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Artykuły w czasopismach na temat "Perseverance rover"
Abhishek, Sujith M.S., Kamalesh Pulluru, Jeevan D, Dr. Sindhu Sree M, Dr. Pavithra G i Dr. T.C.Manjunath. "Mars Exploration Perseverance Rover". international journal of engineering technology and management sciences 7, nr 3 (2023): 436–39. http://dx.doi.org/10.46647/ijetms.2023.v07i03.56.
Pełny tekst źródłaTaylor, E. Jennings, i Gregory S. Jackson. "Perseverance Rover Lands on Mars". Electrochemical Society Interface 30, nr 2 (1.06.2021): 79–80. http://dx.doi.org/10.1149/2.f11212if.
Pełny tekst źródłaJohnson, Paul, i Sanjeev Gupta. "Sanjeev Gupta: Perseverance rover mission scientist". Astronomy & Geophysics 62, nr 1 (1.02.2021): 1.43. http://dx.doi.org/10.1093/astrogeo/atab045.
Pełny tekst źródłaZheng, Naihuan, Chunyu Ding, Yan Su i Roberto Orosei. "Water Ice Resources on the Shallow Subsurface of Mars: Indications to Rover-Mounted Radar Observation". Remote Sensing 16, nr 5 (27.02.2024): 824. http://dx.doi.org/10.3390/rs16050824.
Pełny tekst źródłaAtri, Dimitra, Nour Abdelmoneim, Dattaraj B. Dhuri i Mathilde Simoni. "Diurnal variation of the surface temperature of Mars with the Emirates Mars Mission: a comparison with Curiosity and Perseverance rover measurements". Monthly Notices of the Royal Astronomical Society: Letters 518, nr 1 (26.10.2022): L1—L6. http://dx.doi.org/10.1093/mnrasl/slac094.
Pełny tekst źródłaMangold, N., S. Gupta, O. Gasnault, G. Dromart, J. D. Tarnas, S. F. Sholes, B. Horgan i in. "Perseverance rover reveals an ancient delta-lake system and flood deposits at Jezero crater, Mars". Science 374, nr 6568 (5.11.2021): 711–17. http://dx.doi.org/10.1126/science.abl4051.
Pełny tekst źródłaDoyle, S. "News - Briefing. The Measure of: Perseverance Mars rover". Engineering & Technology 15, nr 4 (1.05.2020): 92–93. http://dx.doi.org/10.1049/et.2020.0433.
Pełny tekst źródłaJaakonaho, Iina, Maria Hieta, Maria Genzer, Jouni Polkko, Terhi Mäkinen, Agustín Sánchez-Lavega, Ricardo Hueso i in. "Pressure sensor for the Mars 2020 Perseverance rover". Planetary and Space Science 239 (grudzień 2023): 105815. http://dx.doi.org/10.1016/j.pss.2023.105815.
Pełny tekst źródłaVoosen, Paul. "Mars rover probes ancient shoreline for signs of life". Science 383, nr 6689 (22.03.2024): 1277–78. http://dx.doi.org/10.1126/science.adp3268.
Pełny tekst źródłaCrane, Leah. "The Perseverance rover is on its way to Mars". New Scientist 247, nr 3294 (sierpień 2020): 14. http://dx.doi.org/10.1016/s0262-4079(20)31353-1.
Pełny tekst źródłaRozprawy doktorskie na temat "Perseverance rover"
Knutsen, Elise Wright. "A spectroscopic study of water vapor on Mars". Electronic Thesis or Diss., université Paris-Saclay, 2023. http://www.theses.fr/2023UPASP136.
Pełny tekst źródłaWater vapor is a minor species in the atmosphere of Mars, yet plays a significant role in shaping the current climate of the planet. Water was once much more abundant, evident today from features such as dry riverbeds, outflow channels and hydrated minerals, prompting extensive research into its disappearance. Atmospheric water vapor has been monitored and studied extensively in the past decades, and most of its chemical and dynamical behaviors are now known, but one of the few remaining challenges is related to its vertical distribution. Missions like Mars Express, MAVEN, and the ExoMars Trace gas Orbiter ushered in a new era in water vertical profile studies and have all provided valuable insights, but access to the lowest part of the atmosphere has remained limited. Water vapor is commonly assumed to have a uniform distribution below the cloud condensation layer, but some measurements are challenging this view, suggesting a more complex profile near the surface, where regolith-atmosphere exchanges might play a role.The main work of this thesis is related to water vapor, with the objective of investigating the near-surface water content in both a seasonal and geographical context. To do this, we have explored two unconventional techniques; a spectral synergy method applied to nadir observations, and infrared spectroscopic surface observations. This thesis also contains one chapter about Martian space weather, which contains a collection of smaller projects conducted throughout the duration of this PhD.The spectral synergy uses near- and thermal-infrared spectra from SPICAM and PFS respectively on Mars Express. Water vapor is retrieved simultaneously from both spectral bands, and since these two wavelength intervals are sensitive to separate atmospheric altitude regions, the resulting increased degree of freedom allows for information on the vertical distribution to be gained. The synergy was applied to almost 200 000 co-located observations, sampled across roughly eight Mars year. Composite climatologies of very accurate column abundances and vertical profiles were assembled. The column abundances were in good agreement with previous studies, but the results exhibited some significant differences from the Mars Climate Database, both with respect to the column abundances and the vertical distribution. The spring sublimation peak was observed to be less extreme, and the sublimation onset occurred later than the model. The vertical confinement is observed to be stronger compared to the model at almost all seasons and latitudes, and the distribution is rarely uniform. The confinement as a function of season and latitude was studied in details, and a latitudinal wave-like behavior was discovered in both hemispheres, as well as a prevailing double-layer structure in the northern hemisphere.For the surface observations, we make use of the infrared spectrometer part of SuperCam on the Perseverance rover, and conduct so-called passive sky measurements. To date, we have 64 observations taken regularly across one Martian year. In the passive sky technique, infrared spectra are acquired at two elevation angles and then ratioed in order to remove continuum and instrumental effects. The resulting spectrum is mainly sensitive to the atmosphere below 15 km, and can therefore directly probe altitudes rarely accessible from orbit. Here we outline the progress made so far regarding data processing and the development of a retrieval pipeline. A forward model and minimization routine has been composed, and is currently undergoing testing and further maturing
Royer, Clément. "Etude des performances des spectromètres miniatures infrarouge à base d'AOTF Pre-launch radiometric calibration of the infrared spectrometer onboard SuperCam for the Mars2020 rover". Thesis, université Paris-Saclay, 2020. http://www.theses.fr/2020UPASP085.
Pełny tekst źródłaDuring the past 20 years, reflectance near-infrared spectroscopy applied to planetary exploration has brought a new sight on planetary surfaces, mainly thanks to the discovery of Martian phyllosilicates by OMEGA (Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité) on-board the European probe Mars Express, and CRISM (Compact Reconnaissance Infrared Spectrometer for Mars) equipping the probe Mars Reconnaissance Orbiter, in 2005 and 2007. These two space missions have paved the way to the thorough study of the surface of planetary bodies in the near-infrared (between 1 and 5 µm), searching for their mineral composition and past/present alteration processes.In order to board a infrared spectrometer in every interplanetary, and even in-situ probes, it is necessary to design a new generation of instruments both compact and efficient. The AOTF-based (Acousto-Optic Tunable Filter) monochromator is a key technology to fulfill this objective. The two spectrometers studied in the frame of my PhD thesis, IRS (Infrared Spectrometer) on-board the SuperCam instrument on Perseverance rover, and ExoCam, in R&T at the IAS (Institut d'Astrophysique Spatiale), benefit from this subsystem to produce high quality science data with a small volume occupation.My PhD thesis has been thus divided in two main parts: the preparation and performance of the radiometric calibration of the IRS/SuperCam qualification and flight models, and the design of an infrared observation simulator for the future Perseverance operations; the study of the performance of hyperspectral near-infrared imagery using an AOTF in transmission, throught the ExoCam R&T program, along with the development of a radiometric model of the R&T breadboard allowing to extrapolate lab results to future space operations
Chide, Baptiste. "Le premier microphone sur Mars : contribution à la spectroscopie de plasma induit par laser et à la science atmosphérique". Thesis, Toulouse, ISAE, 2020. http://www.theses.fr/2020ESAE0041.
Pełny tekst źródłaIn February 2021 the Mars 2020 Perseverance rover will land in Jezero to search for traces of past life.Part of the Perseverance payload, the SuperCam instrument suite includes four spectroscopy techniques,a high resolution imager and a microphone. This microphone will be the first microphone to record audible acoustic waves on the surface on Mars between 100 Hz to 10 kHz. It will open a new field of investigation which is the subject of this thesis. The scientific objectives of this thesis are organized around the sounds that will be recorded by this microphone : atmospheric phenomena in the close vicinity of the rover and artificial noises generated by SuperCam itself. Among the latest, the laser-induced breakdown spectroscopy technique (LIBS) ablates Martian rocks and soils with a pulsed laser. It creates an acoustic signal due tothe expansion of this plasma. These two topics are experimentally explored thanks to the development of laboratory test benches that simulate the conditions likely to be encountered by the microphone on Mars.On the one hand a LIBS setup under Mars atmosphere is used to compare acoustic signal from several minerals. A metrological study of the sensitivity of the acoustic signal with respect to LIBS experimental parameters is conducted : the acoustic energy is proportional to the CO2 background pressure and to the irradiance deposited on the sample. These two relationships will help to normalize the acoustic signal from multiple LIBS targets on Mars. Moreover, it is noticed that the decrease of the acoustic energy along a LIBS burst is linearly linked to the ablated volume. The decrease rate is correlated to the rock hardness.It provides new information relative to the ablation process that is independent from the LIBS emission spectrum. It could be used to better characterize geologic targets and rock, in particular the ones with asurface coating or a weathering rind.On the other hand, a test campaign in a Martian wind tunnel is dedicated to link wind properties withwind-induced signal recorded by the microphone. It is demonstrated that the microphone can determinethe flow velocity by studying the low frequency range of the acoustic spectrum whereas the wind directioncan be retrieved by looking at the high frequency range. An in situ cross-calibration with the weather station on board Perseverance, MEDA, will be required to validate these results. It is also shown that the synchronization of the microphone with the LIBS laser can be used to measure the speed of sound and therefore to estimate the atmospheric temperature close to the surface of Mars.This work also describes some progresses in the microphone development including the performances' validation, the implementation of operating modes and the preparation of SuperCam operations at the surface of Mars
Książki na temat "Perseverance rover"
Owen, Ruth. Mars Rover: Perseverance. Ruby Tuesday Books Limited, 2022.
Znajdź pełny tekst źródłaOwen, Ruth. Mars Rover: Perseverance. Ruby Tuesday Books Limited, 2022.
Znajdź pełny tekst źródłaNASA Mars Rover Perseverance: Mars 2020. Independently Published, 2020.
Znajdź pełny tekst źródłaSaving Tracker Perseverance Mars Rover Landing Day Commemorative. Independently Published, 2021.
Znajdź pełny tekst źródłaLawrence Sinclair, Stewart. Space Rover. Bloomsbury Publishing Plc, 2024. http://dx.doi.org/10.5040/9781501399985.
Pełny tekst źródłaCLARKE, Latoya. Office Organizer - Dare Mighty Things Perseverance Mars Rover Landing Pattern. Independently Published, 2021.
Znajdź pełny tekst źródłaSaving Tracker Perseverance the New NASA Mars Rover 202Mission: 6 X 9 Size, 114 Pages. Independently Published, 2021.
Znajdź pełny tekst źródłaDaily Fitness Sheet Perseverance Mars Rover Landing 202Nasa Mission: 6 X 9 Size, 114 Pages. Independently Published, 2021.
Znajdź pełny tekst źródłaBody Progress Tracker Perseverance Mars Rover Landing 202Nasa Mission: 6 X 9 Size, 114 Pages. Independently Published, 2021.
Znajdź pełny tekst źródłaHexagonal Graph Paper Perseverance Mars Rover Landing 202Nasa Mission: 6 X 9 Size, 114 Pages. Independently Published, 2021.
Znajdź pełny tekst źródłaStreszczenia konferencji na temat "Perseverance rover"
Schulte, Mitchell. "THE MARS 2020 PERSEVERANCE ROVER MISSION". W Northeastern Section - 57th Annual Meeting - 2022. Geological Society of America, 2022. http://dx.doi.org/10.1130/abs/2022ne-373862.
Pełny tekst źródłaDuffy, Elizabeth, Brian Franz, Matthew Orzewalla, Greg Mathy, David Parsons, Louise Jandura, Robert Moeller i Todd Krafchak. "Mars 2020 Perseverance Rover SHERLOC Instrument Isolation System". W 2022 IEEE Aerospace Conference (AERO). IEEE, 2022. http://dx.doi.org/10.1109/aero53065.2022.9843817.
Pełny tekst źródłaHickman-Lewis, Keyron, Christopher Herd, Tanja Bosak, Kathryn Stack, Vivian Sun, Kathleen Benison, Andrew Czaja i in. "Perseverance rover notional caches for Mars Sample Return". W Goldschmidt2021. France: European Association of Geochemistry, 2021. http://dx.doi.org/10.7185/gold2021.4400.
Pełny tekst źródłaDodge, Randy, David Parsons, Mohamed Abid, Kyle Chrystal i Boyan Kartolov. "Dynamics associated with the Corer on M2020 Perseverance Rover". W 2021 IEEE Aerospace Conference. IEEE, 2021. http://dx.doi.org/10.1109/aero50100.2021.9438361.
Pełny tekst źródłaLange, Robert, Luke Walker, Matt Lenda, Chaz Morantz, Torsten Zorn, Farah Alibay, Lauren DuCharme i Justin Koch. "Mars 2020 Perseverance Rover Surface Operations Commissioning Phase Overview". W 2022 IEEE Aerospace Conference (AERO). IEEE, 2022. http://dx.doi.org/10.1109/aero53065.2022.9843314.
Pełny tekst źródłaDeliz, Ivy, Andrea Connell, Chet Joswig, Jessica J. Marquez i Bob Kanefsky. "COCPIT: Collaborative Activity Planning Software for Mars Perseverance Rover". W 2022 IEEE Aerospace Conference (AERO). IEEE, 2022. http://dx.doi.org/10.1109/aero53065.2022.9843397.
Pełny tekst źródłaCzaja, Andrew, Sunanda Sharma, Abigail Allwood, Kathleen Benison, Andrea Corpolongo, Felipe Gómez, Lisa E. Mayhew, Mark Sephton, Sandra Siljeström i Amy Williams. "SAMPLING POTENTIAL BIOSIGNATURES WITH THE MARS 2020 PERSEVERANCE ROVER". W Joint 56th Annual North-Central/ 71st Annual Southeastern Section Meeting - 2022. Geological Society of America, 2022. http://dx.doi.org/10.1130/abs/2022nc-375223.
Pełny tekst źródłaVerma, Vandi, Justin Huang, Philip Bailey, Joseph Carsten i Douglas Klein. "Perseverance Rover Collision Model for a range of Autonomous Behaviors". W 2022 IEEE Aerospace Conference (AERO). IEEE, 2022. http://dx.doi.org/10.1109/aero53065.2022.9843632.
Pełny tekst źródłaBailey, Philip, Douglas Klein, Torsten Zorn, Thirupathi Srinivasan, Ethan W. Schaler, Sawyer Brooks, Luther Beegle i in. "Perseverance Rover Robotic Arm and Turret Mounted Instruments Surface Commissioning". W 2022 IEEE Aerospace Conference (AERO). IEEE, 2022. http://dx.doi.org/10.1109/aero53065.2022.9843702.
Pełny tekst źródłaSiegfriedt, Rebekah Sosland, Emily Bohannon, Andre Girerd, Ian Trettel i Brian Roth. "Making or Breaking a Rover- Systems Engineering Parameters On-Board the Mars 2020 Perseverance Rover". W 2022 IEEE Aerospace Conference (AERO). IEEE, 2022. http://dx.doi.org/10.1109/aero53065.2022.9843325.
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