c. may 12, 1997 interplanetary event
DESCRIPTION
C. May 12, 1997 Interplanetary Event. Ambient Solar Wind Models. SAIC 3-D MHD steady state coronal model based on photospheric field maps. CU/CIRES-NOAA/SEC 3-D solar wind model based on potential and current-sheet source surface empirical models. CME Cone Model. Conceptual model: - PowerPoint PPT PresentationTRANSCRIPT
C. May 12, 1997 Interplanetary Event
Ambient Solar Wind Models
SAIC 3-D MHD steady state coronal model based on photospheric field maps
CU/CIRES-NOAA/SEC 3-D solar wind model based on potential
and current-sheet source surface empirical models
CME Cone Model
Conceptual model:CME as a shell-like region
of enhanced densityGeometrical and kinematical fitting:
Dependence of predicted CME haloson the latitude, longitude, angular
width, and velocity[ Zhao et al., 2001 ]
CME Cone Model
[ Zhao et al., 2001 ]
Best fitting for May 12, 1997 halo CME
• latitude: N3.0• longitude: W1.0• angular width: 50 deg
• velocity:650 km/s at 24 Rs
(14:15 UT)• acceleration: 18.5 m/s2
Boundary Conditions
Ambient Solar WindAmbient Solar Wind
+ Plasma Cloud
CASE - 1 CASE - 2
Evolution of Parameters at Earth
Ambient Solar WindAmbient Solar Wind
+ Plasma Cloud
CASE - 1 CASE - 2
May 12, 1997 Interplanetary Event
ICME propagates into bi-modal solar wind
May 12, 1997 Interplanetary Event
Fast stream follows the ICME
May 12, 1997 Interplanetary Event
ICME propagates into enhanced density at CIR
May 12, 1997 Interplanetary Event
IMF is distorted by shock compression and draping around ICME
May 12, 1997 Interplanetary Event
May 12, 1997 Interplanetary Event