@article{14dcead4d7dc4213b1c51dff682178c0,
title = "Energy Conversion by Parallel Electric Fields During Guide Field Reconnection in Scaled Laboratory and Space Experiments",
abstract = " We present direct and scaled comparisons between laboratory and in situ space observations of magnetic reconnection with a guide field, comparing results from the Magnetospheric Multiscale Mission and the Magnetic Reconnection eXperiment (MRX). While Magnetospheric Multiscale Mission observations obtain high-resolution and fully kinetic data, MRX observations fully cover the 2-D reconnection plane near the current sheet, removing uncertainties in situating the measurements compared to the reconnection region. Through scaling transformations, we show a quantitative agreement in magnetic field and current density profiles, which agree within a factor of 2 from each other. The introduction of the guide field causes the energy conversion J·E in the current sheet to be dominated by J || E || in both cases. However, parallel electric fields reported by recent spacecraft crossings are significantly (5–10 times) larger than values obtained on MRX, highlighting an important issue for understanding energy conversion by reconnection.",
keywords = "energy conversion, experiment, guide field, magnetic reconnection, magnetosphere",
author = "W. Fox and Wilder, {F. D.} and S. Eriksson and J. Jara-Almonte and F. Pucci and J. Yoo and H. Ji and M. Yamada and Ergun, {R. E.} and M. Oieroset and Phan, {T. D.}",
note = "Funding Information: This work was supported by the Max-Planck Princeton Center for Plasma Physics, funded by the U.S. Department of Energy under Contract No. DE-AC0204CH11466 and NASA under Agreements No. NNH15AB29I, NNH14AX631, 80NSSC18K0157, and NNX17AE12G. F.P. was supported by the Strategic International Research Exchange Promotion Program in National Institutes of Natural Sciences, Japan. MRX digital data is available from http://arks.princeton.edu/ark:/88435/ dsp01X920g025r. MMS data is available from the MMS Science Data Center. Funding Information: This work was supported by the Max-Planck Princeton Center for Plasma Physics, funded by the U.S. Department of Energy under Contract No. DE-AC0204CH11466 and NASA under Agreements No. NNH15AB29I, NNH14AX631, 80NSSC18K0157, and NNX17AE12G. F.P. was supported by the Strategic International Research Exchange Promotion Program in National Institutes of Natural Sciences, Japan. MRX digital data is available from http://arks.princeton.edu/ark:/88435/dsp01X920g025r. MMS data is available from the MMS Science Data Center. Publisher Copyright: {\textcopyright}2018. American Geophysical Union. All Rights Reserved.",
year = "2018",
month = dec,
day = "16",
doi = "10.1029/2018GL079883",
language = "English (US)",
volume = "45",
pages = "12,677--12,684",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "American Geophysical Union",
number = "23",
}