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Taiwan Oscillation Network |
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| Authors: | Dean-Yi Chou Ming-Tsung Sun Teng-Yi Huang Shih-Ping Lai Pi-Jen Chi Knight-Tien Ou Chang-Chi Wang Jui-Yang Lu " target="_blank">An-Li Chu and Chi-Seng Niu |
| Institution: | (1) Physics Department, Tsing Hua University, 30043 Hsinchu, Taiwan, R.O. China;(2) Observatorio del Teide, Instituto Astrofisica de Canarias, Tenerife, Spain;(3) Department of Electro-Optics Engineering, Lien-Ho Junior College of Technology, 36012 Miaoli, Taiwan, R.O. China;(4) Huairou Solar Observing Station, Beijing Observatory, Beijing, P.R. China;(5) Big Bear Solar Observatory, California Institute of Technology, 91125 Pasadena, CA, USA;(6) Present address: Department of Mechanical Engineering, Chang-Gung College of Medical and Technology, Kwei-San, Taiwan, R.O. China |
| Abstract: | The Taiwan Oscillation Network (TON) is a ground-based network to measure solar intensity oscillations to study the internal structure of the Sun. K-line full-disk images of 1000 pixels diameter are taken at a rate of one image per minute. Such data would provide information onp-modes withl as high as 1000. The TON will consist of six identical telescope systems at proper longitudes around the world. Three telescope systems have been installed at Teide Observatory (Tenerife), Huairou Solar Observing Station (near Beijing), and Big Bear Solar Observatory (California). The telescopes at these three sites have been taking data simultaneously since October of 1994. Anl – v diagram derived from 512 images is included to show the quality of the data. |
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