| Reconstructing solar magnetic fields from historical observations-VIII. AIA 1600 Å contrast as a proxy of solar magnetic fields I Tähtinen, II Virtanen, AA Pevtsov, K Mursula Astronomy & Astrophysics 664, A2, 2022 | 4 | 2022 |
| Transition to a weaker Sun: Changes in the solar atmosphere during the decay of the Modern Maximum K Mursula, AA Pevtsov, T Asikainen, I Tähtinen, AR Yeates Astronomy & Astrophysics 685, A170, 2024 | | 2024 |
| Effect of magnetic field inclination on SDO/AIA 1600 Å emission I Tähtinen, A Pevtsov, T Asikainen, K Mursula EGU24, 2024 | | 2024 |
| A change in solar radio spectrum during the decay of the Modern Maximum K Mursula, A Pevtsov, T Asikainen, I Tähtinen, A Yeates EGU24, 2024 | | 2024 |
| Clarifying the relation between chromospheric emissions and photospheric magnetic fields using AIA 1600 Å and HMI data I Tähtinen, I Virtanen, A Pevtsov, K Mursula EGU General Assembly Conference Abstracts, EGU22-9622, 2022 | | 2022 |
| Abrupt shrinking of solar corona in late 1990s and related changes in solar magnetic structure K Mursula, I Virtanen, J Koskela, I Tähtinen EGU2020, 2020 | | 2020 |
| Auringon aktiivisuus ja sen indeksit I Tähtinen I. Tähtinen, 2019 | | 2019 |
| The Ca II K emissions as a proxy of the solar magnetic field I Tähtinen I. Tähtinen, 2017 | | 2017 |
