DECoDE: The Dual-channel EUV Coronal Dynamics Explorer

Details DECoDE: The Dual-channel EUV Coronal Dynamics Explorer DECoDE: The Dual-channel EUV Coronal Dynamics Explorer

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spd....34.2005d&link_type=abstract

American Astronomical Society, SPD meeting #34, #20.05; Bulletin of the American Astronomical Society, Vol. 35, p.845

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Scientific paper

DECoDE, the Dual-channel EUV Coronal Dynamics Explorer, is designed to achieve a specific set of mission objectives which are crucial to an improved understanding of fundamental processes in plasma astrophysics and the drivers of space weather.
\begin{bf} Establish the magnetic connectivity, energy and mass transport between the solar chromosphere and corona.
Resolve the internal structure of coronal loops, the basic elements of coronal EUV and soft X-ray emission.
Explore the relationship between small scale reconnection, changes in magnetic topology, and the global scale instabilites that drive space weather.
These science objectives follow logically from NASA's objectives laid out in the `2003 Strategic Plan for NASA,' and in the 2002 SEC Roadmap.

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