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1. Drying of the Martian mesosphere during aphelion induced by lower temperatures

Author

Toledo, Daniel, Rannou, Pascal, Apéstigue, Victor, Rodriguez-Veloso, Raul, Arruego, Ignacio, Martínez, German, Tamppari, Leslie, Munguira, Asier, Lorenz, Ralph, Stcherbinine, Aurélien, Montmessin, Franck, Sanchez-Lavega, Agustin, Patel, Priya, Smith, Michael, Lemmon, Mark, Vicente-Retortillo, Alvaro, Newman, Claire, Viudez-Moreiras, Daniel, Hueso, Ricardo, Bertrand, Tanguy, Pla-Garcia, Jorge, Yela, Margarita, de la Torre Juarez, Manuel, and Rodriguez-Manfredi, Jose Antonio

Published
2024
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2. Present-day thermal and water activity environment of the Mars Sample Return collection

Author

Zorzano, Maria-Paz, Martínez, Germán, Polkko, Jouni, Tamppari, Leslie K., Newman, Claire, Savijärvi, Hannu, Goreva, Yulia, Viúdez-Moreiras, Daniel, Bertrand, Tanguy, Smith, Michael, Hausrath, Elisabeth M., Siljeström, Sandra, Benison, Kathleen, Bosak, Tanja, Czaja, Andrew D., Debaille, Vinciane, Herd, Christopher D. K., Mayhew, Lisa, Sephton, Mark A., Shuster, David, Simon, Justin I., Weiss, Benjamin, Randazzo, Nicolas, Mandon, Lucia, Brown, Adrian, Hecht, Michael H., and Martínez-Frías, Jesús

Published
2024
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6. Terrestrial Planets Comparative Climatology (TPCC) mission concept

Author

Tamppari, Leslie K., Brecht, Amanda, Baines, Kevin, Drouin, Brian, Esposito, Larry, Guzewich, Scott, Hofer, Richard, Jessup, Kandis Lea, Kleinböhl, Armin, Kremic, Tibor, Mischna, Michael, Schneider, Nicholas, and Spiga, Aymeric

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

The authors and co-signers of the Terrestrial Planets Comparative Climatology (TPCC) mission concept white paper advocate that planetary science in the next decade would greatly benefit from comparatively studying the fundamental behavior of the atmospheres of Venus and Mars, contemporaneously and with the same instrumentation, to capture atmospheric response to the same solar forcing, and with a minimum of instrument-related variability. Thus, this white paper was created for the 2023-2032 Planetary Science Decadal Survey process. It describes the science rationale for such a mission, and a mission concept that could achieve such a mission., Comment: 8 pages including cover page with one figure on cover page

Published
2020

16. Photogeologic Map of the Perseverance Rover Field Site in Jezero Crater Constructed by the Mars 2020 Science Team

Author

Stack, Kathryn M., Williams, Nathan R., Calef, III, Fred, Sun, Vivian Z., Williford, Kenneth H., Farley, Kenneth A., Eide, Sigurd, Flannery, David, Hughes, Cory, Jacob, Samantha R., Kah, Linda C., Meyen, Forrest, Molina, Antonio, Nataf, Cathy Quantin, Rice, Melissa, Russell, Patrick, Scheller, Eva, Seeger, Christina H., Abbey, William J., Adler, Jacob B., Amundsen, Hans, Anderson, Ryan B., Angel, Stanley M., Arana, Gorka, Atkins, James, Barrington, Megan, Berger, Tor, Borden, Rose, Boring, Beau, Brown, Adrian, Carrier, Brandi L., Conrad, Pamela, Dypvik, Henning, Fagents, Sarah A., Gallegos, Zachary E., Garczynski, Brad, Golder, Keenan, Gomez, Felipe, Goreva, Yulia, Gupta, Sanjeev, Hamran, Svein-Erik, Hicks, Taryn, Hinterman, Eric D., Horgan, Briony N., Hurowitz, Joel, Johnson, Jeffrey R., Lasue, Jeremie, Kronyak, Rachel E., Liu, Yang, Madariaga, Juan Manuel, Mangold, Nicolas, McClean, John, Miklusicak, Noah, Nunes, Daniel, Rojas, Corrine, Runyon, Kirby, Schmitz, Nicole, Scudder, Noel, Shaver, Emily, SooHoo, Jason, Spaulding, Russell, Stanish, Evan, Tamppari, Leslie K., Tice, Michael M., Turenne, Nathalie, Willis, Peter A., and Aileen Yingst, R.

Published
2020
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17. Perseverance MEDA Atmospheric Pressure Observations—Initial Results.

Author

Harri, Ari‐Matti, Paton, Mark, Hieta, Maria, Polkko, Jouni, Newman, Claire, Pla‐Garcia, Jorge, Leino, Joonas, Mäkinen, Terhi, Kauhanen, Janne, Jaakonaho, Iina, Sánchez‐Lavega, Agustin, Hueso, Ricardo, Genzer, Maria, Lorenz, Ralph, Lemmon, Mark, Vicente‐Retortillo, Alvaro, Tamppari, Leslie K., Viudez‐Moreiras, Daniel, Torre‐Juarez, Manuel de la, and Savijärvi, Hannu

Subjects
ATMOSPHERIC pressure, MARTIAN atmosphere, MARTIAN craters, MARTIAN surface, DUST, ATMOSPHERE
Abstract

The Mars2020 Perseverance Rover landed successfully on the Martian surface on the Jezero Crater floor (18.44°N, 77.45°E) at Martian solar longitude, Ls, ∼5° in February 2021. Since then, it has produced highly valuable environmental measurements with a versatile scientific payload including the MEDA (Mars Environmental Dynamics Analyzer) suite of environmental sensors. One of the MEDA systems is the PS pressure sensor system, which weighs 40 g and has an estimated absolute accuracy of better than 3.5 Pa and a resolution of 0.13 Pa. We present initial results from the first 414 sols of Martian atmospheric surface pressure observations by the PS, whose performance was found to meet its specifications. Observed sol‐averaged atmospheric pressures follow an anticipated pattern of pressure variation in the course of the advancing season and are consistent with data from other landing missions. The observed daily pressure amplitude varies by ∼2%–5 % of the sol‐averaged pressure, with absolute amplitude 10–35 Pa in an approximately direct relationship with airborne dust. During a regional dust storm, which began at Ls ∼ 135°, the daily pressure amplitude roughly doubled. The daily pressure variations were found to be remarkably sensitive to the seasonal evolution of the atmosphere. In particular, analysis of the daily pressure signature revealed diagnostic information likely related to the regional scale structure of the atmosphere. Comparison of Perseverance pressure observations with data from other landers reveals the global scale seasonal behavior of Mars' atmosphere. Plain Language Summary: Mars2020 Perseverance Rover successfully arrived on Mars in February 2021. It landed in an early Martian spring afternoon in a crater north of Mars' equator called Jezero crater. The rover is equipped with meteorological instruments that have so far produced extensive and valuable data for understanding the Martian atmosphere. One of the meteorological instruments is an accurate and precise pressure sensor. The pressure sensor has revealed large changes in the pressure over the seasons that are related to large changes in the actual mass of the Martian atmosphere. This is in line with seasonal pressure changes measured during previous Mars missions and can be explained as the condensation of the atmosphere onto the Martian poles and its subsequent sublimation. On a shorter time scale, the pressure sensor revealed complex pressure changes over a Martian day. These variations are thought to be related to atmospheric dust, whose ubiquitous nature is known to have a strong influence on the Martian climate. As the seasons progressed, the daily pressure variations morphed to exhibit different patterns likely related to the large‐scale regional changes in the atmosphere. Comparison of Perseverance pressure observations with other landers revealed the global nature of the atmosphere. Key Points: The atmospheric pressure observations by Perseverance Rover have proved to be of excellent quality fulfilling expectationsJezero crater pressure exhibits significant differences to other Martian areas likely due to varying regional geography and solar forcingOverall, the diurnal and seasonal atmospheric pressure cycles at Jezero Crater follow an anticipated pattern of pressure variation [ABSTRACT FROM AUTHOR]

Published
2024
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28. Perseverance MEDA Atmospheric Pressure Observations - Initial Results

Author

Harri, Ari-Matti, primary, Paton, Mark, additional, Hieta, Maria, additional, Polkko, Jouni, additional, Newman, Claire, additional, Pla-García, Jorge, additional, Leino, Joonas, additional, Mäkinen, Terhi, additional, Kauhanen, Janne, additional, Jaakonaho, Iina, additional, Sánchez-Lavega, Agustín, additional, Hueso, Ricardo, additional, Genzer, Maria, additional, Lorenz, Ralph D., additional, Lemmon, Mark T, additional, Vicente-Retortillo, Alvaro, additional, Tamppari, Leslie, additional, Viúdez-Moreiras, Daniel, additional, Juárez, Manuel de la Torre, additional, Savijärvi, Hannu, additional, Rodríguez-Manfredi, Jose Antonio, additional, and Martinez, German, additional

Published
2023
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29. The diverse meteorology of Jezero crater over the first 250 sols of Perseverance on Mars

Author

Universitat Politècnica de Catalunya. Departament d'Enginyeria Electrònica, Universitat Politècnica de Catalunya. MNT-Solar - Grup de Micro i Nano Tecnologies per Energia Solar, Rodríguez Manfredi, José Antonio, De la Torre Juárez, M., Sanchez Lavega, Agustin, Hueso, Ricardo, Martinez, German, Lemmon, Mark T., Newman, Claire, Munguira, Asier, Hieta, Maria, Tamppari, Leslie K., Polkko, J., Toledo Melgar, Daniel, Sebastián Martínez, Eduardo, Smith, Michael Doyle, Jaakonaho, Iina, Domínguez Pumar, Manuel, Jiménez Serres, Vicente, Universitat Politècnica de Catalunya. Departament d'Enginyeria Electrònica, Universitat Politècnica de Catalunya. MNT-Solar - Grup de Micro i Nano Tecnologies per Energia Solar, Rodríguez Manfredi, José Antonio, De la Torre Juárez, M., Sanchez Lavega, Agustin, Hueso, Ricardo, Martinez, German, Lemmon, Mark T., Newman, Claire, Munguira, Asier, Hieta, Maria, Tamppari, Leslie K., Polkko, J., Toledo Melgar, Daniel, Sebastián Martínez, Eduardo, Smith, Michael Doyle, Jaakonaho, Iina, Domínguez Pumar, Manuel, and Jiménez Serres, Vicente

Abstract

NASA’s Perseverance rover’s Mars Environmental Dynamics Analyzer is collecting data at Jezero crater, characterizing the physical processes in the lowest layer of the Martian atmosphere. Here we present measurements from the instrument’s first 250 sols of operation, revealing a spatially and temporally variable meteorology at Jezero. We find that temperature measurements at four heights capture the response of the atmospheric surface layer to multiple phenomena. We observe the transition from a stable night-time thermal inversion to a daytime, highly turbulent convective regime, with large vertical thermal gradients. Measurement of multiple daily optical depths suggests aerosol concentrations are higher in the morning than in the afternoon. Measured wind patterns are driven mainly by local topography, with a small contribution from regional winds. Daily and seasonal variability of relative humidity shows a complex hydrologic cycle. These observations suggest that changes in some local surface properties, such as surface albedo and thermal inertia, play an influential role. On a larger scale, surface pressure measurements show typical signatures of gravity waves and baroclinic eddies in a part of the seasonal cycle previously characterized as low wave activity. These observations, both combined and simultaneous, unveil the diversity of processes driving change on today’s Martian surface at Jezero crater., This work has been funded by the Spanish Ministry of Economy and Competitiveness, through the projects no. ESP2014-54256-C4- 1-R (also -2-R, -3-R and -4-R); Ministry of Science, Innovation and Universities, projects no. ESP2016-79612-C3-1-R (also -2-R and -3-R); Ministry of Science and Innovation/State Agency of Research (10.13039/501100011033), projects no. ESP2016-80320-C2-1-R, RTI2018-098728-B-C31 (also -C32 and -C33), RTI2018-099825-B-C31, PID2019-109467GB-I00 and PRE2020-092562; Instituto Nacional de Técnica Aeroespacial; Ministry of Science and Innovation’s Centre for the Development of Industrial Technology; Spanish State Research Agency (AEI) Project MDM-2017-0737 Unidad de Excelencia “María de Maeztu”—Centro de Astrobiología; Grupos Gobierno Vasco IT1366- 19; and European Research Council Consolidator Grant no 818602. The US co-authors performed their work under sponsorship from NASA’s Mars 2020 project, from the Game Changing Development programme within the Space Technology Mission Directorate and from the Human Exploration and Operations Directorate. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). G.M. acknowledges JPL funding from USRA Contract Number 1638782. A.G.F. is supported by the European Research Council, Consolidator Grant no. 818602., Peer Reviewed, Postprint (published version)

Published
2023

30. Twilight Mesospheric Clouds in Jezero as Observed by MEDA Radiation and Dust Sensor (RDS)

Author

Física aplicada I, Fisika aplikatua I, Toledo, Daniel, Gomez Martín, Laura, Apestigue, Victor, Arruego, Ignacio, Smith, Michael D., Munguira Ruiz, Asier, Martínez, Germán, Patel, Priyaben, Sánchez Lavega, Agustín María, Lemmon, Mark T., Tamppari, Leslie, Viúdez Moreiras, Daniel, Hueso Alonso, Ricardo, Vicente Retortillo, Álvaro, Newman, Claire E., Lorenz, Ralph D., Yela, Margarita, de la Torre Juárez, Manuel, Rodríguez Manfredi, José Antonio, Física aplicada I, Fisika aplikatua I, Toledo, Daniel, Gomez Martín, Laura, Apestigue, Victor, Arruego, Ignacio, Smith, Michael D., Munguira Ruiz, Asier, Martínez, Germán, Patel, Priyaben, Sánchez Lavega, Agustín María, Lemmon, Mark T., Tamppari, Leslie, Viúdez Moreiras, Daniel, Hueso Alonso, Ricardo, Vicente Retortillo, Álvaro, Newman, Claire E., Lorenz, Ralph D., Yela, Margarita, de la Torre Juárez, Manuel, and Rodríguez Manfredi, José Antonio

Abstract

The Mars Environmental Dynamics Analyzer instrument, on board NASA's Mars 2020 Perseverance rover, includes a number of sensors to characterize the Martian atmosphere. One of these sensors is the Radiation and Dust Sensor (RDS) that measures the solar irradiance at different wavelengths and geometries. We analyzed the RDS observations made during twilight for the period between sol 71 and 492 of the mission (Ls 39°–262°, Mars Year 36) to characterize the clouds over the Perseverance rover site. Using the ratio between the irradiance at zenith at 450 and 750 nm, we inferred that the main constituent of the detected high-altitude aerosol layers was ice from Ls = 39°–150° (cloudy period), and dust from Ls 150°–262°. A total of 161 twilights were analyzed in the cloudy period using a radiative transfer code and we found: (a) signatures of clouds/hazes in the signals in 58% of the twilights; (b) most of the clouds had altitudes between 40 and 50 km, suggesting water ice composition, and had particle sizes between 0.6 and 2 µm; (c) the cloud activity at sunrise is slightly higher that at sunset, likely due to the differences in temperature; (d) the time period with more cloud detections and with the greatest cloud opacities is during Ls 120°–150°; and (e) a notable decrease in the cloud activity around aphelion, along with lower cloud altitudes and opacities. This decrease in cloud activity indicates lower concentrations of water vapor or cloud condensation nuclei (dust) around this period in the Martian mesosphere.

Published
2023

31. Mars 2020 Perseverance Rover Studies of the Martian Atmosphere Over Jezero From Pressure Measurements

Author

Física aplicada I, Fisika aplikatua I, Sánchez Lavega, Agustín María, Del Río Gaztelurrutia, María Teresa, Hueso Alonso, Ricardo, de la Torre Juárez, Manuel, Martínez, Germán M., Harri, Ari Matti, Genzer, Maria, Hieta, Maria, Polkko, J., Rodríguez Manfredi, José Antonio, Lemmon, Mark T., Plá García, Jorge, Toledo, Daniel, Vicente Retortillo, Álvaro, Viúdez Moreiras, Daniel, Munguira Ruiz, Asier, Tamppari, Leslie, Newman, Claire E., Gómez Elvira, Javier, Guzewich, Scott, Bertrand, Tanguy, Apestigue, Victor, Arruego, Ignacio, Wolff, Michael J., Banfield, Don, Jaakonaho, I., Makinen, T., Física aplicada I, Fisika aplikatua I, Sánchez Lavega, Agustín María, Del Río Gaztelurrutia, María Teresa, Hueso Alonso, Ricardo, de la Torre Juárez, Manuel, Martínez, Germán M., Harri, Ari Matti, Genzer, Maria, Hieta, Maria, Polkko, J., Rodríguez Manfredi, José Antonio, Lemmon, Mark T., Plá García, Jorge, Toledo, Daniel, Vicente Retortillo, Álvaro, Viúdez Moreiras, Daniel, Munguira Ruiz, Asier, Tamppari, Leslie, Newman, Claire E., Gómez Elvira, Javier, Guzewich, Scott, Bertrand, Tanguy, Apestigue, Victor, Arruego, Ignacio, Wolff, Michael J., Banfield, Don, Jaakonaho, I., and Makinen, T.

Abstract

The pressure sensors on Mars rover Perseverance measure the pressure field in the Jezero crater on regular hourly basis starting in sol 15 after landing. The present study extends up to sol 460 encompassing the range of solar longitudes from Ls ∼ 13°–241° (Martian Year (MY) 36). The data show the changing daily pressure cycle, the sol-to-sol seasonal evolution of the mean pressure field driven by the CO2 sublimation and deposition cycle at the poles, the characterization of up to six components of the atmospheric tides and their relationship to dust content in the atmosphere. They also show the presence of wave disturbances with periods 2–5 sols, exploring their baroclinic nature, short period oscillations (mainly at night-time) in the range 8–24 min that we interpret as internal gravity waves, transient pressure drops with duration ∼1–150 s produced by vortices, and rapid turbulent fluctuations. We also analyze the effects on pressure measurements produced by a regional dust storm over Jezero at Ls ∼ 155°.

Published
2023

32. One Martian Year of MEDA/TIRS observations at the Mars 2020 landing site

Author

Martinez, German, primary, Sebastian, Eduardo, additional, Smith, Michael, additional, Savijärvi, Hannu, additional, Gillespie, Hartzel, additional, Vicente-Retortillo, Alvaro, additional, Munguira, Asier, additional, Hueso, Ricardo, additional, Toledo, Daniel, additional, Tamppari, Leslie, additional, Newman, Claire, additional, Sanchez-Lavega, Agustin, additional, Lemmon, Mark, additional, Apestigue, Victor, additional, Arruego, Ignacio, additional, Fischer, Erik, additional, Pla-Garcia, Jorge, additional, Mora-Sotomayor, Luis, additional, de la Torre Juarez, Manuel, additional, and Rodriguez-Manfredi, Jose Antonio, additional

Published
2023
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34. THE FIRST FROST DETECTION CAMPAIGN BY THE MARS 2020 PERSEVERANCE ROVER: IMPLEMENTATION AND RESULTS

Author

Martínez, Germán, Lasue, Jérémie, Meslin, Pierre-Yves, Chide, Baptiste, Caravaca, Gwénaël, López-Reyes, Guillermo, Tamppari, Leslie K., Beyssac, Olivier, Polkko, J., Hieta, M., Genzer, M., Harri, A.-M., Newman, Claire, Gillespie, Hartzel, Fischer, Erik, Mora, Luis, Sebastián, Eduardo, Wiens, Roger, Rodríguez Manfredi, Jose, Lunar and Planetary Institute [Houston] (LPI), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Los Alamos National Laboratory (LANL), Universidad de Valladolid [Valladolid] (UVa), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Institut de minéralogie, de physique des matériaux et de cosmochimie (IMPMC), Muséum national d'Histoire naturelle (MNHN)-Institut de recherche pour le développement [IRD] : UR206-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Finnish Meteorological Institute (FMI), Aeolis Research, University of Michigan [Ann Arbor], University of Michigan System, Centro de Astrobiologia [Madrid] (CAB), Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, and Lunar and Planetary Institute

Subjects
Jezero crater, [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, SuperCam, [SDU]Sciences of the Universe [physics], [SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy, Mars 2020, Mars, [SDU.STU]Sciences of the Universe [physics]/Earth Sciences, frost
Abstract

International audience; Here we describe the first campaign launched by the Perseverance rover to detect frost during the first Martian year of operations (669 sols as of Jan 5, 2023). This campaign was conceived, developed and executed following lessons learnt from the Mars Science Laboratory Mission, where frost was likely detected [1].Between sols 546 and 548 during northern winter (Ls ~297), measurements of ground temperature and relative humidity by the Mars Environmental Dynamics Analyzer (MEDA, [2]) were used to predict frost formation, while SuperCam laser-induced breakdown spectroscopy (LIBS) and Raman spectrometer measurements [3,4] were used to detect frost formation on a target informally called Snowy Mountain. While the measured ground temperature fell below the estimated frost point, and therefore frost was predicted by MEDA, neither H enrichment in LIBS measurements nor Raman peaks associated with water ice were detected by SuperCam.

Published
2023

42. Underlining the Image Processing Techniques Used to Analyze Martian Water Ice Clouds Observed at Jezero Crater by the NavCam Instrument on board the Mars2020 Rover, Perseverance.

Author

Patel, Priya, primary, Coates, Andrew, additional, Tamppari, Leslie, additional, de la Torre Juárez, Manuel, additional, Lemmon, Mark, additional, Toledo, Daniel, additional, Wolff, Michael, additional, Moores, John, additional, Campbell, Charissa, additional, and Brown, Adrian, additional

Published
2022
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45. Surface Energy Budget, Albedo and Thermal Inertia at Jezero Crater, Mars, as Observed from the Mars 2020 MEDA Instrument

Author

Martinez, German, primary, Sebastian Martínez, Eduardo, additional, Vicente-Retortillo, Alvaro, additional, Smith, Michael D., additional, Johnson, Jeffrey R., additional, Fischer, Erik, additional, Savijärvi, Hannu, additional, Toledo, Daniel, additional, Hueso, Ricardo, additional, Mora Sotomayor, Luis, additional, Gillespie, Hartzel Edmond, additional, Munguira, Asier, additional, Sánchez-Lavega, Agustín, additional, Lemmon, Mark T, additional, Gómez, Felipe, additional, Polkko, Jouni, additional, Mandon, Lucia, additional, Apéstigue, Víctor, additional, Arruego, Ignacio, additional, Ramos, Miguel, additional, Conrad, Pamela G., additional, Newman, Claire, additional, de la Torre Juarez, Manuel, additional, Jordan, Francisco, additional, Tamppari, Leslie, additional, McConnochie, Timothy, additional, Harri, Ari-Matti, additional, Genzer, Maria, additional, Hieta, Maria, additional, Zorzano, Maria-Paz, additional, Siegler, Matthew Adam, additional, Prieto-Ballesteros, Olga, additional, Molina, Antonio, additional, and Rodriguez-Manfredi, Jose A., additional

Published
2022
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46. Convective vortices and dust devils detected and characterized by Mars 2020

Author

Hueso, Ricardo, primary, Newman, Claire, additional, del Rio-Gaztelurrutia, Teresa, additional, Munguira, Asier, additional, Sánchez-Lavega, Agustín, additional, Toledo, Daniel, additional, Apéstigue, Víctor, additional, Arruego, Ignacio, additional, Vicente-Retortillo, Alvaro, additional, Martinez, German, additional, Lemmon, Mark T, additional, Lorenz, Ralph D., additional, Richardson, Mark Ian, additional, Viúdez-Moreiras, Daniel, additional, de la Torre Juárez, Manuel, additional, Rodríguez-Manfredi, Jose Antonio, additional, Tamppari, Leslie, additional, Murdoch, Naomi, additional, Navarro López, Sara, additional, Gomez-Elvira, Javier, additional, Baker, Mariah, additional, Pla-García, Jorge, additional, Harri, Ari-Matti, additional, Hieta, Maria, additional, Genzer, Maria, additional, Polkko, Jouni, additional, Jaakonaho, Iina, additional, Mäkinen, Teemu J T, additional, Stott, Alexander, additional, Mimoun, David, additional, Chide, Baptiste, additional, Sebastian Martínez, Eduardo, additional, Banfield, Donald, additional, and Lepinette Malvitte, Alain, additional

Published
2022
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