96-antenna radioheliograph

Abstract

Here we briefly present some design approaches for a multifrequency 96-antenna radioheliograph. The array antenna configuration, transmission lines and digital receivers are the main focus of this work. The radioheliograph is a T-shaped centrally-condensed radiointerferometer operating at the frequency range 4-8~GHz. The justification for the choice of such a configuration is discussed. The antenna signals are transmitted to a workroom by analog optical links. The dynamic range and phase errors of the microwave-over-optical signal are considered. The signals after downconverting are processed by the digital receivers for delay tracking and fringe stopping. The required delay tracking step and data rates are considered. Two 3-bit data streams (I and Q) are transmitted to a correlator with the transceivers embedded in FPGA (Field Programmed Gate Array) chips and with PCI Express cables.

References in corpus (1)

• The multifrequency Siberian Radioheliograph

Cited by in corpus (7)

• Solar Physics with the Square Kilometre Array
• Multi-instrument view on solar eruptive events observed with the Siberian Radioheliograph: From detection of small jets up to development of a shock wave and CME
• Common origin of quasi-periodic pulsations in microwave and decimetric solar radio bursts
• Flare SOL2012-07-06: on the origin of the circular polarization reversal between 17 GHz and 34 GHz
• The 26 December 2001 Solar Event Responsible for GLE63. I. Observations of a Major Long-Duration Flare with the Siberian Solar Radio Telescope
• Antenna system characteristic and solar radio burst observation
• Twin Null-Point-Associated Major Eruptive Three-Ribbon Flares with Unusual Microwave Spectra