Rachmeler, L. A.; Winebarger, A. R.; Savage, S. L.; Golub, L.; Kobayashi, K.; Vigil, G. D.; Brooks, D. H.; Cirtain, J. W.; Pontieu, B. D.; McKenzie, D. E.et al.; Morton, R. J.; Peter, H.; Testa, P.; Tiwari, S. K.; Walsh, R. W.; Warren, H. P.; Alexander, C.; Ansell, D.; Beabout, B. L.; Beabout, D. L.; Bethge, C. W.; Champey, P. R.; Cheimets, P. N.; Cooper, M. A.; Creel, H. K.; Gates, R.; Gomez, C.; Guillory, A.; Haight, H.; Hogue, W. D.; Holloway, T.; Hyde, D. W.; Kenyon, R.; Marshall, J. N.; McCracken, J. E.; McCracken, K.; Mitchell, K. O.; Ordway, M.; Owen, T.; Ranganathan, J.; Robertson, B. A.; Payne, M. J.; Podgorski, W.; Pryor, J.; Samra, J.; Sloan, M. D.; Soohoo, H. A.; Steele, D. B.; Thompson, F. V.; Thornton, G. S.; Watkinson, B.; Windt, D.: The High-Resolution Coronal Imager, Flight 2.1. Solar Physics 294 (12), 174 (2019)
Tiwari, S. K.; Panesar, N. K.; Moore, R. L.; Pontieu, B. D.; Winebarger, A. R.; Golub, L.; Savage, S. L.; Rachmeler, L. A.; Kobayashi, K.; Testa, P.et al.; Warren, H. P.; Brooks, D. H.; Cirtain, J. W.; McKenzie, D. E.; Morton, R. J.; Peter, H.; Walsh, R. W.: Fine-scale Explosive Energy Release at Sites of Prospective Magnetic Flux Cancellation in the Core of the Solar Active Region Observed by Hi-C 2.1, IRIS, and SDO. Astrophysical Journal 887 (1), 56 (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)
Kayshap, P.; Tripathi, D.; Solanki, S. K.; Peter, H.: Quiet-Sun and Coronal Hole in Mg II k Line as Observed by IRIS. The Astrophysical Journal 864 (1), 21 (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)
Li, L.; Zhang, J.; Peter, H.; Chitta, L. P.; Su, J.; Xia, C.; Song, H.; Hou, Y.: Coronal Condensations Caused by Magnetic Reconnection between Solar Coronal Loops. The Astrophysical Journal Letters 864 (1), L4 (2018)
Yang, L.; Peter, H.; He, J.; Tu, C.; Wang, L.; Zhang, L.; Yan, L.: Formation of Cool and Warm Jets by Magnetic Flux Emerging from the Solar Chromosphere to Transition Region. The Astrophysical Journal 852 (1), 16 (2018)
Yang, Z.; Tian, H.; Peter, H.; Su, Y.; Samanta, T.; Zhang, J.; Chen, Y.: Two Solar Tornadoes Observed with the Interface Region Imaging Spectrograph. The Astrophysical Journal 852 (2), 79 (2018)
Young, P. R.; Keenan, F. P.; Milligan, R. O.; Peter, H.: A Si iv/O iv Electron Density Diagnostic for the Analysis of IRIS Solar Spectra. The Astrophysical Journal 857 (1), 5 (2018)
Young, P. R.; Tian, H.; Peter, H.; Rutten, R. J.; Nelson, C. J.; Huang, Z.; Schmieder, B.; Vissers, G. J. M.; Toriumi, S.; van der Voort, L. H. M. R.et al.; Madjarska, M. S.; Danilovic, S.; Berlicki, A.; Chitta, L. P.; Cheung, M. C. M.; Madsen, C.; Reardon, K. P.; Katsukawa, Y.; Heinzel, P.: Solar Ultraviolet Bursts. Space Science Reviews 214, 120 (2018)
Aschwanden, M. J.; Peter, H.: The Width Distribution of Loops and Strands in the Solar Corona - Are We Hitting Rock Bottom? Astrophysical Journal 840 (24), 4 (2017)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
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.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...