Figure 4From: Dynamic bifurcation for the granulation convection in the solar photosphere The graph of \(\pmb{L_{kl}}\) . The curl \(L_{kl}\) passes through the point \((R_{1},F_{1})\) and intersects with the R-axis at \(R_{C_{1}}\), it is easy to find that \(R_{C}> R_{C_{1}}\).Back to article page