The original paper is in English. Non-English content has been machine-translated and may contain typographical errors or mistranslations. ex. Some numerals are expressed as "XNUMX".
Copyrights notice
The original paper is in English. Non-English content has been machine-translated and may contain typographical errors or mistranslations. Copyrights notice
Makmal Penyelidikan Komunikasi (CRL), Balai Cerap Astronomi Kebangsaan (NAO), Institut Angkasa Lepas dan Sains Astronoutikal (ISAS), dan Kumpulan Makmal Rangkaian Telekomunikasi Nippon Telegraph and Telephone Corporation (NTT) telah membangunkan garis dasar yang sangat panjang. tatasusunan interferometri bersambung, panjang garis dasar maksimum ialah 208 km, menggunakan rangkaian mod pemindahan tak segerak (ATM) berkelajuan tinggi dengan AAL1 yang sepadan dengan protokol kadar bit malar. Data cerapan interferometri garis dasar (VLBI) yang sangat panjang dihantar melalui rangkaian ATM 2.488-Gbps [STM-16/OC-48] dan bukannya dirakam pada pita magnetik. Dengan menggabungkan antena melalui rangkaian ATM berkelajuan tinggi, sistem teleskop maya (radio) yang sangat sensitif telah direalisasikan. Sistem ini terdiri daripada dua rangkaian VLBI masa nyata: rangkaian Key-Stone-Project (KSP) CRL (yang digunakan untuk mengukur ubah bentuk kerak di kawasan metropolitan Tokyo), dan rangkaian OLIVE (percubaan VLBI yang dipautkan secara optik) NAO dan ISAS yang digunakan untuk astronomi (angkasa-VLBI). Rangkaian ini beroperasi dengan kerjasama NTT. Untuk merealisasikan teleskop maya, data VLBI yang diperoleh telah diperbetulkan melalui rangkaian ATM dan disintesis menggunakan teknik VLBI. Pemprosesan korelasi silang dan pemerhatian data dilakukan secara serentak dalam sistem ini dan suar radio pada sumber radio yang lemah (HR1099) telah dikesan.
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
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Salinan
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
Salinan
@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},}
Salinan
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 -