Yao, X.; Muñoz Sepúlveda, P. A.; Büchner, J.: Non-thermal electron velocity distribution functions due to 3D kinetic magnetic reconnection for solar coronal plasma conditions. Physics of Plasmas 29 (2), 022104 (2022)
Manthei, A.C.; Benáček, J.; Muñoz, P.A.; Büchner, J.: Refining pulsar radio emission due to streaming instabilities: Linear theory and PIC simulations in a wide parameter range. Astronomy and Astrophysics 649, A145 (2021)
Zhou, X.; Munoz, P. A.; Büchner, J.; Liu, S.; Yao, X.: Wave Excitation by Power-law-Distributed Energetic Electrons with Pitch-angle Anisotropy in the Solar Corona. The Astrophysical Journal 920 (2), 147 (2021)
Muñoz Sepúlveda, P. A.; Jain, N.; Kilian, P.; Büchner, J.: A new hybrid code (CHIEF) implementing the inertial electron fluid equation without approximation. Computer Physics Communications 224, pp. 245 - 264 (2018)
Doctoral candidates joining the Solar System School are offered attractive funding, clear prospects and optimal career conditions. IMPRS-funded students receive a three-year doctoral support contract at 65% pay level. Additional funds are available for travel to international conferences. Following their PhD period, graduates are offered postdoc wrap-up funding.