EGU2020-5547, updated on 16 May 2023
https://doi.org/10.5194/egusphere-egu2020-5547
EGU General Assembly 2020
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Overview of the Instellar Mapping and Acceleration Probe (IMAP) Mission

David McComas
David McComas
  • Princeton University, Astrophysics, United States of America (spacephysics@princeton.edu)

This talk provides an overview of the Interstellar Mapping and Acceleration Probe (IMAP) mission and what we hope and expect to learn from it. IMAP is currently in Phase B and is slated to launch in the fall of 2024. IMAP simultaneously investigates two of the most important, and intimately coupled, research areas in Heliophysics today: 1) the acceleration of energetic particles and 2) the interaction of the solar wind with the local interstellar medium. IMAP’s ten instruments provide a complete set of observations to simultaneously examine the particle injection and acceleration processes at 1 AU while remotely dissecting the global heliospheric interaction and its response to particle populations generated through these processes. For more information about IMAP, see: McComas, D.J., et al., Interstellar mapping and acceleration Probe (IMAP): A New NASA Mission, Space Science Review, 214:116, doi:10.1007/s11214-018-0550-1, 2018.

Open Access: https://link.springer.com/article/10.1007%2Fs11214-018-0550-1 

How to cite: McComas, D.: Overview of the Instellar Mapping and Acceleration Probe (IMAP) Mission, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-5547, https://doi.org/10.5194/egusphere-egu2020-5547, 2020.