Explore the words cloud of the SOLVe project. It provides you a very rough idea of what is the project "SOLVe" about.
The following table provides information about the project.
Coordinator |
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
Organization address contact info |
Coordinator Country | Germany [DE] |
Project website | http://www2.mps.mpg.de/projects/solve/ |
Total cost | 1˙443˙000 € |
EC max contribution | 1˙443˙000 € (100%) |
Programme |
1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC)) |
Code Call | ERC-2016-STG |
Funding Scheme | ERC-STG |
Starting year | 2017 |
Duration (year-month-day) | from 2017-01-01 to 2021-12-31 |
Take a look of project's partnership.
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1 | MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV | DE (Munich) | coordinator | 1˙443˙000.00 |
The proposed project aims at answering four general questions of high scientific importance: - How typical is the Sun as active star? - What is the solar role in climate change? - What are the limitations for detectability of Earth-type planets in habitable zones? - Can the solar paradigm help us to explain variability of other stars and to better detect and characterize exoplanets? These exciting questions can now be addressed thanks to recent progress in solar and stellar physics. On the observational side, the unprecedented precision of broadband stellar photometry achieved with the CNES CoRoT and the NASA Kepler satellites initiated a new era in studying stellar photometric variabilities. Recent surveys with ground-based automated telescopes have significantly increased the number of stars observed over their activity cycles. On the theoretical side, solar irradiance models have matured to reproduce solar brightness variability in great detail. The enormous progress in magnetohydrodynamic simulations of solar and stellar atmospheres as well as the development of new computationally efficient radiative transfer schemes makes it finally possible to extend physics-based solar irradiance models to other stars, thus opening an entirely new horizon for solar-stellar and solar-terrestrial connection studies.
year | authors and title | journal | last update |
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2020 |
A. I. Shapiro, E. M. Amazo-Gómez, N. A. Krivova, S. K. Solanki Inflection point in the power spectrum of stellar brightness variations published pages: A32, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201936018 |
Astronomy & Astrophysics 633 | 2020-03-05 |
2020 |
Amazo-Gómez E. M., Shapiro A. I., Solanki S. K., Krivova N. A., Kopp G., Reinhold T., Oshagh M., Reiners A. Rotation periods from the inflection point in the power spectrum of stellar brightness variations: II. The Sun published pages: in press, ISSN: 0004-6361, DOI: |
Astronomy and Astrophysics | 2020-03-05 |
2020 |
V. Witzke, T. Reinhold, A. I. Shapiro, N. A. Krivova, S. K. Solanki Effect of metallicity on the detectability of rotational periods in solar-like stars published pages: L9, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201936608 |
Astronomy & Astrophysics 634 | 2020-03-05 |
2020 |
Shapiro, Anna V.; Shapiro, Alexander I.; Gizon, Laurent; Krivova, Natalie A.; Solanki, Sami K. Solar-cycle irradiance variations over the last four billion years published pages: in press, ISSN: 0004-6361, DOI: |
Astronomy and Astrophysics | 2020-03-05 |
2019 |
R. V. Tagirov, A. I. Shapiro, N. A. Krivova, Y. C. Unruh, K. L. Yeo, S. K. Solanki Readdressing the UV solar variability with SATIRE-S: non-LTE effects published pages: A178, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201935121 |
Astronomy & Astrophysics 631 | 2020-03-05 |
2020 |
Nèmec N. -E., Shapiro A. I., Krivova N. A., Solanki S. K., Tagirov R. V., Cameron R. H., Dreizler S. Power spectra of solar brightness variations at different inclinations published pages: in press, ISSN: 0004-6361, DOI: |
Astronomy and Astrophysics | 2020-03-05 |
2018 |
V. Witzke, A. I. Shapiro, S. K. Solanki, N. A. Krivova, W. Schmutz From solar to stellar brightness variations published pages: A146, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833936 |
Astronomy & Astrophysics 619 | 2019-08-29 |
2019 |
M. Cernetic, A. I. Shapiro, V. Witzke, N. A. Krivova, S. K. Solanki, R. V. Tagirov Opacity distribution functions for stellar spectra synthesis published pages: A157, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201935723 |
Astronomy & Astrophysics 627 | 2019-08-29 |
2019 |
Timo Reinhold, Keaton J. Bell, James Kuszlewicz, Saskia Hekker, Alexander I. Shapiro Transition from spot to faculae domination published pages: A21, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833754 |
Astronomy & Astrophysics 621 | 2019-08-29 |
2018 |
E. Işık, S. K. Solanki, N. A. Krivova, A. I. Shapiro Forward modelling of brightness variations in Sun-like stars published pages: A177, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833393 |
Astronomy & Astrophysics 620 | 2019-08-29 |
2018 |
T. Egorova, W. Schmutz, E. Rozanov, A. I. Shapiro, I. Usoskin, J. Beer, R. V. Tagirov, T. Peter Revised historical solar irradiance forcing published pages: A85, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731199 |
Astronomy & Astrophysics 615 | 2019-06-13 |
2018 |
Christoffer Karoff, Travis S. Metcalfe, Ângela R. G. Santos, Benjamin T. Montet, Howard Isaacson, Veronika Witzke, Alexander I. Shapiro, Savita Mathur, Guy R. Davies, Mikkel N. Lund, Rafael A. Garcia, Allan S. Brun, David Salabert, Pedro P. Avelino, Jennifer van Saders, Ricky Egeland, Margarida S. Cunha, Tiago L. Campante, William J. Chaplin, Natalie Krivova, Sami K. Solanki, Maximilian Stritzinger, Mads F. Knudsen The Influence of Metallicity on Stellar Differential Rotation and Magnetic Activity published pages: 46, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aaa026 |
The Astrophysical Journal 852/1 | 2019-06-13 |
2017 |
A. I. Shapiro, S. K. Solanki, N. A. Krivova, R. H. Cameron, K. L. Yeo, W. K. Schmutz The nature of solar brightness variations published pages: 612-616, ISSN: 2397-3366, DOI: 10.1038/s41550-017-0217-y |
Nature Astronomy 1/9 | 2019-06-13 |
2018 |
T. Dudok de Wit, G. Kopp, A. Shapiro, V. Witzke, M. Kretzschmar Response of Solar Irradiance to Sunspot-area Variations published pages: 197, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aa9f19 |
The Astrophysical Journal 853/2 | 2019-06-13 |
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The information about "SOLVE" are provided by the European Opendata Portal: CORDIS opendata.