论文标题

部分可观测时空混沌系统的无模型预测

TANSPEC: TIFR-ARIES Near Infrared Spectrometer

论文作者

Sharma, Saurabh, Ojha, Devendra K., Ghosh, Arpan, Ninan, Joe P., Ghosh, Supriyo, Ghosh, Swarna K., Manoj, P., Naik, Milind B., D'Costa, Savio L. A., Reddy, B. Krishna, Nanjappa, Nandish, Pandey, Rakesh, Sinha, Tirthendu, Panwar, Neelam, Antony, Susmitha, Kaur, Harmeen, Sahu, Sanjit, Bangia, Tarun, Poojary, Satheesha S., Jadhav, Rajesh B., Bhagat, Shailesh B., Meshram, Ganesh S., Shah, Harshit, Rayner, John T., Toomey, Douglas W., Sandimani, Pradeep R.

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。

We present the design and performance of the TANSPEC, a medium-resolution $0.55-2.5~μ$m cryogenic spectrometer and imager, now in operation at the 3.6-m Devasthal Optical Telescope (DOT), Nainital, India. The TANSPEC provides three modes of operation which include, photometry with broad- and narrow-band filters, spectroscopy with short slits of 20$^{\prime \prime}$ length and different widths (from 0.5$^{\prime \prime}$ to 4.0$^{\prime \prime}$) in cross-dispersed mode at a resolving power R of $\sim$2750, and spectroscopy with long slits of 60$^{\prime \prime}$ length and different widths (from 0.5$^{\prime \prime}$ to 4.0$^{\prime \prime}$) in prism mode at a resolving power R of $\sim$100-350. TANSPEC's imager mode provides a field of view of 60$^{\prime \prime} \times 60^{\prime \prime}$ with a plate scale of 0.245$^{\prime \prime}$/pixel on the 3.6-m DOT. The TANSPEC was successfully commissioned during April-May 2019 and the subsequent characterization and astronomical observations are presented here. The TANSPEC has been made available to the worldwide astronomical community for science observations from October 2020.

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