Space Science Reviews最新文献

{"title":"Tidal Deformation and Dissipation Processes in Icy Worlds.","authors":"G Tobie, P Auclair-Desrotour, M Běhounková, M Kervazo, O Souček, K Kalousová","doi":"10.1007/s11214-025-01136-y","DOIUrl":"10.1007/s11214-025-01136-y","url":null,"abstract":"<p><p>Tidal interactions play a key role in the dynamics and evolution of icy worlds. The intense tectonic activity of Europa and the eruption activity on Enceladus are clear examples of the manifestation of tidal deformation and associated dissipation. While tidal heating has long been recognized as a major driver in the activity of these icy worlds, the mechanism controlling how tidal forces deform the different internal layers and produce heat by tidal friction still remains poorly constrained. As tidal forcing varies with orbital characteristics (distance to the central planet, eccentricity, obliquity), the contribution of tidal heating to the internal heat budget can strongly change over geological timescales. In some circumstances, the tidally-produced heat can result in internal melting and surface activity taking various forms. Even in the absence of significant heat production, tidal deformation can be used to probe the interior structure, the tidal response of icy moons being strongly sensitive to their hydrosphere structure. In the present paper, we review the methods to compute tidal deformation and dissipation in the different layers composing icy worlds. After summarizing the main principle of tidal deformation and the different rheological models used to model visco-elastic tidal response, we describe the dissipation processes expected in rock-dominated cores, subsurface oceans and icy shells and highlight the potential effects of tidal heating in terms of thermal evolution and activity. We finally anticipate how data collected by future missions to Jupiter's and Saturn's moons could be used to constrain their tidal response and the consequences for past and present activities.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"221 1","pages":"6"},"PeriodicalIF":9.1,"publicationDate":"2025-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11739232/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143011925","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":"Solar Wind Magnetosphere Ionosphere Link Explorer (SMILE): Science and Mission Overview.","authors":"Chi Wang, Graziella Branduardi-Raymont, C Philippe Escoubet, Colin Forsyth","doi":"10.1007/s11214-024-01126-6","DOIUrl":"https://doi.org/10.1007/s11214-024-01126-6","url":null,"abstract":"<p><p>The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) was proposed to the Chinese Academy of Science (CAS) and the European Space Agency (ESA) following a joint call for science missions issued in January 2015. SMILE was proposed by a team of European and Chinese scientists, led by two mission Co-PIs, one from China and one from Europe. SMILE was selected in June 2015, and its budget adopted by the Chinese Academy of Sciences in November 2016 and the ESA Science Programme Committee in March 2019, respectively. SMILE will investigate the connection between the Sun and the Earth using a new technique that will image the magnetopause and polar cusps: the key regions where the solar wind impinges on Earth's magnetic field. Simultaneously, SMILE will image the auroras borealis in an ultraviolet waveband, providing long-duration continuous observations of the northern polar regions. In addition, the ion and magnetic field characteristics of the magnetospheric lobes, magnetosheath and solar wind will be measured by the in-situ instrument package. Here, we present the science goals, instruments and planned orbit. In addition the Working Groups that are supporting the preparation of the mission and the coordination with other magnetospheric missions are described.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"221 1","pages":"9"},"PeriodicalIF":9.1,"publicationDate":"2025-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11772532/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143068031","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":"Jets Downstream of Collisionless Shocks: Recent Discoveries and Challenges.","authors":"Eva Krämer, Florian Koller, Jonas Suni, Adrian T LaMoury, Adrian Pöppelwerth, Georg Glebe, Tara Mohammed-Amin, Savvas Raptis, Laura Vuorinen, Stefan Weiss, Niki Xirogiannopoulou, Martin Archer, Xóchitl Blanco-Cano, Herbert Gunell, Heli Hietala, Tomas Karlsson, Ferdinand Plaschke, Luis Preisser, Owen Roberts, Cyril Simon Wedlund, Manuela Temmer, Zoltán Vörös","doi":"10.1007/s11214-024-01129-3","DOIUrl":"10.1007/s11214-024-01129-3","url":null,"abstract":"<p><p>Plasma flows with enhanced dynamic pressure, known as magnetosheath jets, are often found downstream of collisionless shocks. As they propagate through the magnetosheath, they interact with the surrounding plasma, shaping its properties, and potentially becoming geoeffective upon reaching the magnetopause. In recent years (since 2016), new research has produced vital results that have significantly enhanced our understanding on many aspects of jets. In this review, we summarise and discuss these findings. Spacecraft and ground-based observations, as well as global and local simulations, have contributed greatly to our understanding of the causes and effects of magnetosheath jets. First, we discuss recent findings on jet occurrence and formation, including in other planetary environments. New insights into jet properties and evolution are then examined using observations and simulations. Finally, we review the impact of jets upon interaction with the magnetopause and subsequent consequences for the magnetosphere-ionosphere system. We conclude with an outlook and assessment on future challenges. This includes an overview on future space missions that may prove crucial in tackling the outstanding open questions on jets in the terrestrial magnetosheath as well as other planetary and shock environments.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"221 1","pages":"4"},"PeriodicalIF":9.1,"publicationDate":"2025-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11680644/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142903543","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":"Effects of Oxytocin on Glutamate Mediated Neurotoxicity in Neuroblastoma Cell Culture.","authors":"Börte Gürbüz Özgür, Kamil Vural, Mehmet İbrahim Tuğlu","doi":"10.29399/npa.28377","DOIUrl":"10.29399/npa.28377","url":null,"abstract":"<p><strong>Introduction: </strong>We aimed to investigate the effects of oxytocin on neurite growth, cell viability, cell proliferation and apoptosis to demonstrate its neuroprotective effect on glutamate induced neurotoxicity in human neuroblastoma SH-SY5Y cell culture.</p><p><strong>Method: </strong>The effect of oxytocin on the toxic effects of glutamate in human neuroblastoma SH-SY5Y cell line with the Neurotoxicity Screening Test (NTT), apoptotic effects by Terminal Transferase dUTP Nick End Labeling (TUNEL) method and cell viability test by 3-(4.5-dimethylthiazol-2-yl)-2.5-diphenyltetrazolium bromide (MTT) method. In the NTT test; Neurotoxicity was induced by adding glutamate at a concentration of 32 μM to the cell culture. Oxytocin was added at 1, 3, 10, 30 and 100 μM concentrations and its effect on neurite elongation was investigated. It was demonstrated by TUNEL method that application of glutamate caused apoptosis. Afterwards, when glutamate and different doses of oxytocin were given, antiapoptotic effect was evaluated with the apoptotic index.</p><p><strong>Results: </strong>Glutamate was found to have a dose-dependent neurotoxic effect and reduced neurite elongation by 50% at a concentration of 32 μM. It was shown that the inhibition of neurite elongation caused by glutamate decreased in a dose-dependent manner by applying oxytocin. Especially oxytocin was found to significantly reduce neurite inhibition and show a neuroprotective effect starting from 10 μM concentrations. The concentration at which glutamate reduces cell proliferation by 50% was determined as 54 μM in MTT. Subsequently, it was observed that the adverse effect of glutamate on cell proliferation significantly decreased with oxytocin administration, depending on the dose.</p><p><strong>Conclusion: </strong>It was found that different concentrations of glutamate have a significant toxic effect on cell proliferation and viability, glutamate inhibits neurite elongation in a dose-dependent manner; oxytocin reduces neurite inhibition caused by glutamate, has a neuroprotective effect, increases cell viability and has antiapoptotic effects.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"187 1","pages":"24-29"},"PeriodicalIF":1.1,"publicationDate":"2024-02-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10943934/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"74735295","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":"Presolar Grains as Probes of Supernova Nucleosynthesis.","authors":"Nan Liu, Maria Lugaro, Jan Leitner, Bradley S Meyer, Maria Schönbächler","doi":"10.1007/s11214-024-01122-w","DOIUrl":"10.1007/s11214-024-01122-w","url":null,"abstract":"<p><p>We provide an overview of the isotopic signatures of presolar supernova grains, specifically focusing on ⁴⁴Ti-containing grains with robustly inferred supernova origins and their implications for nucleosynthesis and mixing mechanisms in supernovae. Recent technique advancements have enabled the differentiation between radiogenic (from ⁴⁴Ti decay) and nonradiogenic ⁴⁴Ca excesses in presolar grains, made possible by enhanced spatial resolution of Ca-Ti isotope analyses with the Cameca NanoSIMS (Nano-scale Secondary Ion Mass Spectrometer) instrument. Within the context of presolar supernova grain data, we discuss (<i>i</i>) the production of ⁴⁴Ti in supernovae and the impact of interstellar medium heterogeneities on the galactic chemical evolution of ⁴⁴Ca/⁴⁰Ca, (<i>ii</i>) the nucleosynthesis processes of neutron bursts and explosive H-burning in Type II supernovae, and (<i>iii</i>) challenges in identifying the progenitor supernovae for ⁵⁴Cr-rich presolar nanospinel grains. Drawing on constraints and insights derived from presolar supernova grain data, we also provide an overview of our current understanding of the roles played by various supernova types - including Type II, Type Ia, and electron capture supernovae - in accounting for the diverse array of nucleosynthetic isotopic variations identified in bulk meteorites and meteoritic components. We briefly overview the potential mechanisms that have been proposed to explain these nucleosynthetic variations by describing the transport and distribution of presolar dust carriers in the protoplanetary disk. We highlight existing controversies in the interpretation of presolar grain data and meteoritic nucleosynthetic isotopic variations, while also outlining potential directions for future research.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 8","pages":"88"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11557683/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142627949","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 Gravitational Lensing and Microlensing of Supernovae.","authors":"Sherry H Suyu, Ariel Goobar, Thomas Collett, Anupreeta More, Giorgos Vernardos","doi":"10.1007/s11214-024-01044-7","DOIUrl":"10.1007/s11214-024-01044-7","url":null,"abstract":"<p><p>Strong gravitational lensing and microlensing of supernovae (SNe) are emerging as a new probe of cosmology and astrophysics in recent years. We provide an overview of this nascent research field, starting with a summary of the first discoveries of strongly lensed SNe. We describe the use of the time delays between multiple SN images as a way to measure cosmological distances and thus constrain cosmological parameters, particularly the Hubble constant, whose value is currently under heated debates. New methods for measuring the time delays in lensed SNe have been developed, and the sample of lensed SNe from the upcoming Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to provide competitive cosmological constraints. Lensed SNe are also powerful astrophysical probes. We review the usage of lensed SNe to constrain SN progenitors, acquire high-z SN spectra through lensing magnifications, infer SN sizes via microlensing, and measure properties of dust in galaxies. The current challenge in the field is the rarity and difficulty in finding lensed SNe. We describe various methods and ongoing efforts to find these spectacular explosions, forecast the properties of the expected sample of lensed SNe from upcoming surveys particularly the LSST, and summarize the observational follow-up requirements to enable the various scientific studies. We anticipate the upcoming years to be exciting with a boom in lensed SN discoveries.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 1","pages":"13"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11297109/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141890169","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":"Apollo Next Generation Sample Analysis (ANGSA): an Apollo Participating Scientist Program to Prepare the Lunar Sample Community for Artemis.","authors":"C K Shearer, F M McCubbin, S Eckley, S B Simon, A Meshik, F McDonald, H H Schmitt, R A Zeigler, J Gross, J Mitchell, C Krysher, R V Morris, R Parai, B L Jolliff, J J Gillis-Davis, K H Joy, S K Bell, P G Lucey, L Sun, Z D Sharp, C Dukes, A Sehlke, A Mosie, J Allton, C Amick, J I Simon, T M Erickson, J J Barnes, M D Dyar, K Burgess, N Petro, D Moriarty, N M Curran, J E Elsila, R A Colina-Ruiz, T Kroll, D Sokaras, H A Ishii, J P Bradley, D Sears, B Cohen, O Pravdivseva, M S Thompson, C R Neal, R Hana, R Ketcham, K Welten","doi":"10.1007/s11214-024-01094-x","DOIUrl":"10.1007/s11214-024-01094-x","url":null,"abstract":"<p><p>As a first step in preparing for the return of samples from the Moon by the Artemis Program, NASA initiated the Apollo Next Generation Sample Analysis Program (ANGSA). ANGSA was designed to function as a low-cost sample return mission and involved the curation and analysis of samples previously returned by the Apollo 17 mission that remained unopened or stored under unique conditions for 50 years. These samples include the lower portion of a double drive tube previously sealed on the lunar surface, the upper portion of that drive tube that had remained unopened, and a variety of Apollo 17 samples that had remained stored at -27 °C for approximately 50 years. ANGSA constitutes the first preliminary examination phase of a lunar \"sample return mission\" in over 50 years. It also mimics that same phase of an Artemis surface exploration mission, its design included placing samples within the context of local and regional geology through new orbital observations collected since Apollo and additional new \"boots-on-the-ground\" observations, data synthesis, and interpretations provided by Apollo 17 astronaut Harrison Schmitt. ANGSA used new curation techniques to prepare, document, and allocate these new lunar samples, developed new tools to open and extract gases from their containers, and applied new analytical instrumentation previously unavailable during the Apollo Program to reveal new information about these samples. Most of the 90 scientists, engineers, and curators involved in this mission were not alive during the Apollo Program, and it had been 30 years since the last Apollo core sample was processed in the Apollo curation facility at NASA JSC. There are many firsts associated with ANGSA that have direct relevance to Artemis. ANGSA is the first to open a core sample previously sealed on the surface of the Moon, the first to extract and analyze lunar gases collected <i>in situ</i>, the first to examine a core that penetrated a lunar landslide deposit, and the first to process pristine Apollo samples in a glovebox at -20 °C. All the ANGSA activities have helped to prepare the Artemis generation for what is to come. The timing of this program, the composition of the team, and the preservation of unopened Apollo samples facilitated this generational handoff from Apollo to Artemis that sets up Artemis and the lunar sample science community for additional successes.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 6","pages":"62"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11335912/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142037012","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 Lunar Environment Heliophysics X-ray Imager (LEXI) Mission.","authors":"B M Walsh, K D Kuntz, S Busk, T Cameron, D Chornay, A Chuchra, M R Collier, C Connor, H K Connor, T E Cravens, N Dobson, M Galeazzi, H Kim, J Kujawski, C K Paw U, F S Porter, V Naldoza, R Nutter, R Qudsi, D G Sibeck, S Sembay, M Shoemaker, K Simms, N E Thomas, E Atz, G Winkert","doi":"10.1007/s11214-024-01063-4","DOIUrl":"https://doi.org/10.1007/s11214-024-01063-4","url":null,"abstract":"<p><p>The Lunar Environment heliospheric X-ray Imager (LEXI) is a wide field-of-view soft X-ray telescope developed to study solar wind-magnetosphere coupling. LEXI is part of the Blue Ghost 1 mission comprised of 10 payloads to be deployed on the lunar surface. LEXI monitors the dayside magnetopause position and shape as a function of time by observing soft X-rays (0.1-2 keV) emitted from solar wind charge-exchange between exospheric neutrals and high charge-state solar wind plasma in the dayside magnetosheath. Measurements of the shape and position of the magnetopause are used to test temporal models of meso- and macro-scale magnetic reconnection. To image the boundary, LEXI employs lobster-eye optics to focus X-rays to a microchannel plate detector with a 9.1<math><mmultiscripts><mo>×</mo><mprescripts></mprescripts><none></none><mo>∘</mo></mmultiscripts><msup><mn>9.1</mn><mo>∘</mo></msup></math> field of view.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 4","pages":"37"},"PeriodicalIF":10.3,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11093736/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140959508","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":"Time-Delay Cosmography: Measuring the Hubble Constant and Other Cosmological Parameters with Strong Gravitational Lensing.","authors":"S Birrer, M Millon, D Sluse, A J Shajib, F Courbin, S Erickson, L V E Koopmans, S H Suyu, T Treu","doi":"10.1007/s11214-024-01079-w","DOIUrl":"10.1007/s11214-024-01079-w","url":null,"abstract":"<p><p>Multiply lensed images of a same source experience a relative time delay in the arrival of photons due to the path length difference and the different gravitational potentials the photons travel through. This effect can be used to measure absolute distances and the Hubble constant ( <math><msub><mi>H</mi> <mn>0</mn></msub> </math> ) and is known as time-delay cosmography. The method is independent of the local distance ladder and early-universe physics and provides a precise and competitive measurement of <math><msub><mi>H</mi> <mn>0</mn></msub> </math> . With upcoming observatories, time-delay cosmography can provide a 1% precision measurement of <math><msub><mi>H</mi> <mn>0</mn></msub> </math> and can decisively shed light on the current reported 'Hubble tension'. This manuscript details the general methodology developed over the past decades in time-delay cosmography, discusses recent advances and results, and, foremost, provides a foundation and outlook for the next decade in providing accurate and ever more precise measurements with increased sample size and improved observational techniques.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 5","pages":"48"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11182856/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141427666","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 Lucy Thermal Emission Spectrometer (L'TES) Instrument.","authors":"P R Christensen, V E Hamilton, G L Mehall, S Anwar, H Bowles, S Chase, Z Farkas, T Fisher, A Holmes, I Kubik, I Lazbin, W O'Donnell, C Ortiz, D Pelham, S Rogers, K Shamordola, T Tourville, R Woodward","doi":"10.1007/s11214-023-01029-y","DOIUrl":"10.1007/s11214-023-01029-y","url":null,"abstract":"<p><p>The Lucy Thermal Emission Spectrometer (L'TES) will provide remote measurements of the thermophysical properties of the Trojan asteroids studied by the Lucy mission. L'TES is build-to-print hardware copy of the OTES instrument flown on OSIRIS-REx. It is a Fourier Transform spectrometer covering the spectral range 5.71-100 μm (1750-100 cm^-1) with spectral sampling intervals of 8.64, 17.3, and 34.6 cm^-1 and a 7.3-mrad field of view. The L'TES telescope is a 15.2-cm diameter Cassegrain telescope that feeds a flat-plate Michelson moving mirror mounted on a linear voice-coil motor assembly to a single uncooled deuterated l-alanine doped triglycine sulfate (DLATGS) pyroelectric detector. A significant firmware change from OTES is the ability to acquire interferograms of different length and spectral resolution with acquisition times of 0.5, 1, and 2 seconds. A single ∼0.851 μm laser diode is used in a metrology interferometer to provide precise moving mirror control and IR sampling at 772 Hz. The beamsplitter is a 38-mm diameter, 1-mm thick chemical vapor deposited diamond with an antireflection microstructure to minimize surface reflection. An internal calibration cone blackbody target, together with observations of space, provides radiometric calibration. The radiometric precision in a single spectrum is ≤2.2 × 10^-8 W cm^-2 sr^-1 /cm^-1 between 300 and 1350 cm^-1. The absolute temperature error is <2 K for scene temperatures >75 K. The overall L'TES envelope size is 37.6 × 29.0 × 30.4 cm, and the mass is 6.47 kg. The power consumption is 12.6 W average. L'TES was developed by Arizona State University with AZ Space Technologies developing the electronics. L'TES was integrated, tested, and radiometrically calibrated on the Arizona State University campus in Tempe, AZ. Initial data from space have verified the instrument's radiometric and spatial performance.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 1","pages":"1"},"PeriodicalIF":10.3,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10730683/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138831556","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}