IMAP’s Role in Understanding Particle Injection and Energization Throughout the Heliosphere

The payload of the Interstellar Mapping and Acceleration Probe (IMAP) includes sophisticated in situ instruments to measure solar wind plasma and magnetic fields, suprathermal and energetic particles at 1 au as well as unprecedented remote sensing instruments to observe the energetic neutral atoms (ENAs) in the outer heliosphere and the ultraviolet glow of the interstellar neutral H interacting with the three-dimensional solar wind. This unique combination of sensors on a single platform allows connections to be made between the inner and outer heliosphere to an extent never before possible. This article focuses on the scientific theme of connecting the physics of particle acceleration and transport throughout the heliosphere. Such studies enabled by IMAP are organized into three broad categories: i) fundamental particle acceleration and transport processes, ii) heliospheric variability that affects those processes, and iii) inner heliospheric science.

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Publication Details

Journal
Space Science Reviews
Published
2026-01-07
DOI
https://doi.org/10.1007/s11214-025-01257-4
Citations
2
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
23.83

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article

IMAP’s Role in Understanding Particle Injection and Energization Throughout the Heliosphere

T. S. Horbury, J. S. Rankin, I. Kowalska, G. P. Zank et al.
2 citations
Space Science Reviews
Solar and Space Plasma Dynamics
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article

IMAP’s Role in Understanding Particle Injection and Energization Throughout the Heliosphere

T. S. Horbury, J. S. Rankin, I. Kowalska, G. P. Zank, D. L. Turner, R. M. Skoug, Fuqiang Guo, E. Mœbius, M. Bzowski, M. Gkioulidou, S. Dalla, J. Giacalone, D. N. Baker, B. L. Alterman, H. A. Elliott, E. R. Christian, E. J. Zirnstein, J. G. Mitchell, S. G. Kanekal, A. Bruno, N. A. Schwadron, G. I. Livadiotis, C. M. S. Cohen, C. O. Lee, M. I. Desai, J. G. Luhmann, M. A. Dayeh, W. H. Matthaeus, D. J. McComas, I. J. Cohen, J. D. Richardson
article en
2 citations

Abstract

The payload of the Interstellar Mapping and Acceleration Probe (IMAP) includes sophisticated in situ instruments to measure solar wind plasma and magnetic fields, suprathermal and energetic particles at 1 au as well as unprecedented remote sensing instruments to observe the energetic neutral atoms (ENAs) in the outer heliosphere and the ultraviolet glow of the interstellar neutral H interacting with the three-dimensional solar wind. This unique combination of sensors on a single platform allows connections to be made between the inner and outer heliosphere to an extent never before possible. This article focuses on the scientific theme of connecting the physics of particle acceleration and transport throughout the heliosphere. Such studies enabled by IMAP are organized into three broad categories: i) fundamental particle acceleration and transport processes, ii) heliospheric variability that affects those processes, and iii) inner heliospheric science.

Space Science ReviewsVol. 222(1)
California Institute of Technology (US), Centrum Badań Kosmicznych (PL), Southwest Research Institute (US), Goddard Space Flight Center (US), Los Alamos National Laboratory (US), University of Arizona (US), University of New Hampshire (US), University of America (US), University of Lancashire (GB), Princeton University (US), Johns Hopkins University Applied Physics Laboratory (US), Heliophysics (US), Laboratory for Atmospheric and Space Physics (US), Imperial College London (GB), Massachusetts Institute of Technology (US), University of Alabama in Huntsville (US), Catholic University of America (US), University of Delaware (US), University of California, Berkeley (US)
National Aeronautics and Space Administration, Nuclear Safety and Security Commission, Goddard Space Flight Center
Affordable and clean energy
Openalex Percentile: Top 2%
Solar and Space Plasma Dynamics
23.83
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