Cheng, X.; Xing, C.; Aulanier, G.; Solanki, S. K.; Peter, H.; Ding, M. D.: Deciphering the Slow-rise Precursor of a Major Coronal Mass Ejection. The Astrophysical Journal 954, p. L47 (2023)
Zhang, J.; Tian, H.; Zarka, P.; Louis, C. K.; Lu, H.; Gao, D.; Sun, X.; Yu, S.; Chen, B.; Cheng, X.et al.; Wang, K.: Fine Structures of Radio Bursts from Flare Star AD Leo with FAST Observations. The Astrophysical Journal 953, p. 65 (2023)
Wang, W.Y.; Cheng, X.; Ren, Z.N.; Ding, M.D.: Current-sheet Oscillations Caused by the Kelvin-Helmholtz Instability at the Loop Top of Solar Flares. Astrophysical Journal Letters 931 (2) (2022)
Li, Z. F.; Cheng, X.; Chen, F.; Chen, J.; Ding, M. D.: Three-dimensional Magnetic and Thermodynamic Structures of Solar Microflares. The Astrophysical Journal 930, p. L7 (2022)
Chitta, L. P.; Priest, E. R.; Cheng, X.: From Formation to Disruption: Observing the Multiphase Evolution of a Solar Flare Current Sheet. The Astrophysical Journal 911 (2), 133 (2021)
Li, Z. F.; Cheng, X.; Ding, M. D.; Reeves, K. K.; Kittrell, D.; Weber, M.; McKenzie, D. E.: Thermodynamic Evolution of Solar Flare Supra-arcade Downflows. The Astrophysical Journal 915 (2), 124 (2021)
Huang, Z.W.; Cheng, X.; Ding, M.D.: The kinematic evolution of erupting structures in confined solar flares. The Astrophysical Journal Letters 904 (1), L2 (2020)
Kou, Y. K.; Jing, Z. C.; Cheng, X.; Pan, W. Q.; Liu, Y.; Li, C.; Ding, M. D.: What Determines Solar Flares Producing Interplanetary Type III Radio Bursts? The Astrophysical Journal Letters 898 (1), L24 (2020)
Nindos, A.; Patsourakos, S.; Vourlidas, A.; Cheng, X.; Zhang, J.: When do solar erupting hot magnetic flux ropes form? Astronomy and Astrophysics 642, A109 (2020)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.