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Articles de revues sur le sujet "Volatiles Elements"
Tian, Zhen, Tomáš Magna, James M. D. Day, Klaus Mezger, Erik E. Scherer, Katharina Lodders, Remco C. Hin, Piers Koefoed, Hannah Bloom et Kun Wang. « Potassium isotope composition of Mars reveals a mechanism of planetary volatile retention ». Proceedings of the National Academy of Sciences 118, no 39 (20 septembre 2021) : e2101155118. http://dx.doi.org/10.1073/pnas.2101155118.
Texte intégralDay, James M. D., Frédéric Moynier et Charles K. Shearer. « Late-stage magmatic outgassing from a volatile-depleted Moon ». Proceedings of the National Academy of Sciences 114, no 36 (21 août 2017) : 9547–51. http://dx.doi.org/10.1073/pnas.1708236114.
Texte intégralZhang, Youxue. « Review of melt inclusions in lunar rocks : constraints on melt and mantle composition and magmatic processes ». European Journal of Mineralogy 36, no 1 (26 janvier 2024) : 123–38. http://dx.doi.org/10.5194/ejm-36-123-2024.
Texte intégralChen, Zuxing, Landry Soh Tamehe, Haiyan Qi, Yuxiang Zhang, Zhigang Zeng et Mingjiang Cai. « Using Apatite to Track Volatile Evolution in the Shallow Magma Chamber below the Yonaguni Knoll IV Hydrothermal Field in the Southwestern Okinawa Trough ». Journal of Marine Science and Engineering 11, no 3 (9 mars 2023) : 583. http://dx.doi.org/10.3390/jmse11030583.
Texte intégralMiller, Johanna L. « Krypton isotopes tell the early story of Earth’s life-giving elements ». Physics Today 75, no 3 (1 mars 2022) : 16–18. http://dx.doi.org/10.1063/pt.3.4956.
Texte intégralLiu, Xuena, Jinghua Guo, Zijing Chen, Kun Xu et Kang Xu. « Detection of Volatile Compounds and Their Contribution to the Nutritional Quality of Chinese and Japanese Welsh Onions (Allium fistulosum L.) ». Horticulturae 10, no 5 (26 avril 2024) : 446. http://dx.doi.org/10.3390/horticulturae10050446.
Texte intégralDegruyter, Wim, Andrea Parmigiani, Christian Huber et Olivier Bachmann. « How do volatiles escape their shallow magmatic hearth ? » Philosophical Transactions of the Royal Society A : Mathematical, Physical and Engineering Sciences 377, no 2139 (7 janvier 2019) : 20180017. http://dx.doi.org/10.1098/rsta.2018.0017.
Texte intégralDay, James M. D., et Frederic Moynier. « Evaporative fractionation of volatile stable isotopes and their bearing on the origin of the Moon ». Philosophical Transactions of the Royal Society A : Mathematical, Physical and Engineering Sciences 372, no 2024 (13 septembre 2014) : 20130259. http://dx.doi.org/10.1098/rsta.2013.0259.
Texte intégralNunes, Ana R., Ana C. Gonçalves, Edgar Pinto, Filipa Amaro, José D. Flores-Félix, Agostinho Almeida, Paula Guedes de Pinho, Amílcar Falcão, Gilberto Alves et Luís R. Silva. « Mineral Content and Volatile Profiling of Prunus avium L. (Sweet Cherry) By-Products from Fundão Region (Portugal) ». Foods 11, no 5 (4 mars 2022) : 751. http://dx.doi.org/10.3390/foods11050751.
Texte intégralMarty, Bernard. « Origins and Early Evolution of the Atmosphere and the Oceans ». Geochemical Perspectives 9, no 2 (octobre 2020) : 135–313. http://dx.doi.org/10.7185/geochempersp.9.2.
Texte intégralThèses sur le sujet "Volatiles Elements"
Collins, S. J. « Degassing of volatiles and semi-volatile trace elements at basaltic volcanoes ». Thesis, University of Cambridge, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.597860.
Texte intégralGomez-Ulla, Rubira Alejandra. « Historical eruptions of Lanzarote, Canary Islands : Inference of magma source and melt generation from olivine and its melt inclusions ». Thesis, Université Clermont Auvergne (2017-2020), 2018. http://www.theses.fr/2018CLFAC023.
Texte intégralThe study of oceanic island basalts (OIB) reveals the complexity of the mantle, which composition is highly variable. Deciphering the source lithologies and processes involved in the OIB formation is challenging since the magmas are transformed on their way to the surface. This is especially critical at Canary Islands where the lithosphere is thought to be remarkably thick (>110 km Fullea et al., 2015). In order to better constrain the composition of primitive magmas and the plausible mantle lithologies involved, two historical eruptions recorded at Lanzarote island, Timanfaya 1730-1736 and 1824 eruptions have been investigated. Indeed, these two eruptions offer a unique opportunity to investigate the mechanisms of magma generation and composition in the context of mantle heterogeneity. The Timanfaya, 1730-1736 historical eruption emitted magmas that evolved from basanites through alkali basalts, finally reaching tholeiitic compositions at the end of the eruption. In 1824 the last eruption on the island produced extremely volatile-rich basanite. The heterogeneity of the mantle is demonstrated to the extreme in Lanzarote where a single eruption exhibits compositional variations similar to the span of the OIB worldwide. The extreme heterogeneity is systematic from whole rock lava and tephra at eruption scale but amplified at mineral and melt inclusion scale within a single tephra sample of the eruption.The use of trace element concentrations and ratios of olivine (e.g. Ni, Mn, and Ca) are valuable indicators of the mantle source lithology, namely, the fractionation-corrected Ni x (FeO/MgO) and Fe/Mn as probes of olivine absent or present lithologies, often taken as pyroxenite-derived component in mixtures of primary melts. The measured trace element concentrations in olivine from the 1730-1736 and 1824 eruptions reveal variable mantle lithologies involved in the magma generation with time. Higher Ni and lower Mn and Ca contents are expected when melting Ol-free source, such as pyroxenite lithologies. The basanites exhibit the largest variation covering the range of olivine in MORB and OIB worldwide whereas later produced alkali-basalts and tholeites have values typically expected from pyroxenite derived melts. The Fo content decreases systematically with time during the 1730-36 eruption and the proportion of silica-saturated primary melt increased in the parental magma mixture with time. At the end of the eruption, tholeiite magmas crystallized olivine with lower Fo content, whereas those concentrations of Mn and Ca increased together with Ca/Al at relatively uniform Ni x (FeO/MgO) and Fe/Mn, all of which is readily explained by increased decompression melting at slightly lower temperature. The basanite from the eruption that took place in 1824 has olivine with the highest Fo content and trace element variability expanding the range of the Timanfaya basanite. The fact that Lanzarote basanites contain olivine with trace element systematic spanning that of MORB and pyroxenite melt is explained by CO2-flux melting of a lithologically heterogeneous source, generating the diverse compositions. In addition, early reactive porous flow through the depleted oceanic lithosphere and equilibration with harzburgite restite caused Ni depletion of the earliest percolating pyroxenite melt from which olivine crystallized and probably leaving dunite channels. After the channel formation mantle nodules could be brought to the surface. The fact that olivine compositions and basanite magma were reproduced approximately a century later may reflect episodic carbonatic fluxing in the slowly uprising Canarian mantle plume. (...)
Severs, Matthew Jeremiah. « Applications of Melt Inclusions to Problems in Igneous Petrogenesis ». Diss., Virginia Tech, 2007. http://hdl.handle.net/10919/28310.
Texte intégralPh. D.
Debret, Baptiste. « Serpentinites, vecteurs des circulations fluides et des transferts chimiques de l'océanisation à la subduction : exemple dans les Alpes occidentales ». Phd thesis, Université Blaise Pascal - Clermont-Ferrand II, 2013. http://tel.archives-ouvertes.fr/tel-01037950.
Texte intégralDeligny, Cécile. « Origine des éléments volatils et chronologie de leur accrétion au sein du Système Solaire interne : Apport de l'analyse in-situ des achondrites ». Electronic Thesis or Diss., Université de Lorraine, 2021. http://www.theses.fr/2021LORR0329.
Texte intégralVolatile elements such as hydrogen and nitrogen control the evolution of planetary bodies and their atmospheres, and are essential elements for the development of life on Earth. Nevertheless, the origin of volatile elements and the timing of their accretion by terrestrial planets formed in the inner solar system remains a subject of debate and controversy in planetary science. To answer these questions, the isotopic ratios of hydrogen (D/H) and nitrogen (15N/14N) are powerful tools to trace the origin (solar, chondritic or cometary) of volatile elements trapped in planetary bodies. Therefore, to constrain the source(s) of volatile elements trapped in rocky planets, we analyzed hydrogen and nitrogen contents and isotopic compositions by ion microprobe (LGSIMS) in achondrites that originate from asteroids or from planets that are assumed to have formed in the inner solar system. These meteorites preserve a record of the initial stages of the formation of their parent bodies and can constrain the early evolution of planetary volatile elements. In-situ analysis by SIMS is a quasi-non-destructive technique, which permits to measure the abundance and the isotopic composition of volatile elements of different phases in terrestrial, extraterrestrial and synthetic samples. The recent development of the protocol of nitrogen analysis in silicate samples by ion probe allows us to target tens of micron- sized objects (i.e., glassy melt inclusions). Volatile elements were measured in melt inclusions trapped in minerals and in interstitial glasses. Although the analysis of nitrogen in aubrites was unsuccessful, the analysis performed on Martian meteorites and angrites revealed the presence of a large amount of water and nitrogen within these meteorites. In particular, the study of angrites and more precisely the meteorite D'Orbigny allowed us to highlight the presence of water and nitrogen having isotopic composition similar to those of the primitive meteorites formed in the outer solar system (i.e., CM-like carbonaceous chondrites). These results imply that these volatile elements must have been present in the inner solar system within the first ~4 Ma after CAI formation (i.e., the first solids to form in the solar system) and may have been trapped by the terrestrial planets during their formation. Furthermore, the analysis of Martian meteorites and more particularly of Chassigny revealed the presence of nitrogen with an isotopic composition enriched in 15N compared to enstatite chondrites and terrestrial diamonds which are believed to record the most primitive value of nitrogen on Earth
Leroy, Clémence. « L'iode et le xénon dans les magmas : deux comportements différents ». Thesis, Paris 6, 2016. http://www.theses.fr/2016PA066094/document.
Texte intégralThe presence of magmas at depth helps to constrain past and actual geological processes. Magmas (i.e. silicate melts) participate in geochemical cycles of volatile elements, as vectors of chemical transfers. We study two complementary volatile elements: iodine (I), a halogen, and xenon (Xe), a noble gas. Their extinct 129I/129Xe isotopic system (half-life of 15.7Ma) is used to date Hadean processes and Earth’s atmosphere formation since the atmosphere originated from the Magma Ocean’s evolution. However, little is known about the behavior of both iodine and xenon in silicate melts at depth, under HT and HP conditions. Our experimental protocol aims at elucidating the incorporation process of xenon and iodine in silicate melts, and their solubility. To understand the incorporation of iodine and xenon in magmas, the structure of silicate melts was investigated by in situ diamond anvil cells and Paris-Edinburgh press experiments coupled with X-ray diffraction characterization. Iodine and xenon’s solubility, along with water content are obtained by PIXE and ERDA methods using a nuclear microprobe. At high pressure, iodine has a high solubility (about few wt.%) in magmas. Preliminary results on iodine incorporation in basaltic melt show an absence of covalent bond. At high pressure and temperature conditions (T>300°C – P>1GPa), xenon forms a Xe-O covalent bond with the oxygens of the 6-membered-rings of the melt network. Its solubility in silicate melts is also high (about 4wt.% in haplogranite melts at 1600°C and 3.5GPa). Considering the xenon and iodine differential behavior in melts at depth, a revision of dating models in xenon and iodine cycles must be considered
Rutter, P. « A new non-volatile MNOS memory element ». Thesis, University of Southampton, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.377953.
Texte intégralAldridge, Simon. « Studies of some volatile compounds of main group elements ». Thesis, University of Oxford, 1996. http://ora.ox.ac.uk/objects/uuid:832a8ba8-4b6f-45f3-8a23-403efa9cd6e1.
Texte intégralLeroy, Clémence. « L'iode et le xénon dans les magmas : deux comportements différents ». Electronic Thesis or Diss., Paris 6, 2016. https://accesdistant.sorbonne-universite.fr/login?url=https://theses-intra.sorbonne-universite.fr/2016PA066094.pdf.
Texte intégralThe presence of magmas at depth helps to constrain past and actual geological processes. Magmas (i.e. silicate melts) participate in geochemical cycles of volatile elements, as vectors of chemical transfers. We study two complementary volatile elements: iodine (I), a halogen, and xenon (Xe), a noble gas. Their extinct 129I/129Xe isotopic system (half-life of 15.7Ma) is used to date Hadean processes and Earth’s atmosphere formation since the atmosphere originated from the Magma Ocean’s evolution. However, little is known about the behavior of both iodine and xenon in silicate melts at depth, under HT and HP conditions. Our experimental protocol aims at elucidating the incorporation process of xenon and iodine in silicate melts, and their solubility. To understand the incorporation of iodine and xenon in magmas, the structure of silicate melts was investigated by in situ diamond anvil cells and Paris-Edinburgh press experiments coupled with X-ray diffraction characterization. Iodine and xenon’s solubility, along with water content are obtained by PIXE and ERDA methods using a nuclear microprobe. At high pressure, iodine has a high solubility (about few wt.%) in magmas. Preliminary results on iodine incorporation in basaltic melt show an absence of covalent bond. At high pressure and temperature conditions (T>300°C – P>1GPa), xenon forms a Xe-O covalent bond with the oxygens of the 6-membered-rings of the melt network. Its solubility in silicate melts is also high (about 4wt.% in haplogranite melts at 1600°C and 3.5GPa). Considering the xenon and iodine differential behavior in melts at depth, a revision of dating models in xenon and iodine cycles must be considered
Sarafian, Adam Robert 1986. « Water and volatile element accretion to the inner planets ». Thesis, Massachusetts Institute of Technology, 2018. http://hdl.handle.net/1721.1/115785.
Texte intégralCataloged from PDF version of thesis.
Includes bibliographical references.
This thesis investigates the timing and source(s) of water and volatile elements to the inner solar system by studying the basaltic meteorites angrites and eucrites. In chapters 2 and 3, I present the results from angrite meteorites. Chapter 2 examines the water and volatile element content of the angrite parent body and I suggest that some water and other volatile elements accreted to inner solar system bodies by ~2 Myr after the start of the solar system. Chapter 3 examines the D/H of this water and I suggest it is derived from carbonaceous chondrites. Chapter 4, 5, 6, and 7 addresses eucrite meteorites. Chapter 4 expands on existing models to explain geochemical trends observed in eucrites. In Chapter 5, I examine the water and F content of the eucrite parent body, 4 Vesta. In chapter 6, I determine the source of water for 4 Vesta and determine that carbonaceous chondrites delivered water to this body. Chapter 7 discusses degassing on 4 Vesta while it was forming.
by Adam Robert Sarafian.
Ph. D.
Livres sur le sujet "Volatiles Elements"
Kallenbach, R., T. Encrenaz, J. Geiss, K. Mauersberger, T. C. Owen et F. Robert, dir. Solar System History from Isotopic Signatures of Volatile Elements. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8.
Texte intégralB, McConnell James, United States. Dept. of the Army., US Army Signal Center and Fort Gordon. Environmental and Natural Resources Management Office. et Geological Survey (U.S.), dir. Trace elements and semi-volatile organic compounds in bed sediments from streams and impoundments at Fort Gordon, Georgia. Atlanta, Ga : U.S. Dept. of the Interior, U.S. Geological Survey, 2000.
Trouver le texte intégralB, Lowenstern Jacob, et Geological Survey (U.S.), dir. Major-element, trace-element, and volatile concentrations in silicate melt inclusions from the tuff of Pine Grove, Wah Wah Mountains, Utah. [Menlo Park, Calif.?] : U.S. Dept. of the Interior, U.S. Geological Survey, 1994.
Trouver le texte intégralB, Lowenstern Jacob, et Geological Survey (U.S.), dir. Major-element, trace-element, and volatile concentrations in silicate melt inclusions from the tuff of Pine Grove, Wah Wah Mountains, Utah. [Menlo Park, Calif.?] : U.S. Dept. of the Interior, U.S. Geological Survey, 1994.
Trouver le texte intégralB, Lowenstern Jacob, et Geological Survey (U.S.), dir. Major-element, trace-element, and volatile concentrations in silicate melt inclusions from the tuff of Pine Grove, Wah Wah Mountains, Utah. [Menlo Park, Calif.?] : U.S. Dept. of the Interior, U.S. Geological Survey, 1994.
Trouver le texte intégralB, Lowenstern Jacob, et Geological Survey (U.S.), dir. Major-element, trace-element, and volatile concentrations in silicate melt inclusions from the tuff of Pine Grove, Wah Wah Mountains, Utah. [Menlo Park, Calif.?] : U.S. Dept. of the Interior, U.S. Geological Survey, 1994.
Trouver le texte intégralB, Lowenstern Jacob, et Geological Survey (U.S.), dir. Major-element, trace-element, and volatile concentrations in silicate melt inclusions from the tuff of Pine Grove, Wah Wah Mountains, Utah. [Menlo Park, Calif.?] : U.S. Dept. of the Interior, U.S. Geological Survey, 1994.
Trouver le texte intégralHoughton, Robert L. Volatile trace-element concentrations in snowmelt contributions to streams monitored by hydrologic bench-mark network stations in the conterminous United States where average annual snowfall exceeds 12 inches. Bismarck, N.D : U.S. Dept. of the Interior, Geological Survey, 1985.
Trouver le texte intégralB, McConnell James, United States. Dept. of the Army, US Army Signal Center and Fort Gordon. Environmental and Natural Resources Management Office et Geological Survey (U.S.), dir. Trace elements and semi-volatile organic compounds in bed sediments from streams and impoundments at Fort Gordon, Georgia. Atlanta, Ga : U.S. Dept. of the Interior, U.S. Geological Survey, 2000.
Trouver le texte intégralB, McConnell James, United States. Dept. of the Army, US Army Signal Center and Fort Gordon. Environmental and Natural Resources Management Office et Geological Survey (U.S.), dir. Trace elements and semi-volatile organic compounds in bed sediments from streams and impoundments at Fort Gordon, Georgia. Atlanta, Ga : U.S. Dept. of the Interior, U.S. Geological Survey, 2000.
Trouver le texte intégralChapitres de livres sur le sujet "Volatiles Elements"
Jambon, Albert. « Chapter 12. EARTH DEGASSING AND LARGE-SCALE GEOCHEMICAL CYCLING OF VOLATILE ELEMENTS ». Dans Volatiles in Magmas, sous la direction de Michael R. Carroll et John R. Holloway, 479–518. Berlin, Boston : De Gruyter, 1994. http://dx.doi.org/10.1515/9781501509674-019.
Texte intégralBecker, R. H., R. N. Clayton, E. M. Galimov, H. Lammer, B. Marty, R. O. Pepin et R. Wieler. « Isotopic Signatures of Volatiles in Terrestrial Planets ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 377–410. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_22.
Texte intégralOtt, Ulrich. « Isotopes of Volatiles in Pre-Solar Grains ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 33–48. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_3.
Texte intégralGeiss, Johannes, et George Gloeckler. « Isotopic Composition of H, He and Ne in the Protosolar Cloud ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 3–18. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_1.
Texte intégralAltwegg, Kathrin, et Dominique Bockelée-Morvan. « Isotopic Abundances in Comets ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 139–54. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_10.
Texte intégralMessenger, S., F. J. Stadermann, C. Floss, L. R. Nittler et S. Mukhopadhyay. « Isotopic Signatures of Presolar Materials in Interplanetary Dust ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 155–72. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_11.
Texte intégralMarty, B., K. Hashizume, M. Chaussidon et R. Wieler. « Nitrogen Isotopes on the Moon : Archives of the Solar and Planetary Contributions to the Inner Solar System ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 175–96. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_12.
Texte intégralWieler, R., et V. S. Heber. « Noble Gas Isotopes on the Moon ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 197–210. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_13.
Texte intégralPepin, R. O. « On Noble Gas Processing in the Solar Accretion Disk ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 211–30. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_14.
Texte intégralGrady, Monica M., et Ian P. Wright. « Elemental and Isotopic Abundances of Carbon and Nitrogen in Meteorites ». Dans Solar System History from Isotopic Signatures of Volatile Elements, 231–48. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0145-8_15.
Texte intégralActes de conférences sur le sujet "Volatiles Elements"
Liu, Zhong, Wei-Ping Yan, Li Zhao et Xiao-Min Wang. « Volatiles and Elements Release Characters of Micronized Coal at High Temperature ». Dans ASME 2005 Power Conference. ASMEDC, 2005. http://dx.doi.org/10.1115/pwr2005-50338.
Texte intégralCrosby, James, Sally A. Gibson, Fin Stuart, Teal Riley et Luigia Di Nicola. « Illuminating the long-term storage of fluid-hosted volatiles in the SCLM from 3He/4He, major- and trace elements in global mantle xenolith suites ». Dans Goldschmidt2021. France : European Association of Geochemistry, 2021. http://dx.doi.org/10.7185/gold2021.7412.
Texte intégralHasan, Mahmudul, et Yousef Haseli. « Modeling Woody Biomass Torrefaction Process ». Dans ASME 2018 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2018. http://dx.doi.org/10.1115/imece2018-87974.
Texte intégralBraukmüller, Ninja, Claudia Funk, Carsten Münker et Frank Wombacher. « Volatile Elements in Chondrites ». Dans Goldschmidt2020. Geochemical Society, 2020. http://dx.doi.org/10.46427/gold2020.256.
Texte intégralLodders, K., et B. Fegley. « The origin and evolution of the terrestrial alkali element budget ». Dans Volatiles in the Earth and solar system. AIP, 1995. http://dx.doi.org/10.1063/1.48754.
Texte intégralRussell, Michael J. « On Irish bacteriometallogenesis and its wider connotations ». Dans Irish-type Zn-Pb deposits around the world. Irish Association for Economic Geology, 2023. http://dx.doi.org/10.61153/pbic1076.
Texte intégralLoewen, Matt, Adam Kent et Pavel Izbekov. « Tracking magmatic volatile and non-volatile trace elements with amphibole in arc magmas ». Dans Goldschmidt2022. France : European Association of Geochemistry, 2022. http://dx.doi.org/10.46427/gold2022.10654.
Texte intégralRoland, Jérôme, Vinciane Debaille et Steven Goderis. « Moderately volatile elements in CB and CH chondrites ». Dans Goldschmidt2023. France : European Association of Geochemistry, 2023. http://dx.doi.org/10.7185/gold2023.15337.
Texte intégralFumarola, Alessandro, Y. Leblebici, P. Narayanan, R. M. Shelby, L. L. Sanchez, G. W. Burr, K. Moon, J. Jang, H. Hwang et S. Sidler. « Non-filamentary non-volatile memory elements as synapses in neuromorphic systems ». Dans 2019 19th Non-Volatile Memory Technology Symposium (NVMTS). IEEE, 2019. http://dx.doi.org/10.1109/nvmts47818.2019.8986194.
Texte intégralNie, Nicole, Xinyang Chen, Timo Hopp, Justin Hu, Zhe Zhang, Fang-Zhen Teng, Anat Shahar et Nicolas Dauphas. « Incomplete condensation of volatile elements as the cause for volatile depletion in carbonaceous chondrites ». Dans Goldschmidt2022. France : European Association of Geochemistry, 2022. http://dx.doi.org/10.46427/gold2022.10750.
Texte intégralRapports d'organisations sur le sujet "Volatiles Elements"
Wimpenny, J. Assessing the Behavior of Moderately Volatile Elements on the Moon in order to Constrain Processes of Magmatic Evolution and Planetary Accretion. Office of Scientific and Technical Information (OSTI), novembre 2023. http://dx.doi.org/10.2172/2229028.
Texte intégralSoltani Dehnavi, A., D. R. Lentz et C. R. M. McFarlane. LA-ICP-MS analysis of volatile trace elements in massive sulphides and host rocks of selected VMS deposits of the Bathurst Mining Camp, New Brunswick : methodology and application to exploration. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2015. http://dx.doi.org/10.4095/296545.
Texte intégralJung, Carina, Karl Indest, Matthew Carr, Richard Lance, Lyndsay Carrigee et Kayla Clark. Properties and detectability of rogue synthetic biology (SynBio) products in complex matrices. Engineer Research and Development Center (U.S.), septembre 2022. http://dx.doi.org/10.21079/11681/45345.
Texte intégralBourdeau, J. E., et R. D. Dyer. Regional-scale lake-sediment sampling and analytical protocols with examples from the Geological Survey of Canada. Natural Resources Canada/CMSS/Information Management, 2023. http://dx.doi.org/10.4095/331911.
Texte intégralDehnavi, A. S., C. R. M. McFarlane, S. H. McClenaghan et D. R. Lentz. In situ LA-ICP-MS of sulfide minerals in VMS deposits throughout the Bathurst Mining Camp, New Brunswick, Canada : volatile trace-element contents and distribution with implications for their syngenetic to polyphase metamorphic history. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2014. http://dx.doi.org/10.4095/293681.
Texte intégralKyllönen, Katriina, Karri Saarnio, Ulla Makkonen et Heidi Hellén. Verification of the validity of air quality measurements related to the Directive 2004/107/EC in 2019-2020 (DIRME2019). Finnish Meteorological Institute, 2020. http://dx.doi.org/10.35614/isbn.9789523361256.
Texte intégral