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.

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Publication Details

Published
2025-01-01
DOI
https://doi.org/10.46620/ursiaprasc25/bskf7080
Primary Topic
Astronomical Observations and Instrumentation
Type
article
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Research progress on MUSER and IPS telescope for space weather

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Research progress on MUSER and IPS telescope for space weather

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Abstract

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.

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Astronomical Observations and Instrumentation
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