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Taiwan Oscillation Network

Chou, Dean-Yi and Sun, Ming-Tsung and Huang, Teng-Yi and Jimenez, Antonio and Lai, Shih-Ping and Chi, Pi-Jen and Ou, Knight-Tien and Wang, Chang-Chi and Lu, Jui-Yang and Chu, An-Li and Niu, Chi-Seng and Mu, Tao-Mo and Chen, Kuan-Rong and Chou, Yung-Ping and Chao, Horance and Rabello-Soares, Maria Cristina and Ai, Guoxiang and Wang, Gwo-Ping and Zirin, Harold and Marquette, William and Nenow, Jeff (1995) Taiwan Oscillation Network. Solar Physics, 160 (2). pp. 237-243. ISSN 0038-0938. https://resolver.caltech.edu/CaltechAUTHORS:20200518-080645838

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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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/bf00732806DOIArticle
https://ui.adsabs.harvard.edu/abs/1995SoPh..160..237C/abstractADSArticle
Additional Information:© 1995 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 27 February, 1995; in revised form 18 April, 1995. The TON project is supported by NSC of ROC under grants NSC-83-NSPO-B-RDD-007-01 and NSC-84-2612-M-007-001. MTS is also supported by NSC-84-2612-M-182-001. AJ and MCR are supported by Spanish CICYT under grants ESP 90-0969 and PB 91-0530; MCR receives partial support from the Brazilian Institution: CNPq (202504/91-3). We deeply thank all observers who were dedicated to this long-term observation. We are grateful to the GONG Data Team, especially to Drs E. R. Anderson, F. Hill, and J. Leibacher, for providing the software and helping in the data reduction.
Funders:
Funding AgencyGrant Number
National Science Council (Taipei)NSC-83-NSPO-B-RDD-007-01
National Science Council (Taipei)NSC-84-2612-M-007-001
National Science Council (Taipei)NSC-84-2612-M-182-001
Comisión Interministerial de Ciencia y Tecnología (CICYT)ESP 90-0969
Comisión Interministerial de Ciencia y Tecnología (CICYT)PB 91-0530
Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)202504/91-3
Subject Keywords:Internal Structure; Solar Observatory; Oscillation Network; Intensity Oscillation; Solar Intensity
Issue or Number:2
Record Number:CaltechAUTHORS:20200518-080645838
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200518-080645838
Official Citation:Chou, D., Sun, M., Huang, T. et al. Taiwan Oscillation Network. Sol Phys 160, 237–243 (1995). https://doi.org/10.1007/BF00732806
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103261
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:18 May 2020 15:30
Last Modified:18 May 2020 15:30

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