Specific Entropy During Substorms Observed With Themis

Details Specific Entropy During Substorms Observed With Themis Specific Entropy During Substorms Observed With Themis

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm41a1843n&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SM41A-1843

Physics

[2740] Magnetospheric Physics / Magnetospheric Configuration And Dynamics, [2760] Magnetospheric Physics / Plasma Convection, [2790] Magnetospheric Physics / Substorms

Scientific paper

The method described in Wolf et al. [J. Geophys. Res., 111, A12218, doi: 10.1029/2006JA012010] is used to obtain the instantaneous pV5/3 (specific entropy) of flux tubes from single-satellite measurements of the magnetic field and plasma pressure. Fast, earthward flows are comprised of flux tubes of reduced pV5/3, i.e., ``bubbles”. Magnetic field and plasma data from the multi-satellite THEMIS mission are used to investigate the size of and the azimuthal dependence of pV5/3 within substorm bubbles in the near-Earth plasma sheet.

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