy; Esposito, F.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Fiocco, G.; Dipartimento di Fisica, Universita di Roma La Sapienza, Roma, Italy; Fuà, D.; Dipartimento di Fisica, Universita di Roma La Sapienza, Roma, Italy; Grieco, G.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Maestri, T.; Dipartimento di Fisica, Universita` di Bologna, Bologna, Italy; Masiello, G.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Muscari, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Palchetti, L.; Istituto di Fisica Applicata Nello Carrara, CNR, Sesto Fiorentino, Italy; Papandrea, E.; Dipartimento di Chimica Fisica ed Inorganica, Universita` di Bologna, Bologna, Italy; Pavese, G.; Istituto di Metodologie per l’Analisi Ambientale, CNR, Tito Scalo, Italy; Restieri, R.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Rizzi, R.; Dipartimento di Fisica, Universita` di Bologna, Bologna, Italy; Romano, F.; Istituto di Metodologie per l’Analisi Ambientale, CNR, Tito Scalo, Italy; Serio, C.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Summa, D.; Dipartimento di Ingegeneria e Fisica dell’Ambiente, Universita` della Basilicata, Potenza, Italy; Todini, G.; Dipartimento di Fisica, Universita` di Bologna, Bologna, Italy; Tosi, E.; Dipartimento di Fisica, Universita` di Bologna, Bologna, Italy
&lt;br/&gt;
&lt;br/&gt;Abstract: This paper presents the project Earth Cooling by Water&#xD;
Vapor Radiation, an observational programme, which aims at&#xD;
developing a database of spectrally resolved far infrared&#xD;
observations, in atmospheric dry conditions, in order to&#xD;
validate radiative transfer models and test the quality of water&#xD;
vapor continuum and line parameters. The project provides&#xD;
the very first set of far-infrared spectral downwelling&#xD;
radiance measurements, in dry atmospheric conditions,&#xD;
which are complemented with Raman Lidar-derived&#xD;
temperature and water vapor profiles.</description>
      <pubDate>Tue, 29 Jan 2008 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>The effect of recent Venus transit on Earth’s atmosphere</title>
      <link>http://hdl.handle.net/2122/3505</link>
      <description>Title: The effect of recent Venus transit on Earth’s atmosphere
&lt;br/&gt;
&lt;br/&gt;Authors: De, S. S.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India; De, B. K.; Department of Physics, Tripura University, Agartala, India; Adhikari, S. K.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India; Sarkar, B. K.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India; Sarkar, S. K.; Department of Physics, University of Calcutta, Kolkata, India; Guha, A.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India; Mandal, P. K.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India; Mandal, S. K.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India; Sardar, H. P.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India; Ray, M.; Centre of Advanced Study in Radio Physics and Electronics, University of Calcutta, Kolkata, India
&lt;br/&gt;
&lt;br/&gt;Abstract: Some experiments on June 8, 2004, the day of transit of Venus across the Sun, were undertaken at Kolkata (latitude:&#xD;
22°34lN) to observe the effect, if any, of transit of Venus on FWF, ELF and VLF amplitudes. The result&#xD;
shows a good correlation between their temporal variations during the transit. The observation was unbelievable&#xD;
as the Venus subtends only 1/32th of the cone subtended by Sun on Earth. This anomaly may be explained on&#xD;
the assumption that the height of Venusian atmosphere with high content of CO2, and nitrogen which absorbs&#xD;
electromagnetic and corpuscular radiations from Sun, depleting the solar radiation reaching the Earth to a considerable&#xD;
extent. As a result, relevant parameters of Earth’s atmosphere are modulated and here we show how&#xD;
these changes are reflected in identical behaviour of fair weather field and ELF and VLF spectra.</description>
      <pubDate>Tue, 28 Nov 2006 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>A numerical simulation study of dissolved organic carbon accumulation in the northern Adriatic Sea</title>
      <link>http://hdl.handle.net/2122/3452</link>
      <description>Title: A numerical simulation study of dissolved organic carbon accumulation in the northern Adriatic Sea
&lt;br/&gt;
&lt;br/&gt;Authors: Polimene, L.; Centro Interdipartimentale per la Ricerca sulle Scienze Ambientali, Università di Bologna, Ravenna, Italy; Pinardi, N.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italia; Zavatarelli, M.; Centro Interdipartimentale per la Ricerca sulle Scienze Ambientali, Università di Bologna, Ravenna, Italy; Allen, J. I.; Plymouth Marine Laboratory, Plymouth, UK; Giani, M.; Istituto Centrale per la Ricerca scientifica e tecnologica Applicata al Mare (ICRAM) sts Chioggia, Chioggia, Italy; Vichi, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italia
&lt;br/&gt;
&lt;br/&gt;Abstract: A mechanistic explanation for the accumulation of dissolved organic carbon (DOC), observed in coastal seas such as the Northern Adriatic Sea, is proposed here on the basis of numerical simulations of the marine ecosystem dynamics carried out with a coupled biogeochemical-circulation model. The biogeochemical model is based on the European Regional Seas Ecosystem Model (ERSEM) upgraded with a more detailed representation of the DOC-bacteria interactions and resolving different level of DOC lability/refractivity. The circulation model is the Adriatic Sea implementation of the Princeton Ocean Model. The analysis of simulations confirms the important role of the Po river nutrient input on the ecosystem dynamics and highlights the presence of a strong across-shelf trophic gradient that, affecting the Bacterial Growth Efficiency (BGE), could be a key factor for the DOC accumulation. The simulations show the importance of circulation features in modulating the exchanges between areas having different trophic structure such as the western coastal strip, strongly influenced by the Po river runoff, and the open sea areas in the centre of the northern Adriatic sub-basin. The DOC produced in the high energy system of the Po runoff coastal strip, characterized by high BGE, is transported toward the open areas, which is a more oligotrophic environment with lower BGE. In this area the DOC turnover time is strongly increased giving rise to the DOC accumulation.</description>
      <pubDate>Tue, 06 Mar 2007 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Una nuova procedura per le correzioni atmosferiche: applicazione sulla Solfatara di Pozzuoli.</title>
      <link>http://hdl.handle.net/2122/3322</link>
      <description>Title: Una nuova procedura per le correzioni atmosferiche: applicazione sulla Solfatara di Pozzuoli.
&lt;br/&gt;
&lt;br/&gt;Authors: Musacchio, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia; Amici, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia; Teggi, S.; Pompilio, L; Sgavetti, M.; Buongiorno, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia
&lt;br/&gt;
&lt;br/&gt;Abstract: This paper describes CIRILLO, a new software for the correction of spaceborne images acquired in the VIS-SWIR spectral range. Moreover the capability to retrieve minerals composing the Solfatara di Pozzuoli surface using ASTER multispectral data is shown.&#xD;
In order to identify the mineralogical composition of the collected sample, mineralogy analysis (X-ray fluorescence and X-ray diffratometry) have been done.&#xD;
The reflectance spectra of the collected sample, obtained using a FieldSpec Pro spectrometer (INAF-LASF) has been compared with measurements performed directly on the Solftara di Pozzuoli using a portable ASD-Fieldspec spectrometer.</description>
      <pubDate>Tue, 07 Aug 2007 22:58:59 GMT</pubDate>
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