Relaxation of Sheared Magnetic fields — a Process of Contraction

Relaxation of Sheared Magnetic fields — a Process of Contraction

Events List

• The M1.2 flare of 2002-04-15 (Sui and Holman 2003)

• The M2.1 flare of 2002-09-09 (Ji, Wang, and Goode et al. 2004)

• The X3.1 flare of 2002-08-24 (Li and Gan 2005)

• The X3.9 flare of 2003-11-03 (Veronig, Karlicky, and Vrsnak et al. 2006)

• The M1.2 flare of 2004-11-01 (Ji, Huang, and Wang et al. 2006)

• The M6.8 flare of 2003-06-13 (Ji, Huang, and Wang 2007)

• The X10 flare of 2003-10-29 (Zhou, Ji and Huang 2006)

• The M5.7 flare of 2002-03-14 (Zhou, Ji and Huang 2006)

• The M1.0 flare of 2002-07-26 (Ji & Wang 2007)

2002/04/15

in the early phase of the flares, the looptop sources moves down

Velocity ~ tens of kilometers per second

10-25 keVThe M1.2 flare of 2002-04-15: Motion of looptop sources

The M2.1 flare of 2002-09-09: Motion of looptop sources and flare kernels

The X3.1 flare of 2002-08-24: shrinkage of flaring loops

The M3.9 flare of 2003-11-03: Motion of looptop sources

Flare shear

The M1.2 flare of 2004-11-01: Motion of looptop sources and flare kernels – Unshear motion

03:18:44 – 03:18:56 03:19:08 – 03:19:20

The M1.2 flare of 2004-11-01: Motion of looptop sources and flare kernels – Unshear motion

The M6.8 flare of 2003-06-17: Motion of looptop sources, EUV flaring loops and flare kernels

– Unshear motion

The M6.8 flare of 2003-06-17: Motion of looptop sources, EUV flaring loops and flare kernels

– Unshear motion

The M6.8 flare of 2003-06-17: Motion of looptop sources, EUV flaring loops and flare kernels

– Unshear motion

The flare of 2002-03-14 – unshear motion

The flare of 2002-03-14 – unshear motion

The flare of 2002-03-14

The flare of 2003-10-29

The flare of 2003-10-29

Expansion of flaring loops

☆ inward motion of conjugate flaring kernels ☆ shrinkage of flaring loops (radio, EUV) ☆ descending of HXR looptop sources

Unshear motion during contraction and expansion!

Contraction of flaring loops

☆ outward motion of conjugate flaring kernels ☆ expansion of flaring loops (radio, EUV)

☆ upward motion of HXR looptop sources

Interpretation of Loop Contraction10-25 keV

1. Current sheet formation (Sui & Holman 2003, Sui et al. 2004)

2. Magnetic shrinkage (Acton & Forbes1996,

Lin 2004)

3. Collapsing magnetic trap (Veronig et al. 2005)

4. Magnetic Implosion (Hudson 2000)

V dVB )8/( 2 reduced

V dVB )8/( 2

Mapping effectfrom

the Photosphere

Modifying effect caused by

Our interpretation (ApJ, 2007)

220 ),( kkykxFB z

zeyxBzyxB ),(),,( 0

constk 22

Unshear rate and HXR spikes

The M1.0 flare of2002-07-26

What I am doing

★ A statistical study using old BBSO H-alpha data to study the contracting motion

★ A statistical study using HXR data to study the contracting motion

★ Analyzing the change of flare shear, and its relationship

with magnetic shear using more events.

★ The correlation between the unshear rate with HXR spikes.

★ Verifying the analytical model from existing flare data.

…★ .

We can estimate the energy releasing rate of a flare

Proportional to the GOES magnitude

e.g.

estimated by the contraction motion

an integral over flaring region

The M1.1 flare The M6.7 flare

What is the physical meaning of flare shear?

e.g.

THANKS!