COFFIES
Consequences Of Fields and Flows in the Interior and Exterior of the Sun
CET
COFFIES Effectiveness Team
CV
Convection (Team)
DY
Dynamo (Team)
HS
Helioseismology (Team)
MI
Modeling Integration (Team)
AAS
American Astronomical Society
ADA
Americans with Disabilities Act
aDRS
Anelastic Dynamo in Rotation Spheres model (DY)
AFT
Advective Flux Transport model (SL)
AGU
American Geophysical Union
AISES
American Indian Science and Engineering Society
AR
Active Region
Baristas
COFFIES leadership (executive and Team leads)
Beans
Students, Postdocs, and (self-identified) early career researchers
BLFT Dynamo
3D Babcock-Leighton Flux Transport model (DY)
CCMC
Community Coordinated Modeling Center
Coffieholics
CET members
Coffienators
COFFIES members
CtL
Center-to-Limb [effect]
CZ
Convection Zone
DART
Data Assimilation Research Testbed
DEIA
Diversity, Equity, Inclusion, Accessibility
DL
Deep Learning
DMP
Data Management Plan
DNS
Direct Numerical Simulation
DR
Differential Rotation
DSC
DRIVE Science Center
EL
Executive Leadership
EMF
ElectroMotive Force
EULAG
EULer-LAGrange; 3D Anelastic Global Model of Solar-Type Stars (DY)
FD
Finite Differences (modeling method)
FT&E
Flux Transport and Emergence (THEME)
FTE
Full Time Equivalent
FV
Finite Volumes (modeling method)
GALE
Global Acoustic Linearized Euler model (DY)
GONG
Global Oscillation Network Group (Solar Telescope)
GSU
Georgia State University
HMI
Helioseismic and Magnetic Imager
Holography
Helioseismology method (HS)
HPS
Hybrid Pseudo-Spectral model (CV)
IB
Impact Broadening
JSOC
Joint Science Operations Center
LHS
Lawrence Hall of Science
MC
Meridional Circulation
MFE
Mean Field Electrodynamics
MHD
MagnetoHydroDynamics
MHD-SWT
MHD Shallow-Water Tachocline model (DY)
ML
Machine Learning
MUREP
Minority University Research and Education Project
NAMFID
Non-Axisymmetric Mean-FIeld Dynamo model (DY)
NAS
NASA Advanced Supercomputing
NASA
National Aeronautics and Space Administration
NASEM
National Academies of Sciences, Engineering & Medicine
NCWIT
National Center for Women & Information Technology
NISP
NSO Integrated Synoptic Program
NOAA
National Oceanic and Atmospheric Administration
NRC
National Research Council
NSBP
National Society of Black Physicists
NSF
National Science Foundation
NSO
National Solar Observatory
NSSL
Near-Surface Shear Layer (THEME); Subsurface (Rotational) Shear Layer (terminology defined by D. Haber)
Pencil
3D Compressible (FD) model (DY)
PI
Principal Investigator
PM
Program Manager
POISE
Public Outreach and Informal Science Education
RADMHD
RADiative MHD convective model (CV)
RANS
Reynolds Averaged Navier-Stokes (model)
Rayleigh
Spherical Anelastic MHD code (CV)
RD
Ring Diagram helioseismology method (HS)
REU
Research Experiences for Undergraduates
Rotational Inversion
Helioseismology tool (HS)
SACNAS
Soc. for Advancement of Chicanos/Hispanics & Native Americans in Sci.
SAGA
Stellar Adaptive Global Activity code (FV; prelim.) (MI)
SB
Science Breakthrough [Objective]
SC
Solar Cycle
SDAC
Solar Data Analysis Center
SDO
Solar Dynamics Observatory
SFT
[Global] Surface Flux Transport model (SL)
SHHR
Solar Hemispherical Helicity Rules
SOHO
SOlar and Heliospheric Observatory
SOS
Science on a Sphere ®
SPDF
Space Physics Data Facility
SPEAR
Solar Photospheric Ephemeral and Active Region (catalog)
SQ
Science Question
SSL
Space Sciences Laboratory
ST
Science Team
StellarBox
3D Radiative MHD model (MI)
STEM
Science Technology Engineering & Math
Tachocline
A thin layer of rotational shear at the bottom of the convection zone (THEME)
TD
Time Distance helioseismology method (HS)
Turbulent Pumping
The transport of magnetic flux due to the presence of density and turbulence gradients in convectively unstable layers (Guerrero et al., 2008)
UC
University of California
UCB
University of California, Berkeley
UCSC
University of California, Santa Cruz
URG
Under-Represented Groups
WG
Working Group