Schunker, H.; Gizon, L.; Cameron, R. H.; Birch, A. C.: Helioseismology of sunspots: how sensitive are travel times to the Wilson depression and to the subsurface magnetic field? Astronomy and Astrophysics 558, A130 (2013)
Woodard, M.; Schou, J.; Birch, A. C.; Larson, T. P.: Global-oscillation eigenfunction measurements of solar meridional flow. Solar Physics 287 (1-2), pp. 129 - 147 (2013)
Felipe, T.; Braun, D.; Crouch, A.; Birch, A.: Scattering of the f-mode by small magnetic flux elements from observations and numerical simulations. Astrophysical Journal 757, 148 (2012)
Birch, A.; Gizon, L.; Hanasoge, S.; Langfellner, J.: Ist die Konvektion im Sonneninneren langsamer als gedacht? In: Jahrbuch 2013, n/a. Max-Planck-Gesellschaft, München (2013)
Gottschling, N.; Schunker, H.; Birch, A.; Gizon, L.: Evolution of Flows around Emerging Active Regions. Astronomical Institute at the Ruhr-University Bochum, Bochum, Germany (2019)
Gottschling, N.; Schunker, H.; Birch, A.; Gizon, L.: Evolution of Flows around Emerging Active Regions. 234th Meeting of the American Astronomical Society , St. Louis, Missouri, USA (2019)
Proxauf, B.; Gizon, L.; Löptien, B.; Birch, A.; Schou, J.; Bogart, R. S.: On the latitude dependence of Rossby waves in the Sun. 234th Meeting of the American Astronomical Society, St. Louis, USA (2019)
Proxauf, B.; Gizon, L.; Löptien, B.; Birch, A.; Schou, J.; Bogart, R. S.: Exploring the latitude and depth dependence of solar Rossby waves. 2nd Max Planck Partner Group Workshop on Solar Physics, Mumbai, India (2019)
Ferret, R. Z.; Gizon, L.; Birch, A.; Cameron, R.: New insights on the depth of an average supergranule through forward modeling in time-distance helioseismology. Rocks \& Stars II, Göttingen, Germany (2017)
Langfellner, J.; Birch, A. C.; Gizon, L.: The wave-like nature of solar supergranulation - revisited. Rocks and Stars II Conference, Goettingen, Germany (2017)
Liang, Z.-C.; Birch, A. C.; Duvall Jr., T. L.; Gizon, L.; Schou, J.: Helioseismic travel-time measurements of solar meridional from SDO/HMI and SOHO/MDI. 15th European Solar Physics Meeting, Budapest, Hungary (2017)
Langfellner, J.; Gizon, L.; Birch, A. C.: Evolution of solar intermediate-scale convection. Seismology of the Sun and Distant Stars (HELAS8/SPACEINN/TASC2/KASC9), Angra do Heroismo, Portugal (2016)
Löptien, B.; Birch, A. C.; Duvall{} Jr., T. L.; Gizon, L.; Schou, J.: Measuring active region inflows with local correlation tracking. Solar and Stellar Magnetic Fields - a conference in honor of Manfred Schuessler, Goslar, Germany (2016)
Schunker, H.; Birch, A. C.; Braun, D. C.: Constraining the common properties of active region formation using the SDO/HEAR dataset. SDO 2016: Unraveling the Sun's Complexity, Burlington, Vermont, USA (2016)
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).
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
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.
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).
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
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.
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).