Difference between revisions of "Storm"

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The M3-I2 focus group leaders are committed to helping the GEM/CEDAR community in the collection of reduced data sets including ground-based and space-based data sets:
 
The M3-I2 focus group leaders are committed to helping the GEM/CEDAR community in the collection of reduced data sets including ground-based and space-based data sets:
  
Ground-based:
 
  
- TEC
+
- Space-based:
  
- Magnetometers
+
* AMPERE currents
  
- Incoherent Scatter Radar Ne, Te, Ti profiles
+
* DMSP j/4 electron precipitation & cross-track drifts
  
- SuperDARN line-of-sight
+
* MMS
  
 +
* Van Allen Probes
  
Space-based:
+
* Other satellites as available (Geotail, ...)
  
- AMPERE currents
 
  
- DMSP j/4 electron precipitation & cross-track drifts
+
- Ground-based:
  
- MMS
+
* Magnetometers
  
- Van Allen Probes
+
* Incoherent Scatter Radar Ne, Te, Ti profiles
  
- Other satellites as available (Geotail, ...)
+
* SuperDARN line-of-sight
  
 +
* TEC
  
  
Line 44: Line 44:
 
The M3-I2 focus group leaders are also committed to helping the GEM/CEDAR community in the merging of models and sharing of results. We anticipate several nominal output fields but are open to new suggestions of important shared fields and benchmark results.
 
The M3-I2 focus group leaders are also committed to helping the GEM/CEDAR community in the merging of models and sharing of results. We anticipate several nominal output fields but are open to new suggestions of important shared fields and benchmark results.
  
N/S high-latitude ionosphere fields (in order of importance to M3-I2):
 
  
- Topside ion upflow
+
-Magnetosphere:
  
- Ionospheric convection potential
+
* MMS predictions
  
- Electron precipitation
 
  
- Vertical TEC Structuring
+
-Inner Magnetosphere:
  
- Temperature structure
+
* Calculated Dst and Ring Current
  
- Penetration electric fields
+
* 2D Ne, [O+], [H+], [He+] densities in equatorial plane
  
 +
* Van Allen Probe predictions of HOPE instrument
  
N/S Polar Wind fields:
 
  
- 2D Ion outflow flux at 2.5 Re
+
- N/S high-latitude ionosphere fields:
  
- 2D Ion N, V, T at 2.5 Re
+
* Topside ion upflow
  
Inner Magnetosphere:
+
* Ionospheric convection potential
  
- Calculated Dst and Ring Current
+
* Electron precipitation
  
- 2D Ne, [O+], [H+], [He+] densities in equatorial plane
+
* Vertical TEC Structuring
  
- Van Allen Probe predictions of HOPE instrument
+
* Temperature structure
  
Magnetosphere:
+
* Penetration electric fields
  
- MMS predictions
+
 
 +
- N/S Polar Wind fields:
 +
 
 +
* 2D Ion outflow flux at 2.5 Re
 +
 
 +
* 2D Ion N, V, T at 2.5 Re

Latest revision as of 12:39, 24 February 2017

M3-I2 Community Storm Study #1


Storm #1: 2016 Mar 4-9 (64-68) KDst = -98, Kp=6.3, F10.7=96, F107A=90

We propose modeling and measuring the two quiet days prior to the storm (4,5), the day of the storm main phase (6), and two recovery days (7,8).

The choice of this storm is based on the excellent measurement support of ground-based instrumentation and the reasonable support of magnetospheric satellites (MMS, Van Allen Probes). I choosing these two recent storms to encourage other validation focus groups within NSF-GEM and NSF-CEDAR communities to join in these model-measurement studies. This invitation includes magnetosphere, inner magnetosphere, ring current, polar wind outflow, high-latitude ionosphere & electrodynamics, and the full coupled system.




The M3-I2 focus group leaders are committed to helping the GEM/CEDAR community in the collection of reduced data sets including ground-based and space-based data sets:


- Space-based:

  • AMPERE currents
  • DMSP j/4 electron precipitation & cross-track drifts
  • MMS
  • Van Allen Probes
  • Other satellites as available (Geotail, ...)


- Ground-based:

  • Magnetometers
  • Incoherent Scatter Radar Ne, Te, Ti profiles
  • SuperDARN line-of-sight
  • TEC




The M3-I2 focus group leaders are also committed to helping the GEM/CEDAR community in the merging of models and sharing of results. We anticipate several nominal output fields but are open to new suggestions of important shared fields and benchmark results.


-Magnetosphere:

  • MMS predictions


-Inner Magnetosphere:

  • Calculated Dst and Ring Current
  • 2D Ne, [O+], [H+], [He+] densities in equatorial plane
  • Van Allen Probe predictions of HOPE instrument


- N/S high-latitude ionosphere fields:

  • Topside ion upflow
  • Ionospheric convection potential
  • Electron precipitation
  • Vertical TEC Structuring
  • Temperature structure
  • Penetration electric fields


- N/S Polar Wind fields:

  • 2D Ion outflow flux at 2.5 Re
  • 2D Ion N, V, T at 2.5 Re