ALBERT

Description: Extending magnetic resonance imaging to the atomic scale has been a long-standing aspiration, driven by the prospect of directly mapping atomic positions in molecules with three-dimensional spatial resolution. We report detection of individual, isolated proton spins by a nitrogen-vacancy (NV) center in a diamond chip covered by an inorganic salt. The single-proton identity was confirmed by the Zeeman effect and by a quantum coherent rotation of the weakly coupled nuclear spin. Using the hyperfine field of the NV center as an imaging gradient, we determined proton-NV distances of less than 1 nm.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Loretz, M -- Rosskopf, T -- Boss, J M -- Pezzagna, S -- Meijer, J -- Degen, C L -- New York, N.Y. -- Science. 2014 Oct 16. pii: 1259464. doi: 10.1126/science.1259464. Epub 2014 Oct 16.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics, ETH Zurich, Otto Stern Weg 1, 8093 Zurich, Switzerland. ; Institute for Experimental Physics II, Department of Nuclear Solid State Physics, Universitat Leipzig, Linnestrasse 5, D-04103 Leipzig, Germany. ; Department of Physics, ETH Zurich, Otto Stern Weg 1, 8093 Zurich, Switzerland. degenc@ethz.ch.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25323696" target="_blank"〉PubMed〈/a〉

Description: Agulhas rings provide the principal route for ocean waters to circulate from the Indo-Pacific to the Atlantic basin. Their influence on global ocean circulation is well known, but their role in plankton transport is largely unexplored. We show that, although the coarse taxonomic structure of plankton communities is continuous across the Agulhas choke point, South Atlantic plankton diversity is altered compared with Indian Ocean source populations. Modeling and in situ sampling of a young Agulhas ring indicate that strong vertical mixing drives complex nitrogen cycling, shaping community metabolism and biogeochemical signatures as the ring and associated plankton transit westward. The peculiar local environment inside Agulhas rings may provide a selective mechanism contributing to the limited dispersal of Indian Ocean plankton populations into the Atlantic.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Villar, Emilie -- Farrant, Gregory K -- Follows, Michael -- Garczarek, Laurence -- Speich, Sabrina -- Audic, Stephane -- Bittner, Lucie -- Blanke, Bruno -- Brum, Jennifer R -- Brunet, Christophe -- Casotti, Raffaella -- Chase, Alison -- Dolan, John R -- d'Ortenzio, Fabrizio -- Gattuso, Jean-Pierre -- Grima, Nicolas -- Guidi, Lionel -- Hill, Christopher N -- Jahn, Oliver -- Jamet, Jean-Louis -- Le Goff, Herve -- Lepoivre, Cyrille -- Malviya, Shruti -- Pelletier, Eric -- Romagnan, Jean-Baptiste -- Roux, Simon -- Santini, Sebastien -- Scalco, Eleonora -- Schwenck, Sarah M -- Tanaka, Atsuko -- Testor, Pierre -- Vannier, Thomas -- Vincent, Flora -- Zingone, Adriana -- Dimier, Celine -- Picheral, Marc -- Searson, Sarah -- Kandels-Lewis, Stefanie -- Tara Oceans Coordinators -- Acinas, Silvia G -- Bork, Peer -- Boss, Emmanuel -- de Vargas, Colomban -- Gorsky, Gabriel -- Ogata, Hiroyuki -- Pesant, Stephane -- Sullivan, Matthew B -- Sunagawa, Shinichi -- Wincker, Patrick -- Karsenti, Eric -- Bowler, Chris -- Not, Fabrice -- Hingamp, Pascal -- Iudicone, Daniele -- New York, N.Y. -- Science. 2015 May 22;348(6237):1261447. doi: 10.1126/science.1261447.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Aix Marseille Universite, CNRS, IGS UMR 7256, 13288 Marseille, France. villar@igs.cnrs-mrs.fr not@sb-roscoff.fr hingamp@igs.cnrs-mrs.fr iudicone@szn.it karsenti@embl.de cbowler@biologie.ens.fr. ; CNRS, UMR 7144, Station Biologique de Roscoff, Place Georges Teissier, 29680 Roscoff, France. Sorbonne Universites, Universite Pierre et Marie Curie UPMC, Universite Paris 06, UMR 7144, Station Biologique de Roscoff, Place Georges Teissier, 29680 Roscoff, France. ; Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA. ; Laboratoire de Physique des Oceans (LPO) UMR 6523 CNRS-Ifremer-IRD-UBO, Plouzane, France. Department of Geosciences, Laboratoire de Meteorologie Dynamique (LMD) UMR 8539, Ecole Normale Superieure, 24 Rue Lhomond, 75231 Paris Cedex 05, France. ; CNRS, UMR 7144, Station Biologique de Roscoff, Place Georges Teissier, 29680 Roscoff, France. Sorbonne Universites, Universite Pierre et Marie Curie UPMC, Universite Paris 06, UMR 7144, Station Biologique de Roscoff, Place Georges Teissier, 29680 Roscoff, France. Ecole Normale Superieure, Institut de Biologie de l'ENS (IBENS), and Inserm U1024, and CNRS UMR 8197, F-75005 Paris, France. ; Laboratoire de Physique des Oceans (LPO) UMR 6523 CNRS-Ifremer-IRD-UBO, Plouzane, France. ; Department of Ecology and Evolutionary Biology, University of Arizona, Tucson, AZ 85721, USA. ; Stazione Zoologica Anton Dohrn, Villa Comunale, 80121 Naples, Italy. ; School of Marine Sciences, University of Maine, Orono, ME, USA. ; Sorbonne Universites, UPMC Universite Paris 06, Observatoire Oceanologique, F-06230 Villefranche-sur-Mer, France. INSU-CNRS, UMR 7093, LOV, Observatoire Oceanologique, F-06230 Villefranche-sur-Mer, France. ; Universite de Toulon, Laboratoire PROTEE-EBMA E.A. 3819, BP 20132, 83957 La Garde Cedex, France. ; CNRS, UMR 7159, Laboratoire d'Oceanographie et du Climat LOCEAN, 4 Place Jussieu, 75005 Paris, France. ; Aix Marseille Universite, CNRS, IGS UMR 7256, 13288 Marseille, France. ; Ecole Normale Superieure, Institut de Biologie de l'ENS (IBENS), and Inserm U1024, and CNRS UMR 8197, F-75005 Paris, France. ; Commissariat a l'Energie Atomique et aux Energies Alternatives (CEA), Institut de Genomique, Genoscope, 2 Rue Gaston Cremieux, 91057 Evry, France. CNRS, UMR 8030, CP5706, Evry, France. Universite d'Evry, UMR 8030, CP5706, Evry, France. ; Structural and Computational Biology, European Molecular Biology Laboratory, Meyerhofstrasse 1, 69117 Heidelberg, Germany. Directors' Research, European Molecular Biology Laboratory, Meyerhofstrasse 1, 69117 Heidelberg, Germany. ; Department of Marine Biology and Oceanography, Institute of Marine Sciences (ICM), CSIC, Passeig Maritim de la Barceloneta, 37-49, Barcelona E08003, Spain. ; Structural and Computational Biology, European Molecular Biology Laboratory, Meyerhofstrasse 1, 69117 Heidelberg, Germany. Max-Delbruck-Centre for Molecular Medicine, 13092 Berlin, Germany. ; PANGAEA, Data Publisher for Earth and Environmental Science, University of Bremen, Bremen, Germany. MARUM, Center for Marine Environmental Sciences, University of Bremen, Bremen, Germany. ; Structural and Computational Biology, European Molecular Biology Laboratory, Meyerhofstrasse 1, 69117 Heidelberg, Germany. ; Ecole Normale Superieure, Institut de Biologie de l'ENS (IBENS), and Inserm U1024, and CNRS UMR 8197, F-75005 Paris, France. Directors' Research, European Molecular Biology Laboratory, Meyerhofstrasse 1, 69117 Heidelberg, Germany. villar@igs.cnrs-mrs.fr not@sb-roscoff.fr hingamp@igs.cnrs-mrs.fr iudicone@szn.it karsenti@embl.de cbowler@biologie.ens.fr. ; Ecole Normale Superieure, Institut de Biologie de l'ENS (IBENS), and Inserm U1024, and CNRS UMR 8197, F-75005 Paris, France. villar@igs.cnrs-mrs.fr not@sb-roscoff.fr hingamp@igs.cnrs-mrs.fr iudicone@szn.it karsenti@embl.de cbowler@biologie.ens.fr. ; CNRS, UMR 7144, Station Biologique de Roscoff, Place Georges Teissier, 29680 Roscoff, France. Sorbonne Universites, Universite Pierre et Marie Curie UPMC, Universite Paris 06, UMR 7144, Station Biologique de Roscoff, Place Georges Teissier, 29680 Roscoff, France. villar@igs.cnrs-mrs.fr not@sb-roscoff.fr hingamp@igs.cnrs-mrs.fr iudicone@szn.it karsenti@embl.de cbowler@biologie.ens.fr. ; Stazione Zoologica Anton Dohrn, Villa Comunale, 80121 Naples, Italy. villar@igs.cnrs-mrs.fr not@sb-roscoff.fr hingamp@igs.cnrs-mrs.fr iudicone@szn.it karsenti@embl.de cbowler@biologie.ens.fr.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25999514" target="_blank"〉PubMed〈/a〉

Description: One fundamental controversy about terrestrial planet and asteroid formation is the discrepancy between meteoritical evidence for high temperatures (1500 K to 2000 K) in the inner solar nebula, and much lower theoretical temperature predictions on the basis of models of viscous accretion disks that neglect compressional heating of infalling gas. It is shown here that rigorous numerical calculations of the collapse of a rotating, three-dimensional presolar nebula are capable of producing temperatures on the order of 1500 K in the asteroid region (2.5 astronomical units), in either nearly axisymmetric or strongly nonaxisymmetric nebula models. The latter models may permit significant thermal cycling of solid components in the early inner solar nebula.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Boss, A P -- New York, N.Y. -- Science. 1988 Jul 29;241(4865):565-7.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17774577" target="_blank"〉PubMed〈/a〉

Description: The origin of the moon is considered within the theory of formation of the terrestrial planets by accumulation of planetesimals. The theory predicts the occurrence of giant impacts, suggesting that the moon formed after a roughly Mars-sized body impacted on the protoearth. The impact blasted portions of the protoearth and the impacting body into geocentric orbit, forming a prelunar disk from which the moon later accreted. Although other mechanisms for formation of the moon appear to be dynamically impossible or implausible, fundamental questions must be answered before a giant impact origin can be considered both possible and probable.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Boss, A P -- New York, N.Y. -- Science. 1986 Jan 24;231(4736):341-5.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17735007" target="_blank"〉PubMed〈/a〉

Description: Quantum sensing takes advantage of well-controlled quantum systems for performing measurements with high sensitivity and precision. We have implemented a concept for quantum sensing with arbitrary frequency resolution, independent of the qubit probe and limited only by the stability of an external synchronization clock. Our concept makes use of quantum lock-in detection to continuously probe a signal of interest. Using the electronic spin of a single nitrogen-vacancy center in diamond, we demonstrate detection of oscillating magnetic fields with a frequency resolution of 70 microhertz over a megahertz bandwidth. The continuous sampling further guarantees an enhanced sensitivity, reaching a signal-to-noise ratio in excess of 10 4 for a 170-nanotesla test signal measured during a 1-hour interval. Our technique has applications in magnetic resonance spectroscopy, quantum simulation, and sensitive signal detection.