GP51A:
ESA's Swarm Mission, One Year in Space III Posters

Session ID#: 2642

Friday, 19 December 2014: 8:00 AM-12:20 PM
Poster Hall (Moscone_South)
Chairs:  Gauthier Hulot, Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France and David J Knudsen, University of Calgary, Calgary, AB, Canada
Primary Convener:  Gauthier Hulot, IPGP, Paris, France
Co-conveners:  Hermann Luhr, Deutsches GeoForschungsZentrum, GFZ, Potsdam, Germany, Eigil A Friis-Christensen, DTU, Kongens Lyngby, Denmark and David J Knudsen, University of Calgary, Calgary, AB, Canada
OSPA Liaison:  David J Knudsen, University of Calgary, Calgary, AB, Canada
Co-Sponsor(s):
  • DI - Study of the Earth's Deep Interior
  • G - Geodesy
  • SA - SPA-Aeronomy
  • SM - SPA-Magnetospheric Physics
  • T - Tectonophysics
  • V - Volcanology, Geochemistry and Petrology
Virtual Option?: No

Abstracts Submitted to this Session:

 
In-flight calibration of the experimental Absolute Scalar Magnetometer vector mode on board the Swarm satellites (15700)
Jean-Michel Leger1, Thomas Jager2, Francois Bertrand2, Viviane Cattin1, Isabelle Fratter3, Laura Brocco4, Pierre Vigneron5, Xavier Lalanne4 and Gauthier Hulot6, (1)CEA-LETI, Grenoble, France, (2)CEA-Léti, Université Grenoble Alpes, MINATEC, Grenoble, France, (3)CNES French National Center for Space Studies, Toulouse Cedex 09, France, (4)Institut de Physique du Globe de Paris, Paris, France, (5)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (6)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France
 
Swarm's Absolute Scalar Magnetometers Burst Mode Results (6826)
Pierdavide Coïsson1, Pierre Vigneron2, Gauthier Hulot3, Raul Crespo Grau4,5, Laura Brocco4, Xavier Lalanne4, Olivier Sirol6, Jean-Michel Leger7, Thomas Jager8, Francois Bertrand8, Axel Boness7 and Isabelle Fratter9, (1)Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, UMR 7154 CNRS/INSU, Paris, France, (2)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (3)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, (4)Institut de Physique du Globe de Paris, Paris, France, (5)Observatorio Geofisico Central, Instituto Geografico Nacional, Madrid, Spain, (6)Université de Paris, Institut de physique du globe de Paris, Paris, France, (7)CEA-LETI, Grenoble, France, (8)CEA-Léti, Université Grenoble Alpes, MINATEC, Grenoble, France, (9)CNES French National Center for Space Studies, Toulouse Cedex 09, France
 
Comparing Swarm's Nominal Level1b Magnetic Data and ASM Vector Field Experimental Data: a Convenient Tool for Understanding Data Quality Issues. (15435)
Laura Brocco1, Gauthier Hulot2, Pierre Vigneron3, Vincent Lesur4, Jean-Michel Leger5, Thomas Jager6, Francois Bertrand6, Olivier Sirol7, Xavier Lalanne1, Axel Boness5, Viviane Cattin5 and Isabelle Fratter8, (1)Institut de Physique du Globe de Paris, Paris, France, (2)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, (3)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (4)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, (5)CEA-LETI, Grenoble, France, (6)CEA-Léti, Université Grenoble Alpes, MINATEC, Grenoble, France, (7)Université de Paris, Institut de physique du globe de Paris, Paris, France, (8)CNES French National Center for Space Studies, Toulouse Cedex 09, France
 
A 2015 Igrf Candidate Model Based on Swarm’s Experimental ASM Vector Mode Data (10124)
Pierre Vigneron1, Gauthier Hulot2, Nils Olsen3, Jean-Michel Leger4, Thomas Jager5, Laura Brocco6, Olivier Sirol7, Pierdavide Coïsson8, Xavier Lalanne6, Arnaud Chulliat9, Francois Bertrand5, Axel Boness4 and Isabelle Fratter10, (1)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (2)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, (3)Technical University of Denmark - Space, Kongens Lyngby, Denmark, (4)CEA-LETI, Grenoble, France, (5)CEA-Léti, Université Grenoble Alpes, MINATEC, Grenoble, France, (6)Institut de Physique du Globe de Paris, Paris, France, (7)Université de Paris, Institut de physique du globe de Paris, Paris, France, (8)Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, UMR 7154 CNRS/INSU, Paris, France, (9)National Geophysical Data Center, Boulder, United States, (10)CNES French National Center for Space Studies, Toulouse Cedex 09, France
 
The Swarm Initial Field Model – a Model of the Earth’s Magnetic Field for 2014 Determined From One Year of Swarm Satellite Constellation Data (22655)
Nils Olsen, Technical University of Denmark - Space, Kongens Lyngby, Denmark, Gauthier Hulot, Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, Vincent Lesur, Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, Christopher C Finlay, DTU Space, Lyngby, Denmark, Ciaran Beggan, British Geological Survey, Geomagnetism, Edinburgh, United Kingdom, Arnaud Chulliat, National Geophysical Data Center, Boulder, United States, Terence J Sabaka, NASA Goddard Space Flight Center, Greenbelt, United States and SIFM Team
 
Updating the CHAOS series of field models using Swarm data and resulting candidate models for IGRF-12 (15467)
Christopher C Finlay, Nils Olsen and Lars Tøffner-clausen, Technical University of Denmark - Space, Kongens Lyngby, Denmark
 
Describing Temporal Variations of the Geomagnetic Field through a Modified Virtual Observatory Scheme: Application to SWARM Measurements (6376)
Diana Saturnino, LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France, Benoit Langlais, LPG Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France, Hagay Amit, Nantes Université, Univ Angers, Le Mans Université, Laboratoire de Planétologie et Géosciences, Nantes, France and Mioara Mandea, CNES French National Center for Space Studies, Toulouse Cedex 09, France
 
Jerks in Stochastic Synthetic Magnetic Fields (7858)
William J Brown, University of Leeds, Leeds, LS2, United Kingdom, Jonathan E Mound, University of Leeds, School of Earth and Environment, Leeds, United Kingdom and Philip W Livermore, University of Leeds, School of Earth and Environment, Leeds, LS2, United Kingdom
 
Forward Modeling of the Fennoscandian Lithospheric Field Using Spherical Prisms (7771)
Eldar Baykiev1, Joerg Ebbing2, Marco Broenner3 and Karl W J Fabian3, (1)Norwegian University of Science and Technology, Trondheim, Norway, (2)University of Kiel, Kiel, Germany, (3)Geological Survey of Norway, Trondheim, Norway
 
Possibilities for Observations of Electromagnetic Perturbations Related to Seismic Activity with Swarm Satellites (9496)
Angelo De Santis, Istituto Nazionale di Geofisica e Vulcanologia, Palermo, Italy, Mioara Mandea, CNES French National Center for Space Studies, Toulouse Cedex 09, France and Georgios Balasis, National Observatory of Athens (NOA), Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing (IAASARS), Athens, Greece
 
Equatorial Electric Fields Derived from Swarm Magnetometer Data (7437)
Patrick Alken, University of Colorado Boulder, CIRES, Boulder, CO, United States, Stefan Maus, University of Colorado at Boulder, Boulder, CO, United States, Pierre Vigneron, Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, Olivier Sirol, Université de Paris, Institut de physique du globe de Paris, Paris, France, Gauthier Hulot, Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France and Arnaud Chulliat, National Geophysical Data Center, Boulder, United States
 
Comparing IRI and IRI-Real-Time with SWARM Electron Density Data (17732)
Dieter Bilitza, George Mason University Fairfax, Department of Physics and Astronomy, Fairfax, VA, United States; NASA Goddard Space Flight Center, Greenbelt, MD, United States, Ivan A Galkin, Borealis Global Designs, Varna, Bulgaria, Claudia Stolle, Leibniz Institute of Atmospheric Physics at the University of Rostock, Kühlungsborn, Germany, Artem Vesnin, Univ Massachusetts Lowell, Lowell, MA, United States and Bodo W Reinisch, Lowell Digisonde International, Lowell, MA, United States; University of Massachusetts Lowell, Lowell, MA, United States
 
Can we derive the current density from three point LEO measurements of the magnetic field perturbations? (30243)
Matthew Potter1, Jesper W Gjerloev2, Marc Muhleisen3, Matthew Michael Friel3, Polly Martin3, Guan Le4, Claudia Stolle5 and Hermann Luhr6, (1)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (3)Georgetown Day School, Washington DC, DC, United States, (4)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (5)Leibniz Institute of Atmospheric Physics at the University of Rostock, Kühlungsborn, Germany, (6)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany
 
Field-aligned Currents’ Scale Analysis Performed by the Swarm Constellation (15351)
Hermann Luhr1, Jaeheung Park1, Jesper W Gjerloev2, Jan Rauberg3, Ingo Michaelis4, Guan Le5, Jose MG Merayo6 and Peter Brauer7, (1)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (3)GFZ Helmholtz Centre for Geosciences, 2.3 Geomagnetism, Potsdam, Germany, (4)Helmholtz Centre Potsdam GFZ German Research Center for Geosciences, 2.8 Magnetospheric Physics, Potsdam, Germany, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)DTU Space, Lyngby, Denmark, (7)Technical University of Denmark, DTU Space, Kongens Lyngby, Denmark
 
Structure of small-scale field-aligned currents at middle and low latitudes having lower atmospheric origin (20966)
Kunihito Nakanishi1, Toshihiko Iyemori1, Hermann Luhr2,3 and Tadashi Aoyama1, (1)Kyoto University, Kyoto, Japan, (2)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, (3)Deutsches GeoForschungsZentrum, GFZ, Potsdam, Germany
 
Small-scale field-aligned currents caused by tropical cyclones as observed by the SWARM satellites above the ionosphere (21212)
Tadashi Aoyama, Toshihiko Iyemori and Kunihito Nakanishi, Kyoto University, Graduate School of Science, Kyoto, Japan
 
On the Magnetic Field Spatial Fluctuation Features at Swarm’s Orbit (20994)
Paola De Michelis, Istituto Nazionale di Geofisica e Vulcanologia, Palermo, Italy, Giuseppe Consolini, INAF- Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy and Roberta Tozzi, Istituto Nazionale di Geofisica e Vulcanologia, Roma, Italy
 
Investigating Night-time Ionospheric Currents by Swarm Magnetic Data (16231)
Roberta Tozzi1, Michael Pezzopane1 and Paola De Michelis2, (1)Istituto Nazionale di Geofisica e Vulcanologia, Roma, Italy, (2)Istituto Nazionale di Geofisica e Vulcanologia, Palermo, Italy
 
Swarm Observations of Low-altitude Cusp Ion Upflow (20661)
Johnathan K Burchill1, David J Knudsen1 and Stephan C Buchert2, (1)University of Calgary, Calgary, AB, Canada, (2)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden
 
Observation of Polar Cap Patches and Calculation of Gradient Drift Instability Growth Times: A Swarm Case Study (12782)
Andres Spicher1, Taylor Grant Cameron2, Eric Grono2, Kateryna Yakymenko3, Stephan C Buchert4, Lasse Boy Novock Clausen5, David J Knudsen2, Kathryn A McWilliams6 and Joran Idar Moen1, (1)University of Oslo, Physics Department, Oslo, Norway, (2)University of Calgary, Calgary, AB, Canada, (3)Los Alamos National Laboratory, Los Alamos, NM, United States, (4)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (5)University of Oslo, Department of Physics, Oslo, Norway, (6)University of Saskatchewan, Saskatoon, SK, Canada
 
Swarm In Situ Observations of F-Region Polar Cap Patches Created by Cusp Ionization (20472)
Lindsay Victoria Goodwin1, Blessing Iserhienrhien2, David Miles3, Swadesh Patra4, Christer van der Meeren5, Stephan C Buchert6, Johnathan K Burchill7, Lasse Boy Novock Clausen8, David J Knudsen7, Kathryn A McWilliams2 and Joran Moen8, (1)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, (2)University of Saskatchewan, Saskatoon, SK, Canada, (3)University of Iowa, Physics and Astronomy, Iowa City, United States, (4)University of Oslo, Oslo, Norway, (5)University of Bergen, Bergen, Norway, (6)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (7)University of Calgary, Calgary, AB, Canada, (8)University of Oslo, Department of Physics, Oslo, Norway