The m=1 high-latitude inertial mode frequency implies solar rotation of 365.3 nHz at 75° latitude and 0.8 R_sun, exceeding the p-mode reference by 8.1 nHz.
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Spectral decomposition of sunspot numbers from 1700-2023 yields a forecast of a grand solar minimum from 2030 to 2110 with peak amplitudes roughly half those of recent cycles.
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Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun
The m=1 high-latitude inertial mode frequency implies solar rotation of 365.3 nHz at 75° latitude and 0.8 R_sun, exceeding the p-mode reference by 8.1 nHz.
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Combining spectral analysis and narrow band pass filtering to predict solar cycle parameters in the next solar grand minimum
Spectral decomposition of sunspot numbers from 1700-2023 yields a forecast of a grand solar minimum from 2030 to 2110 with peak amplitudes roughly half those of recent cycles.