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The main objective of this paper is to introduce the STABLE (Surface flux Transport And Babcock–LEighton) solar dynamo model. STABLE is a 3D Babcock–Leighton/Flux Transport dynamo model in which the source of poloidal field is the explicit emergence, distortion, and dispersal of bipolar magnetic regions (BMRs). Here we describe the STABLE model in more detail than we have previously and we verify...
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