DASI

The coupled layers of Earth's upper atmosphere, ionosphere, and magnetosphere
form an interacting system. Continuous observations of the characteristics and
features of this system are needed to study, understand and predict its effects.
Arrays of ground-based instruments fielded to produce continuous overlapping
observations of these important regions, combined with innovative
signal-processing and display techniques, are providing a new look at
Earthspace. The NAS Solar and Space Physics Decadal Survey has recommended that
the next major ground-based instrumentation initiative for space science
research be the deployment of widely-distributed arrays of small instruments.
Such arrays will provide continuous real-time observations with the resolution
needed resolve mesoscale phenomena and their dynamic evolution. The ground-based
DASI program (Distributed Arrays of Small Instruments) provides an opportunity
to address the earthward boundaries of the space weather connection. DASI will
address the need for observations to support the next generation of space
weather data-assimilation models and will push our understanding of the physical
processes which interconnect the spheres of Earthspace to a new level. This
next-generation space research program involves synergy with cyberinfrastructure
development, since DASI has strong needs in this area in order to communicate
and coordinate distributed instrument and research activities from around the
world. As this program develops over the next decade, it is envisioned that DASI
instrumentation will provide real-time data for a wide variety of research,
applications, and educational users.
At the Haystack Observatory, work has begun to address these problems using
distributed ground-based instrument arrays. The network of GPS receivers is
providing a capability to map the overlying ionosphere and to investigate the
effects of solar storms on communications and navigation systems. A distribution
of ISIS software radio receivers is being fielded to study the electric fields
which drive the ionospheric effects, as well as to observe the characteristics
and severity of their space weather impact.