…with help from: michael gehmeyr (lasp),

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Towards real-time Space Weather forecasts using CMIT: Geomagnetic variations and regional K indexes George Millward …with help from: Michael Gehmeyr (LASP), Mike Wiltberger, Wenbin Wang, Pete Schmitt, Art Richmond, Astrid Maute (HAO) ….and: Terry Onsager, Howard Singer, Chris Balch (SWPC)

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Towards real-time Space Weather forecasts using CMIT: Geomagnetic variations and regional K indexes George Millward. …with help from: Michael Gehmeyr (LASP), Mike Wiltberger, Wenbin Wang, Pete Schmitt, Art Richmond, Astrid Maute (HAO) ….and: - PowerPoint PPT Presentation

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Page 1: …with help from: Michael Gehmeyr (LASP),

Towards real-time Space Weather forecasts using CMIT: Geomagnetic variations and regional K indexes

George Millward

…with help from:

Michael Gehmeyr (LASP),

Mike Wiltberger, Wenbin Wang, Pete Schmitt, Art Richmond, Astrid Maute (HAO)

….and:

Terry Onsager, Howard Singer, Chris Balch (SWPC)

Page 2: …with help from: Michael Gehmeyr (LASP),

LFM

TIE-GCM

Magnetosphere -Ionosphere Coupler

Electric PotentialParticle Precipitation

ConductivitiesWinds

•CMIT: First principles, physics-based, 3D, time-dependent model. Consists of a coupling between the Lyon-Fedder-Mobarry MHD Magnetospheric model(LFM) and the NCAR Thermosphere Ionosphere Electrodynamics General Circulation Model (TIE-GCM)

•Present: Medium resolution mode. Running on “Bluesky”: NCAR IBM Cluster 1600 - 8 proc (OpenMP)

•Future: High resolution fast-mode (MPI). Next generation multi-processor computing resources

Real-time Solar Wind Data at L1

CISM Knowledge Transfer:

Transitioning CMIT

for Real-Time Forecasting

Space-Weather Forecast (SWPC)

Current Geospace Conditions

Coupled Magnetosphere Ionosphere Thermosphere model (CMIT 2.0)

•Initial: Real-time solar wind data from the ACE spacecraft. Lead time: about 1 hour

•Future: Solar wind model driven by solar observations Lead-time: 3 to 5 days

Real-time Inputs

Solar Wind Model

Output Products, User Benefits

•Initial: 1 hour forecast of geomagnetic activity, global ionospheric electron content, magnetopause location

•Users: Power utilities, Satellite operators, communication, precision GPS

•Future: 3 day forecast using solar model and observations.

Sun

Earth

Page 3: …with help from: Michael Gehmeyr (LASP),

CMIT 2.5 development on NOAA wJET computer

•wJET: LINUX Cluster (1400 cores)

•Utilizes Intel compilers

•Supports parallel processing via MPI (Not OpenMP)

•LFM and LFM-MIX running in parallel on wJET

•Tiegcm v 1.9 running on wJET

CMIT 2.5 (LFM MPI - TIEGCM1.9) on wJET 98% built

Page 4: …with help from: Michael Gehmeyr (LASP),

LFM

TIE-GCM

Magnetosphere -Ionosphere Coupler

Electric PotentialParticle Precipitation

ConductivitiesWinds

Real-time Solar Wind Data at L1

Space-Weather Forecast (SWPC)

Current Geospace Conditions

Page 5: …with help from: Michael Gehmeyr (LASP),

LFM

TIE-GCM

Magnetosphere -Ionosphere Coupler

Electric PotentialParticle Precipitation

ConductivitiesWinds

Real-time Solar Wind Data at L1

Space-Weather Forecast (SWPC)

Current Geospace Conditions

“in house” (NOAA SWPC)

Page 6: …with help from: Michael Gehmeyr (LASP),

Real-time Solar Wind Data at L1

Page 7: …with help from: Michael Gehmeyr (LASP),

LFM

TIE-GCM

Magnetosphere -Ionosphere Coupler

Electric PotentialParticle Precipitation

ConductivitiesWinds

Page 8: …with help from: Michael Gehmeyr (LASP),

Outputs/Products

Current Geospace Conditions

Page 9: …with help from: Michael Gehmeyr (LASP),
Page 10: …with help from: Michael Gehmeyr (LASP),
Page 11: …with help from: Michael Gehmeyr (LASP),

April 2006 Magnetic Storm

2nd 20thApril 20065 9 14

Page 12: …with help from: Michael Gehmeyr (LASP),

April 2006: Magnetometer data

Page 13: …with help from: Michael Gehmeyr (LASP),

April 2006: CMIT model output

Page 14: …with help from: Michael Gehmeyr (LASP),

JN

JE

JHorizontal

Page 15: …with help from: Michael Gehmeyr (LASP),
Page 16: …with help from: Michael Gehmeyr (LASP),
Page 17: …with help from: Michael Gehmeyr (LASP),

Summary / Comments:

Exciting initial results: CMIT clearly responding well during storm conditions:

Some problems.

Future:

Running CMIT 2.5 on NOAA wJET (soon !!)

Further runs needed for calibration/tuning

Inclusion of magnetospheric currents (LFM/RCM)