1. Introduction
The capabilities of Earth Observation (EO) missions have seen steady growth in the past many years, assisted by developments of small-satellite bus (e.g. the 3U, 6U, 12U CubeSat and microsat bus from Blue Canyon [1]), new instruments (e.g. compact Ka band precipitation radar [2]), large inter-connected ground-station networks (e.g. Amazon Web Service Ground Station [3]), intersatellite communications [4], onboard data processing (e.g. SpaceCube [5]) and reduced launch costs (e.g. launch services from SpaceX, Rocketlabs). These technological capabilities further allow development of new observation systems involving intelligent and collaborative constellations [6].