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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)
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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)
The M1.2 flare of 2002-04-15: Motion of looptop sources 10-25 keV • in the early phase of the flares, the looptop sources moves down • Velocity ~ tens of kilometers per second 2002/04/15
The M2.1 flare of 2002-09-09: Motion of looptop sources and flare kernels
The M1.2 flare of 2004-11-01: Motion of looptop sources and flare kernels – Unshear motion 03:19:08 – 03:19:20 03:18:44 – 03:18:56
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
Expansion of flaring loops • ☆ outward motion of conjugate flaring kernels • ☆ expansion of flaring loops (radio, EUV) • ☆ upward motion of HXR looptop sources Contraction 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!
Interpretation of Loop Contraction 10-25 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) reduced
Our interpretation (ApJ, 2007) Modifying effect caused by Mapping effect from the Photosphere
Unshear rate and HXR spikes The M1.0 flare of 2002-07-26
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. ★ ….
e.g. We can estimate the energy releasing rate of a flare an integral over flaring region estimated by the contraction motion Proportional to the GOES magnitude
The M1.1 flare The M6.7 flare
e.g. What is the physical meaning of flare shear?