Explore the words cloud of the RESOLVE project. It provides you a very rough idea of what is the project "RESOLVE" about.
The following table provides information about the project.
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
|Coordinator Country||Germany [DE]|
|Total cost||171˙460 €|
|EC max contribution||171˙460 € (100%)|
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
|Duration (year-month-day)||from 2017-01-01 to 2018-12-31|
Take a look of project's partnership.
|1||MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV||DE (MUENCHEN)||coordinator||171˙460.00|
Sun-like stars possess magnetically confined, upper atmospheres. These coronae have temperatures of several million degrees and thus are much hotter than the underlying stellar surfaces (photospheres) which have temperatures of the order of 6000 degrees. The coronae are hotter than the photospheres because magnetic energy is generated by convective motions beneath the stellar surface and then transported through the photosphere into the corona where it is dissipated. The key to understanding the heating of the corona is to determine how, and at which spatial and temporal scales, energy is being transported into the stellar atmosphere. Both theory and simulations suggest that a substantial fraction of the energy transfer happens at spatial scales smaller than those currently observationally resolvable. The main goal of the proposed research is to bridge this gap between what we expect from theory and what we can observe. The proposed research will use numerical simulations to characterize the energy flux and look for its (spectropolarimetric) signature. This signature will then be used to create maps of the energy flux on the actual Sun using the highest-resolution observations (50-70 km) which are available: those from the 1-meter Sunrise balloon-borne observatory, and the 1.5-meter GREGOR, Europe's largest solar telescope. We will validate the diagnostics by comparing these maps of the observed energy flux into the solar atmosphere with co-spatial observations of the hot plasma structures seen in the upper atmosphere. Understanding the energy transfer combines the strengths of advanced simulations and the unprecedented observations as well as combining the expertise of world-leading solar groups in Germany and Spain. This research will have a major impact on our understanding of the heating of upper atmosphere. It is the ideal project and set of collaborations to further the experienced researcher's scientific career.
|year||authors and title||journal||last update|
H. N. Smitha, L. P. Chitta, T. Wiegelmann, S. K. Solanki
Observations of solar chromospheric heating at sub-arcsec spatial resolution
published pages: A128, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833276
|Astronomy & Astrophysics 617||2019-06-13|
E. R. Priest, L. P. Chitta, P. Syntelis
A Cancellation Nanoflare Model for Solar Chromospheric and Coronal Heating
published pages: L24, ISSN: 2041-8213, DOI: 10.3847/2041-8213/aad4fc
|The Astrophysical Journal 862/2||2019-06-13|
L. P. Chitta, H. Peter, S. K. Solanki
Nature of the energy source powering solar coronal loops driven by nanoflares
published pages: L9, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833404
|Astronomy & Astrophysics 615||2019-06-13|
K. Barczynski, H. Peter, L.P. Chitta, S.K. Solanki
Emission of solar chromospheric and transition region features related to the underlying magnetic field
published pages: A5, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731650
|Astronomy & Astrophysics 619||2019-06-13|
L. P. Chitta, H. Peter, P. R. Young, Y.-M. Huang
Compact solar UV burst triggered in a magnetic field with a fan-spine topology
published pages: A49, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201730830
|Astronomy & Astrophysics 605||2019-06-13|
L. P. Chitta, H. Peter, S. K. Solanki, P. Barthol, A. Gandorfer, L. Gizon, J. Hirzberger, T. L. RiethmÃ¼ller, M. van Noort, J. Blanco RodrÃguez, J. C. Del Toro Iniesta, D. Orozco SuÃ¡rez, W. Schmidt, V. MartÃnez Pillet, M. KnÃ¶lker
Solar Coronal Loops Associated with Small-scale Mixed Polarity Surface Magnetic Fields
published pages: 4, ISSN: 1538-4365, DOI: 10.3847/1538-4365/229/1/4
|The Astrophysical Journal Supplement Series 229/1||2019-06-13|
Leping Li, Jun Zhang, Hardi Peter, Lakshmi Pradeep Chitta, Jiangtao Su, Chun Xia, Hongqiang Song, Yijun Hou
Coronal Condensations Caused by Magnetic Reconnection between Solar Coronal Loops
published pages: L4, ISSN: 2041-8213, DOI: 10.3847/2041-8213/aad90a
|The Astrophysical Journal 864/1||2019-06-13|
Leping Li, Jun Zhang, Hardi Peter, Lakshmi Pradeep Chitta, Jiangtao Su, Hongqiang Song, Chun Xia, Yijun Hou
Quasi-periodic Fast Propagating Magnetoacoustic Waves during the Magnetic Reconnection Between Solar Coronal Loops
published pages: L33, ISSN: 2041-8213, DOI: 10.3847/2041-8213/aaf167
|The Astrophysical Journal 868/2||2019-06-05|
Peter R. Young, Hui Tian, Hardi Peter, Robert J. Rutten, Chris J. Nelson, Zhenghua Huang, Brigitte Schmieder, Gregal J. M. Vissers, Shin Toriumi, Luc H. M. Rouppe vanÂ der Voort, Maria S. Madjarska, Sanja Danilovic, Arkadiusz Berlicki, L. P. Chitta, Mark C. M. Cheung, Chad Madsen, Kevin P. Reardon, Yukio Katsukawa, Petr Heinzel
Solar Ultraviolet Bursts
published pages: , ISSN: 0038-6308, DOI: 10.1007/s11214-018-0551-0
|Space Science Reviews 214/8||2019-06-05|
L. P. Chitta, A. R. C. Sukarmadji, L. Rouppe van der Voort, H. Peter
Energetics of magnetic transients in solar active region plage
published pages: , ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834548
|Astronomy & Astrophysics||2019-06-05|
P. Syntelis, E. R. Priest, L. P. Chitta
A Cancellation Nanoflare Model for Solar Chromospheric and Coronal Heating. II. 2D Theory and Simulations
published pages: 32, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aafaf8
|The Astrophysical Journal 872/1||2019-06-05|
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