Jiang, J.; Cameron, R. H.; Schmitt, D.; Işık, E.: Modeling solar cycles 15 to 21 using a flux transport dynamo. Astronomy and Astrophysics 553, A128 (2013)
Jiang, J.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The solar magnetic field since 1700 I. Characteristics of sunspot group emergence and reconstruction of the butterfly diagram. Astronomy and Astrophysics 528, A82 (2011)
Jiang, J.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The solar magnetic field since 1700 II. Physical reconstruction of total, polar and open flux. Astronomy and Astrophysics 528, A83 (2011)
Cameron, R. H.; Jiang, J.; Schmitt, D.; Schüssler, M.: Surface flux transport modeling for solar cycles 15-21: effects of cycle-dependent tilt angles of sunspot groups. Astrophysical Journal 719, pp. 264 - 270 (2010)
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The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.