Guo, Y.; Pariat, E.; Valori, G.; Anfinogentov, S.; Chen, F.; Georgoulis, M. K.; Liu, Y.; Moraitis, K.; Thalmann, J. K.; Yang, S.: Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. III. Twist Number Method. Astrophysical Journal 840 (1), 40 (2017)
Hong, J.; Ding, M. D.; Li, Y.; Yang, K.; Cheng, X.; Chen, F.; Fang, C.; Cao, W.: Bidirectional Outflows as Evidence Of Magnetic Reconnection Leading to a Solar Microflare. Astrophysical Journal 820 (1), L17 (2016)
Valori, G.; Pariat, E.; Anfinogentov, S.; Chen, F.; Georgoulis, M. K.; Guo, Y.; Liu, Y.; Moraitis, K.; Thalmann, J. K.; Yang, S.: Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. Part I: Finite Volume Methods. Space Science Reviews 201 (1-4), pp. 147 - 200 (2016)
Chen, F.; Peter, H.: Using coronal seismology to estimate the magnetic field strength in a realistic coronal model. Astronomy and Astrophysics 581, A137 (2015)
Cheung, M. C. M.; Boerner, P.; Schrijver, C. J.; Testa, P.; Chen, F.; Peter, H.; Malanushenko, A.: Thermal Diagnostics with the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory: A Validated Method for Differential Emission Measure Inversions. Astrophysical Journal 807, 143 (2015)
Zhang, J.; Zhang, B.; Li, T.; Yang, S.; Zhang, Y.; Li, L.; Chen, F.; Peter, H.: Coronal Heating By the Interaction between Emerging Active Regions and the Quiet Sun Observed By the Solar Dynamics Observatory. Astrophysical Journal 799, L27 (2015)
Chen, F.; Peter, H.; Bingert, S.; Cheung, M. C. M.: A model for the formation of the active region corona driven by magnetic flux emergence. Astronomy and Astrophysics 564, A12 (2014)
Li, L. P.; Peter, H.; Chen, F.; Zhang, J.: Conversion from mutual helicity to self-helicity observed with IRIS. Astronomy and Astrophysics 570, A93 (2014)
Chen, F.; Peter, H.: Using coronal seismology to estimate the magnetic field strength in a realistic coronal model. 2nd International Sino-German Symposium of Solar Physics: Multi Waveband Observations and Modeling of Solar Activity, Bad Honnef, Germany (2015)
Chen, F.; Peter, H.; Bingert, S.: Magnetic Field Lines and Coronal Loops A Difficult Relation. Living With a Star / Iris / Hinode Meeting, Portland, USA (2014)
Chen, F.; Peter, H.; Bingert, S.; Cheung, M. C. M.: Magnetic field lines and coronal loops. 14th European Solar Physics Meeting, Dublin, Ireland (2014)
Chen, F.; Peter, H.: Using coronal seismology to estimate the magnetic field strength in a realistic coronal model. Hinode 9 Science Meeting, Belfast, Ireland (2015)
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).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Two scientific associations have awarded Prof. Dr. Thorsten Kleine the title "Geochemistry Fellow" for his contributions to the understanding of how the Solar System was formed.
Call for applications: PhD positions in planetary science, solar physics, stellar physics, with a starting date in September 2024, at the IMPRS in Göttingen.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
The MPS instruments on board ESA’s JUICE spacecraft have successfully completed their commissioning in space - and delivered their first observational data.