Taiwan Oscillation Network

Dean Yi Chou; Ming Tsung Sun; Teng Yi Huang; Shih Ping Lai; Pi Jen Chi; Knight Tien Ou; Chang Chi Wang; Jui Yang Lu; An Li Chu; Chi Seng Niu; Tao Mo Mu; Kuan Rong Chen; Yung Ping Chou; Antonio Jimenez; Maria Cristina Rabello-Soares; Horance Chao; Guoxiang Ai; Gwo Ping Wang; Harold Zirin; William Marquette; Jeff Nenow

doi:10.1007/BF00732806

Taiwan Oscillation Network

Dean Yi Chou^*, Ming Tsung Sun, Teng Yi Huang, Shih Ping Lai, Pi Jen Chi, Knight Tien Ou, Chang Chi Wang, Jui Yang Lu, An Li Chu, Chi Seng Niu, Tao Mo Mu, Kuan Rong Chen, Yung Ping Chou, Antonio Jimenez, Maria Cristina Rabello-Soares, Horance Chao, Guoxiang Ai, Gwo Ping Wang, Harold Zirin, William MarquetteJeff Nenow

^*Corresponding author for this work

Research output: Contribution to journal › Journal Article › peer-review

45 Scopus citations

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 on p-modes with l 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. An l - v diagram derived from 512 images is included to show the quality of the data.

Original language	English
Pages (from-to)	237-243
Number of pages	7
Journal	Solar Physics
Volume	160
Issue number	2
DOIs	https://doi.org/10.1007/BF00732806
State	Published - 09 1995
Externally published	Yes

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title = "Taiwan Oscillation Network",

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 on p-modes with l 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. An l - v diagram derived from 512 images is included to show the quality of the data.",

author = "Chou, {Dean Yi} and Sun, {Ming Tsung} and Huang, {Teng Yi} 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 Antonio Jimenez and Rabello-Soares, {Maria Cristina} and Horance Chao and Guoxiang Ai and Wang, {Gwo Ping} and Harold Zirin and William Marquette and Jeff Nenow",

year = "1995",

month = sep,

doi = "10.1007/BF00732806",

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volume = "160",

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T1 - Taiwan Oscillation Network

AU - Chou, Dean Yi

AU - Sun, Ming Tsung

AU - Huang, Teng Yi

AU - Lai, Shih Ping

AU - Chi, Pi Jen

AU - Ou, Knight Tien

AU - Wang, Chang Chi

AU - Lu, Jui Yang

AU - Chu, An Li

AU - Niu, Chi Seng

AU - Mu, Tao Mo

AU - Chen, Kuan Rong

AU - Chou, Yung Ping

AU - Jimenez, Antonio

AU - Rabello-Soares, Maria Cristina

AU - Chao, Horance

AU - Ai, Guoxiang

AU - Wang, Gwo Ping

AU - Zirin, Harold

AU - Marquette, William

AU - Nenow, Jeff

PY - 1995/9

Y1 - 1995/9

N2 - 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 on p-modes with l 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. An l - v diagram derived from 512 images is included to show the quality of the data.

AB - 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 on p-modes with l 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. An l - v diagram derived from 512 images is included to show the quality of the data.

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DO - 10.1007/BF00732806

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SN - 0038-0938

VL - 160

SP - 237

EP - 243

JO - Solar Physics

JF - Solar Physics

IS - 2

ER -

Taiwan Oscillation Network

Abstract

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