We present new global 3D MHD simulations of the solar convection zone that exhibit two distinct states of the dynamo coexisting simultaneously. We discuss our results in terms of the solar active longitudes and hemispheric asymmetry.
BT - Astrophysics and Space Science Proceedings DA - 2020-12 DO - 10.1007/978-3-030-55336-4_27 N2 -We present new global 3D MHD simulations of the solar convection zone that exhibit two distinct states of the dynamo coexisting simultaneously. We discuss our results in terms of the solar active longitudes and hemispheric asymmetry.
PB - Springer International Publishing PY - 2020 SE - 197 SN - 9783030553357/1570-6591, 1570-6605 SP - 197 EP - 199 T2 - Astrophysics and Space Science Proceedings TI - Dynamo States with Strikingly Different Symmetries Coexisting in Global Solar Simulations UR - https://link.springer.com/chapter/10.1007/978-3-030-55336-4_27 VL - 57 ER -