Langfellner, J.; Gizon, L.; Birch, A. C.: Spatially resolved vertical vorticity in solar supergranulation using helioseismology and local correlation tracking. Astronomy and Astrophysics 581, A67 (2015)
Langfellner, J.; Gizon, L.; Birch, A. C.: Anisotropy of the solar network magnetic field around the average supergranule. Astronomy and Astrophysics 579, L7 (2015)
Nielsen, M. B.; Schunker, H.; Gizon, L.; Ball, W. H.: Constraining differential rotation of Sun-like stars from asteroseismic and starspot rotation periods. Astronomy and Astrophysics 582, A10 (2015)
Ball, W. H.; Gizon, L.: A new correction of stellar oscillation frequencies for near-surface effects (Corrigendum). Astronomy and Astrophysics 569, C2 (2014)
Cameron, R. H.; Jiang, J.; Schuessler, M.; Gizon, L.: Physical causes of solar cycle amplitude variability. Journal of Geophysical Research: Space Physics 119, pp. 680 - 688 (2014)
Deheuvels, S.; Doğan, G.; Goupil, M. J.; Appourchaux, T.; Benomar, O.; Bruntt, H.; Campante, T. L.; Casagrande, L.; Ceillier, T.; Davies, G. R.et al.; De Cat, P.; Fu, J. N.; García, R. A.; Lobel, A.; Mosser, B.; Reese, D. R.; Regulo, C.; Schou, J.; Stahn, T.; Thygesen, A. O.; Yang, X. H.; Chaplin, W. J.; Christensen-Dalsgaard, J.; Eggenberger, P.; Gizon, L.; Mathis, S.; Molenda-Żakowicz, J.; Pinsonneault, M.: Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants. Astronomy and Astrophysics 564, A27 (2014)
Fournier, D.; Gizon, L.; Hohage, T.; Birch, A.: Generalization of the noise model for time‐distance helioseismology. Astronomy and Astrophysics 567, A137 (2014)
Jiang, J.; Hathaway, D. H.; Cameron, R. H.; Solanki, S. K.; Gizon, L.; Upton, L.: Magnetic Flux Transport at the Solar Surface. Space Science Reviews 186, pp. 491 - 523 (2014)
Langfellner, J.; Gizon, L.; Birch, A. C.: Time-distance helioseismology: A new averaging scheme for measuring flow vorticity. Astronomy and Astrophysics 570, A90 (2014)
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.
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