@article{3712306551b042218569c42c7e5d3fa0,
title = "Associating ground magnetometer observations with current or voltage generators",
abstract = "A circuit analogy for magnetosphere-ionosphere current systems has two extremes for drivers of ionospheric currents: ionospheric electric fields/voltages constant while current/conductivity vary—the “voltage generator”—and current constant while electric field/conductivity vary—the “current generator.” Statistical studies of ground magnetometer observations associated with dayside Transient High Latitude Current Systems (THLCS) driven by similar mechanisms find contradictory results using this paradigm: some studies associate THLCS with voltage generators, others with current generators. We argue that most of this contradiction arises from two assumptions used to interpret ground magnetometer observations: (1) measurements made at fixed position relative to the THLCS field-aligned current and (2) negligible auroral precipitation contributions to ionospheric conductivity. We use observations and simulations to illustrate how these two assumptions substantially alter expectations for magnetic perturbations associated with either a current or a voltage generator. Our results demonstrate that before interpreting ground magnetometer observations of THLCS in the context of current/voltage generators, the location of a ground magnetometer station relative to the THLCS field-aligned current and the location of any auroral zone conductivity enhancements need to be taken into account.",
keywords = "TCV, current generator, ground magnetometer, magnetosphere-ionosphere coupling, sudden commencement, voltage generator",
author = "Hartinger, {M. D.} and Z. Xu and Clauer, {C. R.} and Y. Yu and Weimer, {D. R.} and Hyomin Kim and V. Pilipenko and Welling, {D. T.} and R. Behlke and Willer, {A. N.}",
note = "Funding Information: M.D. Hartinger was supported by NSF grants AGS-1049403 and PLR-1543364. V. Pilipenko was supported by NSF AGS-1264146. We acknowledge high-performance computing support from Yellowstone (ark:/85065/d7wd3xhc) provided by NCAR's Computational and Information Systems Laboratory, sponsored by the National Science Foundation. This work was carried out using the SWMF/BATS-R-US tools developed at The University of Michigan Center for Space Environment Modeling (CSEM). Magnetometer observations and simulation output files are available upon request from the corresponding author (M.D. Hartinger, mdhartin@vt.edu). Most ground magnetometer measurements and SPEDAS software for plotting can be obtained from the THEMIS website (http://themis.ssl.berkeley.edu/index.shtml). AGO and BAS magnetometer data are available upon request from NJIT and BAS. The authors thank Andrew Gerrard (PI, NJIT, under NSF grant PLR-1443507) for providing fluxgate magnetometer data from the AGO station. We thank the British Antarctic Survey for providing the low-power magnetometer data (PI Mervyn Freeman) from B14 (m81-338) and B16 (m83-347). We thank the National Space Institute at the Technical University of Denmark (DTU Space) for providing magnetometer data from the Greenland Magnetometer Array. We thank the NASA Space Science Data facility for use of Virtual Ionosphere, Thermosphere, Mesosphere Observatory models via the OMNIWeb interface. M.D. Hartinger thanks Mark Engebretson, Jennifer Posch, and Aaron Ridley for informative discussions. Publisher Copyright: {\textcopyright}2017. American Geophysical Union. All Rights Reserved.",
year = "2017",
month = jul,
doi = "10.1002/2017JA024140",
language = "English (US)",
volume = "122",
pages = "7130--7141",
journal = "Journal of Geophysical Research: Space Physics",
issn = "2169-9380",
number = "7",
}