The ISS as a Launch Platform for Phenomena of Interest

Details The ISS as a Launch Platform for Phenomena of Interest The ISS as a Launch Platform for Phenomena of Interest

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsa11a1566s&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SA11A-1566

Physics

[0358] Atmospheric Composition And Structure / Thermosphere: Energy Deposition, [2427] Ionosphere / Ionosphere/Atmosphere Interactions, [2494] Ionosphere / Instruments And Techniques

Scientific paper

The Ionosphere-Thermosphere-Mesosphere (ITM) region serves as the cross-over boundary between the heliophysical and atmospheric regions of Earth. As such, both electro-dynamic and fluid-dynamic processes operate in this region. The coupling between these processes, acting both as a system driver and feedback element in the ITM region, is still poorly understood. NASA’s International Space Station (ISS) has the potential to play a major role in facilitating long-term studies of the ITM region. The ISS serves as a unique and stable platform for deploying multiple small satellites in a responsive or long-term approach. This approach, along with the ISS’s convenient location within the heart of the ITM, enables the scripted creation of localized and global sensor constellations targeted at key ITM measurement parameters. In this paper we present a small satellite constellation design example that can be developed from the ISS. The constellation design targets global ITM measurements, including considerable observation time in the lower thermosphere (often termed the “inaccessible region” due to high levels of satellite drag that ensures a quick end to satellite lifetimes). The ISS’s established accessibility provides for consistent refurbishment of the constellation and for responsive deployment scenarios based on manual control from within the ISS or the ground, enabling affordable long-term geo-space, space weather, and climate studies.

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