Examinando por Autor "Reina, M."

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OSIRIS – The Scientific Camera System Onboard Rosetta
(Springer Link, 2007-01-12) Keller, H. U.; Barbieri, C.; Lamy, Philippe; Rickman, H.; Rodrigo, Rafael; Wenzel, K. P.; Sierks, H.; A´Hearn, M. F.; Angrilli, F.; Angulo, M.; Bailey, M. E.; Barthol, P.; Barucci, M. A.; Bertaux, J. L.; Bianchini, G.; Boit, J. L.; Brown, V.; Burns, J. A.; Büttner, I.; Castro, J. M.; Cremonese, G.; Curdt, W.; Da Deppo, V.; Debei, S.; De Cecco, M.; Dohlen, K.; Fornasier, S.; Fulle, M.; Germerott, D.; Gliem, F.; Guizzo, G. P.; Hviid, S. F.; Ip, W. H.; Jorda, L.; Koschny, D.; kramm, J. R.; Kührt, E.; Küppers, M.; Lara, L. M.; Llebaria, A.; López, A.; López Jiménez, A.; López Moreno, J. J.; Meller, R.; Michalik, H.; Díaz Michelena, M.; Müller, R.; Naletto, G.; Origné, A.; Parzianello, G.; Pertile, M.; Quintana, C.; Ragazzoni, R.; Ramous, P.; Reiche, K. U.; Reina, M.; Rodríguez, J.; Rousset, G.; Sabau, L.; Sivan, J. P.; Stöckner, K.; Telljohann, U.; Thomas, N.; Timón, V.; Tomasch, G.; Wittrock, T.; Zaccariotto, M.; Sanz de la Rosa, Andrea
The Optical, Spectroscopic, and Infrared Remote Imaging System OSIRIS is the scientific camera system onboard the Rosetta spacecraft (Figure 1). The advanced high performance imaging system will be pivotal for the success of the Rosetta mission. OSIRIS will detect 67P/Churyumov-Gerasimenko from a distance of more than 106 km, characterise the comet shape and volume, its rotational state and find a suitable landing spot for Philae, the Rosetta lander. OSIRIS will observe the nucleus, its activity and surroundings down to a scale of ~2 cm px−1. The observations will begin well before the onset of cometary activity and will extend over months until the comet reaches perihelion. During the rendezvous episode of the Rosetta mission, OSIRIS will provide key information about the nature of cometary nuclei and reveal the physics of cometary activity that leads to the gas and dust coma. OSIRIS comprises a high resolution Narrow Angle Camera (NAC) unit and a Wide Angle Camera (WAC) unit accompanied by three electronics boxes. The NAC is designed to obtain high resolution images of the surface of comet 67P/Churyumov-Gerasimenko through 12 discrete filters over the wavelength range 250–1000 nm at an angular resolution of 18.6 μrad px−1. The WAC is optimised to provide images of the near-nucleus environment in 14 discrete filters at an angular resolution of 101 μrad px−1. The two units use identical shutter, filter wheel, front door, and detector systems. They are operated by a common Data Processing Unit. The OSIRIS instrument has a total mass of 35 kg and is provided by institutes from six European countries.
Acceso Abierto
OWLS: a ten-year history in optical wireless links for intra-satellite communications
(Institute of Electrical and Electronics Engineers 27(9): 1599-1611(2009), 2009-12-10) Arruego, I.; Guerrero, H.; Rodríguez, Santiago; Martínez Oter, J.; Jiménez, J. J.; Domínguez, J. A.; Rivas, J.; Álvarez, M. T.; Gallego, P.; Azcue, J.; Ruiz de Galarreta, C.; Martín, B.; Álvarez Herrero, A.; Díaz Michelena, M.; Martín, I.; Tamayo, R.; Reina, M.; Gutiérrez, M. J.; Sabau, L.; Torres, J.; Martín-Ortega, Alberto; Martín-Ortega, Alberto; de Mingo Martín, José Ramón; Apéstigue, Víctor; Sánchez - Valdepeñas García - Moreno, Jesús; Samblas Iglesias, Juan
The application of Optical Wireless Links to intra- Spacecraft communications (OWLS) is presented here. This work summarizes ten years of developments, ranging from basic optoelectronic parts and front-end electronics, to different inorbit demonstrations. Several wireless applications were carried out in representative environments at ground level, and on in-flight experiments. A completely wireless satellite will be launched at the beginning of 2010. The benefits of replacing standard data wires and connectors with wireless systems are: mass reduction, flexibility, and simplification of the Assembly, Integration and Tests phases (AIT). However, the Aerospace and Defense fields need high reliability solutions. The use of COTS (Commercial-Off-The- Shelf) parts in these fields require extensive analyses in order to attain full product assurance. The current commercial optical wireless technology needs a deep transformation in order to be fully applicable in the aforementioned fields. Finally, major breakthroughs for the implementation of optical wireless links in Space will not be possible until dedicated circuits such as mixed analog/digital ASICs are developed. Once these products become available, it will also be possible to extend optical wireless links to other applications, such as Unmanned Air and Underwater Vehicles (UAV and UUV). The steps taken by INTA to introduce Optical Wireless Links in the Space environment are presented in this paper.
Acceso Abierto
Radiation and Dust Sensor for Mars Environmental Dynamic Analyzer Onboard M2020 Rover
(Multidisciplinary Digital Publishing Institute (MDPI), 2022-04-10) Jiménez, J. J.; Boland, J.; Lemmon, M. T.; García Menéndez, Elisa; Rivas, J.; Azcue, J.; Bastide, L.; Andrés Santiuste, N.; Martínez Oter, J.; González Guerrero, M.; Toledo, D.; Álvarez Rios, F. J.; Serrano, F.; Martín Vodopivec, B.; Manzano, J.; López Heredero, R.; Carrasco, I.; Aparicio, S.; Carretero, Á.; MacDonald, D. R.; Moore, L. B.; Alcacera Gil, María Ángeles; Fernández Viguri, J. A.; Martín, I.; Yela González, M.; Álvarez, M.; Manzano, P.; Martín, J. A.; Reina, M.; Urquí, R.; Rodríguez Manfredi, J. A.; De la Torre Juárez, M.; Córdoba, E.; Leiter, R.; Thompson, A.; Madsen, S.; Smith, M. D.; Viúdez Moreiras, Daniel; Saix López, A.; Sánchez Lavega, A.; Apéstigue, Víctor; Gómez Martín, L.; Gonzalo Melchor, Alejandro; Martínez, G. M.; de Mingo Martín, José Ramón; Gómez Elvira, J.; Martín-Ortega, Alberto; Arruego, I.; del Hoyo Gordillo, Juan Carlos; Martín-Ortega, Alberto; González Hernández, Carmen; Martín-Ortega, Alberto; Instituto Nacional de Técnica Aeroespacial (INTA); Comunidad de Madrid; Gobierno Vasco; Ministerio de Economía y Competitividad (MINECO); Agencia Estatal de Investigación (AEI); National Aeronautics and Space Administration (NASA)
The Radiation and Dust Sensor is one of six sensors of the Mars Environmental Dynamics Analyzer onboard the Perseverance rover from the Mars 2020 NASA mission. Its primary goal is to characterize the airbone dust in the Mars atmosphere, inferring its concentration, shape and optical properties. Thanks to its geometry, the sensor will be capable of studying dust-lifting processes with a high temporal resolution and high spatial coverage. Thanks to its multiwavelength design, it will characterize the solar spectrum from Mars’ surface. The present work describes the sensor design from the scientific and technical requirements, the qualification processes to demonstrate its endurance on Mars’ surface, the calibration activities to demonstrate its performance, and its validation campaign in a representative Mars analog. As a result of this process, we obtained a very compact sensor, fully digital, with a mass below 1 kg and exceptional power consumption and data budget features.
Acceso Abierto
The athena x-ray integral field unit: a consolidated design for the system requirement review of the preliminary definition phase
(Springer Link, 2022-08-30) Barret, Didier; Albouys, Vincent; Herderm Jan-Willem den; Piro, Luigi; Cappi, Massimo; Huovelin, Juhani; Kelley, Richard; Mas-Hesse, J. Miguel; Paltani, Stéphane; Rauw, Gregor; Rozanska, Agata; Fiore, Fabrizio; Bonny, Patrick; Boorman, Peter; Boreux, Charles; Bounab, Ayoub; Cuttaia, Francesco; Gabici, Stefano; Boutelier, Martin; Boyce, Kevin; Molin, Alexeï; Etcheverry, Christophe; Brienza, Daniele; Bruijn, Marcel; Bandler, Simon; Puccio, Elena; Bulgarelli, Andrea; Calarco, Simona; Callanan, Paul; D'Ai, Antonino; Camus, Thierry; Canourgues, Florent; Branduardi-Raymont, Graziella; Cavazzuti, Elisabetta; Gant, Florent; Capobianco, Vito; Cardiel, Nicolás; Castellani, Florent; Cheatom, Oscar; Pascale, Ramon; Chervenak, James; D'anca, Fabio; Gastaldello, Fabio; Ettori, Stefano; Dadina, Mauro; Barbera, Marco; Daniel, Christophe; Peille, Philippe; Gloaguen, Emilie; DeNigris, Natalie; Dercksen, Johannes; DiPirro, Michael; Doumayrou, Eric; Dubbeldam, Luc; Finoguenov, Alexis; Bozzo , Enrico; Dupieux, Michel; Monestes, David; Genolet, Ludovic; Ghizzardi, Simona; Plaa, Jelle de; Alcacera Gil, María Ángeles; Dupourqué, Simon; Giovannini, Elisa; Durkin, Malcom; Grosso, Nicolas; Charles, Ivan; Godet, Olivier; Gómez Elvira, J.; Montinaro, Nicola; González, Manuel; González, Raoul; Gottardi, Luciano; Ardellier, Florence; Granat, Dolorès; Gros, Michel; Pinsard, Frederic; Rioland, Guillaume; Guignard, Nicolas; Hieltjes, Paul; Fioretti, Valentina; Mot, Baptiste; Hurtado, Adolfo Jesus; Costantini, Elisa; Irwin, Kent; Jacquey, Christian; Argan, Andrea; Van der Kuur, Jan; Janiuk, Agnieszka; Jaubert, Jean; Rodriguez, Louis; Jolly, Antoine; Smith, Stephen; Jourdan, Thierry; Julien, Sabine; Geoffray, Hervé; Kedziora, Bartosz; Kaastra, Jelle; Korb, Andrew; Van Leeuwen, Bert-Joost; Dauser, Thomas; Kreykenbohm, Ingo; König, Ole; Langer, Mathieu; Murat, David; Roig, Anton; Laudet, Philippe; Laurent, Philippe; Mazzotta, Pasquale; Laurenza, Monica; Lesrel, Jean; Jacques, Lionel; Bellouard, Elise; Ligori, Sebastiano; Lorenz, Maximilian; Luminari, Alfredo; Nagayoshi, Kenichiro; Decourchelle, Anne; Maffei, Bruno; Colonges, Stéphane; Rollet, Bertrand; Maisonnave, Océane; Marelli, Lorenzo; Massonet, Didier; Maussang, Irwin; Carron, Jérôme; Nazé, Yaël; Roudil, Gilles; Noguès, Loïc; Kirsch, Christian; Pailot, Damien; Chiarello, Fabio; Fossecave, Hervé; Duval, Jean-Marc; Panessa, Francesca; Parodi, Luigi; Petit, Pascal; Piconcelli, Enrico; Adams, Joseph; Pinto, Ciro; Miller, Jon; Rudnicki, Tomasz; Gatti, Flavio; Clerc, Nicolas; Sanisidro, Julien; Encinas Plaza, José Miguel; Sciortino, Luisa; Durand, Jean Louis; Hoogeveen, Ruud; Silva, Vitor; Sordet, Michael; Miniutti, Giovanni; Soto Aguilar, Javier; Spizzi, Pierre; Surace, Christian; Clerc, Laurent; Fernández Sánchez, Miguel; Taralli, Emanuele; Fiorini, Mauro; Goldwurm, Andrea; Hartog, Roland den; Eckert, Dominique; Nicastro, Fabrizio; Jackson, Brian; Svoboda, Jiri; Jonker, Peter; Kilbourne, Caroline; Cobo, Beatriz; Korpela, Seppo; Macculi, Claudio; Mendez, Mariano; Khosropanah, Pourya; Mitsuda, Kazuhisa; Finkbeiner, Fred; Molendi, Silvano; Pajot, François; Eiriz, Valvanera; Pointecouteau, Etienne; Porter, Frederick; Gao, Jian-Rong; Van der Hulst, Paul; Pratt, Gabriel W.; Prêle, Damien; Ravera, Laurent; Sciortino, Salvatore; Martin, Sylvain; Sato, Kosuke; Schaye, Joop; Shinozaki, Keisuke; Skup, Konrad; Ercolani, Eric; Coeur-Joly, Odile; Soucek, Jan; Thibert, Tanguy; Vink, Jacco; Yamaguchi, Hiroya; Kiviranta, Mikko; Webb, Natalie; Perry, James; Chaoul, Laurence; Raulin, Desi; Simionescu, Aurora; Torrejón, José Miguel; Coleiro, Alexis; Acero, Fabio; Beaumont, Sophie; Pradines, Alice; Cucchetti, Edoardo; D'Andrea, Matteo; Le Mer, Isabelle; Reina, M.; Ledot, Aurélien; Eckart, Megan; Ferrando, Philippe; Kammoun, Elias; Lotti, Simone; Fiocchi, Maria Teresa; Mesnager, Jean-Michel; Rigano, Manuela; Van Loon, Dennis; Michalski, Lea; Roelfsema, Peter; Natalucci, Lorenzo; Schwander, Denis; Poyatos Martínez, D.; Ceballos, Maria Teresa; Torrioli, Guido; Ullom, Joel; Medinaceli Villegas, Eduardo; Zuchniak, Monika; Millerioux, Jean-Pierre; Brachet, Frank; Lo Cicero, Ugo; Corcione, Leonardo; Lyautey, Bertrand; Parot, Yann; Prouvé, Thomas; Sakai, Kazuhiro; Doriese, William; Weers, Henk van; Wilms, Joern; Mineo, Teresa; Abdoelkariem, Shariefa; Adam, Thomas; Adami, Christophe; Coriat, Mickael; Aicardi, Corinne; Akamatsu, Hiroki; Merino Alonso, Pablo Eleazar; Ptak, Andy; Amato, Roberta; André, Jérôme; Roncarelli, Mauro; Franssen, Philippe; Angelinelli, Matteo; Añón Cancela, M.; Yamasaki, Noriko; Coynel, Alexandre; Anvar, Shebli; Atienza, R.; Attard, Anthony; Auricchio, Natalia; Puccetti, Simonetta; Duband, Lionel; Balado, A.; Bancel, Florian; Ferrari Barusso, Lorenzo; Frericks, Martin; Bernard, Vivian; Barcons, Xavier; Berrocal, A.; Blin, Sylvie; Audard, Marc; Bonino, Donata; Minervini, Gabriele; Bonnet, François; Jiménez, María; Gonzalo Melchor, Alejandro; VERA TRALLERO, ISABEL; Agencia Estatal de Investigación (AEI); Ministerio de Ciencia e Innovación (MICINN); Centre National D'Etudes Spatiales (CNES); Agenzia Spaziale Italiana (ASI); European Space Agency (ESA)
The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer, studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory, a versatile observatory designed to address the Hot and Energetic Universe science theme, selected in November 2013 by the Survey Science Committee. Based on a large format array of Transition Edge Sensors (TES), it aims to provide spatially resolved X-ray spectroscopy, with a spectral resolution of 2.5 eV (up to 7 keV) over an hexagonal field of view of 5 arc minutes (equivalent diameter). The X-IFU entered its System Requirement Review (SRR) in June 2022, at about the same time when ESA called for an overall X-IFU redesign (including the X-IFU cryostat and the cooling chain), due to an unanticipated cost overrun of Athena. In this paper, after illustrating the breakthrough capabilities of the X-IFU, we describe the instrument as presented at its SRR, browsing through all the subsystems and associated requirements. We then show the instrument budgets, with a particular emphasis on the anticipated budgets of some of its key performance parameters. Finally we briefly discuss on the ongoing key technology demonstration activities, the calibration and the activities foreseen in the X-IFU Instrument Science Center, and touch on communication and outreach activities, the consortium organisation, and finally on the life cycle assessment of X-IFU aiming at minimising the environmental footprint, associated with the development of the instrument. Thanks to the studies conducted so far on X-IFU, it is expected that along the design-to-cost exercise requested by ESA, the X-IFU will maintain flagship capabilities in spatially resolved high resolution X-ray spectroscopy, enabling most of the original X-IFU related scientific objectives of the Athena mission to be retained.