Probing the Magnetosheath Boundaries Using Interstellar Boundary Explorer (IBEX) Orbital Encounters

S. T. Hart, M. A. Dayeh, D. B. Reisenfeld, P. H. Janzen, D. J. McComas, F. Allegrini, S. A. Fuselier, K. Ogasawara, J. R. Szalay, H. O. Funsten, S. M. Petrinec

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

Inside the magnetosheath, the IBEX-Hi energetic neutral atom (ENA) imager measures a distinct background count rate that is more than 10 times the typical heliospheric ENA emissions observed when IBEX is outside the magnetosheath. The source of this enhancement is magnetosheath ions of solar wind (SW) origin that deflect around the Earth's magnetopause (MP), scatter and neutralize from the anti-sunward part of the IBEX-Hi sunshade, and continue into the instrument as neutral atoms, behaving indistinguishably from ENAs emitted from distant plasma sources. While this background pollutes observations of outer heliospheric ENAs, it provides a clear signature of IBEX crossings over the magnetospheric boundaries. In this study, we investigate IBEX encounters with the magnetosheath boundaries using ∼8 yr of orbital data, and we determine the MP and bow shock (BS) locations derived from this background signal. We find 280 BS crossings from XGSE ∼ 11 Re to XGSE ∼ −36 Re and 241 MP crossings from XGSE ∼ 6 Re to XGSE ∼ −48 Re. We compare IBEX BS and MP crossing locations to those from IMP-8, Geotail, Cluster, Magion-4, ISEE, and Magnetospheric Multiscale Mission, and we find that IBEX crossing locations overlap with the BS and MP locations inferred from these other data sets. In this paper, we demonstrate how IBEX can be used to identify magnetosheath crossings, and extend boundary observations well past the terminator, thus further constraining future models of magnetosheath boundaries. Furthermore, we use the IBEX data set to show observational evidence of near-Earth magnetotail squeezing during periods of strong interplanetary magnetic field By.

Original languageEnglish
Article numbere2021JA029278
JournalJournal of Geophysical Research: Space Physics
Volume126
Issue number7
DOIs
StatePublished - Jul 2021

Funding

This work is funded by NASA grant NNX17AB98 G, and is partially supported by the IBEX mission as part of the NASA Explorer Program (80NSSC18K0237). S.H. thanks Kimberly Moreland for useful discussions on the topic. IBEX observations are available through the official IBEX release website, https://ibex.princeton.edu/DataRelease12, as well as by contacting the IBEX PI, Prof. D. J. McComas at Princeton University (dmccomas@princeton.edu). This work is funded by NASA grant NNX17AB98 G, and is partially supported by the IBEX mission as part of the NASA Explorer Program (80NSSC18K0237). S.H. thanks Kimberly Moreland for useful discussions on the topic. IBEX observations are available through the official IBEX release website, https://ibex.princeton.edu/ DataRelease12, as well as by contacting the IBEX PI, Prof. D. J. McComas at Princeton University ( dmccomas@princeton.edu ).

FundersFunder number
National Aeronautics and Space Administration80NSSC18K0237, NNX17AB98 G
Princeton University

    Keywords

    • IBEX
    • Solar wind
    • bow shock
    • magnetopause
    • magnetosheath
    • magnetotail

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