A Realtime Observatory for Laboratory Simulation of Planetary Circulation View Full Text


Ontology type: schema:Chapter      Open Access: True


Chapter Info

DATE

2007

AUTHORS

S. Ravela , J. Marshall , C. Hill , A. Wong , S. Stransky

ABSTRACT

We present a physical, laboratory-scale analog of large-scale atmos- pheric circulation and develop an observatory for it. By combining observations of a hydro-dynamically unstable flow with a 3D numerical fluid model, we obtain a real-time estimate of the state of the evolving fluid which is better than either model or observations alone. To the best of our knowledge this is the first such observatory for laboratory simulations of planetary flows that functions in real time. New algorithms in modeling, parameter and state estimation, and observation targeting can be rapidly validated, thus making weather and climate application accessible to computational scientists. Properties of the fluid that cannot be directly observed can be effectively studied by a constrained model, thus facilitating scientific inquiry. More... »

PAGES

1155-1162

Book

TITLE

Computational Science – ICCS 2007

ISBN

978-3-540-72583-1
978-3-540-72584-8

From Grant

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-3-540-72584-8_151

DOI

http://dx.doi.org/10.1007/978-3-540-72584-8_151

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1027375583


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