Publikationen von Hardi Peter

Warnecke, J.; Chen, F.; Bingert, S.; Peter, H.: Current systems of coronal loops in 3D MHD simulations. Astronomy and Astrophysics 607, A 53 (2017)

Bourdin, P. A.; Bingert, S.; Peter, H.: Scaling laws of coronal loops compared to a 3D MHD model of an active region. Astronomy and Astrophysics 589, A86 (2016)

Chitta, L. P.; Peter, H.; Young, P. R.: A closer look at a coronal loop rooted in a sunspot umbra. Astronomy and Astrophysics 587, A20 (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)

Ruan, W.; He, J.; Zhang, L.; Vocks, C.; Marsch, E.; Tu, C.; Peter, H.; Wang, L.: Kinetic Simulation of Slow Magnetosonic Waves and Quasi-Periodic Upflows in the Solar Corona. Astrophysical Journal 825 (1), 58 (2016)

Bourdin, P. A.; Bingert, S.; Peter, H.: Coronal energy input and dissipation in a solar active region 3D MHD model. Astronomy and Astrophysics 580, A72 (2015)

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)

De Pontieu, B.; McIntosh, S.; Martinez-Sykora, J.; Peter, H.; Pereira, T. M. D.: Why is Non-Thermal Line Broadening of Spectral Lines in the Lower Transition Region of the Sun Independent of Spatial Resolution? Astrophysical Journal 799 (1), L12 (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)

Peter, H.: What can large-scale magnetohydrodynamic numerical experiments tell us about coronal heating? Phil. Trans. R. Soc. A 373 (2042), 20150055 (2015)

Peter, H.; Warnecke, J.; Chitta, L. P.; Cameron, R. H.: Limitations of force-free magnetic field extrapolations: Revisiting basic assumptions. Astronomy and Astrophysics 584, A68 (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)

Yang, L.; Zhang, L.; He, J.; Peter, H.; Tu, C.; Wang, L.; Zhang, S.; Feng, X.: Numerical Simulation of Fast-mode Magnetosonic Waves Excited by Plasmoid Ejections in the Solar Corona. Astrophysical Journal 800 (2), 111 (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)

Bourdin, P.-A.; Bingert, S.; Peter, H.: Coronal loops above an active region: Observation versus model. Publ. Astron. Soc. Japan 66, S7 (2014)

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)

Peter, H.; Dwivedi, B. N.: Discovery of the Sun's million-degree hot corona. Frontiers in Astronomy and Space Sciences 1, 2 (2014)