Harriet George

Postdoctoral researcher


Curriculum vitae



Laboratory for Atmospheric and Space Physics

University of Colorado Boulder



A Global Survey of Geospace Electrons with eVlasiator: First Results


Journal article


M. Alho, M. Battarbee, Y. Pfau‐Kempf, U. Ganse, L. Turc, A. Johlander, V. Tarvus, Hongyang Zhou, M. Dubart, M. Grandin, Konstantinos E. Papadakis, J. Suni, H. George, M. Bussov, M. Palmroth
2021

Semantic Scholar DOI
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APA   Click to copy
Alho, M., Battarbee, M., Pfau‐Kempf, Y., Ganse, U., Turc, L., Johlander, A., … Palmroth, M. (2021). A Global Survey of Geospace Electrons with eVlasiator: First Results.


Chicago/Turabian   Click to copy
Alho, M., M. Battarbee, Y. Pfau‐Kempf, U. Ganse, L. Turc, A. Johlander, V. Tarvus, et al. “A Global Survey of Geospace Electrons with EVlasiator: First Results” (2021).


MLA   Click to copy
Alho, M., et al. A Global Survey of Geospace Electrons with EVlasiator: First Results. 2021.


BibTeX   Click to copy

@article{m2021a,
  title = {A Global Survey of Geospace Electrons with eVlasiator: First Results},
  year = {2021},
  author = {Alho, M. and Battarbee, M. and Pfau‐Kempf, Y. and Ganse, U. and Turc, L. and Johlander, A. and Tarvus, V. and Zhou, Hongyang and Dubart, M. and Grandin, M. and Papadakis, Konstantinos E. and Suni, J. and George, H. and Bussov, M. and Palmroth, M.}
}

Abstract

<div> <p>Models of the geospace plasma environment have been proceeding towards more realistic descriptions of the solar wind—magnetosphere interaction, from gas-dynamic to MHD and hybrid ion-kinetic models such as the state-of-the-art Vlasiator model. Advances in computational capabilities have enabled global simulations of detailed physics, but the electron scale has so far been out of reach in a truly global setting. </p> </div><div> <p>In this work we present results from eVlasiator, an offshoot of the Vlasiator model, showing first results from a global 2D+3V kinetic electron geospace simulation. Despite truncation of some electron physics and use of ion-scale spatial resolution, we show that realistic electron distribution functions are obtainable within the magnetosphere and describe these in relation to MMS observations. Electron precipitation to the upper atmosphere from these velocity distributions is estimated.</p> </div>


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