ENLIL 3D-MHD Modeling Support of Heliospheric Missions European Space Weather Week, Liege, Belgium,...
If you can't read please download the document
ENLIL 3D-MHD Modeling Support of Heliospheric Missions European Space Weather Week, Liege, Belgium, 17-21 November 2014 Dusan Odstrcil (GMU & NASA/GSFC)
ENLIL 3D-MHD Modeling Support of Heliospheric Missions European
Space Weather Week, Liege, Belgium, 17-21 November 2014 Dusan
Odstrcil (GMU & NASA/GSFC) in collaboration with UCSD/CASS and
NASA/SWRC space weather teams. NASA/NSF Partnership For
Collaborative Space Weather Modeling
Slide 2
WSA-ENLIL-Cone Modeling System Observationally driven,
near-real time modeling system Routine simulation of corotating
streams and CMEs, event-by event Much faster than real-time
Slide 3
ENLIL Solar Wind Prediction helioweather.net Experimental,
real-time simulation of corotating and transient solar wind
disturbances driven by various coronal models. Results are updated
daily and are used for validation of a research ENLIL version.
MODELS Daily updated results by various driving coronal models (1.7
AU): MISSIONS Daily updates results to support heliospheric
missions (5.3 AU): ARCHIVE Animations and temporal profiles in
2011-2014 (in progress): EVENTS selected CME events simulated in
higher resolution and presented with more details
IPSBDIPSBD-SWRCWSAdub-SWRCWSAduz-SWRCWSAdtb-SWRC
JUNOMAVENMESSENGERROSETTASPITZERSTEREO-ASTEREO-B
Slide 4
helioweather.net Models Prediction of the solar wind parameters
in the inner heliosphere (1.7 AU): - various driving coronal models
(left) - various visualization (right)
Slide 5
helioweather.net Missions Prediction in the mid-heliosphere
(5.3 AU): - various planets/spacecraft (left) - various
visualization (right) ROSETTA
Slide 6
Fitted Parameters of CMEs: 2014 Sep-Oct No.DateLatLonRadVel
012014-09-01T13:3015-1555215002014-09-01T11:24:00-CME-001
022014-09-01T20:33-8-10924 9002014-09-01T16:00:00-CME-001
032014-09-02T00:40-9-120-3414002014-09-01T22:24:00-CME-001
042014-09-02T05:40-10-1103311402014-09-02T02:36:00-CME-001
052014-09-02T20:37-25-5319442014-09-02T17:00:00-CME-001
092014-09-10T20:0015104514002014-09-10T18:18:00-CME-001
112014-09-13T04:50-7-70188302014-09-13T00:36:00-CME-001
202014-09-24T23:0010-1704514002014-09-24T21:54:00-CME-001
212014-09-26T08:054-1145910752014-09-26T04:38:00-CME-001
242014-10-10T20:58-1073448002014-10-10T16:31:00-CME-001
262014-10-13T07:3011-93189812014-10-13T04:30:00-CME-001
272014-10-14T23:32-16-109609502014-10-14T19:00:00-CME-001
282014-10-16T17:26-13-8898602014-10-16T13:26:00-CME-001 37 CMEs
operationally fitted by SWRC (CMEs with Vel > 800 km/s listed
here)
Slide 7
Solar Wind Velocity at Rosetta: 2014-09-04T09 Flank of broad
CME, captured by strong CIR
Slide 8
Solar Wind Velocity at Rosetta: 2014-09-15T02 Flank of broad
narrow CNE at weak CIR
Slide 9
Solar Wind Velocity at Rosetta: 2014-09-17T12 Broad multi-CMEs
with moderate shock in rarefaction
Slide 10
Solar Wind Velocity at Rosetta: 2014-09-23T00 Narrow CME with
weak shock
Slide 11
Solar Wind Velocity at Rosetta: 2014-09-29T06 Broad CME
captured by strong CIR
Slide 12
Solar Wind Velocity at Rosetta: 2014-10-04T12 Broad CME with
moderate shock in rarefaction
Slide 13
Solar Wind Velocity at Rosetta: 2014-10-09T15 Narrow CME, no
shock, in rarefaction
Slide 14
Solar Wind Velocity at Rosetta: 2014-10-16T06 Narrow CME, no
shock
Slide 15
Solar Wind Velocity at Rosetta: 2014-10-17T03 Narrow CME, weak
shock
Slide 16
Solar Wind Velocity at Rosetta: 2014-10-17T21 Narrow CME, no
shock
Slide 17
Solar Wind Velocity at Rosetta: 2014-10-21T16 Broad CME with
strong shock within CIR
Slide 18
Shock IMF Connectivity at Rosetta: 2014-09-16T00 Slowly moving
CMEs, weak velocity jump at IMF-connected shock
Slide 19
Shock IMF Connectivity at Rosetta: 2014-10-11T02 Moderate
velocity jump at IMF-connected shock
Slide 20
Shock IMF Connectivity at Rosetta: 2014-09-01T19 Strong
velocity jump at IMF-connected shock
Slide 21
Predicted ICMEs at Rosetta: 2014 Sep-Oct No.:Forward
shockDriving ejectaComment 012014-09-04T09Flank of broad CME,
captured by strong CIR 022014-09-15T03Flank of narrow CME at weak
CIR 032014-09-17T122014-09-19T06Broad multi-CMEs, moderate shock,
in rarefaction 042014-09-23T002014-09-23T06Narrow CME, weak shock
052014-09-29T06Broad CME, captured by strong CIR
062014-10-04T122014-10-04T21Broad CME, moderate shock, in
rerefaction 072014-10-09T15Narrow CME, no shock, in rarefaction
082014-10-16T09Narrow CME, no shock
092014-10-16T122014-10-17T03Narrow CME, weak shock
102014-10-18T00Narrow CME, no shock
112014-10-21T062014-10-21T16Broad CME, strong shock, within
CIR
Slide 22
Predicted SEP Events at Rosetta: 2014 Sep-Oct
No.:BeginEndComment 012014-09-01T122014-09-03T12Strong
022014-10-10T212014-10-12T00Medium
Slide 23
Summary Routine simulations up to 5 AU are possible by 3D
numerical MHD code ENLIL driven by either WSA-Cone or IPSBD coronal
data at 0.1 AU NASA/GSFC Space Weather Research Center (SWRC)
operationally fits geometric and kinematic parameters of all
observed CMEs: - 37 CMEs in 2014 Sep (9 CMEs > 800 km/s) - 17
CMEs in 2014 Oct (4 CMEs > 800 km/s) HelioWeather testbed system
provides results from various model variants at Earth and at
various heliospheric missions. Predicted disturbances at Rosetta in
2014 Sep-Oct: - complex scenarios involves CMEs overtaken by CIRs -
11 ICMEs: 6 without shock, 5 with shocks (see Table) - 2 SEP events
(Sep 1-3, Oct 10-11), other possible (see Figures) Actual state and
predictions:
http://helioweather.com/missions/rosettahttp://helioweather.com/missions/rosetta
Further calibration and validation needed