Research progress on MUSER and IPS telescope for space weather
The Mingantu Spectral Radioheliograph (MUSER), initially named the Chinese Spectral Radioheliograph (CSRH), was developed from 2009 -2016.Located at the Mingantu Observing Station in Inner Mongolia, it covers the 400 MHz to 15 GHz frequency range.Currently, it consists of two arrays: MUSER -I (400 MHz to 2.0 GHz with 40 4.5 m mesh antennas) and MUSER -II (2 to 15 GHz with 60 2 m dish antennas).Under the Meridian -II Project, it has been expanded with MUSER -L (30 to 400 MHz using 224 Log -Periodic Dipole Antennas).MUSER's mission is to provide solar radio images for monitoring solar bursts from the solar surface to interplanetary space.So far, MUSER has observed dozens of solar radio burst events, which have provided valuable data for solar physics and space weather research.
Authors
- Yihua Yan (ORCID: https://orcid.org/0000-0002-7106-6029)
- Wei Wang (ORCID: https://orcid.org/0000-0003-4023-2845)
- Zhijun Chen (ORCID: https://orcid.org/0000-0001-7023-6519)
- Jin Fan (ORCID: https://orcid.org/0009-0007-5903-0393)
- Linjie Chen (ORCID: https://orcid.org/0000-0002-4721-1812)
- Cang Su
- Ming Xiong (ORCID: https://orcid.org/0000-0001-9427-7366)
Publication Details
- Published
- 2025-01-01
- DOI
- https://doi.org/10.46620/ursiaprasc25/bskf7080
- Primary Topic
- Astronomical Observations and Instrumentation
- Type
- article
- Field-Weighted Citation Impact
- 0.00