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22 results on '"Pincella, C."'

1. The STRIP instrument of the Large Scale Polarization Explorer: microwave eyes to map the Galactic polarized foregrounds

Author

Franceschet, C., Realini, S., Mennella, A., Addamo, G., Baù, A., Battaglia, P. M., Bersanelli, M., Caccianiga, B., Caprioli, S., Cavaliere, F., Cleary, K. A., Cuttaia, F., Del Torto, F., Fafone, V., Farooqui, Z., Santos, R. T. Génova, Gaier, T. C., Gervasi, M., Ghigna, T., Incardona, F., Iovenitti, S., Jones, M., Kangaslahti, P., Mainini, R., Maino, D., Maris, M., Mena, P., Molina, R., Morgante, G., Passerini, A., Perez-de-Taoro, M., Peverini, O. A., Pezzotta, F., Pincella, C., Reyes, N., Rocchi, A., Rubiño-Martín, J. A., Sandri, M., Sartor, S., Soria, M., Tapia, V., Terenzi, L., Tomasi, M., Tommasi, E., Viganó, D. M., Villa, F., Virone, G., Volpe, A., Watkins, B., Zacchei, A., and Zannoni, M.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

In this paper we discuss the latest developments of the STRIP instrument of the "Large Scale Polarization Explorer" (LSPE) experiment. LSPE is a novel project that combines ground-based (STRIP) and balloon-borne (SWIPE) polarization measurements of the microwave sky on large angular scales to attempt a detection of the "B-modes" of the Cosmic Microwave Background polarization. STRIP will observe approximately 25% of the Northern sky from the "Observatorio del Teide" in Tenerife, using an array of forty-nine coherent polarimeters at 43 GHz, coupled to a 1.5 m fully rotating crossed-Dragone telescope. A second frequency channel with six-elements at 95 GHz will be exploited as an atmospheric monitor. At present, most of the hardware of the STRIP instrument has been developed and tested at sub-system level. System-level characterization, starting in July 2018, will lead STRIP to be shipped and installed at the observation site within the end of the year. The on-site verification and calibration of the whole instrument will prepare STRIP for a 2-years campaign for the observation of the CMB polarization., Comment: 17 pages, 15 figures, proceedings of the SPIE Astronomical Telescopes + Instrumentation conference "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX", on June 15th, 2018, Austin (TX)

Published
2018
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2. Cryocooler cooled HTS current leads for a 1 MJ/1 MW-class SMES system

Author

Mariani, M., Ariante, M., Matrone, A., Petrillo, E., Quarantiello, R., Barberis, F., Martini, L., Pincella, C., Canepa, G., Ferrari, P., Ottonello, L., and Vivaldi, F.

Subjects
Magnetic energy storage -- Research, High temperature superconductors -- Research, Superconducting magnets -- Research, Electrical equipment and supplies industry -- Research, Electrical engineering, Business, Electronics, Electronics and electrical industries, European Organization for Nuclear Research -- Conferences, meetings and seminars
Abstract

A prototype of hybrid, resistive and high temperature superconductor (HTS) 1100A current leads, cooled by cryocooler, is described and discussed.

Published
2002

3. DC side filters for multiterminal HVDC systems

Author

Shore, N.L., Adamson, K., Bard, P., Burton, R.S., Clarke, C.D., Coutu, A., Kapoor, S.C., Kent, K.L., Pereira, F.P., Pincella, C., and Sadek, K.

Subjects
Electric power systems -- Equipment and supplies, Electric filters -- Evaluation, Filtering (Electronics) -- Analysis, Electric power system stability -- Research, Business, Computers, Electronics, Electronics and electrical industries
Abstract

Multiterminal HVDC systems present challenges in the specification and design of suitable dc side filtering. This document examines the existing experience and addresses the particular technical problems posed by multiterminal systems. The filtering requirements of small taps are discussed, as is the potential use of active filters. Aspects of calculation and design are considered and recommendations made to guide the planners and designers of future multiterminal schemes. Keywords - HVDC, Multiterminal, DC Filters, Power Transmission, Telephone Interference, Disturbing Current, Tapping, Active Filters, HVDC Specifications.

Published
1996

4. The STRIP instrument of the Large Scale Polarization Explorer: microwave eyes to map the Galactic polarized foregrounds

Author

Iovenitti, S, Zannoni, M, Zacchei, A, Watkins, B, Volpe, A, Virone, G, Villa, F, Vigano', D, Tommasi, E, Tomasi, M, Terenzi, L, Tapia, V, Soria, M, Sartor, S, Sandri, M, Rubino-Martin, J, Rocchi, A, Reyes, N, Realini, S, Pincella, C, Pezzotta, F, Peverini, O, Perez-de-Taoro, M, Passerini, A, Morgante, G, Molina, R, Mennella, A, Mena, P, Maris, M, Maino, D, Mainini, R, Kangaslahti, P, Jones, M, Incardona, F, Ghigna, T, Gervasi, M, Gaier, T, Genova Santos, R, Farooqui, Z, Fafone, V, Del Torto, F, Cuttaia, F, Cleary, K, Cavaliere, F, Caprioli, S, Caccianiga, B, Bersanelli, M, Battaglia, P, Bau', A, Addamo, G, Franceschet, C, Iovenitti, Simone, Zannoni, Mario, Zacchei, Andrea, Watkins, Bob, Volpe, Angela, Virone, Giuseppe, Villa, Fabrizio, Vigano', Daniele M., Tommasi, Elisabetta, Tomasi, Maurizio, Terenzi, Luca, Tapia, Valeria, Soria, Mary, Sartor, Stefano, Sandri, Maura, Rubino-Martin, Jose' A., Rocchi, Alessio, Reyes, Nicolas, Realini, Sabrina, Pincella, Claudio, Pezzotta, Federico, Peverini, Oscar A., Perez-de-Taoro, Maria del Rosario, Passerini, Andrea, Morgante, Gianluca, Molina, Rocio, Mennella, Aniello, Mena, Patricio, Maris, Michele, Maino, Davide, Mainini, Roberto, Kangaslahti, Pekka, Jones, Mike, Incardona, Federico, Ghigna, Tommaso, Gervasi, Massimo, Gaier, Todd C., Genova Santos, Ricardo T., Farooqui, Zunnoorain, Fafone, Viviana, Del Torto, Francesco, Cuttaia, Francesco, Cleary, Kieran A., Cavaliere, Francesco, Caprioli, Silvia, Caccianiga, Barbara, Bersanelli, Marco, Battaglia, Paola M., Bau', Alessandro, Addamo, Giuseppe, Franceschet, Cristian, Iovenitti, S, Zannoni, M, Zacchei, A, Watkins, B, Volpe, A, Virone, G, Villa, F, Vigano', D, Tommasi, E, Tomasi, M, Terenzi, L, Tapia, V, Soria, M, Sartor, S, Sandri, M, Rubino-Martin, J, Rocchi, A, Reyes, N, Realini, S, Pincella, C, Pezzotta, F, Peverini, O, Perez-de-Taoro, M, Passerini, A, Morgante, G, Molina, R, Mennella, A, Mena, P, Maris, M, Maino, D, Mainini, R, Kangaslahti, P, Jones, M, Incardona, F, Ghigna, T, Gervasi, M, Gaier, T, Genova Santos, R, Farooqui, Z, Fafone, V, Del Torto, F, Cuttaia, F, Cleary, K, Cavaliere, F, Caprioli, S, Caccianiga, B, Bersanelli, M, Battaglia, P, Bau', A, Addamo, G, Franceschet, C, Iovenitti, Simone, Zannoni, Mario, Zacchei, Andrea, Watkins, Bob, Volpe, Angela, Virone, Giuseppe, Villa, Fabrizio, Vigano', Daniele M., Tommasi, Elisabetta, Tomasi, Maurizio, Terenzi, Luca, Tapia, Valeria, Soria, Mary, Sartor, Stefano, Sandri, Maura, Rubino-Martin, Jose' A., Rocchi, Alessio, Reyes, Nicolas, Realini, Sabrina, Pincella, Claudio, Pezzotta, Federico, Peverini, Oscar A., Perez-de-Taoro, Maria del Rosario, Passerini, Andrea, Morgante, Gianluca, Molina, Rocio, Mennella, Aniello, Mena, Patricio, Maris, Michele, Maino, Davide, Mainini, Roberto, Kangaslahti, Pekka, Jones, Mike, Incardona, Federico, Ghigna, Tommaso, Gervasi, Massimo, Gaier, Todd C., Genova Santos, Ricardo T., Farooqui, Zunnoorain, Fafone, Viviana, Del Torto, Francesco, Cuttaia, Francesco, Cleary, Kieran A., Cavaliere, Francesco, Caprioli, Silvia, Caccianiga, Barbara, Bersanelli, Marco, Battaglia, Paola M., Bau', Alessandro, Addamo, Giuseppe, and Franceschet, Cristian

Abstract

In this paper we discuss the latest developments of the STRIP instrument of the “Large Scale Polarization Explorer” (LSPE) experiment. LSPE is a novel project that combines ground-based (STRIP) and balloon-borne (SWIPE) polarization measurements of the microwave sky on large angular scales to attempt a detection of the “B-modes” of the Cosmic Microwave Background polarization. STRIP will observe approximately 25% of the Northern sky from the “Observatorio del Teide” in Tenerife, using an array of forty-nine coherent polarimeters at 43 GHz, coupled to a 1.5 m fully rotating crossed-Dragone telescope. A second frequency channel with six-elements at 95 GHz will be exploited as an atmospheric monitor. At present, most of the hardware of the STRIP instrument has been developed and tested at sub-system level. System-level characterization, starting in July 2018, will lead STRIP to be shipped and installed at the observation site within the end of the year. The on-site verification and calibration of the whole instrument will prepare STRIP for a 2-years campaign for the observation of the CMB polarization.

Published
2018

5. The record-breaking Italy--Greece HVDC link. (Transmission & Distribution)

Author

Girogi, A., Rendina, R., Georgantzis, G., Marchiori, C., Pazienza, G., Corsi, S., Pincella, C., Pozzi, M., Danielsson, K., Jonasson, H., and Orini, A.

Subjects
Enel-Terna, Pubic Power Corp. -- Product information, Submarine cables -- Testing, Submarine cables -- Design and construction, Submarine cables -- Product information, Electric utilities -- Product information, Business, Petroleum, energy and mining industries, European Union -- Energy policy
Abstract

The new Italy -- Greece HVDC link is at 1000m the deepest submarine link in existence, and includes one of the longest underground sections in the world. Proving it involved [...]

Published
2002

10. Il progetto Custom Power

Author

Pincella, C., Chiumeo, R., Martini, L., Barberis, F., Cadore, A., DI DOMENICO, F., Faini, E., Furlani, R., Groppelli, P., Albertelli, P., Canepa, G., Ferrari, P., Florio, A., Ottonello, L., Picco, E., Masciarelli, G., Rossi, S., Mariscotti, Andrea, Mazzucchelli, MAURIZIO FRANCO, Torello, Eugenia, and Martinolli, A.

Published
2005

15. The Largest Italian SMES

Author

Ottonello, L., primary, Canepa, G., additional, Albertelli, P., additional, Picco, E., additional, Florio, A., additional, Masciarelli, G., additional, Rossi, S., additional, Martini, L., additional, Pincella, C., additional, Mariscotti, A., additional, Torello, E., additional, Martinolli, A., additional, and Mariani, M., additional

Published
2006
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17. DC Side Filters for Multiterminal HVDC Systems

Author

Shore, N. L., primary, Adamson, K., additional, Bard, P., additional, Kapoor, S., additional, Kent, K. L., additional, Burton, R. S., additional, Clarke, C. D., additional, Pereira, F. P., additional, Pincella, C., additional, Coutu, A., additional, and Sadek, K., additional

Published
1996
Full Text
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22. The STRIP instrument of the Large Scale Polarization Explorer: microwave eyes to map the Galactic polarized foregrounds

Author

Franceschet, Cristian, Realini, Sabrina, Mennella, Aniello, Addamo, Giuseppe, Baù, Alessandro, Battaglia, Paola M., Bersanelli, Marco, Caccianiga, Barbara, Caprioli, Silvia, Cavaliere, Francesco, Cleary, Kieran A., Cuttaia, Francesco, Del Torto, Francesco, Fafone, Viviana, Farooqui, Zunnoorain, Génova Santos, Ricardo T., Gaier, Todd C., Gervasi, Massimo, Ghigna, Tommaso, Incardona, Federico, Iovenitti, Simone, Jones, Mike, Kangaslahti, Pekka, Mainini, Roberto, Maino, Davide, Maris, Michele, Mena, Patricio, Molina, Rocío, Morgante, Gianluca, Passerini, Andrea, Perez-De-Taoro, Maria Del Rosario, Peverini, Oscar A., Pezzotta, Federico, Pincella, Claudio, Reyes, Nicolás, Rocchi, Alessio, Rubiño-Martín, José A., Sandri, Maura, Sartor, Stefano, Soria, Mary, Tapia, Valeria, Terenzi, Luca, Tomasi, Maurizio, Tommasi, Elisabetta, Viganó, Daniele M., Villa, Fabrizio, Virone, Giuseppe, Volpe, Angela, Watkins, Bob, Zacchei, Andrea, Zannoni, Mario, Zmuidzinas, Jonas, Gao, Jian-Rong, Iovenitti, S, Zannoni, M, Zacchei, A, Watkins, B, Volpe, A, Virone, G, Villa, F, Vigano', D, Tommasi, E, Tomasi, M, Terenzi, L, Tapia, V, Soria, M, Sartor, S, Sandri, M, Rubino-Martin, J, Rocchi, A, Reyes, N, Realini, S, Pincella, C, Pezzotta, F, Peverini, O, Perez-de-Taoro, M, Passerini, A, Morgante, G, Molina, R, Mennella, A, Mena, P, Maris, M, Maino, D, Mainini, R, Kangaslahti, P, Jones, M, Incardona, F, Ghigna, T, Gervasi, M, Gaier, T, Genova Santos, R, Farooqui, Z, Fafone, V, Del Torto, F, Cuttaia, F, Cleary, K, Cavaliere, F, Caprioli, S, Caccianiga, B, Bersanelli, M, Battaglia, P, Bau', A, Addamo, G, Franceschet, C, ITA, USA, GBR, ESP, CHL, Electromagnetics, Zmuidzinas, Jonas, and Gao, Jian-Rong

Subjects
media_common.quotation_subject, Cosmic microwave background, FOS: Physical sciences, 02 engineering and technology, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, law.invention, Telescope, FIS/05 - ASTRONOMIA E ASTROFISICA, Optics, law, Cosmic Microwave Background, 0103 physical sciences, 0202 electrical engineering, electronic engineering, information engineering, B-modes, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), media_common, Millimeter, Submillimeter, Far-Infrared, Detectors, Instrumentation, Cosmic Microwave Background, Polarization, Physics, polarization, business.industry, SwIPe, Astrophysics::Instrumentation and Methods for Astrophysics, 020206 networking & telecommunications, Large scale, Polarization (waves), Polarimeter, Cosmic Microwave Background polarization, Sky, Ground-based telescope, business, Astrophysics - Instrumentation and Methods for Astrophysics, Microwave, Galactic foreground
Abstract

In this paper we discuss the latest developments of the STRIP instrument of the "Large Scale Polarization Explorer" (LSPE) experiment. LSPE is a novel project that combines ground-based (STRIP) and balloon-borne (SWIPE) polarization measurements of the microwave sky on large angular scales to attempt a detection of the "B-modes" of the Cosmic Microwave Background polarization. STRIP will observe approximately 25% of the Northern sky from the "Observatorio del Teide" in Tenerife, using an array of forty-nine coherent polarimeters at 43 GHz, coupled to a 1.5 m fully rotating crossed-Dragone telescope. A second frequency channel with six-elements at 95 GHz will be exploited as an atmospheric monitor. At present, most of the hardware of the STRIP instrument has been developed and tested at sub-system level. System-level characterization, starting in July 2018, will lead STRIP to be shipped and installed at the observation site within the end of the year. The on-site verification and calibration of the whole instrument will prepare STRIP for a 2-years campaign for the observation of the CMB polarization., Comment: 17 pages, 15 figures, proceedings of the SPIE Astronomical Telescopes + Instrumentation conference "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX", on June 15th, 2018, Austin (TX)

Published
2018

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