X-Account-Key: account2 X-UIDL: 45591e7f00000002 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from relay19.bu.edu (relay19.bu.edu [128.197.26.136]) by bu-ast2.bu.edu (8.11.6/8.11.6) with ESMTP id kADJ3Ac11197 for ; Mon, 13 Nov 2006 14:03:10 -0500 X-Envelope-From: kkorreck@cfa.harvard.edu Received: from cfa.harvard.edu (cfa.harvard.edu [131.142.10.1]) by relay19.bu.edu (8.13.8/8.13.8) with ESMTP id kADJ5RKn022582 for ; Mon, 13 Nov 2006 14:05:27 -0500 Received: from cfa0 (cfa0 [131.142.24.30]) by cfa.harvard.edu (8.13.7/8.13.7/cfunix Mast-Sol 1.0) with ESMTP id kADJ5Rp3009120 for ; Mon, 13 Nov 2006 14:05:27 -0500 (EST) Date: Mon, 13 Nov 2006 14:05:27 -0500 (EST) From: Kelly Korreck To: siscoe Subject: Re: [Nessc] joint NESSC paper on universal processes In-Reply-To: <4554877C.4050901@bu.edu> Message-ID: References: <4554877C.4050901@bu.edu> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Score-Level: 0 Status: RO Hi George, I could be another possible solar author on 6 and possibily 3. I also volunteer my exo-solar perspective to write a paragraph for an intro or dicussion/conclusion/other work as to how to link the physics with stellar systems, AGN or jets. Kelly Korreck On Fri, 10 Nov 2006, siscoe wrote: > The following topics represent one way to parse the general subject into > bite-size portions: > > 3. Post-eruption processes sunward or earthward of the eruption site > (flares and auroras, particle heating/energization and injection into > closed-field-line volumes) > > 6. Particle acceleration at ICMEs and the terrestrial bow shock and at > flares and reconnection sites in the tail. > > 3a. Solar: John Raymond/Leon Golub > > 3b. Magnetosphere: Harlan Spence/Vania Jordanova > > 6a. Solar: Nathan Schwadron, Marty Lee/Steve Kahler/Ed Cliver > > 6b. Magnetosphere: Marty Lee >