A44G:
Small Satellites Have Scientific Value, but Where Do They Fit In? II
A44G:
Small Satellites Have Scientific Value, but Where Do They Fit In? II
Small Satellites Have Scientific Value, but Where Do They Fit In? II
Submit an Abstract to this Session
Session ID#: 58548
Session Description:
The scientific community and government funding agencies are evaluating the capabilities, limitations, and potential of CubeSats, small satellites, and small satellite constellations for science and long-term data record gap mitigation. Small satellites have demonstrable and in some cases unique scientific value. Their strengths and limitations, which are rapidly evolving as new technologies are developed and demonstrated, are not generally well understood. This session seeks to highlight the state of the art in CubeSat and small satellite science and enabling technologies, specifically as applied to Earth and space science. We invite domestic and international contributions presenting science results obtained from small satellite missions, significant new enabling technologies, commercial platforms and efforts that can be used for scientific research, and new mission concepts that are uniquely suited to small satellites.
Primary Convener: William H Swartz, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Conveners: David M Klumpar, Montana State University - Bozeman, Space Science and Engineering Laboratory, Department of Physics, Bozeman, United States and Pamela Millar, University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Primary Liaisons: William H Swartz, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and David M Klumpar, Montana State University - Bozeman, Space Science and Engineering Laboratory, Department of Physics, Bozeman, United States
Chairs: William H Swartz, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, David M Klumpar, Montana State University - Bozeman, Space Science and Engineering Laboratory, Department of Physics, Bozeman, United States and Pamela Millar, University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
OSPA Liaison: Charles D Norton, NASA Headquarters, Science Mission Directorate, Washington, DC, United States
Co-Organized
with:
Atmospheric Sciences, and SPA-Magnetospheric Physics
Atmospheric Sciences, and SPA-Magnetospheric Physics
Cross-Listed:
- IN - Earth and Space Science Informatics
- SA - SPA-Aeronomy
- SH - SPA-Solar and Heliospheric Physics
- SM - SPA-Magnetospheric Physics
Proposed Co-Organized Session with:
- IN - Earth and Space Science Informatics
- SA - SPA-Aeronomy
- SH - SPA-Solar and Heliospheric Physics
- SM - SPA-Magnetospheric Physics
Index Terms:
0394 Instruments and techniques [ATMOSPHERIC COMPOSITION AND STRUCTURE]
2494 Instruments and techniques [IONOSPHERE]
2794 Instruments and techniques [MAGNETOSPHERIC PHYSICS]
3360 Remote sensing [ATMOSPHERIC PROCESSES]
Abstracts Submitted to this Session:
Recent radio occultation profile results obtained from Spire’s CubeSat GNSS-RO constellation (454531)
See more of: Atmospheric Sciences
