Nobeyama CDAW03 Group 1 1. Event (30-Sep-2000)

1.1 Time profiles

1.2 Images

SXT movie

HXR/SXR images at peak 1

HXR/SXR images at peak 2

HXR/SXR images at peak 2 (diffuse)

2. Analyses

2.1 Above-the-looptop HXR source

Time profiles

comparison with other observations

Spectra

2.2 Outer loop(?) expansion

movie

time series of 1-D integrated image

SXR vs radio in the decay phase

estimatation of radio emission from SXR observations

Radio spectrum maps

EIT movie 3. Summary and Discussion

3.1 What is the above-the-looptop source?

This source is located in the hight-T region.

The M2-source is located at the higher altitude than that of the M1-band.

The spetrum is a little softer than that of the footpoint sources.

3.2 What is the SXR outer loop?

It expanded during the impulsive phase, but the expanding velocity decreased in the gradual phase.

Radio emission can not be explained from the thermal emission estimated from the SXR observations.

Non-thermal electrons might be trapped in the outer loops.