Nelson, C. J.; Auchère, F.; Aznar Cuadrado, R.; Barczynski, K.; Buchlin, E.; Harra, L.; Long, D. M.; Parenti, S.; Peter, H.; Schühle, U.et al.; Schwanitz, C.; Smith, P.; Teriaca, L.; Verbeeck, C.; Zhukov, A. N.; Berghmans, D.: Extreme-ultraviolet brightenings in the quiet-Sun: Signatures in spectral and imaging data from the Interface Region Imaging Spectrograph. Astronomy and Astrophysics 676, A64 (2023)
Schwanitz, C.; Harra, L.; Mandrini, C. H.; Sterling, A. C.; Raouafi, N. E.; Mac Cormack, C.; Berghmans, D.; Auchère, F.; Barczynski, K.; Aznar Cuadrado, R.et al.; Buchlin, É.; Kraaikamp, E.; Long, D. M.; Parenti, S.; Peter, H.; Rodriguez, L.; Schühle, U.; Smith, P.; Teriaca, L.; Verbeeck, C.; Zhukov, A. N.: Small-scale EUV features as the drivers of coronal upflows in the quiet Sun. Astronomy and Astrophysics 674, p. A219 (2023)
Yardley, S. L.; Owen, C. J.; Long, D. M.; Baker, D.; Brooks, D. H.; Polito, V.; Green, L. M.; Matthews, S.; Owens, M.; Lockwood, M.et al.; Stansby, D.; James, A. W.; Valori, G.; Giunta, A.; Janvier, M.; Ngampoopun, N.; Mihailescu, T.; To, A. S. H.; van Driel-Gesztelyi, L.; Démoulin, P.; D'Amicis, R.; French, R. J.; Suen, G. H. H.; Rouillard, A. P.; Pinto, R. F.; Réville, V.; Watson, C. J.; Walsh, A. P.; De Groof, A.; Williams, D. R.; Zouganelis, I.; Müller, D.; Berghmans, D.; Auchère, F.; Harra, L.; Schühle, U. H.; Barczynski, K.; Buchlin, É.; Aznar Cuadrado, R.; Kraaikamp, E.; Mandal, S.; Parenti, S.; Peter, H.; Rodriguez, L.; Schwanitz, C.; Smith, P.; Teriaca, L.; Verbeeck, C.; Zhukov, A. N.; De Pontieu, B.; Horbury, T.; Solanki, S. K.; del Toro Iniesta, J. C.; Woch, J.; Gandorfer, A. M.; Hirzberger, J.; Súarez, D. O.; Appourchaux, T.; Calchetti, D.; Sinjan, J.; Kahil, F.; Albert, K.; Volkmer, R.; Carlsson, M.; Fludra, A.; Hassler, D.; Caldwell, M.; Fredvik, T.; Grundy, T.; Guest, S.; Haberreiter, M.; Leeks, S.; Pelouze, G.; Plowman, J.; Schmutz, W.; Sidher, S.; Thompson, W. T.; Louarn, P.; Federov, A.: Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage. The Astrophysical Journal Supplement Series 267, p. 11 (2023)
Bhatia, T. S.; Cameron, R. H.; Solanki, S. K.; Peter, H.; Przybylski, D.; Witzke, V.; Shapiro, A.: Small-scale dynamo in cool stars. I. Changes in stratification and near-surface convection for main-sequence spectral types. Astronomy and Astrophysics 663, p. A166 (2022)
Brooks, D. H.; Janvier, M.; Baker, D.; Warren, H. P.; Auchère, F.; Carlsson, M.; Fludra, A.; Hassler, D.; Peter, H.; Müller, D.et al.; Williams, D.; Aznar Cuadrado, R.; Barczynski, K.; Buchlin, E.; Caldwell, M.; Fredvik, T.; Giunta, A.; Grundy, T.; Guest, S.; Haberreiter, M.; Harra, L.; Leeks, S.; Parenti, S.; Pelouze, G.; Plowman, J.; Schmutz, W.; Schühle, U.; Sidher, S.; Teriaca, L.; Thompson, W. T.; Young, P. R.: Plasma Composition Measurements in an Active Region from Solar Orbiter/SPICE and Hinode/EIS. The Astrophysical Journal 940, p. 66 (2022)
Chen, H.; Tian, H.; Li, L.; Peter, H.; Chitta, L. P.; Hou, Z.: Coronal condensation as the source of transition-region supersonic downflows above a sunspot. Astronomy and Astrophysics 659, p. A107 (2022)
Chen, Y.; Peter, H.; Przybylski, D.; Tian, H.; Zhang, J.: Doppler shifts of spectral lines formed in the solar transition region and corona. Astronomy and Astrophysics 661, p. A94 (2022)
Hu, H.; Liu, Y. D.; Chitta, L. P.; Peter, H.; Ding, M.: Spectroscopic and Imaging Observations of Spatially Extended Magnetic Reconnection in the Splitting of a Solar Filament Structure. The Astrophysical Journal 940, p. L12 (2022)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.; Xu, Z.; Xiang, Y.: Reconfiguration and Eruption of a Solar Filament by Magnetic Reconnection with an Emerging Magnetic Field. The Astrophysical Journal 935, p. 85 (2022)
Mou, C.; Peter, H.; Xia, L.; Huang, Z.: Anisotropic nonthermal motions in the transition region of solar active regions. Astronomy and Astrophysics 660, p. A3 (2022)
Peter, H.; Chitta, L. P.; Chen, F.; Pontin, D. I.; Winebarger, A. R.; Golub, L.; Savage, S. L.; Rachmeler, L. A.; Kobayashi, K.; Brooks, D. H.et al.; Cirtain, J. W.; De Pontieu, B.; McKenzie, D. E.; Morton, R. J.; Testa, P.; Tiwari, S. K.; Walsh, R. W.; Warren, H. P.: Parallel Plasma Loops and the Energization of the Solar Corona. The Astrophysical Journal 933, p. 153 (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.