Daytime Dynamo Electrodynamics With Spiral Currents Driven by Strong Winds Revealed by Vapor Trails and Sounding Rocket Probes

  • R. Pfaff
    NASA Goddard Space Flight Center Greenbelt MD USA
  • M. Larsen
    Department of Physics and Astronomy Clemson University Clemson SC USA
  • T. Abe
    Japan Aerospace Exploration Agency Tokyo Japan
  • H. Habu
    Japan Aerospace Exploration Agency Tokyo Japan
  • J. Clemmons
    Department of Physics and Astronomy University of New Hampshire Durham NH USA
  • H. Freudenreich
    NASA Goddard Space Flight Center Greenbelt MD USA
  • D. Rowland
    NASA Goddard Space Flight Center Greenbelt MD USA
  • T. Bullett
    Cooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USA
  • M.‐Y. Yamamoto
    School of Systems Engineering Kochi University of Technology Kami Japan
  • S. Watanabe
    Department of Information Media Hokkaido Information University Ebetsu Japan
  • Y. Kakinami
    Department of Information Media Hokkaido Information University Ebetsu Japan
  • T. Yokoyama
    Research Institute for Sustainable Humanosphere Kyoto University Uji Japan
  • J. Mabie
    Cooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USA
  • J. Klenzing
    NASA Goddard Space Flight Center Greenbelt MD USA
  • R. Bishop
    Aerospace Corporation El Segundo CA USA
  • R. Walterscheid
    Aerospace Corporation El Segundo CA USA
  • M. Yamamoto
    Research Institute for Sustainable Humanosphere Kyoto University Uji Japan
  • Y. Yamazaki
    Geo Forschungs Zentrum Potsdam Germany
  • N. Murphy
    Jet Propulsion Laboratory Pasadena CA USA
  • V. Angelopoulos
    Department of Earth, Planetary, and Space Sciences University of California Los Angeles CA USA

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<jats:title>Abstract</jats:title><jats:p>We investigate the forces and atmosphere‐ionosphere coupling that create atmospheric dynamo currents using two rockets launched nearly simultaneously on 4 July 2013 from Wallops Island (USA), during daytime Sq conditions with ΔH of −30 nT. One rocket released a vapor trail observed from an airplane which showed peak velocities of >160 m/s near 108 km and turbulence coincident with strong unstable shear. Electric and magnetic fields and plasma density were measured on a second rocket. The current density peaked near 110 km exhibiting a spiral pattern with altitude that mirrored that of the winds, suggesting the dynamo is driven by tidal forcing. Such stratified currents are obscured in integrated ground measurements. Large electric fields produced a current opposite to that driven by the wind, believed created to minimize the current divergence. Using the observations, we solve the dynamo equation versus altitude, providing a new perspective on the complex nature of the atmospheric dynamo.</jats:p>

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