Space Science Reviews最新文献

{"title":"Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum","authors":"N. Raouafi, L. Matteini, J. Squire, S. Badman, M. Velli, K. Klein, C. H. Chen, W. Matthaeus, A. Szabo, M. Linton, R. Allen, J. Szalay, R. Bruno, R. Decker, M. Akhavan-Tafti, O. Agapitov, S. Bale, R. Bandyopadhyay, K. Battams, L. Bervcivc, S. Bourouaine, T. Bowen, C. Cattell, B. Chandran, R. Chhiber, C. Cohen, R. D’Amicis, J. Giacalone, P. Hess, R. A. Howard, T. Horbury, V. Jagarlamudi, C. Joyce, J. Kasper, J. Kinnison, R. Laker, P. Liewer, D. Malaspina, I. Mann, D. McComas, T. Niembro-Hernandez, O. Panasenco, P. Pokorn'y, A. Pusack, M. Pulupa, J. C. Perez, P. Riley, A. Rouillard, C. Shi, G. Stenborg, A. Tenerani, J. Verniero, N. Viall, A. Vourlidas, B. Wood, Lloyd D. Woodham, T. Woolley","doi":"10.1007/s11214-023-00952-4","DOIUrl":"https://doi.org/10.1007/s11214-023-00952-4","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 1","pages":"1-140"},"PeriodicalIF":10.3,"publicationDate":"2023-01-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"45780556","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":"Herbig Stars","authors":"S. Brittain, I. Kamp, G. Meeus, R. Oudmaijer, L. Waters","doi":"10.1007/s11214-023-00949-z","DOIUrl":"https://doi.org/10.1007/s11214-023-00949-z","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 1","pages":"1-102"},"PeriodicalIF":10.3,"publicationDate":"2023-01-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"47040519","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":"Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Revisited: In-Flight Calibrations, Lessons Learned and Scientific Advances.","authors":"Matina Gkioulidou, Donald G Mitchell, Jerry W Manweiler, Louis J Lanzerotti, Andrew J Gerrard, Aleksandr Y Ukhorskiy, Kunihiro Keika, Christopher G Mouikis, Lynn M Kistler","doi":"10.1007/s11214-023-00991-x","DOIUrl":"10.1007/s11214-023-00991-x","url":null,"abstract":"<p><p>The Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) on both the Van Allen Probes spacecraft is a time-of-flight versus total energy instrument that provided ion composition data over the ring current energy (∼7 keV to ∼1 MeV), and electrons over the energy range ∼25 keV to ∼1 MeV throughout the duration of the mission (2012 - 2019). In this paper we present instrument calibrations, implemented after the Van Allen Probes mission was launched. In particular, we discuss updated rate dependent corrections, possible contamination by \"accidentals\" rates, and caveats concerning the use of certain products. We also provide a summary of the major advances in ring current science, obtained from RBSPICE observations, and their implications for the future of inner magnetosphere exploration.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 8","pages":"80"},"PeriodicalIF":10.3,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10684722/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138462723","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":"Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer.","authors":"Leigh N Fletcher, Thibault Cavalié, Davide Grassi, Ricardo Hueso, Luisa M Lara, Yohai Kaspi, Eli Galanti, Thomas K Greathouse, Philippa M Molyneux, Marina Galand, Claire Vallat, Olivier Witasse, Rosario Lorente, Paul Hartogh, François Poulet, Yves Langevin, Pasquale Palumbo, G Randall Gladstone, Kurt D Retherford, Michele K Dougherty, Jan-Erik Wahlund, Stas Barabash, Luciano Iess, Lorenzo Bruzzone, Hauke Hussmann, Leonid I Gurvits, Ondřej Santolik, Ivana Kolmasova, Georg Fischer, Ingo Müller-Wodarg, Giuseppe Piccioni, Thierry Fouchet, Jean-Claude Gérard, Agustin Sánchez-Lavega, Patrick G J Irwin, Denis Grodent, Francesca Altieri, Alessandro Mura, Pierre Drossart, Josh Kammer, Rohini Giles, Stéphanie Cazaux, Geraint Jones, Maria Smirnova, Emmanuel Lellouch, Alexander S Medvedev, Raphael Moreno, Ladislav Rezac, Athena Coustenis, Marc Costa","doi":"10.1007/s11214-023-00996-6","DOIUrl":"10.1007/s11214-023-00996-6","url":null,"abstract":"<p><p>ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital tour tailored to maximise observing opportunities. We review the Jupiter science enabled by the JUICE mission, building on the legacy of discoveries from the Galileo, Cassini, and Juno missions, alongside ground- and space-based observatories. We focus on remote sensing of the climate, meteorology, and chemistry of the atmosphere and auroras from the cloud-forming weather layer, through the upper troposphere, into the stratosphere and ionosphere. The Jupiter orbital tour provides a wealth of opportunities for atmospheric and auroral science: global perspectives with its near-equatorial and inclined phases, sampling all phase angles from dayside to nightside, and investigating phenomena evolving on timescales from minutes to months. The remote sensing payload spans far-UV spectroscopy (50-210 nm), visible imaging (340-1080 nm), visible/near-infrared spectroscopy (0.49-5.56 μm), and sub-millimetre sounding (near 530-625 GHz and 1067-1275 GHz). This is coupled to radio, stellar, and solar occultation opportunities to explore the atmosphere at high vertical resolution; and radio and plasma wave measurements of electric discharges in the Jovian atmosphere and auroras. Cross-disciplinary scientific investigations enable JUICE to explore coupling processes in giant planet atmospheres, to show how the atmosphere is connected to (i) the deep circulation and composition of the hydrogen-dominated interior; and (ii) to the currents and charged particle environments of the external magnetosphere. JUICE will provide a comprehensive characterisation of the atmosphere and auroras of this archetypal giant planet.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 7","pages":"53"},"PeriodicalIF":9.1,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10511624/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"41179955","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":"Exploring the Interior of Europa with the Europa Clipper.","authors":"James H Roberts,&nbsp;William B McKinnon,&nbsp;Catherine M Elder,&nbsp;Gabriel Tobie,&nbsp;John B Biersteker,&nbsp;Duncan Young,&nbsp;Ryan S Park,&nbsp;Gregor Steinbrügge,&nbsp;Francis Nimmo,&nbsp;Samuel M Howell,&nbsp;Julie C Castillo-Rogez,&nbsp;Morgan L Cable,&nbsp;Jacob N Abrahams,&nbsp;Michael T Bland,&nbsp;Chase Chivers,&nbsp;Corey J Cochrane,&nbsp;Andrew J Dombard,&nbsp;Carolyn Ernst,&nbsp;Antonio Genova,&nbsp;Christopher Gerekos,&nbsp;Christopher Glein,&nbsp;Camilla D Harris,&nbsp;Hamish C F C Hay,&nbsp;Paul O Hayne,&nbsp;Matthew Hedman,&nbsp;Hauke Hussmann,&nbsp;Xianzhe Jia,&nbsp;Krishan Khurana,&nbsp;Walter S Kiefer,&nbsp;Randolph Kirk,&nbsp;Margaret Kivelson,&nbsp;Justin Lawrence,&nbsp;Erin J Leonard,&nbsp;Jonathan I Lunine,&nbsp;Erwan Mazarico,&nbsp;Thomas B McCord,&nbsp;Alfred McEwen,&nbsp;Carol Paty,&nbsp;Lynnae C Quick,&nbsp;Carol A Raymond,&nbsp;Kurt D Retherford,&nbsp;Lorenz Roth,&nbsp;Abigail Rymer,&nbsp;Joachim Saur,&nbsp;Kirk Scanlan,&nbsp;Dustin M Schroeder,&nbsp;David A Senske,&nbsp;Wencheng Shao,&nbsp;Krista Soderlund,&nbsp;Elizabeth Spiers,&nbsp;Marshall J Styczinski,&nbsp;Paolo Tortora,&nbsp;Steven D Vance,&nbsp;Michaela N Villarreal,&nbsp;Benjamin P Weiss,&nbsp;Joseph H Westlake,&nbsp;Paul Withers,&nbsp;Natalie Wolfenbarger,&nbsp;Bonnie Buratti,&nbsp;Haje Korth,&nbsp;Robert T Pappalardo","doi":"10.1007/s11214-023-00990-y","DOIUrl":"10.1007/s11214-023-00990-y","url":null,"abstract":"<p><p>The Galileo mission to Jupiter revealed that Europa is an ocean world. The Galileo magnetometer experiment in particular provided strong evidence for a salty subsurface ocean beneath the ice shell, likely in contact with the rocky core. Within the ice shell and ocean, a number of tectonic and geodynamic processes may operate today or have operated at some point in the past, including solid ice convection, diapirism, subsumption, and interstitial lake formation. The science objectives of the Europa Clipper mission include the characterization of Europa's interior; confirmation of the presence of a subsurface ocean; identification of constraints on the depth to this ocean, and on its salinity and thickness; and determination of processes of material exchange between the surface, ice shell, and ocean. Three broad categories of investigation are planned to interrogate different aspects of the subsurface structure and properties of the ice shell and ocean: magnetic induction, subsurface radar sounding, and tidal deformation. These investigations are supplemented by several auxiliary measurements. Alone, each of these investigations will reveal unique information. Together, the synergy between these investigations will expose the secrets of the Europan interior in unprecedented detail, an essential step in evaluating the habitability of this ocean world.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 6","pages":"46"},"PeriodicalIF":10.3,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10457249/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"10108291","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":"Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory.","authors":"Susanne Aalto,&nbsp;Cara Battersby,&nbsp;Gordon Chin,&nbsp;Leslie K Hunt,&nbsp;Dimitra Rigopoulou,&nbsp;Antony A Stark,&nbsp;Serena Viti,&nbsp;Christopher K Walker","doi":"10.1007/s11214-023-00948-0","DOIUrl":"https://doi.org/10.1007/s11214-023-00948-0","url":null,"abstract":"<p><p>The <i>Orbiting Astronomical Satellite for Investigating Stellar Systems (OASIS)</i>, a proposed Astrophysics MIDEX-class mission concept, has an innovative 14-meter diameter inflatable primary mirror that will provide the sensitivity to study far-infrared continuum and line emission from galaxies at all redshifts with high spectral resolution heterodyne receivers. <i>OASIS</i> will have the sensitivity to follow the water trail from galaxies to the comets that create oceans. It will bring an understanding of the role of water in galaxy evolution and its part of the oxygen budget, by measuring water emission from local to intermediate redshift galaxies, observations that have not been possible from the ground. Observation of the ground-state HD line will accurately measure gas mass in a wide variety of astrophysical objects. Thanks to its exquisite spatial resolution and sensitivity, <i>OASIS</i> will, during its one-year baseline mission, detect water in galaxies with unprecedented statistical significance. This paper reviews the extragalactic science achievable and planned with <i>OASIS</i>.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 1","pages":"9"},"PeriodicalIF":10.3,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9895007/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"10673815","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 Relativistic Proton Spectrometer: A Review of Sensor Performance, Applications, and Science.","authors":"J E Mazur,&nbsp;T P O'Brien,&nbsp;M D Looper","doi":"10.1007/s11214-023-00962-2","DOIUrl":"https://doi.org/10.1007/s11214-023-00962-2","url":null,"abstract":"<p><p>The Relativistic Proton Spectrometer (RPS) on the Van Allen Probes spacecraft was a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from <math><mo>∼</mo> <mn>60</mn> <mspace></mspace> <mtext>MeV</mtext></math> to <math><mo>∼</mo> <mn>2000</mn> <mspace></mspace> <mtext>MeV</mtext></math> . RPS provided new information about the inner Van Allen belt: a nearby region of space that had been relatively unexplored because of the difficulties of making charged particle measurements there and the associated hazards to satellite operations. We met the primary mission objective of providing accurate data for the AP9 radiation specification model at the high energies where there were little to no data prior to the Van Allen Probes mission. Along the way, we were able to demonstrate the long-term stability of parts of the Inner Belt by comparison with short-lived space science missions that operated decades prior to Van Allen Probes. The most significant surprises were the agreement between RPS and some of those historical measurements and the discovery of a trapped population of <math><mo>></mo> <mn>30</mn> <mspace></mspace> <mtext>MeV</mtext></math> leptons at the outer edge of the inner belt. This end-of-mission paper summarizes the instrument performance, calibration, data products, and specific science and engineering results, and includes suggestions for future investigations of intense radiation fields like those found within the inner belt.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 3","pages":"26"},"PeriodicalIF":10.3,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10076393/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"9273556","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":"Simulations of Solar and Stellar Dynamos and Their Theoretical Interpretation.","authors":"Petri J Käpylä,&nbsp;Matthew K Browning,&nbsp;Allan Sacha Brun,&nbsp;Gustavo Guerrero,&nbsp;Jörn Warnecke","doi":"10.1007/s11214-023-01005-6","DOIUrl":"10.1007/s11214-023-01005-6","url":null,"abstract":"<p><p>We review the state of the art of three dimensional numerical simulations of solar and stellar dynamos. We summarize fundamental constraints of numerical modelling and the techniques to alleviate these restrictions. Brief summary of the relevant observations that the simulations seek to capture is given. We survey the current progress of simulations of solar convection and the resulting large-scale dynamo. We continue to studies that model the Sun at different ages and to studies of stars of different masses and evolutionary stages. Both simulations and observations indicate that rotation, measured by the Rossby number which is the ratio of rotation period and convective turnover time, is a key ingredient in setting the overall level and characteristics of magnetic activity. Finally, efforts to understand global 3D simulations in terms of mean-field dynamo theory are discussed.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 7","pages":"58"},"PeriodicalIF":10.3,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10567938/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"41238587","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":"Magnetic Field Modeling and Visualization of the Europa Clipper Spacecraft.","authors":"Corey J Cochrane, Neil Murphy, Carol A Raymond, John B Biersteker, Katherine Dang, Xianzhe Jia, Haje Korth, Pablo Narvaez, Jodie B Ream, Benjamin P Weiss","doi":"10.1007/s11214-023-00974-y","DOIUrl":"10.1007/s11214-023-00974-y","url":null,"abstract":"<p><p>The goal of NASA's Europa Clipper Mission is to investigate the habitability of the subsurface ocean within the Jovian moon Europa using a suite of ten investigations. The Europa Clipper Magnetometer (ECM) and Plasma Instrument for Magnetic Sounding (PIMS) investigations will be used in unison to characterize the thickness and electrical conductivity of Europa's subsurface ocean and the thickness of the ice shell by sensing the induced magnetic field, driven by the strong time-varying magnetic field of the Jovian environment. However, these measurements will be obscured by the magnetic field originating from the Europa Clipper spacecraft. In this work, a magnetic field model of the Europa Clipper spacecraft is presented, characterized with over 260 individual magnetic sources comprising various ferromagnetic and soft-magnetic materials, compensation magnets, solenoids, and dynamic electrical currents flowing within the spacecraft. This model is used to evaluate the magnetic field at arbitrary points around the spacecraft, notably at the locations of the three fluxgate magnetometer sensors and four Faraday cups which make up ECM and PIMS, respectively. The model is also used to evaluate the magnetic field uncertainty at these locations via a Monte Carlo approach. Furthermore, both linear and non-linear gradiometry fitting methods are presented to demonstrate the ability to reliably disentangle the spacecraft field from the ambient using an array of three fluxgate magnetometer sensors mounted along an 8.5-meter (m) long boom. The method is also shown to be useful for optimizing the locations of the magnetometer sensors along the boom. Finally, we illustrate how the model can be used to visualize the magnetic field lines of the spacecraft, thus providing very insightful information for each investigation.</p><p><strong>Supplementary information: </strong>The online version contains supplementary material available at 10.1007/s11214-023-00974-y.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 4","pages":"34"},"PeriodicalIF":9.1,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10220138/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"9710424","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":"Investigating Europa's Habitability with the Europa Clipper.","authors":"Steven D Vance, Kathleen L Craft, Everett Shock, Britney E Schmidt, Jonathan Lunine, Kevin P Hand, William B McKinnon, Elizabeth M Spiers, Chase Chivers, Justin D Lawrence, Natalie Wolfenbarger, Erin J Leonard, Kirtland J Robinson, Marshall J Styczinski, Divya M Persaud, Gregor Steinbrügge, Mikhail Y Zolotov, Lynnae C Quick, Jennifer E C Scully, Tracy M Becker, Samuel M Howell, Roger N Clark, Andrew J Dombard, Christopher R Glein, Olivier Mousis, Mark A Sephton, Julie Castillo-Rogez, Francis Nimmo, Alfred S McEwen, Murthy S Gudipati, Insoo Jun, Xianzhe Jia, Frank Postberg, Krista M Soderlund, Catherine M Elder","doi":"10.1007/s11214-023-01025-2","DOIUrl":"10.1007/s11214-023-01025-2","url":null,"abstract":"<p><p>The habitability of Europa is a property within a system, which is driven by a multitude of physical and chemical processes and is defined by many interdependent parameters, so that its full characterization requires collaborative investigation. To explore Europa as an integrated system to yield a complete picture of its habitability, the Europa Clipper mission has three primary science objectives: (1) characterize the ice shell and ocean including their heterogeneity, properties, and the nature of surface-ice-ocean exchange; (2) characterize Europa's composition including any non-ice materials on the surface and in the atmosphere, and any carbon-containing compounds; and (3) characterize Europa's geology including surface features and localities of high science interest. The mission will also address several cross-cutting science topics including the search for any current or recent activity in the form of thermal anomalies and plumes, performing geodetic and radiation measurements, and assessing high-resolution, co-located observations at select sites to provide reconnaissance for a potential future landed mission. Synthesizing the mission's science measurements, as well as incorporating remote observations by Earth-based observatories, the James Webb Space Telescope, and other space-based resources, to constrain Europa's habitability, is a complex task and is guided by the mission's Habitability Assessment Board (HAB).</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 8","pages":"81"},"PeriodicalIF":9.1,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10687213/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138478607","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}