Mierla, M.; Inhester, B.; Zhukov, A. N.; Shestov, S. V.; Bemporad, A.; Lamy, P.; Koutchmy, S.: Polarimetric Studies of a Fast Coronal Mass Ejection. Solar Physics 297, p. 78 (2022)
Ying, B.; Feng, L.; Inhester, B.; Mierla, M.; Gan, W.; Lu, L.; Li, S.: Three-dimensional analyses of an aspherical coronal mass ejection and its driven shock. Astronomy and Astrophysics 660, p. A23 (2022)
Inhester, B.; Mierla, M.; Shestov, S.; Zhukov, A.: Error Estimation of Linear Polarization Data from Coronagraphs – Application to STEREO-A/SECCHI-COR1 Observations. Solar Physics 296, 72 (2021)
Cheng , X.; Zhang, J.; Kliem, B.; Török, T.; Xing, C.; Zhou, Z. J.; Inhester, B.; Ding, M. D.: Initiation and Early Kinematic Evolution of Solar Eruptions. The Astrophysical Journal 894 (2), 85 (2020)
Dai, X.; Wang, H.; Inhester, B.: Electron Density Reconstruction of Solar Coronal Mass Ejections Based on a Genetic Algorithm: Method and Application. The Astrophysical Journal 896 (2), 155 (2020)
Feng, L.; Li, H.; Inhester, B.; Chen, B.; Ying, B.-L.; Lu, L.; Gan, W.: On the error analyses of polarization measurements of the white-light coronagraph aboard ASO-S. Research in Astronomy and Astrophysics 19 (4), 059 (2019)
Lu, L.; Inhester, B.; Feng, L.; Liu, S.; Zhao, X.: Measure the Propagation of a Halo CME and Its Driven Shock with the Observations from a Single Perspective at Earth. Astrophysical Journal 835 (2), 188 (2017)
Innes, D. E.; Heinrich, P.; Inhester, B.; Guo, L.-J.: Analysis of UV and EUV emission from impacts on the Sun after 2011 June 7 eruptive flare. Astronomy and Astrophysics 592, A17 (2016)
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.
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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.
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