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)
Jiang, J.; Işık, E.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The effect of activity-related meridional flow modulation on the strength of the solar polar magnetic field. Astrophysical Journal 717, pp. 597 - 602 (2010)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.