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Cited article:

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Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode

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Astronomy & Astrophysics 703 L9 (2025)
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Characterizing the Observational Properties of the Sun’s High-latitude m = 1 Inertial Mode

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Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager

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Inertial Waves in a Nonlinear Simulation of the Sun's Convection Zone and Radiative Interior

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The Sun’s differential rotation is controlled by high-latitude baroclinically unstable inertial modes

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Existence of small-scale Rossby waves points to low convective velocity amplitudes in the Sun

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Observed Power and Frequency Variations of Solar Rossby Waves with Solar Cycles

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Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun

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Identification of Inertial Modes in the Solar Convection Zone

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Radial Trapping of Thermal Rossby Waves within the Convection Zones of Low-mass Stars

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