Magnetic fields in the Sun and Low-mass stars

Cool Stars 22 • June 24-28, 2024

Program

The detailed program will be posted below as soon as available. We are looking forward to your contributions to finish the program.
To comply with the 90 minutes limit of the splinter session, we ask our contributing speakers to respect a 10 minute limit for their presentations including questions.

I - Magnetic fields from resolved to unresolved structures

Invited speaker:

S. Solanki [Max-Planck-Institut für Sonnensystemforschung]: The Sun as a resolved magnetic star

Contributed talks:

A. Finley [CEA Paris-Saclay]: How well does surface magnetism represent the dynamo action in cool stars?
F. Chiti [University of Hawaii]: Magnetic Activity and Stellar Spin-Down: Probing the Fully Convective Boundary using WD+MS Binary Systems

II - Techniques, models and results on stellar magnetic fields

Invited speaker:

O. Kochukhov [Uppsala University]: Magnetic Fields in Cool Dwarf Stars

Contributed talks:

C. Garraffo [Center for Astrophysics | Harvard & Smithsonian]: Unraveling the Magnetic Mysteries of Low-Mass Stars: From Youth to Old Age
A. Valio [Mackenzie Presbyterian University]: Unveiling starspots magnetic field from planetary transit mapping