Name: Differential Rotation and Magnetism across the HR Diagram
Start: 2013-04-08T08:00:00+02:00
End: 2013-05-03T18:00:00+02:00
Location: Nordita

Monday, 8 April 2013

07:00 MONDAY
MONDAY
07:00 - 08:30
Room: 132:028

08:30 Registration
Registration
08:30 - 10:00
Room: B3

10:00 BROWNING: Simulations of differential rotation at the bottom of the main sequence
BROWNING: Simulations of differential rotation at the bottom of the main sequence
10:00 - 10:30
Room: B3

10:30 MORIN: Differential rotation in very-low-mass stars: a clue to dynamo bistability?
MORIN: Differential rotation in very-low-mass stars: a clue to dynamo bistability?
10:30 - 11:00
Room: B3

11:00 break
break
11:00 - 11:30
Room: Foyer B

11:30 STRASSMEIER: DI and ZDI of stellar magnetism and surface velocity fields
STRASSMEIER: DI and ZDI of stellar magnetism and surface velocity fields
11:30 - 12:00
Room: B3

12:00 BRUN: Differential rotation and dynamo action in G and K stars
BRUN: Differential rotation and dynamo action in G and K stars
12:00 - 12:30
Room: B3

12:30 Lunch
Lunch
12:30 - 15:00
Room: undefined

15:00 BONANNO: Current-driven Instabilities in Stellar Radiation Zones: linear analysis and nonlinear evolution from DNS
BONANNO: Current-driven Instabilities in Stellar Radiation Zones: linear analysis and nonlinear evolution from DNS
15:00 - 15:30
Room: B3

15:30 MOND: Non-dissipative saturation of the magneto-rotational instability
MOND: Non-dissipative saturation of the magneto-rotational instability
15:30 - 16:00
Room: B3

16:00 HYPOLITE: A two-dimensional model of gravitationally contracting rotating star
HYPOLITE: A two-dimensional model of gravitationally contracting rotating star
16:00 - 16:30
Room: B2

16:30 break
break
16:30 - 17:00
Room: Foyer B

17:00 MIESCH: Meridional circulation in solar and stellar convection zones
MIESCH: Meridional circulation in solar and stellar convection zones
17:00 - 17:30
Room: B2

17:30 SOOD: Dynamic model of dynamo (magnetic activity) and stellar rotation
SOOD: Dynamic model of dynamo (magnetic activity) and stellar rotation
17:30 - 18:00
Room: B3
Tuesday, 9 April 2013

07:00 TUESDAY
TUESDAY
07:00 - 09:30
Room: 132:028

09:30 KITCHATINOV: Mean-field theory of meridional flow and differential rotation
KITCHATINOV: Mean-field theory of meridional flow and differential rotation
09:30 - 10:00
Room: B2

10:00 ZHANG: Consistent Long-term Variation in the Hemispheric Asymmetry of Solar Rotation
ZHANG: Consistent Long-term Variation in the Hemispheric Asymmetry of Solar Rotation
10:00 - 10:20
Room: B2

10:20 ARLT: The solar differential rotation in the 18th century
ARLT: The solar differential rotation in the 18th century
10:20 - 10:40
Room: B2

10:40 FOURNIER: Magnetic flux emergence with differential rotation in compressible shells
FOURNIER: Magnetic flux emergence with differential rotation in compressible shells
10:40 - 11:00
Room: B2

11:00 break
break
11:00 - 11:30
Room: Foyer B

11:30 HACKMAN: Are starspots equivalents to sunspots?
HACKMAN: Are starspots equivalents to sunspots?
11:30 - 12:00
Room: B2

12:00 KOCHUKHOV: Zeeman Doppler imaging: techniques and limitations
KOCHUKHOV: Zeeman Doppler imaging: techniques and limitations
12:00 - 12:30
Room: B2

12:30 BESSOLAZ: Magnetism and differential rotation in pre-main sequence stars
BESSOLAZ: Magnetism and differential rotation in pre-main sequence stars
12:30 - 13:00
Room: B2

13:00 Lunch
Lunch
13:00 - 14:30
Room: undefined

14:30 BASRI: What fraction of Kepler targets show differential rotation?
BASRI: What fraction of Kepler targets show differential rotation?
14:30 - 15:00
Room: B2

15:00 REINHOLD: Rotation and Differential Rotation of the Kepler stars
REINHOLD: Rotation and Differential Rotation of the Kepler stars
15:00 - 15:30
Room: B2

15:30 GARCIA: Studying stellar rotation and magnetic activity cycles with asteroseismic measurements
GARCIA: Studying stellar rotation and magnetic activity cycles with asteroseismic measurements
15:30 - 16:00
Room: B2

16:00 KAROFF: Sounding Stellar Cycles with Kepler
KAROFF: Sounding Stellar Cycles with Kepler
16:00 - 16:30
Room: B2

16:30 break
break
16:30 - 17:00
Room: Foyer B

17:00 CHAN: Rotational effects on convection
CHAN: Rotational effects on convection
17:00 - 17:30
Room: B2

17:30 LEHTINEN: Viability of using photometric period variations as a proxy for stellar surface differential rotation
LEHTINEN: Viability of using photometric period variations as a proxy for stellar surface differential rotation
17:30 - 18:00
Room: B2
Wednesday, 10 April 2013

07:00 WEDNESDAY
WEDNESDAY
07:00 - 09:30
Room: 132:028

09:30 BRANDENBURG: Is solar activity a surface phenomenon?
BRANDENBURG: Is solar activity a surface phenomenon?
09:30 - 10:00
Room: B2

10:00 BENEVOLENSKAYA: Synoptic solar cycle observed by Solar Dynamics Observatory
BENEVOLENSKAYA: Synoptic solar cycle observed by Solar Dynamics Observatory
10:00 - 10:30
Room: B2

10:30 WARNECKE: Solar-like differential rotation in a convective dynamo with a coronal envelope
WARNECKE: Solar-like differential rotation in a convective dynamo with a coronal envelope
10:30 - 11:00
Room: B2

11:00 break
break
11:00 - 11:30
Room: Foyer B

11:30 REINERS: Observational constraints for dynamos in low-mass stars
REINERS: Observational constraints for dynamos in low-mass stars
11:30 - 12:00
Room: B2

12:00 PETITDEMANGE: On the field strength and field topology in anelastic spherical dynamo simulations
PETITDEMANGE: On the field strength and field topology in anelastic spherical dynamo simulations
12:00 - 12:30
Room: B2

12:30 SCHMITT: Surface constraints on the solar dynamo
SCHMITT: Surface constraints on the solar dynamo
12:30 - 13:00
Room: B2

13:00 Lunch
Lunch
13:00 - 14:30
Room: Foyer B

14:30 Free afternoon
Free afternoon
14:30 - 18:00
Room: -
Thursday, 11 April 2013

07:00 THURSDAY
THURSDAY
07:00 - 09:30
Room: 132:028

09:30 CANTIELLO: Pulsations and magnetic fields in massive stars
CANTIELLO: Pulsations and magnetic fields in massive stars
09:30 - 10:00
Room: B2

10:00 GREGORY: Can we predict the global magnetic topology of a pre-main-sequence star from Its position in the Hertzsprung-Russell diagram?
GREGORY: Can we predict the global magnetic topology of a pre-main-sequence star from Its position in the Hertzsprung-Russell diagram?
10:00 - 10:30
Room: B2

10:30 SPADA: Modelling low-mass main, sequence stars: radius discrepancy and magnetic activity
SPADA: Modelling low-mass main, sequence stars: radius discrepancy and magnetic activity
10:30 - 11:00
Room: B2

11:00 break
break
11:00 - 11:30
Room: Foyer B

11:30 SCHRöDER: O.C.Wilson's stars: The aging of stellar activity on the MS
SCHRöDER: O.C.Wilson's stars: The aging of stellar activity on the MS
11:30 - 12:00
Room: B2

12:00 KüKER: Meridional flows in stellar convection zones
KüKER: Meridional flows in stellar convection zones
12:00 - 12:30
Room: B2

12:30 BRAITHWAITE: The Tayler instability in stars
BRAITHWAITE: The Tayler instability in stars
12:30 - 13:00
Room: B3

13:00 Lunch
Lunch
13:00 - 14:30
Room: undefined

14:30 ROGACHEVSKII: New scaling for the alpha effect in slowly rotating turbulence
ROGACHEVSKII: New scaling for the alpha effect in slowly rotating turbulence
14:30 - 15:00
Room: B2

15:00 GUERRERO: Implicit large-eddy simulation of rotating turbulent convection with the EULAG code
GUERRERO: Implicit large-eddy simulation of rotating turbulent convection with the EULAG code
15:00 - 15:30
Room: B2

15:30 KäPYLä: Magnetic cycles and equatorward migration in simulations of turbulent convection
KäPYLä: Magnetic cycles and equatorward migration in simulations of turbulent convection
15:30 - 16:00
Room: B2

16:00 SCHLICKEISER: Cosmic magnetogenesis: from spontaneously emitted aperiodic turbulent to ordered equipartition fields
SCHLICKEISER: Cosmic magnetogenesis: from spontaneously emitted aperiodic turbulent to ordered equipartition fields
16:00 - 16:30
Room: B3

16:30 break
break
16:30 - 17:00
Room: Foyer B

17:00 GAILITIS: The Riga dynamo experiment
GAILITIS: The Riga dynamo experiment
17:00 - 17:30
Room: B2

17:30 TRIANA: Inertial waves driven by differential rotation: a laboratory experiment
TRIANA: Inertial waves driven by differential rotation: a laboratory experiment
17:30 - 18:00
Room: B2
Friday, 12 April 2013

07:00 FRIDAY
FRIDAY
07:00 - 09:30
Room: 132:028

09:30 BENEVOLENSKAYA: Detailed evolution and rotation of the active regions NOAA 11101, 11106 from the SDO/HMI data
BENEVOLENSKAYA: Detailed evolution and rotation of the active regions NOAA 11101, 11106 from the SDO/HMI data
09:30 - 10:00
Room: B2

10:00 SOKOLOFF: Reversals of the solar dipole
SOKOLOFF: Reversals of the solar dipole
10:00 - 10:30
Room: B2

10:30 ILLARIONOV: A new dynamo pattern revealed by the tilt angle of bipolar sunspot groups
ILLARIONOV: A new dynamo pattern revealed by the tilt angle of bipolar sunspot groups
10:30 - 11:00
Room: B2

11:00 break
break
11:00 - 11:30
Room: Foyer B

11:30 COLE: Differential rotation and dynamo in compressible convection simulations
COLE: Differential rotation and dynamo in compressible convection simulations
11:30 - 12:00
Room: B2

12:00 KARAK: Effect of the turbulent pumping of magnetic flux on the predictability of the solar cycle
KARAK: Effect of the turbulent pumping of magnetic flux on the predictability of the solar cycle
12:00 - 12:30
Room: B2
12:30 Resonances for activity waves in spherical mean field dynamos - Dmitry Sokoloff
Resonances for activity waves in spherical mean field dynamos
- Dmitry Sokoloff
12:30 - 13:00
Room: B2
Saturday, 13 April 2013
Sunday, 14 April 2013