Baumgartner, C.; Birch, A. C.; Schunker, H.; Cameron, R. H.; Gizon, L.: Impact of spatially correlated fluctuations in sunspots on metrics related to magnetic twist. Astronomy and Astrophysics 664, p. A183 (2022)
Braun, D. C.; Birch, A. C.; Fan, Y.: Erratum: "Probing the Solar Meridional Circulation Using Fourier Legendre Decomposition" (2021, ApJ, 911, 54). The Astrophysical Journal 924, p. 140 (2022)
Gottschling, N.; Schunker, H.; Birch, A.; Cameron, R. H.; Gizon, L.: Testing solar surface flux transport models in the first days after active region emergence. Astronomy and Astrophysics 660, A6 (2022)
Gottschling, N.; Schunker, H.; Birch, A. C.; Cameron, R.; Gizon, L.: Testing solar surface flux transport models in the first days after active region emergence. Astronomy and Astrophysics 660, p. A6 (2022)
Böning, V. G. A.; Birch, A.; Gizon, L.; Duvall, T.: Helioseismological determination of the subsurface spatial spectrum of solar convection: Demonstration using numerical simulations. Astronomy and Astrophysics 649, A59 (2021)
Braun, D. C.; Birch, A.; Fan, Y.: Probing the Solar Meridional Circulation Using Fourier Legendre Decomposition. The Astrophysical Journal 911 (1), 54 (2021)
Harra, L.; Andretta, V.; Appourchaux, T.; Baudin, F.; Bellot-Rubio, L.; Birch, A.; Boumier, P.; Cameron, R. H.; Carlsson, M.; Corbard, T.et al.; Davies, J.; Fazakerley, A.; Fineschi, S.; Finsterle, W.; Gizon, L.; Harrison, R.; Hassler, D.M.; Leibacher, J.; Liewer, P.; Macdonald, M.; Maksimovic, M.; Murphy, N.; Naletto, G.; Nigro, G.; Owen, C.; Martínez-Pillet, V.; Rochus, P.; Romoli, M.; Sekii, T.; Spadaro, D.; Veronig, A.; Schmutz, W.: A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitude. Experimental Astronomy (2021)
Zaqarashvili V, T.; Albekioni, M.; Ballester, J. L.; Bekki, Y.; Biancofiore, L.; Birch, A. C.; Dikpati, M.; Gizon, L.; Gurgenashvili, E.; Heifetz, E.et al.; Lanza, A. F.; McIntosh, S. W.; Ofman, L.; Oliver, R.; Proxauf, B.; Umurhan, O. M.; Yellin-Bergovoy, R.: Rossby Waves in Astrophysics. Space Science Reviews 217 (1), 15 (2021)
Dhuri, D.B.; Hanasoge, S.M.; Birch, A.; Schunker, H.: Application and interpretation of deep learning for identifying pre-emergence magnetic field patterns. The Astrophysical Journal 903 (1), 27 (2020)
Goddard, C.; Birch, A.; Fournier, D.; Gizon, L.: Predicting frequency changes of global-scale solar Rossby modes due to solar cycle changes in internal rotation. Astronomy and Astrophysics 640, L10 (2020)
Hanson, C. S.; Duvall, T.; Birch, A.; Gizon, L.; Sreenivasan, K. R.: Solar east-west flow correlations that persist for months at low latitudes are dominated by active region inflows. Astronomy and Astrophysics 644, A103 (2020)
Proxauf, B.; Gizon, L.; Löptien, B.; Schou, J.; Birch, A.; Bogart, R. S.: Exploring the latitude and depth dependence of solar Rossby waves using ring-diagram analysis. Astronomy and Astrophysics 634, A44 (2020)
Schou, J.; Birch, A.: Estimating the nonstructural component of the helioseismic surface term using hydrodynamic simulations. Astronomy and Astrophysics 638, A51 (2020)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
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
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.