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On coronal streamer changes N. Goplasmwamy, M. Shimojo, W. Lu, S. Ya shiro, K. Shibasaki, R.A. Howard Advances In Space Research 2004, 33, 676-680 2004 年 6 年 14 年 年年年年年 年年 年年年 () 年年年年年年年年年年

On coronal streamer changes

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On coronal streamer changes. N. Goplasmwamy, M. Shimojo, W. Lu, S. Yashiro, K. Shibasaki, R.A. Howard Advances In Space Research 2004, 33 , 676-680. 2004 年 6 月 14 日 太陽雑誌会 速報 (森本)            プロミネンス爆発ゼミ. How ?. NoRH & SOHO observations on streamer changes with prominence eruptions. - PowerPoint PPT Presentation

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Page 1: On coronal streamer changes

On coronal streamer changes

N. Goplasmwamy, M. Shimojo, W. Lu, S. Yashiro, K. Shibasaki, R.A. Howard

Advances In Space Research2004, 33, 676-680

2004年 6月 14日 太陽雑誌会 速報 (森本)           プロミネンス爆発ゼミ

Page 2: On coronal streamer changes

Abstract

Coronal streamer represents one of the pre-eruption configuration of CMEs. … Characteristics of the streamer-related events.

Motivation :

Streamer-related events are closer to those of prominence eruptions with transverse trajectories.

Main result :

NoRH & SOHO observations on streamer changes with prominence eruptions.

Illustrative examplesstreamer-related VS. general prominence events.

How ?

Page 3: On coronal streamer changes

Introduction

Streamer events : Streamer activities (which show rise motions) with microwave prominence activations or eruptions.

These events do not include CMEs.

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Illustrative examples11 events.

Date P-angle Speed Max. Height

SubsequentCME (Time)

34.3 km/s

-12.8 km/s

1.32 Rs

1.09 Rs

NoRH daily mpeg : 1996-2001Overlapped with SOHO LASCO Lacked white-light CMEsStreamer changes were found

226 prominence eruptions186 5211

Page 5: On coronal streamer changes

2000 Jan 18

NoRH (17/23:11 – 18/06:11 UT)

SOHO LASCO18th all day

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2000 Jan 18 NoRH

1. Mainly transversal motion (radial speed = 5.2 km/s)

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2000 Jan 18 Pic du Midi

2. H prominence eruption

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2000 Jan 18 LASCO

1. Slow Swelling during NoRH Observation (11 hours)

2. Eruption as a CME(CME speed = 143 km/s within C2 FOV)

The streamer changes (corresponding to prominence activation or small scale eruption) is slow swelling.

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1998 Jun 01

NoRH (31/22:46 – 01/06:36 UT)

SOHO LASCO(01th all day)

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1998 Jun 01 NoRH & LASCO

Slow rise (~ 8km/s) Continuous slow swelling from 01th 01:30 UTCME (onset = 02th 08:08 UT)

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1998 Jan 01 EIT

Northern part showed a “failed eruption” (05:00 – 06:56 UT).In emission = heated?

The whole NoRH prominence is seen in absorption

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199 Jan 01 EIT & NoRH

Overlay of the 17GHz contours on an EIT difference image.

EIT ejecta (denoted by the arrow) reached as high as the leading edge of the microwave prominence.

Page 13: On coronal streamer changes

Summary

Transverse events : transversal motion is dominant.Radial event : radial motion is dominant

Transversal motion (prominence activation) is the dominant for the majority of streamer-related events.