IEICE TRANSACTIONS on Communications
Very Long Baseline Connected Interferometry via the STM-16 ATM Network
Summary :
The Communications Research Laboratory (CRL), the National Astronomical Observatory (NAO), the Institute of Space and Astronoutical Science (ISAS), and the Telecommunication Network Laboratory Group of Nippon Telegraph and Telephone Corporation (NTT) have developed a very-long-baseline-connected-interferometry array, maximum baseline-length was 208 km, using a high-speed asynchronous transfer mode (ATM) network with an AAL1 that corresponds to the constant bit-rate protocol. The very long baseline interferometry (VLBI) observed data is transmitted through a 2.488-Gbps [STM-16/OC-48] ATM network instead of being recorded onto magnetic tape. By combining antennas via a high-speed ATM network, a highly-sensitive virtual (radio) telescope system was realized. The system was composed of two real-time VLBI networks: the Key-Stone-Project (KSP) network of CRL (which is used for measuring crustal deformation in the Tokyo metropolitan area), and the OLIVE (optically linked VLBI experiment) network of NAO and ISAS which is used for astronomy (space-VLBI). These networks operated in cooperation with NTT. In order to realize a virtual telescope, the acquired VLBI data were corrected via the ATM networks and were synthesized using the VLBI technique. The cross-correlation processing and data observation were done simultaneously in this system and radio flares on the weak radio source (HR1099) were detected.
- Publication
- IEICE TRANSACTIONS on Communications Vol.E83-B No.2 pp.238-245
- Publication Date
- 2000/02/25
- Publicized
- Online ISSN
- DOI
- Type of Manuscript
- Special Section PAPER (IEICE/IEEE Joint Special Issue on Recent Progress in ATM Technologies)
- Category
- ATM Switch and System Development
Authors
Hitoshi KIUCHI
Yukio TAKAHASHI
Akihiro KANEKO
Hisao UOSE
Sotetsu IWAMURA
Takashi HOSHINO
Noriyuki KAWAGUCHI
Hideyuki KOBAYASHI
Kenta FUJISAWA
Jun AMAGAI
Junichi NAKAJIMA
Tetsuro KONDO
Satoru IGUCHI
Takeshi MIYAJI
Kazuo SORAI
Kouichi SEBATA
Taizoh YOSHINO
Noriyuki KURIHARA
Keyword
Latest Issue
Copyrights notice of machine-translated contents
The copyright of the original papers published on this site belongs to IEICE. Unauthorized use of the original or translated papers is prohibited. See IEICE Provisions on Copyright for details.
Cite this
Copy
Hitoshi KIUCHI, Yukio TAKAHASHI, Akihiro KANEKO, Hisao UOSE, Sotetsu IWAMURA, Takashi HOSHINO, Noriyuki KAWAGUCHI, Hideyuki KOBAYASHI, Kenta FUJISAWA, Jun AMAGAI, Junichi NAKAJIMA, Tetsuro KONDO, Satoru IGUCHI, Takeshi MIYAJI, Kazuo SORAI, Kouichi SEBATA, Taizoh YOSHINO, Noriyuki KURIHARA, "Very Long Baseline Connected Interferometry via the STM-16 ATM Network" in IEICE TRANSACTIONS on Communications,
vol. E83-B, no. 2, pp. 238-245, February 2000, doi: .
Abstract: The Communications Research Laboratory (CRL), the National Astronomical Observatory (NAO), the Institute of Space and Astronoutical Science (ISAS), and the Telecommunication Network Laboratory Group of Nippon Telegraph and Telephone Corporation (NTT) have developed a very-long-baseline-connected-interferometry array, maximum baseline-length was 208 km, using a high-speed asynchronous transfer mode (ATM) network with an AAL1 that corresponds to the constant bit-rate protocol. The very long baseline interferometry (VLBI) observed data is transmitted through a 2.488-Gbps [STM-16/OC-48] ATM network instead of being recorded onto magnetic tape. By combining antennas via a high-speed ATM network, a highly-sensitive virtual (radio) telescope system was realized. The system was composed of two real-time VLBI networks: the Key-Stone-Project (KSP) network of CRL (which is used for measuring crustal deformation in the Tokyo metropolitan area), and the OLIVE (optically linked VLBI experiment) network of NAO and ISAS which is used for astronomy (space-VLBI). These networks operated in cooperation with NTT. In order to realize a virtual telescope, the acquired VLBI data were corrected via the ATM networks and were synthesized using the VLBI technique. The cross-correlation processing and data observation were done simultaneously in this system and radio flares on the weak radio source (HR1099) were detected.
URL: https://global.ieice.org/en_transactions/communications/10.1587/e83-b_2_238/_p
Copy
@ARTICLE{e83-b_2_238,
author={Hitoshi KIUCHI, Yukio TAKAHASHI, Akihiro KANEKO, Hisao UOSE, Sotetsu IWAMURA, Takashi HOSHINO, Noriyuki KAWAGUCHI, Hideyuki KOBAYASHI, Kenta FUJISAWA, Jun AMAGAI, Junichi NAKAJIMA, Tetsuro KONDO, Satoru IGUCHI, Takeshi MIYAJI, Kazuo SORAI, Kouichi SEBATA, Taizoh YOSHINO, Noriyuki KURIHARA, },
journal={IEICE TRANSACTIONS on Communications},
title={Very Long Baseline Connected Interferometry via the STM-16 ATM Network},
year={2000},
volume={E83-B},
number={2},
pages={238-245},
abstract={The Communications Research Laboratory (CRL), the National Astronomical Observatory (NAO), the Institute of Space and Astronoutical Science (ISAS), and the Telecommunication Network Laboratory Group of Nippon Telegraph and Telephone Corporation (NTT) have developed a very-long-baseline-connected-interferometry array, maximum baseline-length was 208 km, using a high-speed asynchronous transfer mode (ATM) network with an AAL1 that corresponds to the constant bit-rate protocol. The very long baseline interferometry (VLBI) observed data is transmitted through a 2.488-Gbps [STM-16/OC-48] ATM network instead of being recorded onto magnetic tape. By combining antennas via a high-speed ATM network, a highly-sensitive virtual (radio) telescope system was realized. The system was composed of two real-time VLBI networks: the Key-Stone-Project (KSP) network of CRL (which is used for measuring crustal deformation in the Tokyo metropolitan area), and the OLIVE (optically linked VLBI experiment) network of NAO and ISAS which is used for astronomy (space-VLBI). These networks operated in cooperation with NTT. In order to realize a virtual telescope, the acquired VLBI data were corrected via the ATM networks and were synthesized using the VLBI technique. The cross-correlation processing and data observation were done simultaneously in this system and radio flares on the weak radio source (HR1099) were detected.},
keywords={},
doi={},
ISSN={},
month={February},}
Copy
TY - JOUR
TI - Very Long Baseline Connected Interferometry via the STM-16 ATM Network
T2 - IEICE TRANSACTIONS on Communications
SP - 238
EP - 245
AU - Hitoshi KIUCHI
AU - Yukio TAKAHASHI
AU - Akihiro KANEKO
AU - Hisao UOSE
AU - Sotetsu IWAMURA
AU - Takashi HOSHINO
AU - Noriyuki KAWAGUCHI
AU - Hideyuki KOBAYASHI
AU - Kenta FUJISAWA
AU - Jun AMAGAI
AU - Junichi NAKAJIMA
AU - Tetsuro KONDO
AU - Satoru IGUCHI
AU - Takeshi MIYAJI
AU - Kazuo SORAI
AU - Kouichi SEBATA
AU - Taizoh YOSHINO
AU - Noriyuki KURIHARA
PY - 2000
DO -
JO - IEICE TRANSACTIONS on Communications
SN -
VL - E83-B
IS - 2
JA - IEICE TRANSACTIONS on Communications
Y1 - February 2000
AB - The Communications Research Laboratory (CRL), the National Astronomical Observatory (NAO), the Institute of Space and Astronoutical Science (ISAS), and the Telecommunication Network Laboratory Group of Nippon Telegraph and Telephone Corporation (NTT) have developed a very-long-baseline-connected-interferometry array, maximum baseline-length was 208 km, using a high-speed asynchronous transfer mode (ATM) network with an AAL1 that corresponds to the constant bit-rate protocol. The very long baseline interferometry (VLBI) observed data is transmitted through a 2.488-Gbps [STM-16/OC-48] ATM network instead of being recorded onto magnetic tape. By combining antennas via a high-speed ATM network, a highly-sensitive virtual (radio) telescope system was realized. The system was composed of two real-time VLBI networks: the Key-Stone-Project (KSP) network of CRL (which is used for measuring crustal deformation in the Tokyo metropolitan area), and the OLIVE (optically linked VLBI experiment) network of NAO and ISAS which is used for astronomy (space-VLBI). These networks operated in cooperation with NTT. In order to realize a virtual telescope, the acquired VLBI data were corrected via the ATM networks and were synthesized using the VLBI technique. The cross-correlation processing and data observation were done simultaneously in this system and radio flares on the weak radio source (HR1099) were detected.
ER -
English
