Bahar, E.; Şenavcı, H. V.; Isik, E.; Hussain, G. A. J.; Kochukhov, O.; Montes, D.; Xiang, Y.: First Chromospheric Activity and Doppler Imaging Study of PW And Using a New Doppler Imaging Code: SpotDIPy. The Astrophysical Journal 960, p. 60 (2024)
Weber, M. A.; Schunker, H.; Jouve, L.; Isik, E.: Understanding Active Region Origins and Emergence on the Sun and Other Cool Stars. Space Science Reviews 219 (8) (2023)
Şenavcı, H. V.; Kılıçoğlu, T.; Isik, E.; Hussain, G. A. J.; Montes, D.; Bahar, E.; Solanki, S. K.: Observing and modelling the young solar analogue EK Draconis: starspot distribution, elemental abundances, and evolutionary status. Monthly Notices of the Royal Astronomical Society 502 (3), pp. 3343 - 3356 (2021)
Isik, E.; Shapiro, A.; Solanki, S. K.; Krivova, N. A.: Amplification of Brightness Variability by Active-region Nesting in Solar-like Stars. The Astrophysical Journal Letters 901, L12 (2020)
Nèmec, N.-E.; Isik, E.; Shapiro, A.; Solanki, S. K.; Krivova, N. A.; Unruh, Y.: Connecting measurements of solar and stellar brightness variations. Astronomy and Astrophysics 638, A56 (2020)
Isik, E.; Solanki, S. K.; Krivova, N. A.; Shapiro, A.: Forward modelling of brightness variations in Sun-like stars: I. Emergence and surface transport of magnetic flux. Astronomy and Astrophysics 620, A177 (2018)
Özavcı, İ.; Şenavcı, H. V.; Isik, E.; Hussain, G. A. J.; O'Neal, D.; Yılmaz, M.; Selam, S. O.: Recurrent star-spot activity and differential rotation in KIC 11560447. Monthly Notices of the Royal Astronomical Society 474 (4), pp. 5534 - 5548 (2018)
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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, ...