论文标题

部分可观测时空混沌系统的无模型预测

From Assembly to the Complete Integration and Verification of the SOXS Common Path

论文作者

Santhakumari, Kalyan Kumar Radhakrishnan, Battaini, Federico, Claudi, Riccardo, Slemer, Alessandra, Biondi, F., Munari, M., Sanchez, R. Z., Aliverti, M., Oggioni, L., Colapietro, M., Ricci, D., Lessio, L., Dima, M., Marafatto, L., Farinato, J., Campana, S., Schipani, P., DOrsi, S., Salasnich, B., Baruffolo, A., Ami, S. Ben, Capasso, G., Cosentino, R., Alessio, F. D, DAvanzo, P., Hershko, O., Kuncarayakti, H., Landoni, M., Pignata, G., Rubin, A., Scuderi, S., Vitali, F., Young, D., Achrn, J., Durn, Jos Antonio Araiza, Arcavi, I., Brucalassi, Anna, Bruch, R., Cappellaro, Enrico, Della Valle, M., Di Benedetto, R., Yam, A. Gal, Genoni, Matteo, Hernandez, M., Kotilainen, J., Causi, G. Li, Marty, L., Mattila, S., Rappaport, Michael, Riva, M., Smartt, S., Stritzingerv, M., Venturae, H.

论文摘要

储层计算是预测湍流的有力工具,其简单的架构具有处理大型系统的计算效率。然而,其实现通常需要完整的状态向量测量和系统非线性知识。我们使用非线性投影函数将系统测量扩展到高维空间,然后将其输入到储层中以获得预测。我们展示了这种储层计算网络在时空混沌系统上的应用,该系统模拟了湍流的若干特征。我们表明,使用径向基函数作为非线性投影器,即使只有部分观测并且不知道控制方程,也能稳健地捕捉复杂的系统非线性。最后,我们表明,当测量稀疏、不完整且带有噪声,甚至控制方程变得不准确时,我们的网络仍然可以产生相当准确的预测,从而为实际湍流系统的无模型预测铺平了道路。

The Son Of X-Shooter (SOXS) is a single object spectrograph offering simultaneous spectral coverage in UV-VIS (350-850 nm) and NIR (800-2000 nm) wavelength regimes with an average of R close to 4500 for a 1 slit. SOXS also has imaging capabilities in the visible wavelength regime. It is designed and optimized to observe all kinds of transients and variable sources. The final destination of SOXS is the Nasmyth platform of the ESO NTT at La Silla, Chile. The SOXS consortium has a relatively large geographic spread, and therefore the Assembly Integration and Verification (AIV) of this medium-class instrument follows a modular approach. Each of the five main sub-systems of SOXS, namely the Common Path, the Calibration Unit, the Acquisition Camera, the UV-VIS Spectrograph, and the NIR Spectrograph, are undergoing (or undergone) internal alignment and testing in the respective consortium institutes. INAF-Osservatorio Astronomico di Padova delivers the Common Path sub-system, the backbone of the entire instrument. We report the Common Path internal alignment starting from the assembly of the individual components to the final testing of the optical quality, and the efficiency of the complete sub-system.

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