Community Workshop on Ground Based Solar Research

White Papers and Reference Materials:

Approaches to optimize scientific productivity of ground-based solar telescopes

Asteroseismology: The next frontier in solar-stellar physics

Causes of solar activity

Coronal magnetic fields

ChroMag: The community synoptic chromospheric magnetograph

Exploring the physics of the corona with total solar eclipse observations

Generation, evolution and destruction of solar magnetic fields

Ground-based solar physics in the era of space astronomy

Ground-based space weather instrument suites

Helioseismology

High-fidelity coronal imaging at low radio frequencies

Next generation space science with the geospace array

Next steps in solar spectral irradiance studies

Particle acceleration and transport on the sun

Science and operation of the advanced technology solar telescope

Solar flares and the chromosphere

The 1.6 m clear aperture optical solar telescope in big bear—The NST

The COronal solar magnetism observatory

The frequency agile solar radiotelescope (FASR)

The importance of ground-based observations of the solar corona

The need for synoptic optical solar observations from the ground

The solar magnetic dynamo and its role in the formation and evolution of the Sun, in the habitability of its planets, and in space weather around Earth

The sun as a star

Uncovering mechanisms of coronal magnetism via advanced 3D modeling of flares and active regions