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Line Profile Line Profile Characteristics of Solar Characteristics of Solar Explosive Event Bursts Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

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Page 1: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

Line Profile Characteristics of Line Profile Characteristics of Solar Explosive Event BurstsSolar Explosive Event Bursts

Z. Ning et al 2004 A&A 419,1141

Speaker: Jinping Dun

Page 2: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

1. Introduction1. Introduction

Explosive Event is a small-scale, short-lifetime phenomenon in the transition region of quiet Sun.

Main Characteristics

Broaden Line Profile

T ~ 105K ( i.e. SiIV 1393 Å) V~100km/s

Size ~ 2” Lifetime ~ 1min

Physical Model

Plasma Jets Produced by Magnetic Reconnection

Page 3: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

2. Observations and Data Reduction (i)2. Observations and Data Reduction (i)

MD

I Magnetogram

The area rastered by SUMER and locations of explosive events

Page 4: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

2. Observations and Data Reduction (ii)2. Observations and Data Reduction (ii)

SiIV 1393 Å Spectrum Slit ~ 1” x120”

Step ~ 6

Interval~ 1.13”

Exposure Time ~5s

Page 5: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

3.3. Examples and Results (i)Examples and Results (i)

Time Variation of Integrated Intensity

Page 6: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

3.3. Examples and Results (ii)Examples and Results (ii) Repetition of Explosive Events

Page 7: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

3.3. Examples and Results (iii)Examples and Results (iii)

2D Time Evolution of 5 Groups of Events

The black dashed line boxes surround events with obvious red-blue wing spatial offset.

(Evidence of reconnection jets, Innes et al.,1997, Nature,386,811)

Page 8: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

3.3. Examples and Results (iv)Examples and Results (iv) The Magnetic Field

Emergence (white) and Cancellation (black)

Page 9: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

4.4. DiscussionDiscussion

2D Structure Evolution of Explosive Events

Repetition of Explosive Events Magnetic reconnection could be triggered by

3~5 min oscillation waves in the chromospheric and transition region.

Page 10: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

Thank YouThank You !!

Page 11: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

Profile of Explosive Event (i)Profile of Explosive Event (i)

Wavelength

Velocity Along Line-of-sight V=0

V>0(red-shift)V<0(blue-Shift)

Explosive Event

Page 12: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

Profile of Explosive Event Profile of Explosive Event (ii)(ii)

Ni 1393.33Ni 1393.33

SiIV 1393.78SiIV 1393.78

Page 13: Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun

three components: stationary and two high-speed (along line-of-sight) sources. (Chae et al.1998,ApJ,497,L109)

stationary component

blue-shift component red-shift components

Profile of Explosive Event (iii)Profile of Explosive Event (iii)