EGU24-6388, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-6388
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

ELMO: ELectron Microburst Observatory mission to study microbursts

Shri Kanekal
Shri Kanekal
  • NASA Goddard Space Flight Center, Heliospheric Physics, Code 672, Greenbelt, United States of America (shrikanth.g.kanekal@nasa.gov)

We describe the ELectron Microburst Observatory mission, ELMO  which is proposed as  a
CubeSat constellation mission to fully characterize microburst event spatial extent systematically for the first time both in latitude  and longitude. ELMO comprises 4 CubeSats two per orbit plane in two orbit planes. ELMO will fly in a high inclination LEO at about 500 km in altitude. The CubeSats will systematically separate both in latitude and longitude over the mission lifetime and will carry MERIT, Miniaturized Electron and Proton Telescope as the the payload. MERIT has been built,tested and delivered  to fly on NASA's HERMES, Lunar Gateway mission. MERIT is a solid state detector particle telescope with two identical sensor heads pointed zenith- and nadir-wards enabling measurement of both downgpoing and upwelling electrons thereby accurately estimating  electron precipitation into the atmosphere.  MERIT  will measure electron and protons over a wide energy range in multiple differential channels with a very time resolution of less than 4 ms.    

ELMO will quantify for the first time the contribution of microbursts to radiation belt electron loss using systematic coordinated multipoint measurements. Energetic electron precipitation affects atmospheric chemistry and therefore climate change. ELMO measures
microbursts with unprecedented time and energy resolution. ELMO provides critical knowledge of electron loss processes required for quantitative prediction of global electron fluxes.

How to cite: Kanekal, S.: ELMO: ELectron Microburst Observatory mission to study microbursts, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-6388, https://doi.org/10.5194/egusphere-egu24-6388, 2024.