"MAGNETIC
FIELDS ACROSS THE HERTZSPRUNG-RUSSELL DIAGRAM"
JANUARY
15 - 19, 2001- SANTIAGO, CHILE
PRELIMINARY
SCIENTIFIC PROGRAMME
Monday, January 15, 2000
9:00 - 09:20 Workshop
opening
0. Introductory talk
9:20 -10:00 Magnetic fields across the Hertzsprung-Russell
diagram [L. Mestel (UK)]
1. The Sun
1.1 Photospheric field
10:00 - 10:40 1.1.1 Large-scale structure of the
sun's magnetic field and solar cycle [E.R. Priest (U.K.)]
10:40-11:20 1.1.2 Sunspot magnetic fields [J.C. del Toro
Iniesta (Spain)]
11:20-11:50 Coffee break
11:50-12:30 1.1.3 Small-scale
structure of the sun's magnetic field: non-spot fields [S.K. Solanki (Germany)
12:30-12:50 C.1 The micro-structure
of the solar magnetic fields [J. Sanchez-Almeida (Spain)]
1.2 Chromospheric and coronal fields
12:50-13:10 1.2.1 Solar
chromospheric magnetic fields [C. Keller (USA)]
13:10-14:40 Lunch
14:40-15:00 1.2.2 Solar
coronal magnetic fields [S.M. White (USA)]
1.3 Magnetic field diagnostic techniques
15:00-15:40 1.3.1 Magnetic field
diagnostic techniques through the Zeeman and Hanle effect
[E. Landi Degl'Innocenti (Italy)]
15:40-16:00 C.2 METASTABLE-level
Atomic Polarization and the Diagnostic Problem of Chromospheric Magnetic Fields
[J. Trujillo-Bueno]
16:00-16:20 C.3 Themis Hanle
and Zeeman effects measurements in second solar spectrum lines [J. Arnaud]
16:30-17:00 Coffee break
16:50-17:10 C.4 A probe
of solar magnetic fields with the molecular Zeeman effect [S. Berdyugina et
al.]
1.4 Theory
17:10-17:50 1.4.1 Solar
magnetic field generation and dynamos [F. Cattaneo (USA)]
18:00- Welcome cocktail
Tuesday, January
16, 2000
9:00-9:40 1.4.3 Theory
of solar chromospheric and coronal magnetic fields [A.A. van Ballegooijen (USA)]
9:40-10:20 1.4.4 Magneto-convection
[M. Knoelker (USA)]
10:20-10:40 C.5 Symmetry
selection in solar cycle dynamo models [M. Dikpati]
10:40-11:10 Coffee break
2. Instrumentation: present
and future
11:10-11:50 2.1 Ground-based
instrumentation for solar magnetic field studies [H.P. Povel (Switzerland)]
11:50-12:30 2.2 Space-based
instrumentation for inference of the solar magnetic field [B.W. Lites (USA)]
2.3 Ground-based instrumentation for stellar
magnetic field studies
12:30-13:10 2.3.1 Polarimetry
and spectropolarimetry on new generation very large telescopes
[J.-F. Donati (France)]
13:10-14:40 Lunch
14:40-15:00 2.3.2 Current
ground-based stellar spectropolarimeters and their use for Zeeman-Doppler imaging
[M. Semel (France)]
15:00-15:20 2.3.3 Resolved
magnetic structures on stellar surfaces: prospects for interfero-spectropolarimetry
[F. Vakili (France)]
15:20-15:40 2.3.4 CRIRES
and VISIR, future tools at ESO's VLT to study magnetic field sensitive lines
in the infrared [H.U. Kaeufl]
15:40-16:20 2.3.5 Pulsar
radiopolarimetry [I.H. Stairs (USA)]
16:20-16:50 Coffee break
16:50-17:30 2.4 Space-based
instrumentation for magnetic field studies of solar and stellar atmospheres
[S. Fineschi (USA)]
17:30-18:10 2.5 Relevance
of instruments and diagnostic techniques used in stellar magnetic field studies
for other areas of astrophysics [K.H. Nordsieck (USA)]
Wednesday, January
17, 2000
3. Non-degenerate stars
3.1 Cool stars
9:00-09:40 3.1.1 Magnetic
field measurements for cool stars [J.A. Valenti (USA)]
9:40-10:20 3.1.2 Stellar
dynamos [P. Charbonneau (USA)]
10:20-10:50 Coffee break
10:50-11:30 3.1.3 Magnetic
activity on cool nondegenerate stars [J.H.M.M. Schmitt (Germany)]
11:30-12:10 3.1.4 Magnetic
fields in binaries [C.G. Campbell (UK)]
12:10-... Workshop tour
Thursday, January
18, 2000
3.2 Ap and Bp stars
9:00-9:40 3.2.1 Magnetic
fields of Ap and Bp stars [G. Mathys (Chile)]
9:40-10:20 3.2.2 Recent
advances in magnetic field diagnostic techniques [J.D. Landstreet (Canada)]
10:20-10:40 3.2.3 Geometrical
structure of Ap and Bp star magnetic fields [S. Bagnulo (Austria)]
10:40-11:00 3.2.4 Zeeman-Doppler
Imaging of magnetic Ap and Bp stars [N. Piskunov (Sweden)]
11:00-11:30 Coffee break
11:30-11:50 C.6 Magnetic
CP stars: catalogue and spatial distribution [I.I. Romanyuk & D.O. Kudryavtsev]
11:50-12:30 3.2.5 Theory:
the origin of Ap and Bp star magnetic fields [D. Moss (UK)]
12:30-12:50 C.7 MHD shearflow
instability as a proxy of Ap star magnetism [G. Ruediger & R. Arlt]
12:50-14:20 Lunch
2.3 Hot stars
14:20-14:40 3.3.1 Detection
of magnetic fields in hot stars using the Zeeman effect [G.A. Wade (Canada)]
14:40-15:00 C.8 Magnetic
field diagnosis in HgMn stars [S. Hubrig et al.]
15:00-15:40 3.3.2 Magnetic
fields in hot stars: indirect indicators [H. Henrichs (Netherlands)]
15:40-16:00 3.3.3 Determination
of magnetic fields in hot stars using the Hanle effect [J.P. Cassinelli (USA)]
16:00-16:30 Coffee break
4. Degenerate stars
16:30-17:10 4.1 Magnetic
fields in isolated white dwarfs: overview [G.D. Schmidt (USA)]
17:10-17:50 4.2 The structure
of magnetic fields of isolated white dwarfs and white dwarfs in magnetic CVs
[D.T. Wickramasinghe (Australia)]
17:50-18:10 C.9 Zeeman-split
lines from magnetised accretion flows in Magnetic Cataclysmic Variables
[L. Ferrario]
18:10-18:30 C.10 MCV's at
extreme low accretion rate - Zeeman and Cyclotron spectra [A. Schwope]
20:30-... Workshop dinner
Friday, January 19, 2000
9:00-9:40 4.3 Magnetic
fields of neutron stars: overview [A. Reisenegger (Chile)]
5. Pre-main sequence (PMS) stars
9:40-10:00 5.1 Magnetic
fields in pre-main sequence stars [E.W. Guenther (Germany)]
10:00-10:40 5.2 Magnetic
flaring in pre-main sequence stars [E.D. Feigelson (USA)]
10:40-11:10 Coffee break
11:10-11:50 5.3 Spindown
of young stars: the role of magnetic fields [K.B. MacGregor (USA)]
11:50-12:30 5.4 Star formation
models with magnetic fields [T.Ch. Mouschovias (USA)]
6. Towards a global picture
12:30-13:10 6.1 Instrumentation
and techniques for magnetic field diagnostics [J.O. Stenflo (Switzerland)]
13:10-14:40 Lunch
6.2 Observable effects induced by or related to
magnetic fields
14:40-15:20 6.2.1 Observable
Effects Produced by Magnetic Fields in the Winds and Envelopes of Hot Stars
[J.P. Cassinelli (USA)]
15:20-16:00 6.2.2 Cool stars
[P.G. Judge (USA)]
16:00-16:30 Coffee break
16:30-17:10 6.3 Theoretical
aspects of stellar magnetic fields and the solar-stellar connection [R. Rosner
(USA)]