Zobrazeno 1 - 10
of 178
pro vyhledávání: '"D. Anger"'
Autor:
Monique Martin, Nicolas Despiegel, Kim Gilchrist, R. Refoios Camejo, D. Anger, Neerav Monga, Q. Cui
Publikováno v:
Value in Health. 17(3)
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Frank D. Anger, Rita V. Rodríguez
Publikováno v:
Constraints. 3:191-202
Numerous AI problems in planning, robot motion, distributed systems, cooperating agents, and intelligence gathering have domains with sub-collections of events or actions over time which are measured on incomparable or unsynchronized time scales from
Publikováno v:
Value in Health. 16(7)
Publikováno v:
Value in Health. 16(3)
Publikováno v:
Physics of Auroral Arc Formation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4907b4d9c58a6e9e1527a9de2ec6549a
https://doi.org/10.1029/gm025p0015
https://doi.org/10.1029/gm025p0015
Publikováno v:
Applied Intelligence. 6:5-9
At the International Joint Conference on Artificial Intelligence (IJCAI) in Chambery, France, the authors organized and ran a Workshop on Spatial and Temporal Reasoning with the purpose of both presenting current research and development in these are
Autor:
Frank D. Anger, Rita V. Rodríguez
Publikováno v:
Applied Intelligence. 6:29-38
Due to increasing interest in representation of temporal knowledge, automation of temporal reasoning, and analysis of distributed systems, literally dozens of temporal models have been proposed and explored during the last decade. Interval-based temp
Autor:
Frank D. Anger, Edmund M. Clarke
Publikováno v:
Applied Intelligence. 3:5-15
TheSpecial Issue on Applications of Temporal Models raises many issues of time: What are the important properties of time? How can time be best represented? How can one reason about time-dependent properties? What are the important directions of temp
Autor:
C. D. Anger, P. B. Hays
Publikováno v:
Applied optics. 17(12)
Satellite observations of the optical emission features in the aurora and nighttime airglow are usually contaminated by scattering from clouds and snow. It is shown here that this contamination can easily be removed when the emission layer is viewed