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)
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.