Radio Imaging Spectroscopy of Physical Processes in the Inner Heliosphere
Abstract
Radio observations below 100 MHz made using an array of small radio antennae on the lunar surface can provide unique insight into non-thermal processes in the corona and heliosphere. Such an array fits within reasonable weight, power, telemetry, and cost constraints.
- Publication:
-
Deep Space Gateway Concept Science Workshop
- Pub Date:
- February 2018
- Bibcode:
- 2018LPICo2063.3185K