Date: Sun, 22 Aug 1999 09:21:11 -0600 (MDT)
From: Richard Canfield <canfield> 

The campaign "Eruptive Flares Associated with Sigmoids during WSM3" (http://solar.physics.montana.edu/max_millennium/ops/op002/op002.html) will continue to follow the backward-S sigmoid in AR 8668, for which coordinates were N22 W25 at 2400 UT on 21-Aug-99. Recent news:

>Date: Sun, 22 Aug 1999 12:26:27 +0900
>From: KUROKAWA Hiroki <kurokawa@kwasan.kyoto-u.ac.jp>
>To: canfield@mithra.physics.montana.edu
>Subject: Re: MMOC002 Target
>
>Dear Canfield san;
>
> I wonder no large flare of more than M-class occurred during the disappearance
>of the southern part of the S-shape filament in NOAA 8668.
> By our Halpha observations around 02 UT of 22 Aug. a small EFR was found
>to be emerging at the site of the disppeared filament.
>
> H. Kurokawa