International low-frequency very-long-baseline interferometry network project milestones
- Molotov, I.
- Kovalenko, A.
- Samodurov, V.
- Lipatov, B.
- Dementiev, A.
- Antipenko, A.
- Snegirev, S.
- Nechaeva, M.
- Reznikova, V.
- Altunin, V.
- Benz, A.
- Mantovani, F.
- Stanghellini, C.
- Tuccari, G.
- Konovalenko, A.
- Falkovich, I.
- Gridin, A.
- Ananthakrishnan, S.
- Balasubramanian, V.
- Sankararaman, M.
- Hong, X.
- Huang, X.
- Shiguang, L.
- Dougherty, S.
- Del Rizzo, D.
- Fink, A.
- Liu, X.
- Na, W.
- Zhang, J.
- Kus, A.
- Borkowski, K.
- Quick, J.
- Nicolson, G.
- Shmeld, I.
- Koyama, Y.
- Sekido, M.
- Gorshenkov, Yu.
- Poperechenko, B.
- Saurin, V.
- Ozolins, G.
- Bezrukov, D.
- Zhang, X.
DOIAbstract
The low-frequency very-long-baseline interferometry network (LFVN) project was started in 1996, having the purpose to arrange the international very-long-baseline interferometry (VLBI) cooperation with participation of former Soviet Union radio telescopes. Currently there are three directions of LFVN development: a Mk 2 subsystem at 92 cm wavelength for solar research, an international S2 ad hoc array at 18 cm for active Galactic nuclei and OH-maser survey, and VLBI radar at 6 cm for investigation of Solar System bodies. 14 VLBI experiments were carried out using various combinations of radio telescopes in Canada, China, England, India, Italy, Japan, Latvia, Poland, Russia, South Africa, Ukraine and USA. The five sessions were processed by ...
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