Relaxation of Sheared Magnetic fields — a Process of Contraction

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Relaxation of Sheared Magnetic fields — a Process of Contraction

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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) - PowerPoint PPT Presentation

Transcript of Relaxation of Sheared Magnetic fields — a Process of Contraction

Page 1: Relaxation of Sheared Magnetic fields  — a Process of Contraction

Relaxation of Sheared Magnetic fields — a Process of Contraction

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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)

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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

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

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

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

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Flare shear

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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

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

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

– Unshear motion

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

– Unshear motion

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

– Unshear motion

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The flare of 2002-03-14 – unshear motion

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The flare of 2002-03-14 – unshear motion

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The flare of 2002-03-14

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The flare of 2003-10-29

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The flare of 2003-10-29

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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

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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

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V dVB )8/( 2

Mapping effectfrom

the Photosphere

Modifying effect caused by

Our interpretation (ApJ, 2007)

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220 ),( kkykxFB z

zeyxBzyxB ),(),,( 0

constk 22

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Unshear rate and HXR spikes

The M1.0 flare of2002-07-26

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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.

…★ .

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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

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The M1.1 flare The M6.7 flare

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What is the physical meaning of flare shear?

e.g.

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THANKS!