| Mo Montag | Di Dienstag | Mi Mittwoch | Do Donnerstag | Fr Freitag | Sa Samstag | So Sonntag |
|---|---|---|---|---|---|---|
|
30
Montag, 30. März 2026
|
31
Dienstag, 31. März 2026
|
1
Mittwoch, 1. April 2026
|
2
Donnerstag, 2. April 2026
|
3
Freitag, 3. April 2026
|
4
Samstag, 4. April 2026
|
5
Sonntag, 5. April 2026
|
|
6
Montag, 6. April 2026
|
7
Dienstag, 7. April 2026
|
8
Mittwoch, 8. April 2026
|
9 Donnerstag, 9. April 2026 |
10
Freitag, 10. April 2026
|
11
Samstag, 11. April 2026
|
12
Sonntag, 12. April 2026
|
|
13
Montag, 13. April 2026
|
14
Dienstag, 14. April 2026
|
15
Mittwoch, 15. April 2026
|
16
Donnerstag, 16. April 2026
|
17
Freitag, 17. April 2026
|
18
Samstag, 18. April 2026
|
19
Sonntag, 19. April 2026
|
|
20
Montag, 20. April 2026
|
21
Dienstag, 21. April 2026
|
22
Mittwoch, 22. April 2026
|
23
Donnerstag, 23. April 2026
|
24
Freitag, 24. April 2026
|
25
Samstag, 25. April 2026
|
26
Sonntag, 26. April 2026
|
|
27
Montag, 27. April 2026
|
28
Dienstag, 28. April 2026
|
29
Mittwoch, 29. April 2026
|
30
Donnerstag, 30. April 2026
|
1
Freitag, 1. Mai 2026
|
2
Samstag, 2. Mai 2026
|
3
Sonntag, 3. Mai 2026
|
Astrophysikalisches Kolloquium
The Department of Astrophysics and Geophysics at the Institute of Physics cordially invites you, as part of the Astrophysical Colloquium series, to a lecture by:
“Superflares on Sun-like stars and TRAPPIST-1”
Dr. Valeriy Vasilyev
Max Planck Institute for Solar System Research, Göttingen
Can superflares occur on the Sun, and if so, how often? One way to approach this is through a solar-stellar comparison. In this colloquium, I will present recent results from an analysis of 56450 Sun-like stars observed by the Kepler space telescope. Our analysis revises the occur-rence rate of superflares for Sun-like stars and finds it to be a factor of 50 higher than previously thought. Connections between superflares and solar energetic particle events are then exam-ined using a probabilistic approach. I will then discuss TRAPPIST-1, an ultracool dwarf and one of JWST's most frequently observed targets, where activity directly impacts exoplanet transmission spectroscopy. Using JWST observations, we find evidence for flare-driven trans-formations of the stellar surface, in particular the disappearance of dark magnetic features. JWST spectroscopic time series allow us to measure their spectra and estimate their temper-atures. Finally, we combine ~87 hours of JWST spectroscopy with K2 photometry to constrain a unified flare-frequency distribution spanning four decades in energy, providing fresh insight into which events dominate the long-term flare energy budget.
Time: Wednesday, 25th March 2026 at 16:00
Place: Bibliothek Experimentalphysik (0005-01-0122) 1. Stock, Universitätsplatz 5, 8010 Graz
Further details can be found in the attached invitation.
Please feel free to use or share this information as needed.