209 results on '"Lopes, R. M."'
Search Results
2. AVALIAÇÃO DA ROTULAGEM DE DIFERENTES MARCAS DE PRODUTOS LÁCTEOS
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Pontes, E. D. S., primary, Rodrigues, M. G. D. S., additional, Lopes, R. M. M., additional, Silva, H. M. F. N., additional, Saraiva, P. C. A., additional, Silva, E. C., additional, and Nascimento, J. A. S., additional
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- 2022
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3. The temporal variability of Io's hotspots.
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Mura, A., Zambon, F., Tosi, F., Lopes, R. M. C., Rathbun, J., Pettine, M., Adriani, A., Altieri, F., Ciarniello, M., Cicchetti, A., Filacchione, G., Grassi, D., Noschese, R., Migliorini, A., Piccioni, G., Plainaki, C., Sordini, R., Sindoni, G., Turrini, D., and Radebaugh, Jani
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INFRARED imaging ,INFRARED spectra ,JUPITER (Planet) ,AURORAS ,ORBITS (Astronomy) - Abstract
We investigate the variability of the power emission of Io's hotspots by using recent Juno/JIRAM infrared observations. The Jovian Infrared Auroral Mapper (JIRAM) is an imaging spectrometer which began observing Jupiter in August 2016. Although observing Jupiter's moons is not its primary objective, JIRAM can use the frequent opportunities to observe Io (up to once per orbit) to gather infrared images and spectra of its surface. The present study uses the data acquired by JIRAM during the last 2 years, including the location and morphology of Io's hotspots, and the temporal variability of the total output. A new photometric model for the hotspots and the dayside surface has been developed, which permits us to disentangle the temporal variability from the changes in the observation geometry. While the latitudinal dependence of the power output is not well constrained, low-latitude hotspots show a significantly more intense temporal variability and greater temperature. [ABSTRACT FROM AUTHOR]
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- 2024
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4. JIRAM Observations of Volcanic Flux on Io: Distribution and Comparison to Tidal Heat Flow Models.
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Pettine, M., Imbeah, S., Rathbun, J., Hayes, A., Lopes, R. M. C., Mura, A., Tosi, F., Zambon, F., and Bertolino, S.
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GRAVITATIONAL interactions ,INFRARED cameras ,SOLAR system ,VOLCANOES ,HARMONIC analysis (Mathematics) - Abstract
Juno has allowed clear, high‐resolution imaging of Io's polar volcanoes using the Jovian Infrared Auroral Mapper (JIRAM) instrument. We have used data from JIRAM's M‐band (4.78 μm) imager from 11 Juno orbits to construct a global map of volcanic flux. This map provides short‐term insight into the spatial distribution of volcanoes and the ways in which high‐ and low‐latitude volcanoes differ. Using spherical harmonic analysis, we quantitatively compare our volcanic flux map to the surface heat flow distribution expected from models of Io's tidal heat deposition (summarized in de Kleer, Park, et al. (2019, https://doi.org/10.26206/d4wc‐6v82). Our observations confirm previously detected systems of bright volcanoes at high latitudes. Our study finds that both poles are comparably active and that the observed flux distribution is inconsistent with an asthenospheric heating model, although the south pole is viewed too infrequently to establish reliable trends. Plain Language Summary: Our study uses data from an infrared camera on Juno called the Jovian Infrared Auroral Mapper (JIRAM) to image Io, the innermost Galilean moon of Jupiter. Io is the most volcanically active body in the Solar System. Io's volcanoes are powered by both the extreme tides from Jupiter and the gravitational interactions between it and Jupiter's other moons. These tides generate friction inside Io. Simulations of Io's interior suggest that, depending on how deep that friction is being generated, the surface heat flow will be higher in certain areas (de Kleer, Park, et al., 2019, https://doi.org/10.26206/d4wc‐6v82). Using JIRAM, we have mapped where volcanoes are producing the most power and compared that to where we expect higher heat flow from the interior models. Our map doesn't agree with any of these models very well. JIRAM observed more volcanic activity at the poles than we expected to see based on previous observations. However, since the south pole was only observed twice, it's possible that these observations don't represent the average volcanic activity of the south pole. Very bright volcanoes that may have been continuously active for decades were also imaged during these Juno fly‐bys, some of which are nearer the poles than the equator. Key Points: We have produced a global volcanic flux map of Io using data from 11 Juno fly‐bysOur flux map doesn't agree well with tidal heat flow models reported in de Kleer, Park, et al. (2019, https://doi.org/10.26206/d4wc‐6v82)The M‐band flux is anti‐correlated with the asthenospheric heating model and has only very weak agreement with the global magma ocean model [ABSTRACT FROM AUTHOR]
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- 2024
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5. A global geomorphologic map of Saturn’s moon Titan
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Lopes, R. M. C., Malaska, M. J., Schoenfeld, A. M., Solomonidou, A., Birch, S. P. D., Florence, M., Hayes, A. G., Williams, D. A., Radebaugh, J., Verlander, T., Turtle, E. P., Le Gall, A., and Wall, S. D.
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- 2020
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6. Predicting Knee Angles from Video: An Initial Experiment with Machine Learning
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Guimarães, I. J. A., Lopes, R. M., Junior, J. F. L. S., Sousa, B. S., Marães, V. R. F. S., Brasil, L. M., Magjarevic, Ratko, Series Editor, Ładyżyński, Piotr, Associate Editor, Ibrahim, Fatimah, Associate Editor, Lackovic, Igor, Associate Editor, Rock, Emilio Sacristan, Associate Editor, Costa-Felix, Rodrigo, editor, Machado, João Carlos, editor, and Alvarenga, André Victor, editor
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- 2019
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7. Er,Cr:YSGG laser associated with acidulated phosphate fluoride gel (1.23% F) for prevention and control of dentin erosion progression
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Bezerra, S. J. C., Trevisan, L. R., Viana, I. E. L., Lopes, R. M., Pereira, D. L., Aranha, A. C. C., and Scaramucci, Taís
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- 2019
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8. Cassini Encounters Enceladus: Background and the Discovery of a South Polar Hot Spot
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Spencer, J. R., Pearl, J. C., Segura, M., Flasar, F. M., Mamoutkine, A., Romani, P., Buratti, B. J., Hendrix, A. R., Spilker, L. J., and Lopes, R. M. C.
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- 2006
9. Predicting Knee Angles from Video: An Initial Experiment with Machine Learning
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Guimarães, I. J. A., primary, Lopes, R. M., additional, Junior, J. F. L. S., additional, Sousa, B. S., additional, Marães, V. R. F. S., additional, and Brasil, L. M., additional
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- 2019
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10. Titan as Revealed by the Cassini Radar
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Lopes, R. M. C., Wall, S. D., Elachi, C., Birch, S. P. D., Corlies, P., Coustenis, A., Hayes, A. G., Hofgartner, J. D., Janssen, M. A., Kirk, R. L., LeGall, A., Lorenz, R. D., Lunine, J. I., Malaska, M. J., Mastroguiseppe, M., Mitri, G., Neish, C. D., Notarnicola, C., Paganelli, F., Paillou, P., Poggiali, V., Radebaugh, J., Rodriguez, S., Schoenfeld, A., Soderblom, J. M., Solomonidou, A., Stofan, E. R., Stiles, B. W., Tosi, F., Turtle, E. P., West, R. D., Wood, C. A., Zebker, H. A., Barnes, J. W., Casarano, D., Encrenaz, P., Farr, T., Grima, C., Hemingway, D., Karatekin, O., Lucas, A., Mitchell, K. L., Ori, G., Orosei, R., Ries, P., Riccio, D., Soderblom, L. A., and Zhang, Z.
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- 2019
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11. Io Hot Spot Distribution Detected by Juno/JIRAM
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Zambon, F., primary, Mura, A., additional, Lopes, R. M. C., additional, Rathbun, J., additional, Tosi, F., additional, Sordini, R., additional, Noschese, R., additional, Ciarniello, M., additional, Cicchetti, A., additional, Adriani, A., additional, Agostini, L., additional, Filacchione, G., additional, Grassi, D., additional, Piccioni, G., additional, Plainaki, C., additional, Sindoni, G., additional, Turrini, D., additional, Brooks, S., additional, Hansen‐Koharcheck, C., additional, and Bolton, S., additional
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- 2023
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12. Geomorphological Map of the Soi Crater Region on Titan
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Schoenfeld, A. M., primary, Solomonidou, A., additional, Malaska, M. J., additional, Lopes, R. M. C., additional, Birch, S. P. D., additional, Le Mouélic, S., additional, Florence, M., additional, Verlander, T., additional, Wall, S. D., additional, and Elachi, C., additional
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- 2023
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13. The Subtropical Estuarine Complex of Paranaguá Bay, Brazil
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Lana, P. C., Marone, E., Lopes, R. M., Machado, E. C., Caldwell, M. M., editor, Heldmaier, G., editor, Lange, O. L., editor, Mooney, H. A., editor, Schulze, E.-D., editor, Sommer, U., editor, Seeliger, Ulrich, editor, and Kjerfve, Björn, editor
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- 2001
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14. Titan's Cold Case Files - Outstanding Questions After Cassini-Huygens
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Nixon, C. A, Lorenz, R. D, Achterberg, R. K, Buch, A, Coll, P, Clark, R. N, Courtin, R, Hayes, A, Less, L, Johnson, R. E, Lopes, R. M. C, Mastrogiuseppe, M, Mandt, K, Mitchell, D. G, Raulin, F, Rymer, A. M, Todd Smith, H, Solomonidou, A, Sotin, C, Turtle, E. P, Vuitton, V, West, R. A, and Yelle, R. V
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Lunar And Planetary Science And Exploration - Abstract
The entry of the Cassini-Huygens spacecraft into orbit around Saturn in July 2004 marked the start of a golden era in the exploration of Titan, Saturn's giant moon. During the prime mission (2004-2008), ground-breaking discoveries were made by the Cassini orbiter including the equatorial dune fields (flyby T3, 2005), northern lakes and seas (T16, 2006), and the large positive and negative ions (T16 & T18, 2006), to name a few. In 2005 the Huygens probe descended through Titan's atmosphere, taking the first close-up pictures of the surface, including large networks of dendritic channels leading to a dried-up seabed, and also obtaining detailed profiles of temperature and gas composition during the atmospheric descent. The discoveries continued through the Equinox mission (2008-2010) and Solstice mission (2010-2017) totaling 127 targeted flybys of Titan in all. Now at the end of the mission, we are able to look back on the high-level scientific questions from the start of the mission, and assess the progress that has been made towards answering these. At the same time, new scientific questions regarding Titan have emerged from the new discoveries that have been made. In this paper we review a cross-section of important scientific questions that remain partially or completely unanswered, ranging from Titan's deep interior to the exosphere. Our intention is to help formulate the science goals for the next generation of planetary missions to Saturn and Titan, and to stimulate new experimental, observation and theoretical investigations in the interim, before such missions arrive again at Titan.
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- 2018
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15. Rapid and Extensive Surface Changes Near Titan's Equator: Evidence of April Showers
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Turtle, E. P., Perry, J. E., Hayes, A. G., Lorenz, R. D., Barnes, J. W., McEwen, A. S., West, R. A., Del Genio, A. D., Barbara, J. M., Lunine, J. I., Schaller, E. L., Ray, T. L., Lopes, R. M. C., and Stofan, E. R.
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- 2011
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16. Corrigendum: The temporal variability of Io's hotspots.
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Mura, A., Zambon, F., Tosi, F., Lopes, R. M. C., Rathbun, J., Pettine, M., Adriani, A., Altieri, F., Ciarniello, M., Cicchetti, A., Filacchione, G., Grassi, D., Noschese, R., Migliorini, A., Piccioni, G., Plainaki, C., Sordini, R., Sindoni, G., and Turrini, D.
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JUNO (Space probe) ,JUPITER (Planet) ,AURORAS ,REFERENCE books ,PUBLISHED articles - Abstract
The document is a corrigendum for an article on Io's hotspots, correcting references to various studies and authors. The corrections ensure accurate citations and do not impact the scientific conclusions of the original article. The authors are from various institutions in Italy, the United States, and other countries, emphasizing international collaboration in space research. [Extracted from the article]
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- 2024
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17. Io Volcanism Seen by New Horizons: A Major Eruption of the Tvashtar Volcano
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Spencer, J. R., Stern, S. A., Cheng, A. F., Weaver, H. A., Reuter, D. C., Retherford, K., Lunsford, A., Moore, J. M., Abramov, O., Lopes, R. M. C., Perry, J. E., Kamp, L., Showalter, M., Jessup, K. L., Marchis, F., Schenk, P. M., and Dumas, C.
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- 2007
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18. Io's Atmospheric Response to Eclipse: UV Aurorae Observations
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Retherford, K. D., Spencer, J. R., Stern, S. A., Saur, J., Strobel, D. F., Steffl, A. J., Gladstone, G. R., Weaver, H. A., Cheng, A. F., Parker, J. Wm., Slater, D. C., Versteeg, M. H., Davis, M. W., Bagenal, F., Throop, H. B., Lopes, R. M. C., Reuter, D. C., Lunsford, A., Conard, S. J., Young, L. A., and Moore, J. M.
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- 2007
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19. Surface, Subsurface and Atmosphere Exchanges on the Satellites of the Outer Solar System
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Tobie, G., Giese, B., Hurford, T. A., Lopes, R. M., Nimmo, F., Postberg, F., Retherford, K. D., Schmidt, J., Spencer, J. R., Tokano, T., and Turtle, E. P.
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- 2010
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20. Atmospheric/Exospheric Characteristics of Icy Satellites
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Coustenis, A., Tokano, T., Burger, M. H., Cassidy, T. A., Lopes, R. M., Lorenz, R. D., Retherford, K. D., and Schubert, G.
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- 2010
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21. TandEM: Titan and Enceladus mission
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Coustenis, A., Atreya, S. K., Balint, T., Brown, R. H., Dougherty, M. K., Ferri, F., Fulchignoni, M., Gautier, D., Gowen, R. A., Griffith, C. A., Gurvits, L. I., Jaumann, R., Langevin, Y., Leese, M. R., Lunine, J. I., McKay, C. P., Moussas, X., Müller-Wodarg, I., Neubauer, F., Owen, T. C., Raulin, F., Sittler, E. C., Sohl, F., Sotin, C., Tobie, G., Tokano, T., Turtle, E. P., Wahlund, J.-E., Waite, J. H., Baines, K. H., Blamont, J., Coates, A. J., Dandouras, I., Krimigis, T., Lellouch, E., Lorenz, R. D., Morse, A., Porco, C. C., Hirtzig, M., Saur, J., Spilker, T., Zarnecki, J. C., Choi, E., Achilleos, N., Amils, R., Annan, P., Atkinson, D. H., Bénilan, Y., Bertucci, C., Bézard, B., Bjoraker, G. L., Blanc, M., Boireau, L., Bouman, J., Cabane, M., Capria, M. T., Chassefière, E., Coll, P., Combes, M., Cooper, J. F., Coradini, A., Crary, F., Cravens, T., Daglis, I. A., de Angelis, E., de Bergh, C., de Pater, I., Dunford, C., Durry, G., Dutuit, O., Fairbrother, D., Flasar, F. M., Fortes, A. D., Frampton, R., Fujimoto, M., Galand, M., Grasset, O., Grott, M., Haltigin, T., Herique, A., Hersant, F., Hussmann, H., Ip, W., Johnson, R., Kallio, E., Kempf, S., Knapmeyer, M., Kofman, W., Koop, R., Kostiuk, T., Krupp, N., Küppers, M., Lammer, H., Lara, L.-M., Lavvas, P., Le Mouélic, S., Lebonnois, S., Ledvina, S., Li, J., Livengood, T. A., Lopes, R. M., Lopez-Moreno, J.-J., Luz, D., Mahaffy, P. R., Mall, U., Martinez-Frias, J., Marty, B., McCord, T., Menor Salvan, C., Milillo, A., Mitchell, D. G., Modolo, R., Mousis, O., Nakamura, M., Neish, C. D., Nixon, C. A., Nna Mvondo, D., Orton, G., Paetzold, M., Pitman, J., Pogrebenko, S., Pollard, W., Prieto-Ballesteros, O., Rannou, P., Reh, K., Richter, L., Robb, F. T., Rodrigo, R., Rodriguez, S., Romani, P., Ruiz Bermejo, M., Sarris, E. T., Schenk, P., Schmitt, B., Schmitz, N., Schulze-Makuch, D., Schwingenschuh, K., Selig, A., Sicardy, B., Soderblom, L., Spilker, L. J., Stam, D., Steele, A., Stephan, K., Strobel, D. F., Szego, K., Szopa, C., Thissen, R., Tomasko, M. G., Toublanc, D., Vali, H., Vardavas, I., Vuitton, V., West, R. A., Yelle, R., and Young, E. F.
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- 2009
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22. Fluvial Features on Titan and Earth: Lessons from Planform Images in Low-resolution SAR
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Miller, J. W., primary, Birch, S. P. D., additional, Hayes, A. G., additional, Malaska, M. J., additional, Lopes, R. M. C., additional, Schoenfeld, A. M., additional, Corlies, P. M., additional, Burr, D. M., additional, Farr, T. G., additional, and Perron, JT, additional
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- 2021
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23. Titan as Revealed by the Cassini Radar
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Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences, Lopes, R. M C, Wall, S. D, Elachi, C., Birch, S. P D, Corlies, P., Coustenis, A., Hayes, A. G, Hofgartner, J. D, Janssen, M. A, Kirk, R. L, LeGall, A., Lorenz, R. D, Lunine, J. I, Malaska, M. J, Mastroguiseppe, M., Mitri, G., Neish, C. D, Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences, Lopes, R. M C, Wall, S. D, Elachi, C., Birch, S. P D, Corlies, P., Coustenis, A., Hayes, A. G, Hofgartner, J. D, Janssen, M. A, Kirk, R. L, LeGall, A., Lorenz, R. D, Lunine, J. I, Malaska, M. J, Mastroguiseppe, M., Mitri, G., and Neish, C. D
- Abstract
Titan was a mostly unknown world prior to the Cassini spacecraft’s arrival in July 2004. We review the major scientific advances made by Cassini’s Titan Radar Mapper (RADAR) during 13 years of Cassini’s exploration of Saturn and its moons. RADAR measurements revealed Titan’s surface geology, observed lakes and seas of mostly liquid methane in the polar regions, measured the depth of several lakes and seas, detected temporal changes on its surface, and provided key evidence that Titan contains an interior ocean. As a result of the Cassini mission, Titan has gone from an uncharted world to one that exhibits a variety of Earth-like geologic processes and surface-atmosphere interactions. Titan has also joined the ranks of “ocean worlds” along with Enceladus and Europa, which are prime targets for astrobiological research.
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- 2021
24. Titan's surface geology
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Aharonson, O., primary, Hayes, A. G., additional, Hayne, P. O., additional, Lopes, R. M., additional, Lucas, A., additional, and Perron, J. T., additional
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- 2014
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25. The science enabled by a dedicated solar system space telescope
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Young, Cindy, primary, Wong, M. H., additional, Sayanagi, K. M., additional, Curry, S., additional, Jessup, K. L., additional, Becker, T., additional, Hendrix, A., additional, Chanover, N., additional, Milam, S., additional, Holler, B. J., additional, Holsclaw, G., additional, Peralta, J., additional, Clarke, J., additional, Spencer, J., additional, Kelley, M. S. P., additional, Luhmann, J., additional, MacDonnell, D., additional, Jr., R. J. Vervack,, additional, Rutherford, K., additional, Fletcher, L. N., additional, Pater, I. de, additional, Vilas, F., additional, Feaga, L., additional, Siegmund, O., additional, Bell, J., additional, Delory, G., additional, Pitman, J., additional, Greathouse, T., additional, Wishnow, E., additional, Schneider, N., additional, Lillis, R., additional, Colwell, J., additional, Bowman, L., additional, Lopes, R. M. C., additional, McGrath, M., additional, Marchis, F., additional, Cartwright, R., additional, and Poston, M. J., additional
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- 2021
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26. Surface, Subsurface and Atmosphere Exchanges on the Satellites of the Outer Solar System
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Tobie, G., primary, Giese, B., additional, Hurford, T. A., additional, Lopes, R. M., additional, Nimmo, F., additional, Postberg, F., additional, Retherford, K. D., additional, Schmidt, J., additional, Spencer, J. R., additional, Tokano, T., additional, and Turtle, E. P., additional
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- 2010
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27. Atmospheric/Exospheric Characteristics of Icy Satellites
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Coustenis, A., primary, Tokano, T., additional, Burger, M. H., additional, Cassidy, T. A., additional, Lopes, R. M., additional, Lorenz, R. D., additional, Retherford, K. D., additional, and Schubert, G., additional
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- 2010
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28. Mapping Io's Surface Composition With Juno/JIRAM
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Tosi, F., primary, Mura, A., additional, Lopes, R. M. C., additional, Filacchione, G., additional, Ciarniello, M., additional, Zambon, F., additional, Adriani, A., additional, Bolton, S. J., additional, Brooks, S. M., additional, Noschese, R., additional, Sordini, R., additional, Turrini, D., additional, Altieri, F., additional, Cicchetti, A., additional, Grassi, D., additional, Hansen, C. J., additional, Migliorini, A., additional, Moriconi, M. L., additional, Piccioni, G., additional, Plainaki, C., additional, and Sindoni, G., additional
- Published
- 2020
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29. The chemical composition of impact craters on Titan
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Solomonidou, A., primary, Neish, C., additional, Coustenis, A., additional, Malaska, M., additional, Le Gall, A., additional, Lopes, R. M. C., additional, Werynski, A., additional, Markonis, Y., additional, Lawrence, K., additional, Altobelli, N., additional, Witasse, O., additional, Schoenfeld, A., additional, Matsoukas, C., additional, Baziotis, I., additional, and Drossart, P., additional
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- 2020
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30. Chatbots for Well-Being: Exploring the Impact of Artificial Intelligence on Mood Enhancement and Mental Health.
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Lopes, R. M., Silva, A. F., Rodrigues, A. C. A., and Melo, V.
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NATURAL language processing , *MENTAL health services , *ACCEPTANCE & commitment therapy , *CHATBOTS , *ARTIFICIAL intelligence , *MOTIVATIONAL interviewing , *DIALECTICAL behavior therapy - Abstract
Introduction: Over the past few years, Psychiatry has undergone a significant transformation with the integration of Artificial Intelligence (AI). This shift has been driven by the increasing demand for mental health services, as well as advances in AI technology. AI analyzes extensive datasets, including text, voice, and behavioral data, aiding in mental health diagnosis and treatment. Consequently, a range of AI-based interventions has been developed, including chatbots, virtual therapists and apps featuring cognitive-behavioral therapy (CBT) modules. Notably, chatbots, as conversational agents, have emerged as valuable tools, assisting users in monitoring emotions and providing evidence-based resources, well-being support, psychoeducation and adaptive coping strategies. Objectives: This study aims to investigate the impact of AI chatbots on improving mental health, evaluate their strengths and weaknesses and explore their potential for early detection and intervention in mental health issues. Methods: A literature review was conducted through PubMed and Google Scholar databases, using keywords 'artificial intelligence', 'chatbot' and 'mental health'. The selection focused on the most relevant articles published between January 2021 and September 2023. Results: Mental health chatbots are highly personalized, with a primary focus on addressing issues such as depression or anxiety within specific clinical population groups. Through the integration of Natural Language Processing (NLP) techniques and rule-based AI algorithms, these chatbots closely simulate human interactions and effectively instruct users in therapeutic techniques. While chatbots integrating CBT principles have gained widespread use and extensive research attention, some also incorporate alternative therapeutic approaches, including dialectical behavior therapy, motivational interviewing, acceptance and commitment therapy, positive psychology or mindfulness-based stress reduction. AI chatbots provide substantial advantages in terms of accessibility, cost-effectiveness and improved access to mental health support services. Nonetheless, they also exhibit limitations, including the absence of human connection, limited expertise, potential for misdiagnosis, privacy concerns, risk of bias and limitations in risk assessment accuracy. Conclusions: AI-based chatbots hold the potential to enhance patient outcomes by enabling early detection and intervention in mental health issues. However, their implementation in mental health should be approached with caution. Further studies are essential to thoroughly evaluate their effectiveness and safety. Disclosure of Interest: None Declared [ABSTRACT FROM AUTHOR]
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- 2024
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31. Exploring the associations between involuntary treatment and gender in a portuguese acute psychiatric unit.
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Silva, A. F., Lopes, R. M., Melo, V. S., Rodrigues, C. A., Coelho, P. M., Santos, F. M. A., Fernandes, I. S., and Delgado, L. P.
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MENTAL health services , *INVOLUNTARY hospitalization , *GENDER identity , *GENDER differences (Psychology) , *INVOLUNTARY treatment - Abstract
Introduction: Involuntary admission rates differ between gender across various countries. In several European Union countries, men are more frequently involuntarily admitted, while an opposite trend, associating women with involuntary care, has been observed in countries like Switzerland, Brazil, and China. Objectives: Considering the contradictory evidence about gender and involuntary care in the literature, we aim to analyze the gender patterns of involuntary care in Centro Hospitalar Médio Tejo's Psychiatric Acute Unit, exploring the gender differences in diagnosis among involuntary patients. Methods: We stored and analyzed the data using Microsoft Excel and IBM SPSS Statistics. We studied psychiatry admissions at Centro Hospitalar Médio Tejo, Portugal over 2 years. The Acute Psychiatric Unit, located within a general hospital, has 24 beds, and offers acute mental healthcare services to adults aged 18 and above, serving a coverage area of approximately 251,000 residents. As part of our data collection process for all admissions to the Acute Psychiatry Unit, we recorded information such as gender, age, diagnosis at discharge, treatment type (voluntary or involuntary), and length of stay. Results: From January 1, 2021, to December 31, 2022, there were 686 psychiatry admissions at Centro Hospitalar Médio Tejo, of which 125 (18,2%) were involuntary. The admission rates were approximately 136.6 per 100,000 people annually, with 24.9 being involuntary admissions per 100,000 people annually. In our analysis of involuntary admissions, women had a lower rate of such admissions, making up 6.4%, while men had a higher rate at 11.8%. No other gender identity was mentioned. Schizophrenia-related disorders were the primary cause for involuntary admissions for both genders, with 67.9% for men and 50% for women. Mood disorders were the second most common reason for involuntary admission, accounting for around 40.9% of cases for women and a significantly lower 16% for men. Involuntarily hospitalized patients exhibited longer lengths of stay independently of the gender. Men hospitalized involuntarily tended to be younger, whereas for women, involuntary hospitalizations were associated with older ages. Conclusions: In conclusion, our study reveals gender differences in psychiatric involuntary admissions, with more men being involuntarily admitted than women. Schizophrenia group disorders were the most common diagnoses among male and female involuntary patients. Furthermore, all hospitalized women exhibited a higher prevalence of mood disorders, a trend that was more pronounced among those admitted involuntarily. These gender trends match the overall patterns seen in the epidemiology of schizophrenia and mood disorders. Additionally, women with schizophrenia generally exhibit better social functioning than men, which may explain the lower needs of involuntary hospitalization. Disclosure of Interest: None Declared [ABSTRACT FROM AUTHOR]
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- 2024
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32. The chemical composition of impact craters on Titan : I. Implications for exogenic processing
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Solomonidou, A., Neish, C., Coustenis, A., Malaska, M., Le Gall, A., Lopes, R. M. C., Werynski, A., Markonis, Y., Lawrence, K., Altobelli, N., Witasse, O., Schoenfeld, A., Matsoukas, Christos, Baziotis, I., Drossart, P., Solomonidou, A., Neish, C., Coustenis, A., Malaska, M., Le Gall, A., Lopes, R. M. C., Werynski, A., Markonis, Y., Lawrence, K., Altobelli, N., Witasse, O., Schoenfeld, A., Matsoukas, Christos, Baziotis, I., and Drossart, P.
- Abstract
We investigate the spectral behavior of nine Titan impact craters in order to constrain their composition. Past studies that have examined the chemical composition of impact craters on Titan have either used qualitative comparisons between craters or combined all craters into a single unit, rather than separating them by geographic location and/or degradation state. Here, we use Visual and Infrared Mapping Spectrometer (VIMS) data and a radiative transfer code to estimate the atmospheric contribution to the data, extract the surface albedos of the impact craters, and constrain their composition by using a library of candidate Titan materials, including essentially water ice, tholin, a dark component, and other possible ices at different grain sizes. Following a general characterization of the impact craters, we study two impact crater subunits, the "crater floor" and the "ejecta blanket". The results show that the equatorial dune craters - Selk, Ksa, Guabonito, and the crater on Santorini Facula - appear to be purely composed of organic material (mainly an unknown dark component). Titan's midlatitude plain craters - Afekan, Soi, and Forseti - along with Menrva and Sinlap, are enriched in water ice within an organic-based mixture. This follows the geographic pattern observed in our previous work with VIMS data, where the uppermost layers of the midlatitude alluvial fans, undifferentiated plains, and labyrinth terrains were found to consist of a mixture of organics and water ice, while the equatorial plains, hummocky terrains, and dunes were found to consist of a mixture of dark material and tholins. Furthermore, we found that the addition of some form of ice improves the fit in the ejecta spectra of Afekan and Sinlap craters. We find no indication for the presence of either NH3 or CO2 ice. Our main results agree with an existing Titan surface evolution scenario, wherein the impact cratering process produces a mixture of organic material and water ice, which is later, QC 20201201
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- 2020
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33. Spectral and emissivity analysis of the raised ramparts around Titan's northern lakes
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Solomonidou, A., Le Gall, A., Malaska, M. J., Birch, S. P. D., Lopes, R. M. C., Coustenis, A., Rodriguez, S., Wall, S. D., Michaelides, R. J., Nasr, M. R., Elachi, C., Hayes, A. G., Soderblom, J. M., Schoenfeld, A. M., Matsoukas, Christos, Drossar, P., Janssen, M. A., Lawrence, K. J., Witasse, O., Yates, J., Radebaugh, J., Solomonidou, A., Le Gall, A., Malaska, M. J., Birch, S. P. D., Lopes, R. M. C., Coustenis, A., Rodriguez, S., Wall, S. D., Michaelides, R. J., Nasr, M. R., Elachi, C., Hayes, A. G., Soderblom, J. M., Schoenfeld, A. M., Matsoukas, Christos, Drossar, P., Janssen, M. A., Lawrence, K. J., Witasse, O., Yates, J., and Radebaugh, J.
- Abstract
Some of Titan's small northern hemisphere lakes show raised rampart features (which are distinct from raised rims), and appear as SAR-bright mound-like annuli extending away from the lake for up to tens of kilometers from the shoreline. We investigate the infrared and microwave characteristics of these features using Cassini Visual and Infrared Mapping Spectrometer (VIMS) and RADAR data. A spectral comparative analysis is performed among the lakes, their ramparts, and the surrounding regions. We overcome the profound difference in spatial resolution between VIMS and SAR data by using a method that provides overlays between the spectral images and SAR, thus enabling the correct selection of VIMS pixels. The surface properties of the selected areas are obtained using a radiative transfer analysis on the selected VIMS pixels, in addition to emissivity obtained from the RADAR in radiometry mode. Analysis of these combined and co-registered data provides constraints for the formation mechanism(s) of raised ramparts. The results show that the emissivity of the raised ramparts is close to that of Titan's labyrinthic terrains and to that of empty lake floors in the northern polar regions. This is confirmed by the VIMS analysis that also shows that the infrared spectral response of the raised ramparts is very similar to that of some empty lake floors. This suggests that both areas are made from or are covered by a similar material. In addition, two out of the eight lakes with raised ramparts show spectral differences at three specific wavelengths, 1.6, 2.0, and 5.0 mu m, between the ramparts and the surrounding terrain. We hypothesize that this could be due to some component, or mixture of components in the ramparts that is less absorbent at these specific wavelengths, or it could be an effect of different grain sizes. These observations provide first insights into the possible mechanisms leading to the formation of the raised ramparts that are discussed here., QC 20200713
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- 2020
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34. Identification of tetracyclic lactams as NMDA receptor antagonists with potential application in neurological disorders
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Fundação para a Ciência e a Tecnologia (Portugal), Ministerio de Ciencia, Innovación y Universidades (España), European Commission, Instituto de Salud Carlos III, Espadinha, Margarida, Viejo, L., Lopes, R. M. R. M., Herrera-Arozamena, Clara, Molins, E., dos Santos, D. J. V. A., Gonçalves, Lídia M., Rodríguez-Franco, María Isabel, Ríos, C. d. l., Santos, Maria M. M., Fundação para a Ciência e a Tecnologia (Portugal), Ministerio de Ciencia, Innovación y Universidades (España), European Commission, Instituto de Salud Carlos III, Espadinha, Margarida, Viejo, L., Lopes, R. M. R. M., Herrera-Arozamena, Clara, Molins, E., dos Santos, D. J. V. A., Gonçalves, Lídia M., Rodríguez-Franco, María Isabel, Ríos, C. d. l., and Santos, Maria M. M.
- Abstract
N-Methyl-D-aspartate receptors (NMDARs) are crucial for the normal function of the central nervous system (CNS), and fundamental in memory and learning-related processes. The overactivation of these receptors is associated with numerous neurodegenerative and psychiatric disorders. Therefore, NMDAR is considered a relevant therapeutic target for many CNS disorders. Herein, we report the synthesis and pharmacological evaluation of a new scaffold with antagonistic activity for NMDAR. Specifically, a chemical library of eighteen 1-aminoindan-2-ol tetracyclic lactams was synthesized and screened as NMDAR antagonists. The compounds were obtained by chiral pool synthesis using enantiomerically pure 1-aminoindan-2-ols as chiral inductors, and their stereochemistry was proven by X-ray crystallographic analysis of two target compounds. Most compounds reveal NMDAR antagonism, and eleven compounds display IC values in a Ca entry-sensitive fluo-4 assay in the same order of magnitude of memantine, a clinically approved NMDAR antagonist. Docking studies suggest that the novel compounds can act as NMDAR channel blockers since there is a compatible conformation with MK-801 co-crystallized with NMDAR channel. In addition, we show that the tetracyclic 1-aminoindan-2-ol derivatives are brain permeable and non-toxic, and we identify promising hits for further optimization as modulators of the NMDAR function.
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- 2020
35. Titan's Surface from Cassini RADAR SAR and High Resolution Radiometry Data of the First Five Flybys
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Paganelli, F, Janssen, M. A, Stiles, B, West, R, Lorenz, R. D, Lunine, J. I, Wall, S. D, Callahan, P, Lopes, R. M, Stofan, E, Kirk, R. L, Johnson, W. T. K, Roth, L, and Elachi, C
- Subjects
Communications And Radar - Abstract
The first five Titan flybys with Cassini's Synthetic Aperture RADAR (SAR) and radiometer are examined with emphasis on the calibration and interpretation of the high-resolution radiometry data acquired during the SAR mode (SAR-radiometry). Maps of the 2-cm wavelength brightness temperature are obtained coincident with the SAR swath imaging, with spatial resolution approaching 6 km. A preliminary calibration shows that brightness temperature in these maps varies from 64 to 89 K. Surface features and physical properties derived from the SAR-radiometry maps and SAR imaging are strongly correlated; in general, we find that surface features with high radar reflectivity are associated with radiometrically cold regions, while surface features with low radar reflectivity correlate with radiometrically warm regions. We examined scatterplots of the normalized radar cross-section sigma(exp o) versus brightness temperature, finding differing signatures that characterize various terrains and surface features. Implications for the physical and compositional properties of these features are discussed. The results indicate that volume scattering is important in many areas of Titan's surface, particularly Xanadu, while other areas exhibit complex brightness temperature variations consistent with variable slopes or surface material and compositional properties.
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- 2007
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36. Developments in the rat adjuvant arthritis model and its use in therapeutic evaluation of novel non-invasive treatment by SOD in Transfersomes
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Simões, S. I., Delgado, T. C., Lopes, R. M., Jesus, S., Ferreira, A. A., Morais, J. A., Cruz, M. E.M., Corvo, M. L., and Martins, M. B.F.
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- 2005
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37. Cryovolcanic Features on Titan's Surface as Revealed by the Cassini RADAR
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Lopes, R. M, Elachi, C, Stofan, E, Paganelli, F, Wood, C, Kirk, R, Lorenz, R, Fortes, A. D, and Lunine, J
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Lunar And Planetary Science And Exploration - Abstract
The Cassini Titan Radar Mapper obtained Synthetic Aperture radar images of about 1.1% of Titan's surface during the spacecraft s first targeted fly-by on October 26, 2004 (referred to as the Ta fly-by). These images revealed that Titan is very complex geologically. Features identified include a possible volcanic dome or shield, craters that appear to be of volcanic origin, and extensive flows. We will discuss these features and others that will likely be revealed during Cassini s T3 Titan fly-by of February 15, 2005, during which a swath covering comparable amount of the surface will be obtained. Additional information is included in the original extended abstract.
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- 2005
38. Channels and Fan-like Features on Titan Surface Imaged by the Cassini RADAR
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Paganelli, F, Elachi, C, Lopes, R. M, West, R, Stiles, B, Janssen, M. A, Stofan, E. R, Wood, C. A, Lorenz, R. D, and Lunine, J. L
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Lunar And Planetary Science And Exploration - Abstract
During two close flybys of Titan on October 26, 2004, and February 15, 2005, the Cassini s radar instrument acquired synthetic-aperture radar (SAR) data revealing Titan s complex surface and intriguing geological features. Fan-like and apparently flow-related features are connected to sinuous and linear features which resemble channels. The fan-like features and channels appear to be relatively SAR-bright and suggest surface roughness properties at the scale and bigger than the Ku-band, and possible volume scattering. A strong correlation between the SAR-bright and radiometric cold regions has been observed. The correlation is consistent with radiometric cold areas being caused by volume scattering at Ku as due to broken low-loss ice and resulting low emissivity as with the surfaces of Europa and Ganymede.
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- 2005
39. Characterization of Activity at Loki from Galileo and Ground-based Observations
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Howell, R. R and Lopes, R. M
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Geophysics - Abstract
While Loki is the most active volcanic center on Io, major questions remain concerning the nature of that activity. Rathbun et al. showed that the activity was semi-periodic, and suggested it was due to a resurfacing wave which swept across a lava lake as the crust cooled and become unstable. However in 2001 new observations showed that an intermediate level, less periodic mode of activity had apparently begun. Galileo-NIMS observations of Loki clearly show that the highest temperatures are found near the edge of the patera, consistent with disruption of a lava lake at the margins. NIMS observations also show gradients in temperature across the patera which, when modeled in terms of lava cooling models, are generally consistent with ages expected for the resurfacing wave but may also be consistent with spreading flows. We present a further analysis of NIMS data from I24 and I32 which help define the nature of the temperature variations present in Loki patera, along with Galileo-SSI images from the G1-I32 flybys which show albedo changes apparently correlated with the "periodic" activity measured from ground-based observations.
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- 2004
40. Caledras (Paterae) on Jupiter's moon Io
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Lopes, R. M. C, Kamp, L. W, Smythe, W. D, and Carlson, R. W
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- 2003
41. Baldur - a cold caldera on Io
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Smythe, W, Lopes, R. M. C, Carlson, R, and Doute, S
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- 2003
42. Mapping of the Culann-Tohil Region of Io
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Turtle, E. P, Keszthelyi, L. P, Jaeger, W. L, Radebaugh, J, Milazzo, M. P, McEwen, A. S, Moore, J. M, Schenk, P. M, and Lopes, R. M. C
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Lunar And Planetary Science And Exploration - Abstract
The Galileo spacecraft completed its observations of Jupiter's volcanic moon Io in October 2001 with the orbit I32 flyby, during which new local (13-55 m/pixel) and regional (130-400 m/pixel) resolution images and spectroscopic data were returned of the antijovian hemisphere. We have combined a I32 regional mosaic (330 m/pixel) with lower-resolution C21 color data (1.4 km/pixel, Figure 1) and produced a geomorphologic map of the Culann-Tohil area of this hemisphere. Here we present the geologic features, map units, and structures in this region, and give preliminary conclusions about geologic activity for comparison with other regions to better understand Io's geologic evolution.
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- 2003
43. Io's Thermal Regions and Non-SO2 Spectral Features
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Smythe, W. D, Soderblom, L. A, and Lopes, R. M. C
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Lunar And Planetary Science And Exploration - Abstract
Several absorptions have been identified in the Galileo NIMS spectra of Io that are not related to SO2. [1,2]. These absorptions have band centers at 2.97, 3.15, 3.85, and 3.91 microns. There are also broad absorptions in the regions 1-1.3 and 3- 3.4 microns. Patterning noise in wavelength registration, arising from the pushbroom imaging and grating motion of the NIMS instrument have previously inhibited reliable mapping of weak absorptions. Recent improvements in techniques to remove the coherent pattern noise from the NIMS dataset have been made by Soderblom. This greatly improves the signal to noise ratio and enables mapping of weak spectral signatures such as the 3.15 micron absorption on Io.
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- 2003
44. Night Time Observations of Io's Thermal Output from the Galileo Near Infrared Mapping Spectrometer
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Smythe, W. D, Lopes, R. M. C, Kamp, L. W, Leader, F, and Carlson, R. W
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Lunar And Planetary Science And Exploration - Abstract
The thermal output of Io is mapped using all nighttime observations obtained by Galileo NIMS. Additional information is contained in the original extended abstract.
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- 2002
45. Galileo's last fly-bys of Io: NIMS observation of Loki, Tupan, and Emakong
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Lopes, R. M. C, Kamp, L. W, Davies, A. G, Smythe, W. D, Carlson, R. W, Doute, S, McEwen, A, Turtle, E. P, Leader, F, Mehlman, R, Shirley, J, and Segura, M
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- 2002
46. Io's diverse styles of volcanic activity: Results from Galileo NIMS
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Geissler, P. E, McEwen, A. S, Carlson, R, Doute, S, Kamp, L. W, Smythe, W. D, and Lopes, R. M. C
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- 2001
47. Io's diverse styles of volcanic activity: Results from Galileo NIMS
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Lopes, R. M. C, Smythe, W. D, Kamp, L. W, Doute, S, Carlson, R, McEwen, A. S, and Geissler, P. E
- Abstract
The Near-Infrared Mapping Spectrometer on Galileo has observed Io since June 1996. In 1999 and 2000, the spacecraft made three close fly-bys to Io, revealing for the first time, the detailed thermal structure of some of Io's hot spots.
- Published
- 2001
48. A global geomorphologic map of Saturn’s moon Titan
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Lopes, R. M. C., primary, Malaska, M. J., additional, Schoenfeld, A. M., additional, Solomonidou, A., additional, Birch, S. P. D., additional, Florence, M., additional, Hayes, A. G., additional, Williams, D. A., additional, Radebaugh, J., additional, Verlander, T., additional, Turtle, E. P., additional, Le Gall, A., additional, and Wall, S. D., additional
- Published
- 2019
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49. Salivary cytokines and oral mucosa cells apoptosis in patients during hematopoietic cell transplantation: Possible relationship with oral mucositis
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Corrêa, L., primary, Bezinelli, L.M., additional, Rosin, F.C.P., additional, Ferreira, M.H., additional, Carvalho, D.L.C., additional, Lopes, R M D G, additional, Hamerschlak, N., additional, and Eduardo, F.D.P., additional
- Published
- 2019
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50. Globally Consistent Quantitative Observations of Planktonic Ecosystems
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Lombard, Fabien, Boss, Emmanuel, Waite, Anya, Vogt, Meike, Uitz, Julia, Stemman, Lars, Sosik, Heidi M., Schulz, Jan, Romagnan, J.-B., Picheral, Marc, Pearlman, Jay, Ohman, M. D., Niehoff, Barbara, Möller, Klas Ove, Miloslavich, Patricia, Lara-Lpez, A., Kudela, R., Lopes, R. M., Kiko, Rainer, Karp-Boss, Lee, Jaffe, J.S., Iversen, Morten, Irisson, J.-O., Fennel, K., Hauss, Helena, Guidi, Lionel, Gorsky, Gaby, Giering, Sarah L. C., Gaube, Peter, Gallager, Scott M., Dubelaar, G., Cowen, R.K., Carlotti, F., Briseno-Avena, C., Berline, Leo, Benoit-Bird, K., Bax, Nicholas J., Batten, Sonia Dawn, Ayata, Sakina-Dorothée, Artigas, L.F., Appeltans, Ward, Lombard, Fabien, Boss, Emmanuel, Waite, Anya, Vogt, Meike, Uitz, Julia, Stemman, Lars, Sosik, Heidi M., Schulz, Jan, Romagnan, J.-B., Picheral, Marc, Pearlman, Jay, Ohman, M. D., Niehoff, Barbara, Möller, Klas Ove, Miloslavich, Patricia, Lara-Lpez, A., Kudela, R., Lopes, R. M., Kiko, Rainer, Karp-Boss, Lee, Jaffe, J.S., Iversen, Morten, Irisson, J.-O., Fennel, K., Hauss, Helena, Guidi, Lionel, Gorsky, Gaby, Giering, Sarah L. C., Gaube, Peter, Gallager, Scott M., Dubelaar, G., Cowen, R.K., Carlotti, F., Briseno-Avena, C., Berline, Leo, Benoit-Bird, K., Bax, Nicholas J., Batten, Sonia Dawn, Ayata, Sakina-Dorothée, Artigas, L.F., and Appeltans, Ward
- Abstract
In this paper we review the technologies available to make globally quantitative observations of particles in general—and plankton in particular—in the world oceans, and for sizes varying from sub-microns to centimeters. Some of these technologies have been available for years while others have only recently emerged. Use of these technologies is critical to improve understanding of the processes that control abundances, distributions and composition of plankton, provide data necessary to constrain and improve ecosystem and biogeochemical models, and forecast changes in marine ecosystems in light of climate change. In this paper we begin by providing the motivation for plankton observations, quantification and diversity qualification on a global scale. We then expand on the state-of-the-art, detailing a variety of relevant and (mostly) mature technologies and measurements, including bulk measurements of plankton, pigment composition, uses of genomic, optical and acoustical methods as well as analysis using particle counters, flow cytometers and quantitative imaging devices. We follow by highlighting the requirements necessary for a plankton observing system, the approach to achieve it and associated challenges. We conclude with ranked action-item recommendations for the next 10 years to move toward our vision of a holistic ocean-wide plankton observing system. Particularly, we suggest to begin with a demonstration project on a GO-SHIP line and/or a long-term observation site and expand from there, ensuring that issues associated with methods, observation tools, data analysis, quality assessment and curation are addressed early in the implementation. Global coordination is key for the success of this vision and will bring new insights on processes associated with nutrient regeneration, ocean production, fisheries and carbon sequestration.
- Published
- 2019
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