Week
Mon. 09
Tue. 10
Wed. 11
List
Mon. 09
Tue. 10
Wed. 11
09:00
10:00
11:00
12:00
13:00
14:00
15:00
16:00
17:00
18:00
19:00
20:00
21:00
22:00
Registration and coffee
13:50 - 14:20 (30min)
Registration and coffee
Location: Fitzgerald Library
Welcome address
14:20 - 14:30 (10min)
Welcome address
Vidotto
Session 1: Prominences and Flares
Surface magnetic field and prominence system of the young Sun-like star AP 149
Tracking coronal structure through prominences
Slingshot prominences evolution for a solar-like star
Coffee break
Flare frequency distributions: power-laws and magneto-convection
Quasi-Periodic Pulsations in Solar and Stellar Flares
Discussion
14:30 - 17:35 (3h05)
Session 1: Prominences and Flares
14:30 - 14:55 (25min)
Surface magnetic field and prominence system of the young Sun-like star AP 149
Petit
14:55 - 15:20 (25min)
Tracking coronal structure through prominences
Jardine
15:20 - 15:45 (25min)
Slingshot prominences evolution for a solar-like star
Villarreal D' Angelo
15:45 - 16:15 (30min)
Coffee break
Fitzgerald Library
16:15 - 16:40 (25min)
Flare frequency distributions: power-laws and magneto-convection
Mullan
16:40 - 17:05 (25min)
Quasi-Periodic Pulsations in Solar and Stellar Flares
Hayes
17:05 - 17:35 (30min)
Discussion
Session 1
Session 2: Stellar activity and characterisation
The MINERVA Australis High-Precision RV Telescope Array
Classification of cool stars using spectroscopic data and advanced models
Search for the onset of complete convection in main sequence stars
Machine learning algorithms applied to the measurement of stellar magnetic fields
Coffee/Tea break
Chromospheric activity of cool stars: the Vaughan-Preston gap and the active/inactive branch of stellar activity cycles
Discussion
9:00 - 12:05 (3h05)
Session 2: Stellar activity and characterisation
9:00 - 9:25 (25min)
The MINERVA Australis High-Precision RV Telescope Array
Mengel
9:25 - 9:50 (25min)
Classification of cool stars using spectroscopic data and advanced models
Kulenthirarajah
9:50 - 10:15 (25min)
Search for the onset of complete convection in main sequence stars
Mullan
10:15 - 10:40 (25min)
Machine learning algorithms applied to the measurement of stellar magnetic fields
Ramirez
10:40 - 11:10 (30min)
Coffee/Tea break
Fitzgerald Library
11:10 - 11:35 (25min)
Chromospheric activity of cool stars: the Vaughan-Preston gap and the active/inactive branch of stellar activity cycles
Boro Saikia
11:35 - 12:05 (30min)
Discussion
Session 2
Session 3: Magnetic field observations
Magnetic fields in F-type stars
Lunch
Spectropolarimetric observations of mildly active M dwarfs from ESPaDOnS to SPIRou
Magnetic fields of weak-line T Tauri stars
The transition from dynamo to fossil magnetic fields in massive supergiants
Coffee/Tea break
Surface magnetic fields on supergiants: the long term monitoring (+7yrs) of Betelgeuse
On the polarised spectrum of the post-AGB binary system 89 Herculis
Discussion
12:05 - 17:35 (5h30)
Session 3: Magnetic field observations
12:05 - 12:30 (25min)
Magnetic fields in F-type stars
Marsden
12:30 - 14:30 (2h)
Lunch
14:30 - 14:55 (25min)
Spectropolarimetric observations of mildly active M dwarfs from ESPaDOnS to SPIRou
Morin
14:55 - 15:20 (25min)
Magnetic fields of weak-line T Tauri stars
Hill
15:20 - 15:45 (25min)
The transition from dynamo to fossil magnetic fields in massive supergiants
Wade
15:45 - 16:15 (30min)
Coffee/Tea break
Fitzgerald Library
16:15 - 16:40 (25min)
Surface magnetic fields on supergiants: the long term monitoring (+7yrs) of Betelgeuse
Lebre
16:40 - 17:05 (25min)
On the polarised spectrum of the post-AGB binary system 89 Herculis
Gangi
17:05 - 17:35 (30min)
Discussion
Session 3
Conference dinner
19:00 - 22:00 (3h)
Conference dinner
Session 4: Magnetic field generation and evolution
Evolution of Solar Photospheric and Coronal Magnetic Fields over Multiple Activity Cycles
The activity cycle of Tau Bootis
Evolving Models of Stellar Surface and Coronal Magnetic Fields
Magnetic field topology in spherical, anelastic dynamo simulations
Coffee/Tea break
Gravity darkening in late-type stars
Observing the Simulations? Applying ZDI to 3D non-potential flux transport simulations
Discussion
9:00 - 12:30 (3h30)
Session 4: Magnetic field generation and evolution
9:00 - 9:25 (25min)
Evolution of Solar Photospheric and Coronal Magnetic Fields over Multiple Activity Cycles
DeRosa
9:25 - 9:50 (25min)
The activity cycle of Tau Bootis
Jeffers
9:50 - 10:15 (25min)
Evolving Models of Stellar Surface and Coronal Magnetic Fields
Cheung
10:15 - 10:40 (25min)
Magnetic field topology in spherical, anelastic dynamo simulations
Petitdemange
10:40 - 11:10 (30min)
Coffee/Tea break
Fitzgerald Library
11:10 - 11:35 (25min)
Gravity darkening in late-type stars
Raynaud
11:35 - 12:00 (25min)
Observing the Simulations? Applying ZDI to 3D non-potential flux transport simulations
Lehmann
12:00 - 12:30 (30min)
Discussion
Session 4
Lunch
12:30 - 14:05 (1h35)
Lunch
Session 5: Stellar winds and their impact on rotation and exoplanets
Rotational evolution in solar-type stars
The Solar Wind in Time
The Effect of Magnetic Variability on Angular Momentum Loss for the Sun and Other Stars
Estimating the mass-loss and angular momentum-loss rates for a sample of Zeeman-Doppler imaged stars
Coffee/Tea break
Magnetised winds and their influence in the escaping upper atmosphere of HD209458b
Stellar wind effects on the multi-planetary system HD219134
Discussion
14:05 - 17:35 (3h30)
Session 5: Stellar winds and their impact on rotation and exoplanets
14:05 - 14:30 (25min)
Rotational evolution in solar-type stars
Amard
14:30 - 14:55 (25min)
The Solar Wind in Time
Ó Fionnagáin
14:55 - 15:20 (25min)
The Effect of Magnetic Variability on Angular Momentum Loss for the Sun and Other Stars
Finley
15:20 - 15:45 (25min)
Estimating the mass-loss and angular momentum-loss rates for a sample of Zeeman-Doppler imaged stars
See
15:45 - 16:15 (30min)
Coffee/Tea break
Fitzgerald Library
16:15 - 16:40 (25min)
Magnetised winds and their influence in the escaping upper atmosphere of HD209458b
Villarreal D'Angelo
16:40 - 17:05 (25min)
Stellar wind effects on the multi-planetary system HD219134
Vidotto
17:05 - 17:35 (30min)
Discussion
Session 5