Anfinogentov, S. A.; Kaltman I, T.; Stupishin, A. G.; Nakariakov, V. M.; Loukitcheva, M. A.: Diagnostics of Plasma Jets in the Solar Corona. Solnechno-Zemnaya Fizika 7 (2), pp. 3 - 10 (2021)
Kaltman, T. I.; Stupishin, A. G.; Anfinogentov, S. A.; Nakariakov, V. M.; Loukitcheva, M.; Shendrik, A. V.: Hot Jets in the Solar Corona: Creating a Catalogue of Events Based on Multi-Instrumental Observations. Geomagnetism and Aeronomy 61, pp. 1083 - 1091 (2021)
Nagnibeda, V. G.; Topchilo, N. A.; Loukitcheva, M.; Rakhimov, I. A.: Features of Radio-Brightness Distribution over the Solar Disk at Millimeter Waves: Models and Observations. Geomagnetism and Aeronomy 61, pp. 1150 - 1158 (2021)
Loukitcheva, M.; White, S. M.; Solanki, S. K.: ALMA Detection of Dark Chromospheric Holes in the Quiet Sun. The Astrophysical Journal Letters 877 (2), L26 (2019)
Bastian, T. S.; Chintzoglou, G.; Pontieu, B. D.; Shimojo, M.; Schmit, D.; Leenaarts, J.; Loukitcheva, M.: Erratum: "A First Comparison of Millimeter Continuum and MgII Ultraviolet Line Emission from the Solar Chromosphere". The Astrophysical Journal Letters 860 (1), L16 (2018)
Bastian, T. S.; Chintzoglou, G.; De Pontieu, B.; Shimojo, M.; Schmit, D.; Leenaarts, J.; Loukitcheva, M.: A First Comparison of Millimeter Continuum and MgII Ultraviolet Line Emission from the Solar Chromosphere. Astrophysical Journal 845 (2), L19 (2017)
Fleishman, G. D.; Anfinogentov, S.; Loukitcheva, M.; Mysh'yakov, I.; Stupishin, A.: Casting the Coronal Magnetic Field Reconstruction Tools in 3D Using the MHD Bifrost Model. Astrophysical Journal 839 (1), 30 (2017)
Iwai, K.; Loukitcheva, M.; Shimojo, M.; Solanki, S. K.; White, S. M.: ALMA Discovery of Solar Umbral Brightness Enhancement at lambda=3 mm. Astrophysical Journal 841 (2), L20 (2017)
Loukitcheva, M.; Iwai, K.; Solanki, S. K.; White, S. M.; Shimojo, M.: Solar ALMA Observations: Constraining the Chromosphere above Sunspots. The Astrophysical Journal 850 (1), 35 (2017)
Loukitcheva, M.; White, S. M.; Solanki, S. K.; Fleishman, G. D.; Carlsson, M.: Millimeter radiation from a 3D model of the solar atmosphere II. Chromospheric magnetic field. Astronomy and Astrophysics 601, A43 (2017)
Shimojo, M.; Bastian, T. S.; Hales, A. S.; White, S. M.; Iwai, K.; Hills, R. E.; Hirota, A.; Phillips, N. M.; Sawada, T.; Yagoubov, P.et al.; Siringo, G.; Asayama, S.; Sugimoto, M.; Brajsa, R.; Skokic, I.; Barta, M.; Kim, S.; de Gregorio-Monsalvo, I.; Corder, S. A.; Hudson, H. S.; Wedemeyer, S.; Gary, D. E.; De Pontieu, B.; Loukitcheva, M.; Fleishman, G. D.; Chen, B.; Kobelski, A.; Yan, Y.: Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): High-Resolution Interferometric Imaging. Solar Physics 292 (7), 87 (2017)
White, S. M.; Iwai, K.; Phillips, N. M.; Hills, R. E.; Hirota, A.; Yagoubov, P.; Siringo, G.; Shimojo, M.; Bastian, T. S.; Hales, A. S.et al.; Sawada, T.; Asayama, S.; Sugimoto, M.; Marson, R. G.; Kawasaki, W.; Muller, E.; Nakazato, T.; Sugimoto, K.; Brajsa, R.; Skokic, I.; Barta, M.; Kim, S.; Remijan, A. J.; de Gregorio, I.; Corder, S. A.; Hudson, H. S.; Loukitcheva, M.; Chen, B.; De Pontieu, B.; Fleishmann, G. D.; Gary, D. E.; Kobelski, A.; Wedemeyer, S.; Yan, Y.: Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): Fast-Scan Single-Dish Mapping. Solar Physics 292 (7), 88 (2017)
Wedemeyer, S.; Bastian, T.; Braja, R.; Hudson, H.; Fleishman, G.; Loukitcheva, M.; Fleck, B.; Kontar, E. P.; De Pontieu, B.; Yagoubov, P.et al.; Tiwari, S. K.; Soler, R.; Black, J. H.; Antolin, P.; Scullion, E.; Gunár, S.; Labrosse, N.; Ludwig, H.-G.; Benz, A. O.; White, S. M.; Hauschildt, P.; Doyle, J. G.; Nakariakov, V. M.; Ayres, T.; Heinzel, P.; Karlicky, M.; Van Doorsselaere, T.; Gary, D.; Alissandrakis, C. E.; Nindos, A.; Solanki, S. K.; Rouppe van der Voort, L.; Shimojo, M.; Kato, Y.; Zaqarashvili, T.; Perez, E.; Selhorst, C. L.; Barta, M.: Solar Science with the Atacama Large Millimeter/Submillimeter ArrayA New View of Our Sun. Space Science Reviews 200 (1-4), pp. 1 - 73 (2016)
Loukitcheva, M.; Solanki, S. K.; Carlsson, M.; White, S. M.: Millimeter radiation from a 3D model of the solar atmosphere. I. Diagnosing chromospheric thermal structure. Astronomy and Astrophysics 575, A15 (2015)
Wedemeyer, S.; Bastian, T.; Brajsa, R.; Barta, M.; Hudson, H.; Fleishman, G.; Loukitcheva, M.; Fleck, B.; Kontar, E.; De Pontieu, B.et al.; Tiwari, S.; Kato, Y.; Soler, R.; Yagoubov, P.; Black, J. H.; Antolin, P.; Gunar, S.; Labrosse, N.; Benz, A. O.; Nindos, A.; Steffen, M.; Scullion, E.; Doyle, J. G.; Zaqarashvili, T.; Hanslmeier, A.; Nakariakov, V. M.; Heinzel, P.; Ayres, T.; Karlicky, M.; The SSALMON Group: SSALMON-The Solar Simulations for the Atacama Large Millimeter Observatory Network. Advances in Space Research 56 (12), pp. 2679 - 2692 (2015)
Nagnibeda, V. G.; Loukitcheva, M. A.: Diagnostics of solar chromosphere plasma based on observations of millimeter radiation. Chem. Phys. 398, pp. 33 - 36 (2012)
Fleishman, G.; Loukitcheva, M.; Nita, G.: Solar ALMA: Observation-Based Simulations of the mm and sub-mm Emissions from Active Regions. In: Revolution in Astronomy with ALMA: The Third Year, Vol. 499, pp. 351 - 352. Astronomical Soc Pacific, San Francisco (2015)
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, ...