Publikationen von F. Chen

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)

Warnecke, J.; Chen, F.; Bingert, S.; Peter, H.: Current systems of coronal loops in 3D MHD simulations. Astronomy and Astrophysics 607, A 53 (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)

Li, L.; Zhang, J.; Peter, H.; Priest, E.; Chen, H.; Guo, L.; Chen, F.; Mackay, D.: Magnetic reconnection between a solar filament and nearby coronal loops. Nature Physics 12 (9), S. 847 - 851 (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), S. 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)

Chen, F.; Peter, H.; Bingert, S.; Cheung, M. C. M.: Magnetic Jam in the Corona of the Sun. Nature Physics 11, S. 492 - 495 (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)

Li, L. P.; Peter, H.; Chen, F.; Zhang, J.: Heating and cooling of coronal loops observed by SDO. Astronomy and Astrophysics 583, A109 (2015)

Yan, L.; Peter, H.; He, J.; Tian, H.; Xia, L.; Wang, L.; Tu, C.; Zhang, L.; Chen, F.; Barczynski, K.: Self-Absorption in the Solar Transition Region. Astrophysical Journal 811, 48 (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)

Chen, F.: Coronal dynamics driven by magnetic flux emergence. Dissertation, Georg-August-Univ. Göttingen, Göttingen (2015)