GP43C:
Swarm Two Years on: Achievements in Unraveling the Earth's Magnetic Field II Posters


Session ID#: 8382

Session Description:
Swarm is an Earth Explorer mission in ESA's Living Planet Programme launched on November 22, 2013 and is dedicated to geomagnetic field exploration. The mission is composed of a lower satellite pair flying in a side-by-side constellation, with a third satellite in an independent higher orbit. The three spacecraft deliver high-accuracy measurements of the strength, direction and time variations of the magnetic field, providing the required observations to unravel the magnetic signals that stem from Earth’s core, mantle, crust and oceans, as well as its ionosphere and magnetosphere.

This session solicits contributions about the results from the mission two years after its launch in terms of data analysis, modeling and interpretation as well as combination and synergies of Swarm with other satellite missions and ground stations in order to provide a comprehensive description of geomagnetic field sources and their variations.

Primary Convener:  Stavros Kotsiaros, DTU Space, Lyngby, Denmark
Conveners:  Patrick Alken, University of Colorado Boulder, CIRES, Boulder, CO, United States and Foteini Vervelidou, Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany
Chairs:  Stavros Kotsiaros, DTU Space, Lyngby, Denmark and Patrick Alken, University of Colorado Boulder, CIRES, Boulder, CO, United States
OSPA Liaison:  Stavros Kotsiaros, DTU Space, Lyngby, Denmark

Cross-Listed:
  • SM - SPA-Magnetospheric Physics
Index Terms:

1507 Core processes [GEOMAGNETISM AND PALEOMAGNETISM]
1515 Geomagnetic induction [GEOMAGNETISM AND PALEOMAGNETISM]
1517 Magnetic anomalies: modeling and interpretation [GEOMAGNETISM AND PALEOMAGNETISM]
1541 Satellite magnetics: main field, crustal field, external field [GEOMAGNETISM AND PALEOMAGNETISM]

Abstracts Submitted to this Session:

The Absolute Vector Magnetometers on Board Swarm, Lessons Learned From Two Years in Space. (65950)
Gauthier Hulot1, Jean-Michel Leger2, Pierre Vigneron3, Laura Brocco4, Nils Olsen5, Thomas Jager6, Francois Bertrand6, Isabelle Fratter7, Olivier Sirol8 and Xavier Lalanne4, (1)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, (2)CEA-LETI, Grenoble, France, (3)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (4)Institut de Physique du Globe de Paris, Paris, France, (5)Technical University of Denmark - Space, Kongens Lyngby, Denmark, (6)CEA-Léti, Université Grenoble Alpes, MINATEC, Grenoble, France, (7)CNES French National Center for Space Studies, Toulouse Cedex 09, France, (8)Université de Paris, Institut de physique du globe de Paris, Paris, France
Core field accelerations from Swarm and ground observatory data (77681)
Christopher C Finlay1, Nils Olsen2, Stavros Kotsiaros1, Nicolas Gillet3 and Lars Tøffner-clausen1, (1)DTU Space, Lyngby, Denmark, (2)Technical University of Denmark - Space, Kongens Lyngby, Denmark, (3)ISTerre Institute of Earth Sciences, Grenoble, France
Small-scale field-aligned currents and ionospheric disturbances induced by vertical acoustic resonance during the 2015 eruption of Chile's Calbuco volcano (77742)
Tadashi Aoyama1, Toshihiko Iyemori1, Kunihito Nakanishi1 and Michi Nishioka2, (1)Kyoto University, Graduate School of Science, Kyoto, Japan, (2)NICT National Institute of Information and Communications Technology, Tokyo, Japan
A Model of the Earth’s Magnetic Field From Two Years of Swarm Satellite Constellation Data (77748)
Nils Olsen1, Christopher C Finlay2 and Stavros Kotsiaros2, (1)Technical University of Denmark - Space, Kongens Lyngby, Denmark, (2)DTU Space, Lyngby, Denmark
SWARM Observations of the Motion of Low-latitude Plasma Depletions Coordinated with Ground-based TEC Measurements (81188)
Rezy Pradipta1, Cesar Enrique Valladares1, Robert E Sheehan2, Pierdavide Coïsson3 and David J Knudsen4, (1)Boston College, Institute for Scientific Research, Chestnut Hill, MA, United States, (2)Boston College, Chestnut Hill, MA, United States, (3)Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, UMR 7154 CNRS/INSU, Paris, France, (4)University of Calgary, Calgary, AB, Canada
Distribution of turbulent plasma in the magnetosphere estimated by the SWARM magnetic data. (76237)
Yoshihiro Yokoyama1, Toshihiko Iyemori2, Kunihito Nakanishi2 and Tadashi Aoyama2, (1)Kyoto University, Kyoto, Japan, (2)Kyoto University, Graduate School of Science, Kyoto, Japan
A lithospheric magnetic field model derived from the Swarm satellite magnetic field measurements (77810)
Erwan Thebault, University of Nantes, Nantes, France, Gauthier Hulot, Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France and Pierre Vigneron, Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France
Analysis of Plasma Irregularities and Electromagnetic Signals Based on Swarm Absolute Scalar Magnetometer Burst Mode Sessions (64278)
Pierdavide Coïsson1, Laura Brocco2, Gauthier Hulot3, Jean-Michel Leger4, Thomas Jager5, Pierre Vigneron6, Francois Bertrand5 and Axel Boness4, (1)Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, UMR 7154 CNRS/INSU, Paris, France, (2)Institut de Physique du Globe de Paris, Paris, France, (3)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, (4)CEA-LETI, Grenoble, France, (5)CEA-Léti, Université Grenoble Alpes, MINATEC, Grenoble, France, (6)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France
New insights from satellite magnetic gradient observations into the determination of Earth's lithospheric field (78961)
Stavros Kotsiaros1, Nils Olsen2 and Christopher C Finlay1, (1)DTU Space, Lyngby, Denmark, (2)Technical University of Denmark - Space, Kongens Lyngby, Denmark
Complexities of determining the Field-Aligned current density from LEO satellites. (82915)
Jesper W Gjerloev1, Matthew Michael Friel2, Shinichi Ohtani3, Marc Muhleisen4, Amalia W Gjerloev5, Polly Martin4 and Robin J Barnes6, (1)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)JHU/APL, Laurel, United States, (4)Georgetown Day School, Washington DC, DC, United States, (5)University of Richmond, Physics, Richmond, VA, United States, (6)JHU/APL, Laurel, MD, United States
What is magnetically quiet time? (82573)
Matthew Michael Friel1, Jesper W Gjerloev1, Shinichi Ohtani1, Polly Martin2, Marc Muhleisen2, Nils Olsen3, Haje Korth1 and Brage Foerland4, (1)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (2)Georgetown Day School, Washington DC, DC, United States, (3)Technical University of Denmark - Space, Kongens Lyngby, Denmark, (4)University of Bergen, Bergen, Norway
Oceanic tidal signals in magnetic satellite data (71987)
Ingo Wardinski, Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany and Vincent Lesur, Institut de Physique du Globe de Paris, Paris, France
An earthquake from space: detection of precursory magnetic anomalies from Swarm satellites before the 2015 M8 Nepal Earthquake (58482)
Angelo De Santis1, Georgios Balasis2, F. Javier Pavón-Carrasco1, Gianfranco Cianchini3 and Mioara Mandea4, (1)Istituto Nazionale di Geofisica e Vulcanologia, Palermo, Italy, (2)National Observatory of Athens (NOA), Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing (IAASARS), Athens, Greece, (3)Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy, (4)CNES French National Center for Space Studies, Toulouse Cedex 09, France

See more of: Geomagnetism and Paleomagnetism