First reported detection of poleward meridional flow at chromospheric heights via long-term 17 GHz radio observations, with motion tracking magnetic flux transport and supporting deep magnetic anchoring.
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astro-ph.SR 2years
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UNVERDICTED 2representative citing papers
Gaussian separation reveals that optimization and CFIT NLFFF models reproduce some coronal current signatures from magnetogram data for AR 11429 but the CFIT model alters a flux rope signature along the lower PIL.
citing papers explorer
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Radio Signature of Higher Atmospheric Meridional Flow and Implications for Magnetic Trees in the Sun
First reported detection of poleward meridional flow at chromospheric heights via long-term 17 GHz radio observations, with motion tracking magnetic flux transport and supporting deep magnetic anchoring.
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Validating Coronal Magnetic Field Models Using Gaussian Separation
Gaussian separation reveals that optimization and CFIT NLFFF models reproduce some coronal current signatures from magnetogram data for AR 11429 but the CFIT model alters a flux rope signature along the lower PIL.