TY - JOUR
T1 - Dynamical recurrent neural networks and pattern recognition methods for time series prediction
T2 - Application to seeing and temperature forecasting in the context of ESO's VLT astronomical weather station
AU - Aussem, A.
AU - Murtagh, F.
AU - Sarazin, M.
PY - 1994
Y1 - 1994
N2 - The European Southern Observatory's planned Astronomical Weather Station for the Very Large Telescope which is currently under construction at Cerro Paranal in Chile includes (i) advance temperature prediction, which would permit air conditioning in the telescope enclosure to be preset as a function of the next night's expected temperature; and (ii) prediction of seeing, a few hours in advance, to allow flexible scheduling of the most appropriate instrumentation. Extensive data, collected since 1985, are being used to appraise various methodologies. A recurrent neural network is described, which uses arbitrary time-delayed connections to capture the dynamic of time series. This endows the model with a memory of its previous states. The resulting network is time- and space-recurrent, and generalizes most recurrent architectures. The performance of this network is discussed. The results are compared with the k-nearest neighbors method.
AB - The European Southern Observatory's planned Astronomical Weather Station for the Very Large Telescope which is currently under construction at Cerro Paranal in Chile includes (i) advance temperature prediction, which would permit air conditioning in the telescope enclosure to be preset as a function of the next night's expected temperature; and (ii) prediction of seeing, a few hours in advance, to allow flexible scheduling of the most appropriate instrumentation. Extensive data, collected since 1985, are being used to appraise various methodologies. A recurrent neural network is described, which uses arbitrary time-delayed connections to capture the dynamic of time series. This endows the model with a memory of its previous states. The resulting network is time- and space-recurrent, and generalizes most recurrent architectures. The performance of this network is discussed. The results are compared with the k-nearest neighbors method.
KW - connectionist networks
KW - correspondance analysis
KW - forecasting
KW - fuzzy methods
KW - k-nearest neighbors
KW - possibility theory
KW - prediction
KW - telescope operations
UR - http://www.scopus.com/inward/record.url?scp=0011878483&partnerID=8YFLogxK
U2 - 10.1016/0083-6656(94)90047-7
DO - 10.1016/0083-6656(94)90047-7
M3 - Article
AN - SCOPUS:0011878483
VL - 38
SP - 357
EP - 374
JO - New Astronomy Reviews
JF - New Astronomy Reviews
SN - 1387-6473
IS - Part 3
ER -