Section 1. Solar and Stellar Convection: Effects of rotation and surface forcing on deep stellar convection zones P. J. Kaepylae; Analyzing magnetic network and its variations over Solar Cycles 23, 24 and 25 based on magnetic power spectra Y. Luo, J. Jiang and R. Wang; Imaging stellar surface features with optical interferometry X. Haubois; Section 2. Differential Rotation and Meridional Circulation: Differential rotation of the solar chromosphere using multidecadal Ca II K spectroheliograms D. K. Mishra et al.; A frequency-dependent method for measuring the Sun's interior meridional circulation R. Chen and J. Zhao; Probing the Sun's near surface shear layer using HMI spherical harmonic coefficients S. C. Tripathy, K. Jain, S. Kholikov and R. Komm; Rotational shear in the low photosphere of the Sun T. Corbard, M. Faurobert et al.; Near-surface shear layer of solar rotation: origin and significance L. Kitchatinov; The near-surface shear layer (NSSL) of the Sun: a theoretical model A. R. Choudhuri and B. K. Jha; Differential rotation of stars from spot transit mapping: dependence on rotation period and effective temperature A. Araujo and A. Valio; Short and long term spot evolution on EI Eri L. Kriskovics et al.; Magnetic activity under tidal influences in the 2+2 hierarchical quadruple system V815 Herculis Zs. K?vari et al.; Section 3. Global dynamo. Solar and Stellar Activity Cycles: Recent developments in the Babcock-Leighton solar dynamo theory B. B. Karak; Nonlinear and stochastic mechanisms of the solar cycle and their implications for the cycle prediction J. Jiang; A new generation of solar dynamo model and its application to explore the stellar magnetic cycle Z. Zhang; Resonance and stellar dynamos D. Sokoloff, E. Yushkov and A. Serenkova; The role of nonlinear toroidal flux loss due to flux emergence in the long-term evolution of the solar cycle A. Biswas; Dominating active regions in the minima of solar activity R. A. Suleymanova and V. I. Abramenko; Solar cycle variability induced by stochastic fluctuations of BMR properties and at different amounts of dynamo supercriticality Pawan Kumar; Exploring the predictability of the solar cycle from the polar field rise rate: Results from observations and simulations A. Biswas; The North-South asymmetry of the number and magnetic fluxes of active regions of different magneto-morphological types in cycles 23 and 24 A. Zhukova; Prognostic opportunity of the shifted correlation Between Wolf numbers and their time derivatives S. V. Starchenko and S. V. Yakovleva; Chromosphere activity: relations with solar cycles S. Koutchmy and E. Tavabi; Modelling the rotation dependence of cycle variability in sun-like stars: Answering why only slowly rotating stars produce grand minima V. Vashishth; On origin of active/inactive branches on moderate rotating solar analogs V. V. Pipin; Section 4. Helioseismology and Asteroseismology: Recent progress in time-distance helioseismology: meridional circulation, far-side imaging, and sunquakes R. Chen and J. Zhao; Convection, rotation, and magnetic activity of solar-like stars from asteroseismology S. Mathur; Solar inertial modes L. Gizon et al.; A 2D model for the excitation of the linearly stable inertial modes of the Sun by turbulent convection J. Philidet and L. Gizon; Temporal variation of solar equatorial Rossby modes with azimuthal orders 6 <= m <= 10 B. Lekshmi et al.; Observational study of Reynolds stresses associated with solar inertial modes Y. Mandowara et al.; Probing the superadiabaticity of the solar convection zone with inertial modes P. Dey et al.; Effects of small-scale magnetic fields in the photosphere on surface effects for solar-like stars G. Lin, Y. Li, T. Wu and S. Jie; The effect of Coulomb interactions on acoustic oscillations in the outer layers of low-mass stars A. Brito and I. Lopes; Section 5. Local Processes of Ma
