Return-Path: Received: (qmail 12460 invoked from network); 26 May 2001 00:51:23 -0000 Received: from unknown (HELO murphys-inbound.servers.plus.net) (212.159.14.225) by excalibur.plus.net with SMTP; 26 May 2001 00:51:23 -0000 Received: (qmail 12453 invoked from network); 26 May 2001 00:50:50 -0000 Received: from unknown (HELO post.thorcom.com) (212.172.148.70) by murphys with SMTP; 26 May 2001 00:50:50 -0000 Received: from majordom by post.thorcom.com with local (Exim 3.16 #2) id 153SCW-0007kj-00 for rsgb_lf_group-outgoing@blacksheep.org; Sat, 26 May 2001 01:45:04 +0100 Received: from tomts6.bellnexxia.net ([209.226.175.26] helo=tomts6-srv.bellnexxia.net) by post.thorcom.com with esmtp (Exim 3.16 #2) id 153SCV-0007kZ-00 for rsgb_lf_group@blacksheep.org; Sat, 26 May 2001 01:45:03 +0100 Received: from server1 ([209.226.189.169]) by tomts6-srv.bellnexxia.net (InterMail vM.4.01.03.16 201-229-121-116-20010115) with SMTP id <20010526004356.ISIB7009.tomts6-srv.bellnexxia.net@server1> for ; Fri, 25 May 2001 20:43:56 -0400 Message-ID: <002f01c0e57c$8f4eb7a0$0a00a8c0@ThreeLakes.ca> From: "Larry Kayser" To: rsgb_lf_group@blacksheep.org References: <001901c0e564$cde1ee00$0165073e@default> Subject: LF: Re: CME directions, and particle energy Date: Fri, 25 May 2001 20:41:07 -0400 MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org X-Listname: rsgb_lf_group Sender: Alan: > Hi Larry, well I am not sure that the professionals know a awful lot about > 'em. I have been chasing this for a while and almost no information is available in the area that I want to find information. >As I understand it a CME is erupted from the surface roughly radially > as far as the main energy is concerned. I suspect it is a little like the > stone-in-the-pond and think there may be some spreading of the energy as the > cme travels. I have a sense from what I have found that the "radially" is a variable as well, the main burst apparently does not have a direct vector out from the center of the sun, it can come out from any point from 0 to 90 degrees from the surface, although many do come fairly close to 90 degrees. I could also be in a position of having totally missunderstood what I was reading of course, but that is what I have so far. >Thus I think the professionals judge whether a CME is going to > make an impact with the Earth's magnetosphere by finding where on the solar > surface it is generated. Thus if near the solar equator and in the middle of > the disc, we are certainly going to get the particles. If however it is > generated off towards the limb, then the main direction will be not pointing > at Earth so we do not get the effect. My interest is not in what is going to give the Earth a blast, my interest is what is going by the Earth at a radius of out to 7.5 million miles. My specific interest is in the near misses, I have no interest in the ones that are going to get us a good one. > There is another problem however, the ejected plasma mass carries a > substantial magnetic field, and the magnitude of the effect on us depends on > the orientation of that field with respect to the Earth's magnetic field. > One direction and it passes harmlessly round the earth magnetosphere, the > other direction and it couples with the Earth's field and then particle > injection is possible. I am not sure at what stage the solar observers are > able to determine this. I believe it is this effect that means that some > supposedly big CMEs seem to have little effect on us, while a smaller one > (with the appropriate orientation) will sometimes produce big auroral > displays. I have a direct interest in anything that is going by the Earth within a radius of 7.5 million miles but far enough away that it is not directly going to give us one on the nose. > So, in my experience, spotting the CMEs is only part of the story. So far I > have tried using the Kp index to see whether there will be (or maybe 'has > been') particle injection. I also believe the Kp index may be a measure of > the particle energy (...current >> Field??)...related to the field (but I > maybe wrong!).... BIG CMEs seem give a high Kp. The point is that it doesnt > immediately correlate with radio effects as it takes the particles a while > to work their way down from the poles to lower latitudes, and diffuse down > into the ionsphere. Excellent. I am wondering if I could take some of these information elements and from them determine the direction that the CME is going and if it is going to come, at any energy level, within the 7.5 million miles from Earth. > I reckon at least 24 hours and maybe longer before the effect is felt in > radio terms. By then the Kp has usually dropped right back to quiet levels > again. Certainly, I can agree, and the time lag can be up to a week from what I saw recently in some data. > I may be talking a load of bilge but that the best I can do from my > observations.....hope it maybe of some help....I am still trying to work up > some correlation attempts. > If anyone knows better please help me correct my naive ideas. If we had certain knowledge of what you are talking about then the subject would be well understood and my querry would have received the response, go read this chapter in some book hi. Since that hasn't happened I can assume we are into a border area of knowledge. One thing that would be a big help is to identify who are the worlds experts in this area and then I can try and engage one of them in a conversation. If anyone has any ideas then I would sure appreciate the help. If anyone is offended at the OFF TOPIC discussion let me know and I will go away hi. Thanks Alan for your time and effort. Larry VA3LK