|
 Thesis title |
 Year of announcement |
 Year of defence |
Thesis type |
Thesis discipline |  Supervisor |
 Author |
 Announced |
Assigned | Department |
Faculty |
 |
Flow structure in supergranules and its dependence on heliographic latitude |
2017/2018 |
|
diploma thesis |
FA | doc. Mgr. Michal Švanda, Ph.D. |
|
06.02.2015 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Flares across Hertzsprung-Russel diagram |
2019/2020 |
|
diploma thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
07.10.2016 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Robustness of the SOLA inversion against the choice of the trade-off parameters |
2016/2017 |
|
Bachelor's thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
25.07.2011 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Observational hints for the dynamicaldisconnection of the solar magnetic regions from their roots |
2025/2026 |
|
rigorosum thesis |
FA | doc. Mgr. Michal Švanda, Ph.D. |
|
23.10.2023 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Properties of the average solar active region in the photosphere |
2014/2015 |
|
diploma thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
25.07.2011 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Advances in helioseismology |
2016/2017 |
|
Bachelor's thesis |
F, FMUZV, FMU2ZV, FOF | doc. Mgr. Michal Švanda, Ph.D. |
|
25.07.2011 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
3-D models of Sun-like stars |
2007/2008 |
|
diploma thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
19.09.2007 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Relation between the X-ray class of solar flare and geomagnetically induced currents |
2018/2019 |
|
diploma thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
25.01.2016 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Average bipolar active region constructed from a set of active regions recorded in HMI/SDO data series |
2014/2015 |
|
Bachelor's thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
25.07.2011 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Optimal target functions for SOLA-type helioseismic inversions |
2014/2015 |
|
diploma thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
25.07.2011 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Perpendicular transport of magnetic fields in stationary MHD: ideal MHD flows and resistive MHD annihilation solutions |
2015/2016 |
|
project |
| doc. Mgr. Michal Švanda, Ph.D. |
|
03.10.2012 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
 |
Helioseismic inversions using point-to-point geometry |
2015/2016 |
|
diploma thesis |
| doc. Mgr. Michal Švanda, Ph.D. |
|
19.08.2012 |
Ne | Astronomický ústav UK (32-AUUK) |
MFF |
|