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  • 1.
    Björling, Marcus
    et al.
    Luleå University of Technology, Department of Engineering Sciences and Mathematics, Machine Elements.
    Habchi, Wassim
    Department of Industrial and Mechanical Engineering, Lebanese American University, Byblos, Lebanon.
    Bair, Scott
    Georgia Institute of Technology, Centre for High Pressure Rheology, G.W. Woodruff School of Mechanical Engineering, Atlanta, GA, 30332-0405, USA.
    Larsson, Roland
    Luleå University of Technology, Department of Engineering Sciences and Mathematics, Machine Elements.
    Marklund, Pär
    Luleå University of Technology, Department of Engineering Sciences and Mathematics, Machine Elements.
    Warm carbon coat reduces friction2014In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 505, no 7483, p. 264-Article in journal (Other academic)
    Abstract [en]

    A coating material made of carbon reduces friction not just by providing a slippery surface, but also by keeping the points of contact warm. Marcus Björling at Luleå University of Technology in Sweden and his team coated steel balls with ``diamond-like-carbon'' - a material in which carbon atoms have a bonding pattern similar to that of diamond. They rolled the balls against a metal disk with an oil lubricant in between, and showed that the carbon coating acts as an insulator, lowering the viscosity of the lubricant and thus reducing the fricion between the ball and the disk. These findings could encourage the development of lubricant coatings made from insulating materials.

  • 2.
    Elming, Sten-åke
    Luleå University of Technology, Department of Civil, Environmental and Natural Resources Engineering, Geosciences and Environmental Engineering.
    Evidence for early Proterozoic plate tectonics from seismic reflection profiles in the Baltic Shield1990In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 348, p. 34-38Article in journal (Refereed)
    Abstract [en]

    Plate tectonics provides the linking framework for all tectonic and magmatic activity seen today, but it is not known when plate tectonics first developed on Earth. New deep seismic reflection and coincident refraction profiles across an exposed, 1.89-Gyr-old volcanic arc complex show a 10-km-thick offset in the Moho and bivergent reflectors in the crust, which were most probably created by plate convergence, subduction and accretion during the Early Proterozoic. Hence, plate tectonic models seem to be applicable for at least the second half of Earth's history.

  • 3. Korablev, Oleg
    et al.
    Martin-Torres, Javier
    Luleå University of Technology, Department of Computer Science, Electrical and Space Engineering, Space Technology.
    Zorzano Mier, María-Paz
    Luleå University of Technology, Department of Computer Science, Electrical and Space Engineering, Space Technology.
    Vago, Jorge L.
    European Space Research and Technology Centre (ESTEC), ESA, Noordwijk, The Netherlands.
    No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations2019In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 568, p. 517-520Article in journal (Refereed)
    Abstract [en]

    The detection of methane on Mars has been interpreted as indicating that geochemical or biotic activities could persist on Mars today1. A number of different measurements of methane show evidence of transient, locally elevated methane concentrations and seasonal variations in background methane concentrations2,3,4,5. These measurements, however, are difficult to reconcile with our current understanding of the chemistry and physics of the Martian atmosphere6,7, which—given methane’s lifetime of several centuries—predicts an even, well mixed distribution of methane1,6,8. Here we report highly sensitive measurements of the atmosphere of Mars in an attempt to detect methane, using the ACS and NOMAD instruments onboard the ESA-Roscosmos ExoMars Trace Gas Orbiter from April to August 2018. We did not detect any methane over a range of latitudes in both hemispheres, obtaining an upper limit for methane of about 0.05 parts per billion by volume, which is 10 to 100 times lower than previously reported positive detections2,4. We suggest that reconciliation between the present findings and the background methane concentrations found in the Gale crater4 would require an unknown process that can rapidly remove or sequester methane from the lower atmosphere before it spreads globally.

  • 4.
    Li, Jian-Yang
    et al.
    Planetary Science Institute, Tucson, AZ, USA.
    Hirabayashi, Masatoshi
    Department of Aerospace Engineering, Department of Geosciences, Auburn University, Auburn, AL, USA.
    Farnham, Tony L.
    Department of Astronomy, University of Maryland, College Park, MD, USA.
    Sunshine, Jessica M.
    Department of Astronomy, University of Maryland, College Park, MD, USA.
    Knight, Matthew M.
    Physics Department, United States Naval Academy, Annapolis, MD, USA.
    Tancredi, Gonzalo
    Departamento de Astronomía, Facultad de Ciencias, Udelar, Uruguay.
    Moreno, Fernando
    Instituto de Astrofísica de Andalucía, CSIC, Granada, Spain.
    Murphy, Brian
    University of Edinburgh, Royal Observatory, Edinburgh, UK.
    Opitom, Cyrielle
    University of Edinburgh, Royal Observatory, Edinburgh, UK.
    Chesley, Steve
    Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
    Scheeres, Daniel J.
    Aerospace Engineering Sciences, Colorado Center for Astrodynamics Research, University of Colorado, Boulder, CO, USA.
    Thomas, Cristina A.
    Northern Arizona University, Flagstaff, AZ, USA.
    Fahnestock, Eugene G.
    Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
    Cheng, Andrew F.
    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.
    Dressel, Linda
    Space Telescope Science Institute, Baltimore, MD, USA.
    Ernst, Carolyn M.
    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.
    Ferrari, Fabio
    Department of Aerospace Science and Technology, Politecnico di Milano, Milan, Italy.
    Fitzsimmons, Alan
    School of Mathematics and Physics, Queen’s University Belfast, Belfast, UK.
    Ieva, Simone
    INAF - Osservatorio Astronomico di Roma, Rome, Italy.
    Ivanovski, Stavro L.
    INAF Osservatorio Astronomico di Trieste, Trieste, Italy.
    Kareta, Theodore
    Lowell Observatory, Flagstaff, AZ, USA; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
    Kolokolova, Ludmilla
    Department of Astronomy, University of Maryland, College Park, MD, USA.
    Lister, Tim
    Las Cumbres Observatory, Goleta, CA, USA.
    Raducan, Sabina D.
    Space Research and Planetary Sciences, Physikalisches Institut, University of Bern, Bern, Switzerland.
    Rivkin, Andrew S.
    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.
    Rossi, Alessandro
    IFAC-CNR, Florence, Italy.
    Soldini, Stefania
    Department of Mechanical, Materials and Aerospace Engineering, University of Liverpool, Liverpool, UK.
    Stickle, Angela M.
    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.
    Vick, Alison
    Space Telescope Science Institute, Baltimore, MD, USA.
    Vincent, Jean-Baptiste
    DLR Institute of Planetary Research, Berlin, Germany.
    Weaver, Harold A.
    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.
    Bagnulo, Stefano
    Armagh Observatory and Planetarium, Armagh, UK.
    Bannister, Michele T.
    School of Physical and Chemical Sciences, Te Kura Matū, University of Canterbury, Christchurch, New Zealand.
    Cambioni, Saverio
    Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA.
    Campo Bagatin, Adriano
    Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante, Alicante, Spain; Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Alicante, Spain.
    Chabot, Nancy L.
    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.
    Cremonese, Gabriele
    INAF Osservatorio Astronomico di Padova, Padua, Italy.
    Daly, R. Terik
    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.
    Dotto, Elisabetta
    INAF - Osservatorio Astronomico di Roma, Rome, Italy.
    Glenar, David A.
    Center for Space Science and Technology, University of Maryland, Baltimore County, Baltimore, MD, USA; Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.
    Granvik, Mikael
    Luleå University of Technology, Department of Computer Science, Electrical and Space Engineering, Space Technology. Department of Physics, University of Helsinki, Helsinki, Finland.
    Hasselmann, Pedro H.
    INAF - Osservatorio Astronomico di Roma, Rome, Italy.
    Herreros, Isabel
    Centro de Astrobiología (CAB), CSIC-INTA, Torrejón de Ardoz, Madrid, Spain.
    Jacobson, Seth
    Department of Earth and Environmental Sciences, Michigan State University, East Lansing, MI, USA.
    Jutzi, Martin
    Space Research and Planetary Sciences, Physikalisches Institut, University of Bern, Bern, Switzerland.
    Kohout, Tomas
    Institute of Geology of the Czech Academy of Sciences, Prague, Czech Republic; Department of Geosciences and Geography, University of Helsinki, Helsinki, Finland.
    La Forgia, Fiorangela
    Dipartimento di Fisica e, Astronomia-Padova University, Padua, Italy.
    Lazzarin, Monica
    Dipartimento di Fisica e, Astronomia-Padova University, Padua, Italy.
    Lin, Zhong-Yi
    Institute of Astronomy, National Central University, Taoyuan City, Taiwan.
    Lolachi, Ramin
    Center for Space Science and Technology, University of Maryland, Baltimore County, Baltimore, MD, USA; Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.
    Lucchetti, Alice
    INAF Osservatorio Astronomico di Padova, Padua, Italy.
    Makadia, Rahil
    Department of Aerospace Engineering, University of Illinois Urbana-Champaign, Urbana, IL, USA.
    Mazzotta Epifani, Elena
    INAF - Osservatorio Astronomico di Roma, Rome, Italy.
    Michel, Patrick
    Laboratoire Lagrange, Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Nice, France.
    Migliorini, Alessandra
    INAF - Institute for Space Astrophysics and Planetology, Rome, Italy.
    Moskovitz, Nicholas A.
    Lowell Observatory, Flagstaff, AZ, USA.
    Ormö, Jens
    Centro de Astrobiología (CAB), CSIC-INTA, Torrejón de Ardoz, Madrid, Spain.
    Pajola, Maurizio
    INAF Osservatorio Astronomico di Padova, Padua, Italy.
    Sánchez, Paul
    Aerospace Engineering Sciences, Colorado Center for Astrodynamics Research, University of Colorado, Boulder, CO, USA.
    Schwartz, Stephen R.
    Planetary Science Institute, Tucson, AZ, USA.
    Snodgrass, Colin
    University of Edinburgh, Royal Observatory, Edinburgh, UK.
    Steckloff, Jordan
    Planetary Science Institute, Tucson, AZ, USA.
    Stubbs, Timothy J.
    Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.
    Trigo-Rodríguez, Josep M.
    Institute of Space Sciences (CSIC-IEEC), UAB Bellaterra, Barcelona, Spain.
    Ejecta from the DART-produced active asteroid Dimorphos2023In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 616, p. 452-456Article in journal (Refereed)
    Abstract [en]

    Some active asteroids have been proposed to be formed as a result of impact events1. Because active asteroids are generally discovered by chance only after their tails have fully formed, the process of how impact ejecta evolve into a tail has, to our knowledge, not been directly observed. The Double Asteroid Redirection Test (DART) mission of NASA2, in addition to having successfully changed the orbital period of Dimorphos3, demonstrated the activation process of an asteroid resulting from an impact under precisely known conditions. Here we report the observations of the DART impact ejecta with the Hubble Space Telescope from impact time T + 15 min to T + 18.5 days at spatial resolutions of around 2.1 km per pixel. Our observations reveal the complex evolution of the ejecta, which are first dominated by the gravitational interaction between the Didymos binary system and the ejected dust and subsequently by solar radiation pressure. The lowest-speed ejecta dispersed through a sustained tail that had a consistent morphology with previously observed asteroid tails thought to be produced by an impact4,5. The evolution of the ejecta after the controlled impact experiment of DART thus provides a framework for understanding the fundamental mechanisms that act on asteroids disrupted by a natural impact1,6.

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  • 5.
    O’Carroll, Conor
    et al.
    European Research Area Steering Group on Human Resources and Mobility, Newry, United Kingdom.
    Scholz, Beate
    Scholz Consulting, Bonn, Germany.
    Nogueira, Maria Manuela
    European Science Foundation, Strasbourg, France.
    Avellis, Gianna
    the m-WiSET Working Group of the Marie Curie Fellows Association, Brussels, Belgium.
    Marin, Laura
    Swedish Research Council, Stockholm, Sweden.
    Dan, Maria Bostenaru
    Ion Mincu University of Architecture and Urbanism, Bucharest, Romania.
    Chmielowski, Riia
    Luleå University of Technology, Department of Civil, Environmental and Natural Resources Engineering, Geosciences and Environmental Engineering.
    di Trapani, Antonella
    European Research Council Executive Agency, Brussels, Belgium.
    Theodoridou, Magdalini
    University of Cyprus, Nicosia, Cyprus.
    Virtual mobility can drive equality2014In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 511, no 292, p. 292-Article in journal (Other academic)
    Download full text (pdf)
    fulltext
  • 6.
    Okada, T.
    et al.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; University of Tokyo, Tokyo, Japan.
    Fukuhara, T.
    Rikkyo University, Tokyo, Japan.
    Tanaka, S.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan; University of Tokyo, Kashiwa, Japan.
    Taguchi, M.
    Rikkyo University, Tokyo, Japan.
    Arai, T.
    Ashikaga University, Ashikaga, Japan.
    Senshu, H.
    Planetary Exploration Research Center, Chiba Institute of Technology, Narashino, Japan.
    Sakatani, N.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Shimaki, Y.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Demura, H.
    University of Aizu, Aizu-Wakamatsu, Japan.
    Ogawa, Y.
    University of Aizu, Aizu-Wakamatsu, Japan.
    Suko, K.
    University of Aizu, Aizu-Wakamatsu, Japan.
    Sekiguchi, T.
    Hokkaido University of Education, Asahikawa, Japan.
    Kouyama, T.
    National Institute of Advanced Industrial Science and Technology (AIST), Tokyo, Japan.
    Takita, J.
    Hokkaido Kitami Hokuto High School, Kitami, Japan.
    Matsunaga, T.
    National Institute for Environmental Studies (NIES), Tsukuba, Japan.
    Imamura, T.
    University of Tokyo, Kashiwa, Japan.
    Wada, T.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Hasegawa, S.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Helbert, J.
    German Aerospace Center (DLR), Berlin, Germany.
    Müller, T. G.
    Max-Planck Institute for Extraterrestrial Physics, Garching, Germany.
    Hagermann, Axel
    University of Stirling, Stirling, UK.
    Biele, J.
    German Aerospace Center (DLR), Cologne, Germany.
    Grott, M.
    German Aerospace Center (DLR), Berlin, Germany.
    Hamm, M.
    German Aerospace Center (DLR), Berlin, Germany; University of Potsdam, Potsdam, Germany.
    Delbo, M.
    Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Nice, France.
    Hirata, N.
    University of Aizu, Aizu-Wakamatsu, Japan.
    Hirata, N.
    Kobe University, Kobe, Japan.
    Yamamoto, Y.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Sugita, S.
    University of Tokyo, Tokyo, Japan; Planetary Exploration Research Center, Chiba Institute of Technology, Narashino, Japan.
    Namiki, N.
    The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan; National Astronomical Observatory of Japan (NAOJ), Mitaka, Japan.
    Kitazato, K.
    University of Aizu, Aizu-Wakamatsu, Japan.
    Arakawa, M.
    Kobe University, Kobe, Japan.
    Tachibana, S.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; University of Tokyo, Tokyo, Japan.
    Ikeda, H.
    Research and Development Directorate, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Ishiguro, M.
    Seoul National University, Seoul, South Korea.
    Wada, K.
    Planetary Exploration Research Center, Chiba Institute of Technology, Narashino, Japan.
    Honda, C.
    University of Aizu, Aizu-Wakamatsu, Japan.
    Honda, R.
    Kochi University, Kochi, Japan.
    Ishihara, Y.
    National Institute for Environmental Studies (NIES), Tsukuba, Japan.
    Matsumoto, K.
    The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan; National Astronomical Observatory of Japan (NAOJ), Mitaka, Japan.
    Matsuoka, M.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Michikami, T.
    Kindai University, Higashi-Hiroshima, Japan.
    Miura, A.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Morota, T.
    University of Tokyo, Tokyo, Japan.
    Noda, H.
    National Astronomical Observatory of Japan (NAOJ), Mitaka, Japan.
    Noguchi, R.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Ogawa, K.
    Kobe University, Kobe, Japan; Space Exploration Center, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Shirai, K.
    Kobe University, Kobe, Japan.
    Tatsumi, E.
    University of Tokyo, Tokyo, Japan; Instituto de Astrofísica de Canarias, University of La Laguna, La Laguna, Tenerife, Spain.
    Yabuta, H.
    Hiroshima University, Higashi-Hiroshima, Japan.
    Yokota, Y.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Yamada, M.
    Planetary Exploration Research Center, Chiba Institute of Technology, Narashino, Japan.
    Abe, M.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Hayakawa, M.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Iwata, T.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Ozaki, M.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Yano, H.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Hosoda, S.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Mori, O.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Sawada, H.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Shimada, T.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Takeuchi, H.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Tsukizaki, R.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Fujii, A.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Hirose, C.
    Research and Development Directorate, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Kikuchi, S.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Mimasu, Y.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Ogawa, N.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; Space Exploration Center, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Ono, G.
    Research and Development Directorate, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Takahashi, T.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Takei, Y.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Yamaguchi, T.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Yoshikawa, K.
    Research and Development Directorate, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Terui, F.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Saiki, T.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Nakazawa, S.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan.
    Yoshikawa, M.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Watanabe, S.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; Nagoya University, Nagoya, Japan.
    Tsuda, Y.
    Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan; The Graduate University for Advanced Studies, SOKENDAI, Hayama, Japan.
    Highly porous nature of a primitive asteroid revealed by thermal imaging2020In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 579, p. 518-522Article in journal (Refereed)
  • 7.
    Parasnis, Dattatray S.
    Luleå University of Technology.
    PhD theses1988In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 333, no 6171, p. 294-Article in journal (Other academic)
  • 8. Paul, Jan
    CO dissociation on potassium promoted aluminum1986In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 323, no 6090, p. 701-703Article in journal (Refereed)
  • 9.
    Stage, Jesper
    Department of Economics, University of Gothenburg, 405 30 Gothenburg, PO Box 640, Sweden.
    Speaking up for economic-sciences modelling2008In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 456, no 7222, p. 470-Article in journal (Other academic)
  • 10.
    Zoback, Mary Lou
    et al.
    US Geological Survey, Menlo Park, California, 94025, USA.
    Zoback, Mark D.
    Department of Geophysics, Stanford University, Stanford, California, 94305, USA.
    Adams, J.
    Geophysics Division, Geological Survey of Canada, 1 Observatory Crescent, Ottawa, Ontario, Canada.
    Assumpção, M.
    Institute Astronômico e Geofísico, Universidade de São Paulo, 01051, São Paulo-SP, Brazil.
    Bell, S.
    Institute of Sedimentary and Petroleum Geology, 3303 33rd St NW, Calgary, Alberta, Canada.
    Bergman, E. A.
    Massachusetts Institute of Technology, Cambridge, Massachusetts, 02139, USA.
    Blümling, P.
    NAGRA, Parkstrasse 23, CH-5401, Baden, Switzerland.
    Brereton, N. R.
    British Geological Survey, Key-worth, Nottinghamshire, NC12 5GG, UK.
    Denham, D.
    Australian Seismological Centre, PO Box 378, Canberra, ACT 2601, Australia.
    Ding, J.
    Institute of Crustal Dynamics, State Seismological Bureau, PO Box 2855, Beijing, China.
    Fuchs, K.
    Universität Karlsruhe, Geophysikalisches Institut, D-7500, Karlsruhe, 21, FRG.
    Gay, N.
    Rock Mechanics Laboratory, Auckland Park 2006, Johannesburg, South Africa.
    Gregersen, S.
    Geodetic Institute, Gamlehave Alle 22, DK-2920, Charlottenlund, Denmark.
    Gupta, H. K.
    Cochin University of Science and Technology, Cochin, 682 022, India.
    Gvishiani, A.
    Institute of Physics of the Earth, Academy of Sciences of the USSR, Moscow, 123810, USSR.
    Jacob, K.
    Lamont-Doherty Geological Observatory, Columbia University, Palisades, New York, 10964, USA.
    Klein, R.
    BP Research International, Sunbury on Thames, Middlesex, TW16 7LN, UK.
    Knoll, P.
    Zentralinstitut fur Physik der Erde, Telegrafenberg A 17, Potsdam, GDR-1561.
    Magee, M.
    US Geological Survey, Menlo Park, California, 94025, USA.
    Mercier, J. L.
    Laboratoire de Géologic Dynamique Interne, Université Paris-Sud, 91405, Orsay, France.
    Müller, B. C.
    Universität Karlsruhe, Geophysikalisches Institut, D-7500, Karlsruhe, 21, FRG.
    Paquin, C.
    Laboratoire de Géophysique et Géodynamique Interne, Université Paris-Sud, 91405, Orsay, France.
    Rajendran, K.
    Department of Geology, University of South Carolina, Columbia, South Carolina, 29208, USA.
    Stephansson, O.
    Luleå University of Technology.
    Suarez, G.
    Institute de Geofisica, Universidad Nacional Autónoma de México, México, DF 04510, Mexico.
    Suter, M.
    Institute de Geologia, Universidad Nacional Autónoma de México, México, DF 04510, Mexico.
    Udias, A.
    Cátedra de Geofísica-Fac. de C. Fisicas, Universidad Complutense, Madrid, 28040, Spain.
    Xu, Z. H.
    Institute of Geophysics, State Seismological Bureau, Beijing, China.
    Zhizhin, M.
    Institute of Physics of the Earth, Academy of Sciences of the USSR, Moscow, 123810, USSR.
    Global patterns of tectonic stress1989In: Nature, ISSN 0028-0836, E-ISSN 1476-4687, Vol. 341, no 6240, p. 291-298Article, review/survey (Refereed)
    Abstract [en]

    Regional patterns of present-day tectonic stress can be used to evaluate the forces acting on the lithosphere and to investigate intraplate seismicity. Most intraplate regions are characterized by a compressional stress regime; extension is limited almost entirely to thermally uplifted regions. In several plates the maximum horizontal stress is subparallel to the direction of absolute plate motion, suggesting that the forces driving the plates also dominate the stress distribution in the plate interior.

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