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CONTENTS Large-Scale Corona (eclipse) - images - models Local Regions of Corona (active regions) - images - models 3. Topology of Corona. SLIDE SHOW 4 - Coronal Loops. ("crown") -- See at ECLIPSE of Sun. 1. LARGE-SCALE CORONA. Another ECLIPSE.
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CONTENTS • Large-Scale Corona (eclipse) - images - models • Local Regions of Corona (active regions) - images - models 3. Topology of Corona SLIDE SHOW 4 - Coronal Loops
("crown") -- See at ECLIPSE of Sun 1. LARGE-SCALE CORONA
How Model Global Corona ? Use observed Br at surface (on grid or treat as series of sources) and construct solutions to j x B = 0 Simplest - assume j = 0, so that
Example Observed Calculated [Colour is velocity]
2. LOCAL REGIONS OF CORONA TRACE (Active region)
Ex 2. Observations of Location of Loops in an Emerging Flux Region
Compare with Potential, Linear fff, Nonlinear fff (2005) Best fit -- nonlinear fff
Ex 3. Magnetic Fragments in Superganule Magnetogram movie (white +ve , black -ve)- 20 hrs • Flux emerges ... cancels • Reprocessed very quickly (14 hrs !!!)
“Magnetic Carpet” Magnetic sources in surface are concentrated Use observed Bn at photosphere to calculate coronal B from Laplace’s equation
From observed magnetograms - construct coronal field lines - statistical properties: most close low down Time for all field lines to change connections only 1.5 hours
3. TOPOLOGY of CORONAL B In 2D -- Separatrix curves In 3D -- Separatrix surfaces -- intersect inSeparator
Structure of Null Point Simplest B = (x, y, -2z) 2 families of field lines through null point: Spine Field Line FanSurface
? Reveal structure of complex field ? plot a few arbitrary B lines E.g. 2 unbalanced sources SKELETON -- set of nulls, separatrices -- from fans
2 Unbalanced Sources Skeleton: null + spine + fan (separatrix dome)
Simplest configuration w. separator: Sources, nulls, fans -> separator
Looking Down on Structure Bifurcations from one state to another