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STELLAR RESEARCH
Task
B:
Stellar
magnetism
across
the
Hertzsprung-Russell
(HR)
diagram:
The
purpose
of
task
B
is
to
model
accurately
stars
that
are
either
less
or
more
massive
than
the
Sun
or
younger
or
more
evolved
(RGB)
in
order
to
map
in
3-D
stellar
magnetism
and
the
HR
diagram .
Task
B1:
Convection,
differential
rotation
and
magnetism
in
low
mass
red
giant
(RGB)
stars
Task
B2:
Young
Suns:
magnetism
of
fastly
rotating
stars,
activity
vs
rotation
scaling
law
Task
B3:
A
stars:
magnetism
in
core
convection
of
massive
stars
and
interaction
with
magnetism
in
radiative
envelope
Task
B4:
K
stars:
convection
and
magnetism
in
deep
convection
shell
for
low
mass
stars
Task
B5:
Introduction
of
averaged
profiles
and
physical
quantities
deduced
from
3-D
simulations
into
1D
stellar
evolution
models
and
2-D
mean
field
stellar
dynamo
models
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