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2. 3D Global climate model of an exo-Venus: a modern Venus-like atmosphere for the nearby super-Earth LP 890-9 c

Author

Quirino, Diogo, Gilli, Gabriella, Kaltenegger, Lisa, Navarro, Thomas, Fauchez, Thomas J., Turbet, Martin, Leconte, Jérémy, Lebonnois, Sébastien, and González-Galindo, Francisco

Subjects
Astrophysics - Earth and Planetary Astrophysics, Physics - Atmospheric and Oceanic Physics
Abstract

The recently discovered super-Earth LP 890-9 c is an intriguing target for atmospheric studies as it transits a nearby, low-activity late-type M-dwarf star at the inner edge of the Habitable Zone. Its position at the runaway greenhouse limit makes it a natural laboratory to study the climate evolution of hot rocky planets. We present the first 3D-GCM exo-Venus model for a modern Venus-like atmosphere (92 bar surface pressure, realistic composition, H$_2$SO$_4$ radiatively-active clouds), applied to the tidally-locked LP 890-9c to inform observations by JWST and future instruments. If LP 890-9 c has developed into a modern exo-Venus, then the modelled temperatures suggest that H$_2$SO$_4$ clouds are possible even in the substellar region. Like on modern Venus, clouds on LP 890-9 c would create a flat spectrum. The strongest CO$_2$ bands in transmission predicted by our model for LP 890-9 c are about 10 ppm, challenging detection, given JWST estimated noise floor. Estimated phase curve amplitudes are 0.9 and 2.4 ppm for continuum and CO$_2$ bands, respectively. While pointing out the challenge to characterise modern exo-Venus analogues, these results provide new insights for JWST proposals and highlight the influence of clouds in the spectrum of hot rocky exoplanet spectra., Comment: 6 pages, 4 figures, MNRAS letter

Published
2023
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6. A Wireless Tree Climbing Robot: REDA-Design and Implementation

Author

Villalpando-Hernandez, Rafaela, Vargas-Rosales, Cesar, Diaz-M., Rene, Gonzalez, J. Jorge Nuñez, Galindo, Francisco Ruvalcaba, Barajas, Isai Fritshe, Kacprzyk, Janusz, Series Editor, Gomide, Fernando, Advisory Editor, Kaynak, Okyay, Advisory Editor, Liu, Derong, Advisory Editor, Pedrycz, Witold, Advisory Editor, Polycarpou, Marios M., Advisory Editor, Rudas, Imre J., Advisory Editor, Wang, Jun, Advisory Editor, Cardona, Manuel N., editor, Baca, José, editor, Garcia, Cecilia, editor, Carrera, Isela G., editor, and Martinez, Carol, editor

Published
2024
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10. Ariel: Enabling planetary science across light-years

Author

Tinetti, Giovanna, Eccleston, Paul, Haswell, Carole, Lagage, Pierre-Olivier, Leconte, Jérémy, Lüftinger, Theresa, Micela, Giusi, Min, Michel, Pilbratt, Göran, Puig, Ludovic, Swain, Mark, Testi, Leonardo, Turrini, Diego, Vandenbussche, Bart, Osorio, Maria Rosa Zapatero, Aret, Anna, Beaulieu, Jean-Philippe, Buchhave, Lars, Ferus, Martin, Griffin, Matt, Guedel, Manuel, Hartogh, Paul, Machado, Pedro, Malaguti, Giuseppe, Pallé, Enric, Rataj, Mirek, Ray, Tom, Ribas, Ignasi, Szabó, Robert, Tan, Jonathan, Werner, Stephanie, Ratti, Francesco, Scharmberg, Carsten, Salvignol, Jean-Christophe, Boudin, Nathalie, Halain, Jean-Philippe, Haag, Martin, Crouzet, Pierre-Elie, Kohley, Ralf, Symonds, Kate, Renk, Florian, Caldwell, Andrew, Abreu, Manuel, Alonso, Gustavo, Amiaux, Jerome, Berthé, Michel, Bishop, Georgia, Bowles, Neil, Carmona, Manuel, Coffey, Deirdre, Colomé, Josep, Crook, Martin, Désjonqueres, Lucile, Díaz, José J., Drummond, Rachel, Focardi, Mauro, Gómez, Jose M., Holmes, Warren, Krijger, Matthijs, Kovacs, Zsolt, Hunt, Tom, Machado, Richardo, Morgante, Gianluca, Ollivier, Marc, Ottensamer, Roland, Pace, Emanuele, Pagano, Teresa, Pascale, Enzo, Pearson, Chris, Pedersen, Søren Møller, Pniel, Moshe, Roose, Stéphane, Savini, Giorgio, Stamper, Richard, Szirovicza, Peter, Szoke, Janos, Tosh, Ian, Vilardell, Francesc, Barstow, Joanna, Borsato, Luca, Casewell, Sarah, Changeat, Quentin, Charnay, Benjamin, Civiš, Svatopluk, Foresto, Vincent Coudé du, Coustenis, Athena, Cowan, Nicolas, Danielski, Camilla, Demangeon, Olivier, Drossart, Pierre, Edwards, Billy N., Gilli, Gabriella, Encrenaz, Therese, Kiss, Csaba, Kokori, Anastasia, Ikoma, Masahiro, Morales, Juan Carlos, Mendonça, João, Moneti, Andrea, Mugnai, Lorenzo, Muñoz, Antonio García, Helled, Ravit, Kama, Mihkel, Miguel, Yamila, Nikolaou, Nikos, Pagano, Isabella, Panic, Olja, Rengel, Miriam, Rickman, Hans, Rocchetto, Marco, Sarkar, Subhajit, Selsis, Franck, Tennyson, Jonathan, Tsiaras, Angelos, Venot, Olivia, Vida, Krisztián, Waldmann, Ingo P., Yurchenko, Sergey, Szabó, Gyula, Zellem, Rob, Al-Refaie, Ahmed, Alvarez, Javier Perez, Anisman, Lara, Arhancet, Axel, Ateca, Jaume, Baeyens, Robin, Barnes, John R., Bell, Taylor, Benatti, Serena, Biazzo, Katia, Błęcka, Maria, Bonomo, Aldo Stefano, Bosch, José, Bossini, Diego, Bourgalais, Jeremy, Brienza, Daniele, Brucalassi, Anna, Bruno, Giovanni, Caines, Hamish, Calcutt, Simon, Campante, Tiago, Canestrari, Rodolfo, Cann, Nick, Casali, Giada, Casas, Albert, Cassone, Giuseppe, Cara, Christophe, Carone, Ludmila, Carrasco, Nathalie, Chioetto, Paolo, Cortecchia, Fausto, Czupalla, Markus, Chubb, Katy L., Ciaravella, Angela, Claret, Antonio, Claudi, Riccardo, Codella, Claudio, Comas, Maya Garcia, Cracchiolo, Gianluca, Cubillos, Patricio, Da Peppo, Vania, Decin, Leen, Dejabrun, Clemence, Delgado-Mena, Elisa, Di Giorgio, Anna, Diolaiti, Emiliano, Dorn, Caroline, Doublier, Vanessa, Doumayrou, Eric, Dransfield, Georgina, Dumaye, Luc, Dunford, Emma, Escobar, Antonio Jimenez, Van Eylen, Vincent, Farina, Maria, Fedele, Davide, Fernández, Alejandro, Fleury, Benjamin, Fonte, Sergio, Fontignie, Jean, Fossati, Luca, Funke, Bernd, Galy, Camille, Garai, Zoltán, García, Andrés, García-Rigo, Alberto, Garufi, Antonio, Sacco, Giuseppe Germano, Giacobbe, Paolo, Gómez, Alejandro, Gonzalez, Arturo, Gonzalez-Galindo, Francisco, Grassi, Davide, Griffith, Caitlin, Guarcello, Mario Giuseppe, Goujon, Audrey, Gressier, Amélie, Grzegorczyk, Aleksandra, Guillot, Tristan, Guilluy, Gloria, Hargrave, Peter, Hellin, Marie-Laure, Herrero, Enrique, Hills, Matt, Horeau, Benoit, Ito, Yuichi, Jessen, Niels Christian, Kabath, Petr, Kálmán, Szilárd, Kawashima, Yui, Kimura, Tadahiro, Knížek, Antonín, Kreidberg, Laura, Kruid, Ronald, Kruijssen, Diederik J. M., Kubelík, Petr, Lara, Luisa, Lebonnois, Sebastien, Lee, David, Lefevre, Maxence, Lichtenberg, Tim, Locci, Daniele, Lombini, Matteo, Lopez, Alejandro Sanchez, Lorenzani, Andrea, MacDonald, Ryan, Magrini, Laura, Maldonado, Jesus, Marcq, Emmanuel, Migliorini, Alessandra, Modirrousta-Galian, Darius, Molaverdikhani, Karan, Molinari, Sergio, Mollière, Paul, Moreau, Vincent, Morello, Giuseppe, Morinaud, Gilles, Morvan, Mario, Moses, Julianne I., Mouzali, Salima, Nakhjiri, Nariman, Naponiello, Luca, Narita, Norio, Nascimbeni, Valerio, Nikolaou, Athanasia, Noce, Vladimiro, Oliva, Fabrizio, Palladino, Pietro, Papageorgiou, Andreas, Parmentier, Vivien, Peres, Giovanni, Pérez, Javier, Perez-Hoyos, Santiago, Perger, Manuel, Pestellini, Cesare Cecchi, Petralia, Antonino, Philippon, Anne, Piccialli, Arianna, Pignatari, Marco, Piotto, Giampaolo, Podio, Linda, Polenta, Gianluca, Preti, Giampaolo, Pribulla, Theodor, Puertas, Manuel Lopez, Rainer, Monica, Reess, Jean-Michel, Rimmer, Paul, Robert, Séverine, Rosich, Albert, Rossi, Loic, Rust, Duncan, Saleh, Ayman, Sanna, Nicoletta, Schisano, Eugenio, Schreiber, Laura, Schwartz, Victor, Scippa, Antonio, Seli, Bálint, Shibata, Sho, Simpson, Caroline, Shorttle, Oliver, Skaf, N., Skup, Konrad, Sobiecki, Mateusz, Sousa, Sergio, Sozzetti, Alessandro, Šponer, Judit, Steiger, Lukas, Tanga, Paolo, Tackley, Paul, Taylor, Jake, Tecza, Matthias, Terenzi, Luca, Tremblin, Pascal, Tozzi, Andrea, Triaud, Amaury, Trompet, Loïc, Tsai, Shang-Min, Tsantaki, Maria, Valencia, Diana, Vandaele, Ann Carine, Van der Swaelmen, Mathieu, Vardan, Adibekyan, Vasisht, Gautam, Vazan, Allona, Del Vecchio, Ciro, Waltham, Dave, Wawer, Piotr, Widemann, Thomas, Wolkenberg, Paulina, Yip, Gordon Hou, Yung, Yuk, Zilinskas, Mantas, Zingales, Tiziano, and Zuppella, Paola

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. During its 4-year mission, Ariel will study what exoplanets are made of, how they formed and how they evolve, by surveying a diverse sample of about 1000 extrasolar planets, simultaneously in visible and infrared wavelengths. It is the first mission dedicated to measuring the chemical composition and thermal structures of hundreds of transiting exoplanets, enabling planetary science far beyond the boundaries of the Solar System. The payload consists of an off-axis Cassegrain telescope (primary mirror 1100 mm x 730 mm ellipse) and two separate instruments (FGS and AIRS) covering simultaneously 0.5-7.8 micron spectral range. The satellite is best placed into an L2 orbit to maximise the thermal stability and the field of regard. The payload module is passively cooled via a series of V-Groove radiators; the detectors for the AIRS are the only items that require active cooling via an active Ne JT cooler. The Ariel payload is developed by a consortium of more than 50 institutes from 16 ESA countries, which include the UK, France, Italy, Belgium, Poland, Spain, Austria, Denmark, Ireland, Portugal, Czech Republic, Hungary, the Netherlands, Sweden, Norway, Estonia, and a NASA contribution., Comment: Ariel Definition Study Report, 147 pages. Reviewed by ESA Science Advisory Structure in November 2020. Original document available at: https://www.cosmos.esa.int/documents/1783156/3267291/Ariel_RedBook_Nov2020.pdf/

Published
2021

11. Consensus document on acute-on-chronic liver failure (ACLF) established by the Mexican Association of Hepatology

Author

Torre, Aldo, Cisneros-Garza, Laura Esthela, Castillo-Barradas, Mauricio, Navarro-Alvarez, Nalu, Sandoval-Salas, Ricardo, González-Huezo, María Sarai, Pérez-Hernández, José Luís, Méndez-Guerrero, Osvely, Ruiz-Manríquez, Jesús Alejandro, Trejo-Estrada, Rafael, Chavez-Tapia, Norberto C., Solís-Gasca, Luis Carlos, Moctezuma-Velázquez, Carlos, Aguirre-Valádez, Jonathan, Flores-Calderón, Judith, Higuera-de-la-Tijera, Fatima, García-Juárez, Ignacio, Canedo-Castillo, Nancy Allin, Malé-Velázquez, René, Montalvo-Gordon, Iaarah, Vilatobá, Mario, Márquez-Guillén, Ernesto, Córdova-Gallardo, Jacqueline, Flores-García, Nayeli Cointa, Miranda-Zazueta, Godolfino, Martínez-Saldívar, Belinda Isela, Páez-Zayas, Víctor Manuel, Muñoz-Espinosa, Linda Elsa, and Solís-Galindo, Francisco Alfonso

Published
2023
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23. The Climatology of Mars Thermospheric Polar Warming at Aphelion

Author

Thiemann, Edward M. B., primary, Trompet, Loïc, additional, Bougher, Stephen W., additional, Yiğit, Erdal, additional, Gasperini, Federico, additional, Montabone, Luca, additional, Gonzalez‐Galindo, Francisco, additional, Eparvier, Francis G., additional, and Vandaele, Anne‐Carine, additional

Published
2024
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29. Cooling of the Martian thermosphere by CO$_2$ radiation and gravity waves: An intercomparison study with two general circulation models

Author

Medvedev, Alexander S., González-Galindo, Francisco, Yiğit, Erdal, Feofilov, Artem G., Forget, François, and Hartogh, Paul

Subjects
Astrophysics - Earth and Planetary Astrophysics, Physics - Atmospheric and Oceanic Physics, Physics - Fluid Dynamics, Physics - Space Physics
Abstract

Observations show that the lower thermosphere of Mars ($\sim$100--140 km) is up to 40 K colder than the current general circulation models (GCMs) can reproduce. Possible candidates for physical processes missing in the models are larger abundances of atomic oxygen facilitating stronger CO$_2$ radiative cooling, and thermal effects of gravity waves. Using two state-of-the-art Martian GCMs, the Laboratoire de M\'et\'eorologie Dynamique and Max Planck Institute models that self-consistently cover the atmosphere from the surface to the thermosphere, these physical mechanisms are investigated. Simulations demonstrate that the CO$_2$ radiative cooling with a sufficiently large atomic oxygen abundance, and the gravity wave-induced cooling can alone result in up to 40 K colder temperature in the lower thermosphere. Accounting for both mechanisms produce stronger cooling at high latitudes. However, radiative cooling effects peak above the mesopause, while gravity wave cooling rates continuously increase with height. Although both mechanisms act simultaneously, these peculiarities could help to further quantify their relative contributions from future observations., Comment: Accepted for publication in Journal of Geophysical Research - Planets

Published
2015

31. Carcinoma gástrico difuso en la juventud: reporte de caso.

Author

González-Aguirre, Rodrigo, Ronaldo Sánchez-Moreno, Héctor, Alberto Gutiérrez-Rodríguez, Eulalio, Alexis Arce-Hernández, Julio, and Alfonso Solis-Galindo, Francisco

Abstract

Copyright of Revista Medica del IMSS is the property of Direccion de Prestaciones Medicas - IMSS and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Published
2024
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38. Temporal Variability of Waves at the Proton Cyclotron Frequency Upstream from Mars: Implications for Mars Distant Hydrogen Exosphere

Author

Bertucci, Cesar, Romanelli, Norberto, Chaufray, Jean-Yves, Gomez, Daniel, Mazelle, Christian, Delva, Magda, Modolo, Ronan, Gonzalez-Galindo, Francisco, and Brain, David Andrew

Subjects
Physics - Space Physics
Abstract

We report on the temporal variability of the occurrence of waves at the local proton cyclotron frequency upstream from the Martian bow shock from Mars Global Surveyor observations during the first aerobraking and science phasing orbit periods. Observations at high southern latitudes during minimum-to-mean solar activity show that the wave occurrence rate is significantly higher around perihelion southern summer solstice and lower around the same hemisphere's spring and autumn equinoxes. A similar trend is observed in the hydrogen (H) exospheric density profiles over the Martian South Pole obtained from a model including UV thermospheric heating effects. In spite of the complexity in the ion pick-up and plasma wave generation and evolution processes, these results support the idea that variations in the occurrence of waves could be used to study the temporal evolution of the distant Martian H corona and its coupling with the thermosphere at altitudes currently inaccessible to direct measurements., Comment: 16 pages, 2 figures, Submitted to Geophysical Research Letters

Published
2013
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39. Osteoporosis en el hombre

Author

Galindo, Blanca Sánchez and Galindo, Francisco José Sánchez

Abstract

•En los varones existe una alta prevalencia de osteoporosis secundaria, por lo que es necesario descartar una causa subyacente de la misma.•El tratamiento de elección en los varones son los bisfosfonatos, siendo estos los únicos fármacos en los que puede plantearse la posibilidad de las vacaciones terapéuticas.•La mayoría de los pacientes con osteoporosis deben de poder ser atendidos en la consulta del médico de atención primaria, siendo necesaria la derivación en determinadas circunstancias.•En todo paciente con osteoporosis deben implementarse como medidas generales de tratamiento la realización de ejercicio físico regular, el cese del tabaquismo, evitar el consumo excesivo de alcohol, ingesta adecuada de calcio y niveles adecuados de vitamina D.

Published
2024
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40. Longitudinal Variations of Mars Thermosphere CO2, Ar, N2, and O Densities From MAVEN: Dependencies on Species Mass, Solar Flux, and Local Time.

Author

Forbes, Jeffrey M., Xiaohua Fang, Xiaoli Zhang, Benna, Mehdi, and González-Galindo, Francisco

Subjects
THERMOSPHERE, ROSSBY waves, STANDING waves, MARTIAN atmosphere, MARS (Planet), ATMOSPHERE
Abstract

Measurements of CO2, Ar, N2, and O densities between 150 and 200 km from the Mars Atmosphere and Volatile Evolution Neutral Gas and Ion Mass Spectrometer during February 2015 to February 2022 are analyzed to provide a comprehensive analysis of their longitudinal wavenumber k = 1, 2, and 3 components. Variations in density amplitudes (Ak) with solar flux are marginally detectable during this period. The Ak binned and averaged in latitude, local solar time and Ls are referenced to diurnal- and zonal-mean backgrounds in accord with how tides and stationary planetary waves (SPWs) are defined in theory and modeling. The resulting global Ak distributions are the interference patterns formed by superposition of diurnal tides, SPWs and/or semidiurnal tides; consequently, a simple dependence on species mass consistent with thermal expansion (diffusive equilibrium) that might exist for some individual wave components is obscured. Additionally, vertical winds likely contribute to deviations from diffusive equilibrium. Complementary analyses of the Mars Climate Database indicate that the major contributors to the Ak are DE2, SE1, DE1, and SPW1, 2, 3; support the absence of significant variability due to solar flux; and indicate a more well-defined sensitivity to species mass. The Ak and their phases (longitudes of maxima) for the whole data set are available as part of Supporting Information S1. [ABSTRACT FROM AUTHOR]

Published
2024
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41. Martian Atmospheric Aerosols Composition and Distribution Retrievals During the First Martian Year of NOMAD/TGO Solar Occultation Measurements: 2. Extended Results, End of MY 34 and First Half of MY 35

Author

Stolzenbach, Aurélien, primary, López Valverde, Miguel‐Angel, additional, Brines, Adrian, additional, Modak, Ashimananda, additional, Funke, Bernd, additional, González‐Galindo, Francisco, additional, Thomas, Ian, additional, Liuzzi, Giuliano, additional, Villanueva, Gerónimo, additional, Luginin, Mikhail, additional, Aoki, Shohei, additional, Grabowski, Udo, additional, Lopez Moreno, José Juan, additional, Rodriguez‐Gomez, Julio, additional, Wolff, Mike, additional, Ristic, Bojan, additional, Daerden, Frank, additional, Bellucci, Giancarlo, additional, Patel, Manish, additional, and Vandaele, Ann‐Carine, additional

Published
2023
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42. Martian Atmospheric Aerosols Composition and Distribution Retrievals During the First Martian Year of NOMAD/TGO Solar Occultation Measurements: 1. Methodology and Application to the MY 34 Global Dust Storm

Author

Stolzenbach, Aurélien, primary, López Valverde, Miguel‐Angel, additional, Brines, Adrian, additional, Modak, Ashimananda, additional, Funke, Bernd, additional, González‐Galindo, Francisco, additional, Thomas, Ian, additional, Liuzzi, Giuliano, additional, Villanueva, Gerónimo, additional, Luginin, Mikhail, additional, Aoki, Shohei, additional, Grabowski, Udo, additional, Lopez Moreno, José Juan, additional, Rodrìguez Gòmez, Julio, additional, Wolff, Mike, additional, Ristic, Bojan, additional, Daerden, Frank, additional, Bellucci, Giancarlo, additional, Patel, Manish, additional, and Vandaele, Ann‐Carine, additional

Published
2023
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44. Loss of glutathione redox homeostasis impairs proteostasis by inhibiting autophagy-dependent protein degradation

Author

Guerrero-Gómez, David, Mora-Lorca, José Antonio, Sáenz-Narciso, Beatriz, Naranjo-Galindo, Francisco José, Muñoz-Lobato, Fernando, Parrado-Fernández, Cristina, Goikolea, Julen, Cedazo-Minguez, Ángel, Link, Christopher D., Neri, Christian, Sequedo, María Dolores, Vázquez-Manrique, Rafael P., Fernández-Suárez, Elena, Goder, Veit, Pané, Roser, Cabiscol, Elisa, Askjaer, Peter, Cabello, Juan, and Miranda-Vizuete, Antonio

Published
2019
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46. A Surface to Exosphere Non‐Orographic Gravity Wave Parameterization for the Mars Planetary Climate Model

Author

Liu, Jiandong, primary, Millour, Ehouarn, additional, Forget, François, additional, Gilli, Gabriella, additional, Lott, François, additional, Bardet, Deborah, additional, González Galindo, Francisco, additional, Bierjon, Antoine, additional, Naar, Joseph, additional, Martinez, Antoine, additional, Lebonnois, Sébastien, additional, Fan, Siteng, additional, Pierron, Thomas, additional, and Vandemeulebrouck, Romain, additional

Published
2023
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