de Oliveira, I.; Sowmya, K.; Nèmec, N. -.; Shapiro, A. I.: Estimation of Spectral Solar Irradiance in the Ecliptic Plane Using Synthetic Solar Surface Magnetograms. Journal of Geophysical Research (Space Physics) 129, p. e2024JA032601 (2024)
Seager, S.; Shapiro, A. I.: Why Observations at Mid-infrared Wavelengths Partially Mitigate M Dwarf Star Host Stellar Activity Contamination in Exoplanet Transmission Spectroscopy. The Astrophysical Journal 970, p. 155 (2024)
Shapiro, A. V.; Egorova, T.; Shapiro, A. I.; Arsenovic, P.; Rozanov, E.; Gizon, L.: Transition of the Sun to a Regime of High Activity: Implications for the Earth Climate and Role of Atmospheric Chemistry. JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES (15) (2024)
Egorova, T. A.; Shapiro, A.; Shapiro, A. I.; Arsenovic, P.; Rozanov, E. V.: Climate implications of the sun transition to higher activity mode. Journal of Atmospheric and Solar-Terrestrial Physics 244, p. 106020 (2023)
Sowmya, K.; Shapiro, A. I.; Rouppe van der Voort, L. H. M.; Krivova, N. A.; Solanki, S. K.: Modeling Stellar Ca II H and K Emission Variations: Spot Contribution to the S-index. The Astrophysical Journal 956, p. L10 (2023)
Bhatia, T. S.; Cameron, R. H.; Solanki, S. K.; Peter, H.; Przybylski, D.; Witzke, V.; Shapiro, A.: Small-scale dynamo in cool stars. I. Changes in stratification and near-surface convection for main-sequence spectral types. Astronomy and Astrophysics 663, p. A166 (2022)
Kaplan-Lipkin, A.; Macintosh, B.; Madurowicz, A.; Sowmya, K.; Shapiro, A. I.; Krivova, N. A.; Solanki, S. K.: Multiwavelength Mitigation of Stellar Activity in Astrometric Planet Detection. The Astronomical Journal 163, p. 205 (2022)
The European Space Agency (ESA) has given the green light to build the flight models of the spacecraft and science payload for the PLATO mission to search for extrasolar planets.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
The longest-serving solar observatory in space has turned 25 and is still making significant contributions to solar research. Its old age has become an important merit.