Space Science Reviews最新文献

{"title":"The Comet Interceptor Mission.","authors":"Geraint H Jones, Colin Snodgrass, Cecilia Tubiana, Michael Küppers, Hideyo Kawakita, Luisa M Lara, Jessica Agarwal, Nicolas André, Nicholas Attree, Uli Auster, Stefano Bagnulo, Michele Bannister, Arnaud Beth, Neil Bowles, Andrew Coates, Luigi Colangeli, Carlos Corral van Damme, Vania Da Deppo, Johan De Keyser, Vincenzo Della Corte, Niklas Edberg, Mohamed Ramy El-Maarry, Sara Faggi, Marco Fulle, Ryu Funase, Marina Galand, Charlotte Goetz, Olivier Groussin, Aurélie Guilbert-Lepoutre, Pierre Henri, Satoshi Kasahara, Akos Kereszturi, Mark Kidger, Matthew Knight, Rosita Kokotanekova, Ivana Kolmasova, Konrad Kossacki, Ekkehard Kührt, Yuna Kwon, Fiorangela La Forgia, Anny-Chantal Levasseur-Regourd, Manuela Lippi, Andrea Longobardo, Raphael Marschall, Marek Morawski, Olga Muñoz, Antti Näsilä, Hans Nilsson, Cyrielle Opitom, Mihkel Pajusalu, Antoine Pommerol, Lubomir Prech, Nicola Rando, Francesco Ratti, Hanna Rothkaehl, Alessandra Rotundi, Martin Rubin, Naoya Sakatani, Joan Pau Sánchez, Cyril Simon Wedlund, Anamarija Stankov, Nicolas Thomas, Imre Toth, Geronimo Villanueva, Jean-Baptiste Vincent, Martin Volwerk, Peter Wurz, Arno Wielders, Kazuo Yoshioka, Konrad Aleksiejuk, Fernando Alvarez, Carine Amoros, Shahid Aslam, Barbara Atamaniuk, Jędrzej Baran, Tomasz Barciński, Thomas Beck, Thomas Behnke, Martin Berglund, Ivano Bertini, Marcin Bieda, Piotr Binczyk, Martin-Diego Busch, Andrei Cacovean, Maria Teresa Capria, Chris Carr, José María Castro Marín, Matteo Ceriotti, Paolo Chioetto, Agata Chuchra-Konrad, Lorenzo Cocola, Fabrice Colin, Chiaki Crews, Victoria Cripps, Emanuele Cupido, Alberto Dassatti, Björn J R Davidsson, Thierry De Roche, Jan Deca, Simone Del Togno, Frederik Dhooghe, Kerri Donaldson Hanna, Anders Eriksson, Andrey Fedorov, Estela Fernández-Valenzuela, Stefano Ferretti, Johan Floriot, Fabio Frassetto, Jesper Fredriksson, Philippe Garnier, Dorota Gaweł, Vincent Génot, Thomas Gerber, Karl-Heinz Glassmeier, Mikael Granvik, Benjamin Grison, Herbert Gunell, Tedjani Hachemi, Christian Hagen, Rajkumar Hajra, Yuki Harada, Johann Hasiba, Nico Haslebacher, Miguel Luis Herranz De La Revilla, Daniel Hestroffer, Tilak Hewagama, Carrie Holt, Stubbe Hviid, Iaroslav Iakubivskyi, Laura Inno, Patrick Irwin, Stavro Ivanovski, Jiri Jansky, Irmgard Jernej, Harald Jeszenszky, Jaime Jimenéz, Laurent Jorda, Mihkel Kama, Shingo Kameda, Michael S P Kelley, Kamil Klepacki, Tomáš Kohout, Hirotsugu Kojima, Tomasz Kowalski, Masaki Kuwabara, Michal Ladno, Gunter Laky, Helmut Lammer, Radek Lan, Benoit Lavraud, Monica Lazzarin, Olivier Le Duff, Qiu-Mei Lee, Cezary Lesniak, Zoe Lewis, Zhong-Yi Lin, Tim Lister, Stephen Lowry, Werner Magnes, Johannes Markkanen, Ignacio Martinez Navajas, Zita Martins, Ayako Matsuoka, Barbara Matyjasiak, Christian Mazelle, Elena Mazzotta Epifani, Mirko Meier, Harald Michaelis, Marco Micheli, Alessandra Migliorini, Aude-Lyse Millet, Fernando Moreno, Stefano Mottola, Bruno Moutounaick, Karri Muinonen, Daniel R Müller, Go Murakami, Naofumi Murata, Kamil Myszka, Shintaro Nakajima, Zoltan Nemeth, Artiom Nikolajev, Simone Nordera, Dan Ohlsson, Aire Olesk, Harald Ottacher, Naoya Ozaki, Christophe Oziol, Manish Patel, Aditya Savio Paul, Antti Penttilä, Claudio Pernechele, Joakim Peterson, Enrico Petraglio, Alice Maria Piccirillo, Ferdinand Plaschke, Szymon Polak, Frank Postberg, Herman Proosa, Silvia Protopapa, Walter Puccio, Sylvain Ranvier, Sean Raymond, Ingo Richter, Martin Rieder, Roberto Rigamonti, Irene Ruiz Rodriguez, Ondrej Santolik, Takahiro Sasaki, Rolf Schrödter, Katherine Shirley, Andris Slavinskis, Balint Sodor, Jan Soucek, Peter Stephenson, Linus Stöckli, Paweł Szewczyk, Gabor Troznai, Ludek Uhlir, Naoto Usami, Aris Valavanoglou, Jakub Vaverka, Wei Wang, Xiao-Dong Wang, Gaëtan Wattieaux, Martin Wieser, Sebastian Wolf, Hajime Yano, Ichiro Yoshikawa, Vladimir Zakharov, Tomasz Zawistowski, Paola Zuppella, Giovanna Rinaldi, Hantao Ji","doi":"10.1007/s11214-023-01035-0","DOIUrl":"10.1007/s11214-023-01035-0","url":null,"abstract":"<p><p>Here we describe the novel, multi-point Comet Interceptor mission. It is dedicated to the exploration of a little-processed long-period comet, possibly entering the inner Solar System for the first time, or to encounter an interstellar object originating at another star. The objectives of the mission are to address the following questions: What are the surface composition, shape, morphology, and structure of the target object? What is the composition of the gas and dust in the coma, its connection to the nucleus, and the nature of its interaction with the solar wind? The mission was proposed to the European Space Agency in 2018, and formally adopted by the agency in June 2022, for launch in 2029 together with the Ariel mission. Comet Interceptor will take advantage of the opportunity presented by ESA's F-Class call for fast, flexible, low-cost missions to which it was proposed. The call required a launch to a halo orbit around the Sun-Earth L2 point. The mission can take advantage of this placement to wait for the discovery of a suitable comet reachable with its minimum <math><mi>Δ</mi></math>V capability of <math><mn>600</mn><msup><mtext> ms</mtext><mrow><mo>-</mo><mn>1</mn></mrow></msup></math>. Comet Interceptor will be unique in encountering and studying, at a nominal closest approach distance of 1000 km, a comet that represents a near-pristine sample of material from the formation of the Solar System. It will also add a capability that no previous cometary mission has had, which is to deploy two sub-probes - B1, provided by the Japanese space agency, JAXA, and B2 - that will follow different trajectories through the coma. While the main probe passes at a nominal 1000 km distance, probes B1 and B2 will follow different chords through the coma at distances of 850 km and 400 km, respectively. The result will be unique, simultaneous, spatially resolved information of the 3-dimensional properties of the target comet and its interaction with the space environment. We present the mission's science background leading to these objectives, as well as an overview of the scientific instruments, mission design, and schedule.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 1","pages":"9"},"PeriodicalIF":10.3,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10808369/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139571374","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The Mapping Imaging Spectrometer for Europa (MISE).","authors":"Diana L Blaney, Karl Hibbitts, Serina Diniega, Ashley Gerard Davies, Roger N Clark, Robert O Green, Matthew Hedman, Yves Langevin, Jonathan Lunine, Thomas B McCord, Scott Murchie, Chris Paranicas, Frank Seelos, Jason M Soderblom, Morgan L Cable, Regina Eckert, David R Thompson, Samantha K Trumbo, Carl Bruce, Sarah R Lundeen, Holly A Bender, Mark C Helmlinger, Lori B Moore, Pantazis Mouroulis, Zachary Small, Hong Tang, Byron Van Gorp, Peter W Sullivan, Shannon Zareh, Jose I Rodriquez, Ian McKinley, Daniel V Hahn, Matthew Bowers, Ramsey Hourani, Brian A Bryce, Danielle Nuding, Zachery Bailey, Alessandro Rettura, Evan D Zarate","doi":"10.1007/s11214-024-01097-8","DOIUrl":"https://doi.org/10.1007/s11214-024-01097-8","url":null,"abstract":"<p><p>The Mapping Imaging Spectrometer for Europa (MISE) is an infrared compositional instrument that will fly on NASA's Europa Clipper mission to the Jupiter system. MISE is designed to meet the Level-1 science requirements related to the mission's composition science objective to \"understand the habitability of Europa's ocean through composition and chemistry\" and to contribute to the geology science and ice shell and ocean objectives, thereby helping Europa Clipper achieve its mission goal to \"explore Europa to investigate its habitability.\" MISE has a mass of 65 kg and uses an energy per flyby of 75.2 W-h. MISE will detect illumination from 0.8 to 5 μm with 10 nm spectral resolution, a spatial sampling of 25 m per pixel at 100 km altitude, and 300 cross-track pixels, enabling discrimination among the two principal states of water ice on Europa, identification of the main non-ice components of interest: salts, acids, and organics, and detection of trace materials as well as some thermal signatures. Furthermore, the spatial resolution and global coverage that MISE will achieve will be complemented by the higher spectral resolution of some Earth-based assets. MISE, combined with observations collected by the rest of the Europa Clipper payload, will enable significant advances in our understanding of how the large-scale structure of Europa's surface is shaped by geological processes and inform our understanding of the surface at microscale. This paper describes the planned MISE science investigations, instrument design, concept of operations, and data products.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 7","pages":"80"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11464581/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142475175","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Characterization of the Surfaces and Near-Surface Atmospheres of Ganymede, Europa and Callisto by JUICE.","authors":"Federico Tosi, Thomas Roatsch, André Galli, Ernst Hauber, Alice Lucchetti, Philippa Molyneux, Katrin Stephan, Nicholas Achilleos, Francesca Bovolo, John Carter, Thibault Cavalié, Giuseppe Cimò, Emiliano D'Aversa, Klaus Gwinner, Paul Hartogh, Hans Huybrighs, Yves Langevin, Emmanuel Lellouch, Alessandra Migliorini, Pasquale Palumbo, Giuseppe Piccioni, Jeffrey J Plaut, Frank Postberg, François Poulet, Kurt Retherford, Ladislav Rezac, Lorenz Roth, Anezina Solomonidou, Gabriel Tobie, Paolo Tortora, Cecilia Tubiana, Roland Wagner, Eva Wirström, Peter Wurz, Francesca Zambon, Marco Zannoni, Stas Barabash, Lorenzo Bruzzone, Michele Dougherty, Randy Gladstone, Leonid I Gurvits, Hauke Hussmann, Luciano Iess, Jan-Erik Wahlund, Olivier Witasse, Claire Vallat, Rosario Lorente","doi":"10.1007/s11214-024-01089-8","DOIUrl":"10.1007/s11214-024-01089-8","url":null,"abstract":"<p><p>We present the state of the art on the study of surfaces and tenuous atmospheres of the icy Galilean satellites Ganymede, Europa and Callisto, from past and ongoing space exploration conducted with several spacecraft to recent telescopic observations, and we show how the ESA JUICE mission plans to explore these surfaces and atmospheres in detail with its scientific payload. The surface geology of the moons is the main evidence of their evolution and reflects the internal heating provided by tidal interactions. Surface composition is the result of endogenous and exogenous processes, with the former providing valuable information about the potential composition of shallow subsurface liquid pockets, possibly connected to deeper oceans. Finally, the icy Galilean moons have tenuous atmospheres that arise from charged particle sputtering affecting their surfaces. In the case of Europa, plumes of water vapour have also been reported, whose phenomenology at present is poorly understood and requires future close exploration. In the three main sections of the article, we discuss these topics, highlighting the key scientific objectives and investigations to be achieved by JUICE. Based on a recent predicted trajectory, we also show potential coverage maps and other examples of reference measurements. The scientific discussion and observation planning presented here are the outcome of the JUICE Working Group 2 (WG2): \"<i>Surfaces and Near-surface Exospheres of the Satellites, dust and rings</i>\".</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 5","pages":"59"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11310297/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141917449","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The Need for Near-Earth Multi-Spacecraft Heliospheric Measurements and an Explorer Mission to Investigate Interplanetary Structures and Transients in the Near-Earth Heliosphere.","authors":"Noé Lugaz, Christina O Lee, Nada Al-Haddad, Robert J Lillis, Lan K Jian, David W Curtis, Antoinette B Galvin, Phyllis L Whittlesey, Ali Rahmati, Eftyhia Zesta, Mark Moldwin, Errol J Summerlin, Davin E Larson, Sasha Courtade, Richard French, Richard Hunter, Federico Covitti, Daniel Cosgrove, J D Prall, Robert C Allen, Bin Zhuang, Réka M Winslow, Camilla Scolini, Benjamin J Lynch, Rachael J Filwett, Erika Palmerio, Charles J Farrugia, Charles W Smith, Christian Möstl, Eva Weiler, Miho Janvier, Florian Regnault, Roberto Livi, Teresa Nieves-Chinchilla","doi":"10.1007/s11214-024-01108-8","DOIUrl":"10.1007/s11214-024-01108-8","url":null,"abstract":"<p><p>Based on decades of single-spacecraft measurements near 1 au as well as data from heliospheric and planetary missions, multi-spacecraft simultaneous measurements in the inner heliosphere on separations of 0.05-0.2 au are required to close existing gaps in our knowledge of solar wind structures, transients, and energetic particles, especially coronal mass ejections (CMEs), stream interaction regions (SIRs), high speed solar wind streams (HSS), and energetic storm particle (ESP) events. The Mission to Investigate Interplanetary Structures and Transients (MIIST) is a concept for a small multi-spacecraft mission to explore the near-Earth heliosphere on these critical scales. It is designed to advance two goals: (a) to determine the spatiotemporal variations and the variability of solar wind structures, transients, and energetic particle fluxes in near-Earth interplanetary (IP) space, and (b) to advance our fundamental knowledge necessary to improve space weather forecasting from <i>in situ</i> data. We present the scientific rationale for this proposed mission, the science requirements, payload, implementation, and concept of mission operation that address a key gap in our knowledge of IP structures and transients within the cost, launch, and schedule limitations of the NASA Heliophysics Small Explorers program.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 7","pages":"73"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11415466/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142295964","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Advanced Methods for Analyzing in-Situ Observations of Magnetic Reconnection.","authors":"H Hasegawa, M R Argall, N Aunai, R Bandyopadhyay, N Bessho, I J Cohen, R E Denton, J C Dorelli, J Egedal, S A Fuselier, P Garnier, V Génot, D B Graham, K J Hwang, Y V Khotyaintsev, D B Korovinskiy, B Lavraud, Q Lenouvel, T C Li, Y-H Liu, B Michotte de Welle, T K M Nakamura, D S Payne, S M Petrinec, Y Qi, A C Rager, P H Reiff, J M Schroeder, J R Shuster, M I Sitnov, G K Stephens, M Swisdak, A M Tian, R B Torbert, K J Trattner, S Zenitani","doi":"10.1007/s11214-024-01095-w","DOIUrl":"10.1007/s11214-024-01095-w","url":null,"abstract":"<p><p>There is ample evidence for magnetic reconnection in the solar system, but it is a nontrivial task to visualize, to determine the proper approaches and frames to study, and in turn to elucidate the physical processes at work in reconnection regions from in-situ measurements of plasma particles and electromagnetic fields. Here an overview is given of a variety of single- and multi-spacecraft data analysis techniques that are key to revealing the context of in-situ observations of magnetic reconnection in space and for detecting and analyzing the diffusion regions where ions and/or electrons are demagnetized. We focus on recent advances in the era of the Magnetospheric Multiscale mission, which has made electron-scale, multi-point measurements of magnetic reconnection in and around Earth's magnetosphere.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 6","pages":"68"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11369046/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142133806","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Strong Lensing by Galaxies.","authors":"A J Shajib, G Vernardos, T E Collett, V Motta, D Sluse, L L R Williams, P Saha, S Birrer, C Spiniello, T Treu","doi":"10.1007/s11214-024-01105-x","DOIUrl":"https://doi.org/10.1007/s11214-024-01105-x","url":null,"abstract":"<p><p>Strong gravitational lensing at the galaxy scale is a valuable tool for various applications in astrophysics and cosmology. Some of the primary uses of galaxy-scale lensing are to study elliptical galaxies' mass structure and evolution, constrain the stellar initial mass function, and measure cosmological parameters. Since the discovery of the first galaxy-scale lens in the 1980s, this field has made significant advancements in data quality and modeling techniques. In this review, we describe the most common methods for modeling lensing observables, especially imaging data, as they are the most accessible and informative source of lensing observables. We then summarize the primary findings from the literature on the astrophysical and cosmological applications of galaxy-scale lenses. We also discuss the current limitations of the data and methodologies and provide an outlook on the expected improvements in both areas in the near future.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 8","pages":"87"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11549236/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142627960","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Geologic Constraints on the Formation and Evolution of Saturn's Mid-Sized Moons.","authors":"Alyssa Rose Rhoden, Sierra N Ferguson, William Bottke, Julie C Castillo-Rogez, Emily Martin, Michael Bland, Michelle Kirchoff, Marco Zannoni, Nicolas Rambaux, Julien Salmon","doi":"10.1007/s11214-024-01084-z","DOIUrl":"10.1007/s11214-024-01084-z","url":null,"abstract":"<p><p>Saturn's mid-sized icy moons have complex relationships with Saturn's interior, the rings, and with each other, which can be expressed in their shapes, interiors, and geology. Observations of their physical states can, thus, provide important constraints on the ages and formation mechanism(s) of the moons, which in turn informs our understanding of the formation and evolution of Saturn and its rings. Here, we describe the cratering records of the mid-sized moons and the value and limitations of their use for constraining the histories of the moons. We also discuss observational constraints on the interior structures of the moons and geologically-derived inferences on their thermal budgets through time. Overall, the geologic records of the moons (with the exception of Mimas) include evidence of epochs of high heat flows, short- and long-lived subsurface oceans, extensional tectonics, and considerable cratering. Curiously, Mimas presents no clear evidence of an ocean within its surface geology, but its rotation and orbit indicate a present-day ocean. While the moons need not be primordial to produce the observed levels of interior evolution and geologic activity, there is likely a minimum age associated with their development that has yet to be determined. Uncertainties in the populations impacting the moons makes it challenging to further constrain their formation timeframes using craters, whereas the characteristics of their cores and other geologic inferences of their thermal evolutions may help narrow down their potential histories. Disruptive collisions may have also played an important role in the formation and evolution of Saturn's mid-sized moons, and even the rings of Saturn, although more sophisticated modeling is needed to determine the collision conditions that produce rings and moons that fit the observational constraints. Overall, the existence and physical characteristics of Saturn's mid-sized moons provide critical benchmarks for the development of formation theories.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 5","pages":"55"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11255024/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141736325","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Editorial to the Topical Collection: Solar and Stellar Dynamos: a New Era","authors":"Manfred Schüssler, Robert Cameron, Paul Charbonneau, M. Dikpati, Hideyuki Hotta, Leonid Kitchatinov","doi":"10.1007/s11214-023-01037-y","DOIUrl":"https://doi.org/10.1007/s11214-023-01037-y","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"2 4","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138948388","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Sedimentary Processes on Venus","authors":"Lynn M. Carter, M. S. Gilmore, R. Ghail, Paul K. Byrne, S. Smrekar, Terra M. Ganey, N. Izenberg","doi":"10.1007/s11214-023-01033-2","DOIUrl":"https://doi.org/10.1007/s11214-023-01033-2","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":" 3","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138611218","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Initial on-Orbit Results from the GOES-18 Spacecraft Science Magnetometer","authors":"P. Loto’aniu, A. Davis, A. Jarvis, M. Grotenhuis, F. J. Rich, S. Califf, F. Inceoglu, A. Pacini, H. J. Singer","doi":"10.1007/s11214-023-01032-3","DOIUrl":"https://doi.org/10.1007/s11214-023-01032-3","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":" 4","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138615982","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}