Towards an algebraic method of solar cycle prediction - I. Calculating the ultimate dipole contributions of individual active regions | Journal of Space Weather and Space Climate

Topical Issue - Space climate: The past and future of solar activity

Open Access

Fig. 1

Solutions of the 1D SFT equation with a bipolar source placed at λ₀ = +15° latitude at time t = 0. Units of the model parameters shown on top of the rows are m/s, km²/s and year, respectively. The meridional flow profile is given by equation (9). Dashed blue lines in the left-hand plots mark the asymptotic solutions D = δD_∞ (top) and D = δD_∞exp(−t/τ) (bottom).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.