Hostname: page-component-cc8bf7c57-llmch Total loading time: 0 Render date: 2024-12-12T06:22:34.397Z Has data issue: false hasContentIssue false

Low Frequency VLBI Project

Published online by Cambridge University Press:  26 May 2016

I.E. Molotov
Affiliation:
Astro Space Center Moscow of LPI RAS, Moscow, Russia
S.F. Likhachev
Affiliation:
Astro Space Center Moscow of LPI RAS, Moscow, Russia
A.A. Chuprikov
Affiliation:
Astro Space Center Moscow of LPI RAS, Moscow, Russia
A. Dementiev
Affiliation:
Radiophysical Research Institute, N. Novgorod, Russia
B. Lipatov
Affiliation:
Radiophysical Research Institute, N. Novgorod, Russia
M. Nechaeva
Affiliation:
Radiophysical Research Institute, N. Novgorod, Russia
S. Snegirev
Affiliation:
Radiophysical Research Institute, N. Novgorod, Russia
N. Dugin
Affiliation:
Radiophysical Research Institute, N. Novgorod, Russia
S. Ananthakrishnan
Affiliation:
National Center for Radioastrophysics of TIFR, Pune, India
V. Balasubramanian
Affiliation:
National Center for Radioastrophysics of TIFR, Pune, India
A. Benz
Affiliation:
Institute of Astronomy of SFIT ETH, Zurich, Switzerland
F. Mantovani
Affiliation:
Instituto di Radioastronomia, del CNR Bologna, Italy
X. Liu
Affiliation:
National Astrnomical Observatories of CAS, China
X. Hong
Affiliation:
National Astrnomical Observatories of CAS, China
A. Kus
Affiliation:
Torun Centre for Astronomy of Nicolaus Copernicus University, Poland
E.P. Molotov
Affiliation:
Russian Institute of Space Device Engineering, Moscow, Russia
S.P. Ignatov
Affiliation:
Russian Institute of Space Device Engineering, Moscow, Russia
B.A. Poperechenko
Affiliation:
Special Research Bureau of MPEI, Moscow, Russia
Y.N. Gorshenkov
Affiliation:
Special Research Bureau of MPEI, Moscow, Russia
A.A. Konovalenko
Affiliation:
Institute of Radio Astronomy, NASU, Kharkiv, Ukraine

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An international Low Frequency VLBI Network (LFVN) has been organized for observations at 327 MHz and 1665 MHz frequencies with MARK-II and S2 recording terminals. Data on the interplanetary medium and spike-like solar bursts were obtained in first preliminary experiments.

Type
Part 9: Instrumentation and Techniques
Copyright
Copyright © Astronomical Society of the Pacific 2002