Chen, Y.; Mandal, S.; Peter, H.; Chitta, L. P.: Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUI. Astronomy and Astrophysics 692, p. A119 (2024)
Chitta, L. P.; Hannah, I.G.; Fletcher, L.; Hudson, H.S.; Young, P.R.; Krucker, S.; Peter, H.: Hard X-rays from the deep solar atmosphere: An unusual UV burst with flare properties. ASTRONOMY & ASTROPHYSICS (2024)
Chitta, L. P.; van Noort, M.; Smitha, H. N.; Priest, E.R.; van der Voort, L.H.M.R.: Photospheric Hot Spots at Solar Coronal Loop Footpoints Revealed by Hyperspectral Imaging Observations. ASTROPHYSICAL JOURNAL (1) (2024)
Chitta, L. P.; Zhukov, A. N.; Berghmans, D.; Peter, H.; Parenti, S.; Mandal, S.; Aznar Cuadrado, R.; Schühle, U.; Teriaca, L.; Auchère, F.et al.; Barczynski, K.; Buchlin, É.; Harra, L.; Kraaikamp, E.; Long, D. M.; Rodriguez, L.; Schwanitz, C.; Smith, P. J.; Verbeeck, C.; Seaton, D. B.: Picoflare jets power the solar wind emerging from a coronal hole on the Sun. Science 38, pp. 867 - 872 (2023)
Li, Z.; Cheng, X.; Ding, M. D.; Chitta, L. P.; Peter, H.; Berghmans, D.; Smith, P. J.; Auchère, F.; Parenti, S.; Barczynski, K.et al.; Harra, L.; Schühle, U.; Buchlin, É.; Verbeeck, C.; Aznar Cuadrado, R.; Zhukov, A. N.; Long, D. M.; Teriaca, L.; Rodriguez, L.: Evidence of external reconnection between an erupting mini-filament and ambient loops observed by Solar Orbiter/EUI. Astronomy and Astrophysics 673, p. A83 (2023)
Chitta, L. P.; Seaton, D. B.; Downs, C.; DeForest, C. E.; Higginson, A. K.: Direct observations of a complex coronal web driving highly structured slow solar wind. Nature Astronomy (2022)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.