Antenna system characteristic and solar radio burst observation
Sha Li, Yihua Yan, Zhijun Chen, Wei Wang, Donghao Liu

TL;DR
The paper describes the development and capabilities of the Chinese Spectral Radio Heliograph (CSRH), an advanced solar radio imaging instrument, and reports successful observations of solar radio bursts and satellite imaging.
Contribution
It introduces the design, technical specifications, and observational achievements of CSRH, including solar burst detection and imaging techniques for surface sources.
Findings
Successful detection of a solar radio burst between 1.2-1.6GHz.
CSRH's gain exceeds 60 dBi and noise temperature is below 120K.
Imaging of a geosynchronous satellite demonstrates error correction methods.
Abstract
Chinese Spectral Radio Heliograph (CSRH) is an advanced aperture synthesis solar radio heliograph, developed by National Astronomical Observatories, Chinese Academy of Sciences independently. It consists of 100 reflector antennas, which are grouped into two antenna arrays (CSRH-I and CSRH-II) for low and high frequency bands respectively. The frequency band of CSRH-I is 0.4-2GHz and for CSRH-II, the frequency band is 2-15GHz. In the antenna and feed system, CSRH uses an Eleven feed to receive signals coming from the Sun, the radiation pattern with lower side lobe and back lobe of the feed is well radiated. The characteristics of gain G and antenna noise temperature T effect the quality of solar radio imaging. For CSRH, measured G is larger than 60 dBi and is less than 120K, after CSRH-I was established, we have successfully captured a solar radio burst between 1.2-1.6GHz on…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
