Received: from MRK2.fjfi.cvut.cz (147.32.9.23) by MRK1.fjfi.cvut.cz (147.32.9.81) with Microsoft SMTP Server (TLS) id 14.3.123.3; Thu, 6 Jun 2013 12:11:24 +0200 Received: from BRK2.fjfi.cvut.cz (147.32.9.22) by MRK2.fjfi.cvut.cz (147.32.9.23) with Microsoft SMTP Server (TLS) id 14.3.123.3; Thu, 6 Jun 2013 12:11:24 +0200 Received: from mailgw1.fjfi.cvut.cz (147.32.9.3) by BRK2.fjfi.cvut.cz (147.32.9.22) with Microsoft SMTP Server (TLS) id 14.3.123.3; Thu, 6 Jun 2013 12:11:23 +0200 Received: from mailgw1.fjfi.cvut.cz (localhost [127.0.0.1]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) by mailgw1.fjfi.cvut.cz (Postfix) with ESMTPS id 609F0C0197 for ; Thu, 6 Jun 2013 12:11:24 +0200 (CEST) Received: from localhost (localhost [127.0.0.1]) by mailgw1.fjfi.cvut.cz (Postfix) with ESMTP id 5237AC0194 for ; Thu, 6 Jun 2013 12:11:24 +0200 (CEST) X-CTU-FNSPE-Virus-Scanned: amavisd-new at fjfi.cvut.cz X-CTU-FNSPE: this_is_mailgw_for_ctu_fnspe_header X-CTU-FNSPE-Helo: mail-qc0-f169.google.com X-CTU-FNSPE-Client-Address: 209.85.216.169 X-CTU-FNSPE-Client-Name: mail-qc0-f169.google.com X-CTU-FNSPE-Sender: markovic6453@gmail.com X-CTU-FNSPE-Recip: svoboda@fjfi.cvut.cz Authentication-Results: mailgw1.fjfi.cvut.cz (amavisd-new); dkim=pass (2048-bit key) header.d=gmail.com Received: from mailgw1.fjfi.cvut.cz ([127.0.0.1]) by localhost (mailgw1.fjfi.cvut.cz [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id f5lh4KymMMtz for ; Thu, 6 Jun 2013 12:11:22 +0200 (CEST) Received: from mail-qc0-f169.google.com (mail-qc0-f169.google.com [209.85.216.169]) (using TLSv1 with cipher RC4-SHA (128/128 bits)) (No client certificate requested) by mailgw1.fjfi.cvut.cz (Postfix) with ESMTPS id C3759C018B for ; Thu, 6 Jun 2013 12:11:20 +0200 (CEST) X-SenderID: Sendmail Sender-ID Filter v1.0.0 mailgw1.fjfi.cvut.cz C3759C018B Received: by mail-qc0-f169.google.com with SMTP id c10so1105757qcz.28 for ; Thu, 06 Jun 2013 03:11:19 -0700 (PDT) DKIM-Signature: v=1; a=rsa-sha256; c=relaxed/relaxed; d=gmail.com; s=20120113; h=mime-version:from:date:message-id:subject:to:cc:content-type; bh=3PQX8oZXvodz9PnzyuK6ULzP3Vrz9QxSqxedlGOC7hk=; b=b4ZBRhxxnfxG7I9fMHAx5gE2cZQdJeLsXQsj0EtUgXKhmphzcSnXr+2yWdHA89aTi6 5b5zMlS3q0rGT+Sgvh6O5AZkLyOpKt/jq8Rf6nxFUlmQ1cvyk+HWdWN/+ZYkrw7d4ZTX cItajykYcayjKI/T7+mSl9CsPUS+BKgj31LE8ePVH2TJqxb0mILIblVRyQicJwfmEhe4 B4InDXBp6niquD/Af8hDctWgJBV2FvPfdEUicwRSjk8d/wWDAHCt+4/lOMuPnLhdxQWv T7z8n1aezcb4ZvFbfk5N+t3gTgahU5O+d/Ba/bki4Kr5B8gcN7w/WvJhuv/ltSUJyay7 8lLQ== X-Received: by 10.49.24.198 with SMTP id w6mr38271348qef.58.1370513479335; Thu, 06 Jun 2013 03:11:19 -0700 (PDT) Received: by 10.49.62.229 with HTTP; Thu, 6 Jun 2013 03:10:59 -0700 (PDT) From: Tomas Markovic Date: Thu, 6 Jun 2013 12:10:59 +0200 Message-ID: Subject: Gomtraic -- new research opportunities To: =?ISO-8859-1?Q?Daniel_Hern=E1ndez_A=2E?= , Mauricio R , Frederik Ostyn CC: =?ISO-8859-1?Q?R=E9fy_D=E1niel?= , "Vojtech Svoboda" Content-Type: multipart/alternative; boundary="047d7b5d8e79188bf804de79896a" Return-Path: markovic6453@gmail.com X-MS-Exchange-Organization-PRD: gmail.com Received-SPF: Neutral (BRK2.fjfi.cvut.cz: 147.32.9.3 is neither permitted nor denied by domain of markovic6453@gmail.com) X-MS-Exchange-Organization-AVStamp-Mailbox: MSFTFF;1;0;0 0 0 X-MS-Exchange-Organization-SenderIdResult: NEUTRAL X-MS-Exchange-Organization-AuthSource: BRK2.fjfi.cvut.cz X-MS-Exchange-Organization-AuthAs: Anonymous MIME-Version: 1.0 --047d7b5d8e79188bf804de79896a Content-Type: text/plain; charset="ISO-8859-1" Hi guys, sorry for being out of reach for past few days (weeks) - I had final exam going on, which is now finally over :-) Meanwhile, there were some discussions about possiblities of new research on GOLEM with some senior physicists from IPP. These also included a joint experiment of magnetic diagnostics and probe diagnostics, in order to investigate poloidal rotation velocity changes during discharges. The main idea is basically the same as we discussed on Gomtraic meeting wile you were all here in Prague (by the way, tokamak was not affected by rent flood, despite being right next to river). Poloidal rotation is mainly E_r x B_phi drift. B_phi is known from magnetics and E_r is known from probe measurements, so v_theta can be calculated. This quantity can be also estimated by detection of magnetic islands using FFT and c-correlation. The question now stands, how much similar will be detected and "calculated" v_theta? Nobody knows for sure... v_theta detection is basically in your hands. You did not include v_theta measurements in your report yet, but it will be necessary to do it at some point, since it is required. You have most of what you need to do so, only little more work is necessary for obtaining v_theta -- the Gomtraic will now be less intensive anyways. Obtaining v_theta is now more in form of "research collaboration" and learning data processing techniques used on research institutes (i.e. learning to do your future work or to get better at it). I would like to help you now with this all -- of course once you are finished with assignments at your own universities. Let me please know how are you standing with this and when can you start. -- Regards, Tomas --047d7b5d8e79188bf804de79896a Content-Type: text/html; charset="ISO-8859-1" Content-Transfer-Encoding: quoted-printable
Hi guys,

sorry for being out of reac= h for past few days (weeks) - I had final exam going on, which is now final= ly over :-)

Meanwhile, there were some discussions= about possiblities of new research on GOLEM with some senior physicists fr= om IPP. These also included a joint experiment of magnetic diagnostics and = probe diagnostics, in order to investigate poloidal rotation velocity chang= es during discharges. The main idea is basically the same as we discussed o= n Gomtraic meeting wile you were all here in Prague (by the way, tokamak wa= s not affected by rent flood, despite being right next to river). Poloidal = rotation is mainly E_r x B_phi drift. B_phi is known from magnetics and E_r= is known from probe measurements, so v_theta can be calculated. This quant= ity can be also estimated by detection of magnetic islands using FFT and c-= correlation. The question now stands, how much similar will be detected and= "calculated" v_theta? Nobody knows for sure...

v_theta detection is basically in your hands= . You did not include v_theta measurements in your report yet, but it will = be necessary to do it at some point, since it is required. You have most of= what you need to do so, only little more work is necessary for obtaining v= _theta -- the Gomtraic will now be less intensive anyways. Obtaining v_thet= a is now more in form of "research collaboration" and learning da= ta processing techniques used on research institutes (i.e. learning to do y= our future work or to get better at it).

I would like to help you now with= this all -- of course once you are finished with assignments at your own u= niversities. Let me please know how are you standing with this and when can= you start.

-- 
Regards,
Tomas
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