Li, L.; Peter, H.; Chitta, L. P.; Song, H.: On-disk Solar Coronal Condensations Facilitated by Magnetic Reconnection between Open and Closed Magnetic Structures. The Astrophysical Journal 910 (2), 82 (2021)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.: Formation of a Solar Filament by Magnetic Reconnection and Coronal Condensation. The Astrophysical Journal Letters 919 (2), L21 (2021)
Li, L.-P.; Peter, H.; Chitta, L. P.; Song, H.-Q.: Revisiting the formation mechanism for coronal rain from previous studies. Research in Astronomy and Astrophysics 21 (10), 255 (2021)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.; Ji, K.; Xiang, Y.: Magnetic Reconnection between Loops Accelerated By a Nearby Filament Eruption. The Astrophysical Journal 908 (2), 213 (2021)
Young, P. R.; Viall, N. M.; Kirk, M. S.; Mason, E. I.; Chitta, L. P.: An Analysis of Spikes in Atmospheric Imaging Assembly (AIA) Data. Solar Physics 296, 181 (2021)
Chitta, L. P.; Lazarian, A.: Onset of Turbulent Fast Magnetic Reconnection Observed in the Solar Atmosphere. Astrophysical Journal, Letters 890 (1), L2 (2020)
Chitta, L. P.; Peter, H.; Priest, E. R.; Solanki, S. K.: Impulsive coronal heating during the interaction of surface magnetic fields in the lower solar atmosphere. Astronomy and Astrophysics 644, A130 (2020)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.: Relation of Coronal Rain Originating from Coronal Condensations to Interchange Magnetic Reconnection. The Astrophysical Journal 905 (1), 26 (2020)
Pontin, D. I.; Peter, H.; Chitta, L. P.: Non-thermal line broadening due to braiding-induced turbulence in solar coronal loops. Astronomy and Astrophysics 639, A21 (2020)
Chitta, L. P.; Sukarmadji, A. R. C.; van der Voort, L. R.; Peter, H.: Energetics of magnetic transients in a solar active region plage. Astronomy and Astrophysics 623, A176 (2019)
Li, L.; Peter, H.; Chitta, L. P.; Zhang, J.; Su, J.; Song, H.; Hou, Y.; Xia, C.: Repeated Coronal Condensations Caused by Magnetic Reconnection between Solar Coronal Loops. The Astrophysical Journal 884 (1), 34 (2019)
Syntelis, P.; Priest, E. R.; Chitta, L. P.: A Cancellation Nanoflare Model for Solar Chromospheric and Coronal Heating. II. 2D Theory and Simulations. Astrophysical Journal 872 (1), 32 (2019)
Barczynski, K.; Peter, H.; Chitta, L. P.; Solanki, S. K.: Emission of solar chromospheric and transition region features related to the underlying magnetic field. Astronomy and Astrophysics 619, A5 (2018)
Chitta, L. P.; Peter, H.; Solanki, S. K.: Nature of the energy source powering solar coronal loops driven by nanoflares. Astronomy and Astrophysics 615, L9 (2018)
Li, L.; Zhang, J.; Peter, H.; Chitta, L. P.; Su, J.; Song, H.; Xia, C.; Hou, Y.: Quasi-periodic Fast Propagating Magnetoacoustic Waves during the Magnetic Reconnection Between Solar Coronal Loops. The Astrophysical Journal Letters 868 (2), L33 (2018)
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.