From gomory@auriga.ta3.sk Wed Mar 28 06:47:55 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.1.8 (2007-02-13) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-4.5 required=5.0 tests=ALL_TRUSTED,AWL,BAYES_00, SPF_HELO_PASS autolearn=ham version=3.1.8 Received: from auriga.ta3.sk (localhost.localdomain [127.0.0.1]) by auriga.ta3.sk (8.13.6/8.13.1) with ESMTP id l2S6lrAL020242 for ; Wed, 28 Mar 2007 06:47:53 GMT Received: (from gomory@localhost) by auriga.ta3.sk (8.13.6/8.13.6/Submit) id l2S6lrtj020241 for choc; Wed, 28 Mar 2007 06:47:53 GMT From: Peter Gomory Message-Id: <200703280647.l2S6lrtj020241@auriga.ta3.sk> Subject: Re: [sot_co:00366] Details about program 25 for the SOHO+HINODE April 2007 campaign (sot_co:) (fwd) To: choc@auriga.ta3.sk (Jan Rybak) Date: Wed, 28 Mar 2007 06:47:53 +0000 (UTC) X-Mailer: ELM [version 2.5 PL6] MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Virus-Scanned: ClamAV version 0.90.1, clamav-milter version 0.90.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean Status: RO >From berger@lmsal.com Wed Mar 28 02:30:36 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.1.8 (2007-02-13) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=0.0 required=5.0 tests=none autolearn=failed version=3.1.8 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.1) with ESMTP id l2S2Tg6S030038 for ; Wed, 28 Mar 2007 02:30:33 GMT Received: from [198.116.7.148] (account berger HELO [192.168.1.104]) by lmsal.com (CommuniGate Pro SMTP 5.0.11) with ESMTPA id 6346280; Tue, 27 Mar 2007 19:29:41 -0700 In-Reply-To: <4609C632.5080306@nao.ac.jp> References: <7.0.0.16.2.20070221162248.04f7f0f0@nao.ac.jp> <4609C632.5080306@nao.ac.jp> Mime-Version: 1.0 (Apple Message framework v752.3) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <9FF1E156-988B-4B8F-8A14-260D310D6865@lmsal.com> Cc: sot_co@plain.isas.jaxa.jp Content-Transfer-Encoding: 7bit From: Thomas Berger Subject: Re: [sot_co:00366] Details about program 25 for the SOHO+HINODE April 2007 campaign (sot_co:) Date: Tue, 27 Mar 2007 19:28:18 -0700 To: gomory@astro.sk X-Mailer: Apple Mail (2.752.3) X-Virus-Scanned: ClamAV version 0.90.1, clamav-milter version 0.90.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean Peter, SOT is planning on supporting all of the SOHO/SUMER campaigns during April so consider your program scheduled in week 15. The exact times of observation will presumably be relayed sometime closer to week 15. Regarding your request for SOT observations, please note that the high cadence and FOV that you request can only be sustained for about an hour due to on-board memory and telemetry restrictions. So in an optimal 7 hour period we may be able to run two high-cadence programs of about 1 hour duration each but no more than that. The FOV you request will be a 1kx2k pixel readout resulting in an exact FOV of 54" x 109" - I trust you won't miss those extra 6 arcseconds. If you have any other requests for coordination with SOT please email either myself or Takashi Sekii, the SOT science scheduling coordinators. Cheers, Tom Berger berger@lmsal.com Takashi Sekii sekii@solar.mtk.nao.ac.jp On Mar 27, 2007, at 6:34 PM, Jan Jurcak wrote: > Hello, > > I am just forwarding the e-mail from Peter Gomory who had problems > with sending it directly to the sot_co. > > Regards, Jan > > ********************************************************************** > ********* > > Dear SOT planners, > > we have already applied for the observing time in a frame of the > joint observing campaign of the SOHO/SUMER and HINODE/EIS > spectrometers > following suggestion of the SUMER PI Werner Curdt. This program was > included to the SOHO+HINODE April 2007 campaign (program 25) > scheduled for week 15. > For our scientific goals it would be great if we can get also > support of the SOT instrument. > > Our main aim is to study upper parts of the solar atmosphere (i.e. > chromosphere, transition region and corona) in order to identify > the most probable physical mechanism responsible for the heating of > the solar corona localized particularly in/above chromospheric > network. The detailed scientific justification of our observing > program and the description of the SUMER and EIS observing details > can be found at http://www.mps.mpg.de/homes/curdt/hinode/ > HINODE_cases.html > (observing program nr. 25). > The main argument to try to acquire also SOT data for this program > is that the filtergrams taken in G-band and blue continuum should > enable us to analyze footpoints of the magnetic field > concentrations. These magnetic elements, visible as the > photospheric bright points concentrated in the network, are > considered to be the prime candidate for drivers of the coronal > heating mechanisms (Muller at al., A&A 283, 232). > Moreover, time series of the SOT filtergrams taken in the Ca II H > spectral line will provide additional information about behaviour > of waves in the chromosphere and they will allow better > identification of the coronal heating mechanism. > > Therefore, SOT measurements will definitely improve the quality and > complexity of our observing campaign. We add here technical details > for > possible SOT support of our program. > SOT observing details (Broad Filter Imager): > -------------------------------------------- > - FOV: 60" x 109" > - spectral channels: G-band, Ca II H, blue continuum > (sequentially in time if > possible, if only one channel could be > selected then G-band channel is preferred) > - cadence of a set of these 3 channels: 10-15 sec > - total run duration: minimum: ~3.5 hours > optimum: ~7.0 hours > - no compensation of the solar rotation > - target: quiet Sun near disk center with the SUMER 1D slit in the > center > of the SOT FOV > - pointing: specified via e-mail a day in advance > > We would be very obliged if the SOT will be able to support > our program with this type of observations. Therefore we > would be obliged to hear from you whether this is realistic > in frame of the SOHO+HINODE campaign scheduled for April > 2007 (week 15 in our case). > > With best wishes and many thanks beforehand > > Peter Gomory, coordinator of the SOHO/HINODE April 2007 program 25 > > Tatranska Lomnica, 26/03/2007 > > ********************************************************************** > **** > * Peter Gomory tel. : ++421 52 7879 166 (111 > secretary) * > * Astronomical Institute fax : ++421 52 4467 > 656 * > * Slovak Academy of Sciences email : > gomory@astro.sk * > * 05960 Tatranska Lomnica WWW : http://www.astro.sk/ > ~gomory * > * Slovak > Republic * > ********************************************************************** > **** > > From berger@lmsal.com Tue May 22 19:10:23 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.1.8 (2007-02-13) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.1.8 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.1) with ESMTP id l4MJ9U40029441 for ; Tue, 22 May 2007 19:10:21 GMT Received: from [71.198.96.163] (account berger HELO [192.168.1.74]) by lmsal.com (CommuniGate Pro SMTP 5.0.11) with ESMTPA id 6680513 for choc@ta3.sk; Tue, 22 May 2007 12:09:27 -0700 Mime-Version: 1.0 (Apple Message framework v752.3) In-Reply-To: <200705221223.l4MCNDTx022289@auriga.ta3.sk> References: <200705221223.l4MCNDTx022289@auriga.ta3.sk> Content-Type: multipart/mixed; boundary=Apple-Mail-9--309785633 Message-Id: From: Thomas Berger Subject: Re: SOT: request for suggestions Date: Tue, 22 May 2007 12:07:57 -0700 To: Jan Rybak X-Mailer: Apple Mail (2.752.3) X-Virus-Scanned: ClamAV version 0.90.2, clamav-milter version 0.90.2 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 8 Status: ROr --Apple-Mail-9--309785633 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Dear Jan, Your calculations are basically correct - it is difficult to run the SOT in uncompressed mode due to data rate restrictions. Instead, we have been running with 2-3 bit JPEG compression with very good results. This allows a 1k x 2k FOV at 1x1 pixel resolution (ie. unsummed camera output) to run at 60 seconds cadence for several hours. Perhaps not as long as five hours as that depends somewhat on the telemetry pass schedule. Also, if you can tolerate 2x2 summing (0.108" pixels in the BFI) you can definitely get 5 hours of uninterrupted observations at 1k x 2k FOV. Actually in this case we'd probably run a 2k x 2k FOV that would produce 1k x 1k images of the 109" x 109" FOV. SOT has in the past provided multi-hour continuous stretches of observations for coordinated observing, although at present we are in eclipse season and the longest uninterrupted observations are only about an hour. By August we'll be out of eclipse though and we should be able to accommodate your request. The next step is for you to submit a proposal to me which I will present to the Science Scheduling Coordinators meeting in June. Your proposal should include a brief science justification followed by specific observing requirements for the Hinode instruments. I've attached a Latex template for making Hinode observing proposals. This is only a guideline so feel free to develop your own proposal outline if this one doesn't fit. Cheers, Tom --Apple-Mail-9--309785633 Content-Transfer-Encoding: 7bit Content-Type: application/octet-stream; x-unix-mode=0644; x-mac-creator=454D4178; name=sample_observing_proposal.tex Content-Disposition: attachment; filename=sample_observing_proposal.tex \documentclass[11pt]{article} \begin{document} \title{Proposal for Hinode/XXX Joint Observing Campaign} \author{J. O. E. Observer} \maketitle \section{Science objectives} \section{Campaign Outline} \subsection{Dates and Times} \subsection{Participating Instruments} \subsection{Observing Program} \subsubsection{Targeting} \subsubsection{Duration} \subsubsection{Hinode Observations} \begin{enumerate} \item{SOT} \begin{itemize} \item BFI \item NFI \item SP \end{itemize} \item{XRT} \item{EIS} \end{enumerate} \subsubsection{XXX Observations} \subsubsection{Data Analysis Requirements} \end{document} --Apple-Mail-9--309785633 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On May 22, 2007, at 5:23 AM, Jan Rybak wrote: > > > Dear Dr. Berger, > > I apologize for my disturbing you for a moment but I would like to ask > you some questions as the SOT SSC. > > Our group was granted by the DOT/LaPalma observing time in August 2007 > (campaign web page with the proposal text is available at > http://www.astro.sk/~choc/open/07_dot/07_dot.html). > > We have already prepared and submitted a SOHO JOP proposal but it is > clear that after Aug 17 there will be no SOHO support available due to > the SOHO keyhole limitations. > > Therefore, we work currently on a proposal for Hinode/EIS+SOT+XRT > support > of our g-b observations (or vice versa) for which we would like to > apply > (observing time since Aug 18). > > Concerning the SOT part I would like to ask the following questions > in advance. > Our idea is to operate SOT for few hours taking series of exposures > like > > - channels: BFI: G-band, Ca II H; NFI Fe I 630.25nm longitudinal > magnetograms > - FOV: 1k x 2k (54" x 109") > - 12bit DPCM lossless data compression > - cadence: ~20s per filtergram (~60s per the sequence) > - time of day : 08:00-13:00 UT > > Using data given at the SOT web page it seems that such program > would provide > ~800 kbps what is much more than the average data rate of only > 300kbps. > This leads to just ~7000s of observations for one run. > > Questions: - is this calculation correct? > - can be the sequence (G-band, Ca II H, Fe I 630.25nm > long. magnetograms) > performed for several hours in such a run > - is an alternative of ~3 bits/pixel the JPEG algorithm > reasonable > (it gives ~5hours we in fact need) or is it really to > much > - is it possible to ask for such time of runs - 5hours > of data acqusition > + downlik after it > > You surely understand that we would like to keep all Hinode > instruments observing > for the mentioned interval when we can expect better seeing > conditions at LaPalma. > On the other hand we do not want to decrease cadence of filtergrams > or number > of the selected channels. Therefore we would like to know your > advice how to > handle this problem in an optimum way if possible. > > With many thanks beforehand > > Jan Rybak > > TL, 22/5/07 > > ********************************************************************** > **** > * Jan Rybak tel. : ++421 52 7879 156 (111 > secretary) * > * Astronomical Institute fax : ++421 52 4467 > 656 * > * Slovak Academy of Sciences email : > choc@astro.sk * > * 05960 Tatranska Lomnica WWW : http://www.astro.sk/ > ~choc * > * Slovak > Republic * > ********************************************************************** > **** > --Apple-Mail-9--309785633-- From berger@lmsal.com Mon Jun 4 20:27:19 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.1.8 (2007-02-13) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.1.8 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.1) with ESMTP id l54KQQZ1029173 for ; Mon, 4 Jun 2007 20:27:17 GMT Received: from [198.116.7.226] (account berger [198.116.7.226] verified) by lmsal.com (CommuniGate Pro SMTP 5.0.11) with ESMTPA id 6754509 for choc@ta3.sk; Mon, 04 Jun 2007 13:26:25 -0700 Mime-Version: 1.0 (Apple Message framework v752.2) In-Reply-To: <200705311119.l4VBJqmO016941@auriga.ta3.sk> References: <200705311119.l4VBJqmO016941@auriga.ta3.sk> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: Tom Berger Subject: Re: Rybak - SOT proposal Date: Mon, 4 Jun 2007 13:34:15 -0700 To: Jan Rybak X-Mailer: Apple Mail (2.752.2) X-Virus-Scanned: ClamAV version 0.90.3, clamav-milter version 0.90.3 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 45 Status: ROr Jan, Thank you for submitting the proposal. It will be discussed during the June SSC meeting. We will strive to schedule your request during the period of something like 15-31 August. I must remind you that in the case of a major flaring active region on the disk, SOT reserves the right to forgo any quiet Sun/network observations that may have been previously scheduled. But other than that restriction, we should be able to coordinate with the DOT during the above dates. Cheers, Tom On May 31, 2007, at 4:19 AM, Jan Rybak wrote: > > Dear Dr. Berger, > > many thanks for your previous answer helping me to prepare the SOT > part of our > Hinode proposal. > > Finally our proposal is ready. I send to you the PDF file of our > proposal > and the simple summary of the SOT requirements we have specified in > the proposal. > > I will send the corresponding information also to other SSCs (EIS - > Dr. Cilhane, > XRT - Dr. Golub), and to the CC J. Davis. > > I hope the enclosed files will give you all relevant information > you need > to consider our application. In case of any question please contact > me via email > (choc@astro.sk). > > We ask for almost 2 weeks of the Hinode support during morning UT > time when > seeing conditions for DOT at La Palma are the most favorable. We > understand that > there are many other applications appearing so we probably will get > much less > that we ask for. Nevertheless we hope you and your colleagues will > find our proposal > interesting and we will get some Hinode support. It is especially > crucial > for us after Aug 17 when SOHO keyhole start and therefore there is > no change > to get CDS or MDI support. > > With many thanks beforehand > > Jan Rybak > > TL, 31/5/07 > > PS: web page of our DOT campaign + SOHO JOP 189: > http://www.astro.sk/~choc/open/07_dot/07_dot.html > > ********************************************************************** > **** > * Jan Rybak tel. : ++421 52 7879 156 (111 > secretary) * > * Astronomical Institute fax : ++421 52 4467 > 656 * > * Slovak Academy of Sciences email : > choc@astro.sk * > * 05960 Tatranska Lomnica WWW : http://www.astro.sk/ > ~choc * > * Slovak > Republic * > ********************************************************************** > **** > > From tarbell@lmsal.com Mon Aug 6 07:41:38 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l767ee0C031955 for ; Mon, 6 Aug 2007 07:41:31 GMT Received: from [133.74.8.195] (account tarbell@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7282956; Mon, 06 Aug 2007 00:40:39 -0700 From: "Ted Tarbell" Subject: Re: [sot_co:01690] sot_co: request for target information To: sot_co@solar.isas.jaxa.jp, choc@auriga.ta3.sk (Jan Rybak), gomory@astro.sk (Peter Gomory), asv@IGAM06WS.kfunigraz.ac.at (Astrid Veronig), manuela.temmer@uni-graz.at (Manuela Temmer), sigrid.stoiser@stud.uni-graz.at (Sigrid Stoiser) X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Mon, 06 Aug 2007 00:40:39 -0700 Message-ID: In-Reply-To: <200708060658.l766whHS029477@auriga.ta3.sk> References: <200708060658.l766whHS029477@auriga.ta3.sk> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean Status: ROr Hello, Actually there is a web page which has the Hinode pointing (which is the center of the SOT FOV) as soon as it decided in the daily meeting. See the Hinode Daily Events page at, for example: http://www.isas.jaxa.jp/home/solar/hinode_op/hinode_daily_events.php?date=20070806 Every day except Sunday, the bottom of this page has a link to the pointing file, if the pointing has been selected yet. Today's file is: http://www.isas.jaxa.jp/home/solar/hinode_op/cmdpln/20070806/re-point_200708068000.txt In this file, the column of coordinates below "/* Memory upload :" show the pointing coordinates at the start of each pointing. If the tracking number is 0, then pointing is fixed at these coordinates; if it is 1-4, then the pointing will continuously follow solar rotation. You can also find a pointing file now for Tuesday 20070807. These coordinates were chosen this morning, but they may be modified in the daily meeting Tu morning at 01:30 UT. Usually any such last minute modifications are fine tuning in the same target region. Each pointing file ends with 24 hours pointing at disk center called the backup plan; ignore this, it will only take effect if the next day's plan can't be uplinked for some reason. Good luck, Ted Tarbell On Mon, 6 Aug 2007 06:58:43 +0000 (UTC) Jan Rybak wrote: > > Dear SOT Chief Observer, > > I apologize for disturbing you for a moment. > > Currently, I am a leader of the currently running SOHO JOP189 with >support of the TRACE, > DOT/LaPalma and other istruments. > > I would like to ask just to inform me (as soon as possible) when >SOT/Hinode decision is made > about the actual pointing of Hinode for individual days of this >week. Or is only the web page > http://solar-b.nao.ac.jp/operation_e/thisweek_e/ the latest >information available? > > My contact is: rybak@astro.sk > > Your cooperation would help us very much to coordinate our >observations using the DOT, TRACE, > SOHO/CDS,MDI with the Hinode data acquisition. > > With best wishes and many thanks for your answer beforehand > > Jan Rybak, on behalf of the JOP189 team > > TL, 07/08/2007 > > ************************************************************************** > * Jan Rybak tel. : ++421 52 7879 156 (111 >secretary) * > * Astronomical Institute fax : ++421 52 4467 656 > * > * Slovak Academy of Sciences email : choc@astro.sk > * > * 05960 Tatranska Lomnica WWW : http://www.astro.sk/~choc > * > * Slovak Republic > * > ************************************************************************** > Dr. Ted Tarbell tarbell@lmsal.com Lockheed Martin Solar & Astrophysics Laboratory phone: (650) 424-4033 fax: (650) 424-3994 From zoe@lmsal.com Wed Aug 15 00:56:45 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7F0tg0r004807 for ; Wed, 15 Aug 2007 00:56:33 GMT Received: from [133.74.8.198] (account zoe@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7366959; Tue, 14 Aug 2007 17:55:41 -0700 From: "Zoe Frank" Subject: sot_co: JOP 189 / HOP 20 To: Sigrid Stoiser , choc@ta3.sk Cc: sot Chief Observer X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Tue, 14 Aug 2007 17:55:41 -0700 Message-ID: In-Reply-To: <46C19426.8030007@stud.uni-graz.at> References: <46C19426.8030007@stud.uni-graz.at> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 102 Status: RO Dear Sigrid and Jan, I am one of the Hinode SOT Chief Observers during your upcoming HOP 20 campaign and I wanted to confirm with you that we will support HOP 20 starting with observations on Saturday, 8/18. The SOT observations you requested were for Ca H, Gband, and 6302 magnetograms, 2Kx2K field of view (~109"x109"), binned 2x2 (to 1kx1k final size) at 30 second cadence per wavelength (10 sec between images). We will try to accomodate this but may have to increase the cadence depending on telemetry restrictions. Please send your targeting information to sot_co@solar.isas.jaxa.jp (include "sot_co:" in the subject line, as in this message). We will need both Saturday and Sunday target pointing before 10 AM JST (01:00 UT) Friday. We wish you continued success with this campaign. Yours, Zoe ======================================================== Zoe Frank Lockheed Martin ATC, O/ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com ======================================================== From sigrid.stoiser@stud.uni-graz.at Wed Aug 15 12:34:43 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=AWL,BAYES_00 autolearn=ham version=3.2.1 Received: from neto.uni-graz.at (NETO.KFUNIGRAZ.AC.AT [143.50.13.43]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7FCXjL1014052 for ; Wed, 15 Aug 2007 12:34:35 GMT Received: from localhost (unknown [127.0.0.1]) by neto.uni-graz.at (Postfix) with ESMTP id 58EBB8002B1 for ; Wed, 15 Aug 2007 12:33:45 +0000 (UTC) X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) Received: from neto.uni-graz.at ([127.0.0.1]) by localhost (neto.uni-graz.at [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id bQJzBoujPFSe for ; Wed, 15 Aug 2007 14:33:44 +0200 (CEST) Received: from [143.50.39.118] (IGAM12DD.KFUNIGRAZ.AC.AT [143.50.39.118]) by neto.uni-graz.at (Postfix) with ESMTP id D4D248002B0 for ; Wed, 15 Aug 2007 14:33:44 +0200 (CEST) Message-ID: <46C2F505.7000701@stud.uni-graz.at> Date: Wed, 15 Aug 2007 14:43:49 +0200 From: Sigrid Stoiser User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.7.12) Gecko/20050915 X-Accept-Language: en-us, en MIME-Version: 1.0 To: dot_jop189_hop020@astro.sk Subject: [Fwd: Re: sot_co: JOP 189 / HOP 20] Content-Type: multipart/mixed; boundary="------------020602080009090809030903" X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 114 Status: RO This is a multi-part message in MIME format. --------------020602080009090809030903 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit --------------020602080009090809030903 Content-Type: message/rfc822; name="Re: sot_co: JOP 189 / HOP 20" Content-Transfer-Encoding: 7bit Content-Disposition: inline; filename="Re: sot_co: JOP 189 / HOP 20" Return-Path: Received: from murder (neto0 [10.0.13.43]) by andarta0 (Cyrus v2.2.12-Invoca-RPM-2.2.12-8.1.RHEL4) with LMTPA; Wed, 15 Aug 2007 14:31:31 +0200 X-Sieve: CMU Sieve 2.2 Received: from neto.uni-graz.at ([unix socket]) by neto.uni-graz.at (Cyrus v2.2.12-Invoca-RPM-2.2.12-8.1.RHEL4) with LMTPA; Wed, 15 Aug 2007 14:31:31 +0200 Received: from localhost (unknown [127.0.0.1]) by neto.uni-graz.at (Postfix) with ESMTP id 5EB338002B0 for ; Wed, 15 Aug 2007 12:31:31 +0000 (UTC) X-Virus-Scanned: amavisd-new at edu.uni-graz.at Received: from neto.uni-graz.at ([127.0.0.1]) by localhost (neto.uni-graz.at [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id zu5kaJBh2tJI for ; Wed, 15 Aug 2007 14:31:30 +0200 (CEST) Received: from mbug18.uni-graz.at (MBUG18.KFUNIGRAZ.AC.AT [143.50.5.18]) by neto.uni-graz.at (Postfix) with ESMTP id 2CE438002A2 for ; Wed, 15 Aug 2007 14:31:30 +0200 (CEST) Received: from mbug18.uni-graz.at (unknown [127.0.0.1]) by mbug18.uni-graz.at (Symantec Mail Security) with ESMTP id 1229F702B54 for ; Wed, 15 Aug 2007 14:31:30 +0200 (CEST) X-AuditID: 8f320512-a25ebbb000001932-39-46c2f221e5c1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by mbug18.uni-graz.at (Symantec Mail Security) with ESMTP id 7566E5B000B for ; Wed, 15 Aug 2007 14:31:29 +0200 (CEST) Received: from [220.212.54.108] (account zoe@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7371414 for sigrid.stoiser@stud.uni-graz.at; Wed, 15 Aug 2007 05:31:28 -0700 From: "Zoe Frank" Subject: Re: sot_co: JOP 189 / HOP 20 To: Sigrid Stoiser X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Wed, 15 Aug 2007 05:31:28 -0700 Message-ID: In-Reply-To: <46C2D39B.9090006@stud.uni-graz.at> References: <46C19426.8030007@stud.uni-graz.at> <46C2D39B.9090006@stud.uni-graz.at> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Brightmail-Tracker: AAAAAA== Dear Sigird, We would like Monday's pointing information on Saturday, if possible. People in Japan take Sunday's rest very seriously. During the week, we construct our observing plans the day before observations. There are no spacecraft uploads on Sunday, though, so we plan for two days (Sat & Sun) on Friday and one day (Mon) on Saturday. I hope this helps and is not too confusing. Yours, Zoe On Wed, 15 Aug 2007 12:21:15 +0200 Sigrid Stoiser wrote: > > Dear Zoe, > > thank you very much for your confirmation. We are already excited >about the start of the Hinode campaign! > > The SOT observations for our HOP020 which you listed in your email >are exactly those we would like to have. As requested, we will send >our target for Saturday 18/08/07 and Sunday 19/08/07 well before the >deadline on Friday at 01:00 UT. > > The only open question for me is by which time you need the target >info for Monday 20/08. Do you have to know on Friday (as is the case >for the TRACE and CDS instrument) or is it sufficient to send the >pointing coordinates on Sunday 19/08/07? > > Kind regards, > > Sigrid (dot_jop189_hop020@astro.sk) > > Zoe Frank wrote: > >> Dear Sigrid and Jan, >> >> I am one of the Hinode SOT Chief Observers during your upcoming HOP >>20 >> campaign and I wanted to confirm with you that we will support HOP >>20 >> starting with observations on Saturday, 8/18. >> >> The SOT observations you requested were for Ca H, Gband, and 6302 >> magnetograms, 2Kx2K field of view (~109"x109"), binned 2x2 (to 1kx1k >> final size) at 30 second cadence per wavelength (10 sec between >> images). We will try to accomodate this but may have to increase the >> cadence depending on telemetry restrictions. >> >> Please send your targeting information to sot_co@solar.isas.jaxa.jp >> (include "sot_co:" in the subject line, as in this message). We >>will >> need both Saturday and Sunday target pointing before 10 AM JST >>(01:00 >> UT) Friday. >> >> We wish you continued success with this campaign. >> >> Yours, >> Zoe >> >> ======================================================== >> Zoe Frank >> Lockheed Martin ATC, O/ADBS, Bldg 252 >> 3251 Hanover St., Palo Alto, CA 94304 >> ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com >> ======================================================== >> > =========================================================== Zoe Frank Lockheed Martin ATC, O/ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com =========================================================== --------------020602080009090809030903-- From zoe@lmsal.com Thu Aug 16 07:53:19 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7G7qICq029293 for ; Thu, 16 Aug 2007 07:53:09 GMT Received: from [133.74.8.198] (account zoe@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7378379; Thu, 16 Aug 2007 00:52:17 -0700 From: "Zoe Frank" Subject: sot_co: JOP 189 / HOP 20 targeting To: Sigrid Stoiser Cc: dot_jop189_hop020@astro.sk, sot_co@solar.isas.jaxa.jp X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Thu, 16 Aug 2007 00:52:17 -0700 Message-ID: In-Reply-To: <46C2D39B.9090006@stud.uni-graz.at> References: <46C19426.8030007@stud.uni-graz.at> <46C2D39B.9090006@stud.uni-graz.at> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 137 Status: RO Dear Sigrid, During the upcoming HOP 20 campaign, we would like to offset your target by a fixed amount (10 arcsec) in our SOT field of view to better position it on our CCD. Would this be acceptable to you? For the SOT team, Zoe =========================================================== Zoe Frank Lockheed Martin ATC, O/ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com =========================================================== From zoe@lmsal.com Thu Aug 16 10:19:07 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7GAI8LY007330 for ; Thu, 16 Aug 2007 10:18:59 GMT Received: from [133.74.8.198] (account zoe@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7379252; Thu, 16 Aug 2007 03:18:08 -0700 From: "Zoe Frank" Subject: Re: sot_co: JOP 189 / HOP 20 targeting To: asv@IGAM06WS.uni-graz.at Cc: dot_jop189_hop020@astro.sk, sot_co@solar.isas.jaxa.jp X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Thu, 16 Aug 2007 03:18:08 -0700 Message-ID: In-Reply-To: <1187252280.46c408381e791@igam01ws.kfunigraz.ac.at> References: <46C19426.8030007@stud.uni-graz.at> <46C2D39B.9090006@stud.uni-graz.at> <1187252280.46c408381e791@igam01ws.kfunigraz.ac.at> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 146 Status: RO Hi Astrid, I'm very sorry. I meant when you do provide pointing information, we would like to shift the image on our CCD. It's an internal shift but it is something you should be aware of for accurate alignment of data from several instuments. However, I made an error in timing. Please send your pointing information to us *two* days before your observations (not the day before). Hinode's observing day starts at 11 UT. Infomation we have by 1 UT on the 17th can be included in the observations starting at 11 UT on the 18th. So, please send your pointing information for both 8/18 and 8/19 by 01:00 UT. Yours, Zoe On Thu, 16 Aug 2007 10:18:00 +0200 asv@IGAM06WS.uni-graz.at wrote: > Dear Zoe, > > I took over the HOP20 coordination from Sigrid. > > As regards your sugggested target offset: I am a little confused. >Our HOP20 > campaign starts 18/8 (and will run until 23/8), and we have not yet >specified a > target but will send our first target info, following your >discussion with > Sigrid, until Fr 17/8 01 UT latest. Did I misunderstand something? > > Best regards, > Astrid > for the HOP20 team > > >> Dear Sigrid, >> >> During the upcoming HOP 20 campaign, we would like to offset your >> target by a fixed amount (10 arcsec) in our SOT field of view to >> better position it on our CCD. Would this be acceptable to you? >> >> For the SOT team, >> Zoe >> >> =========================================================== >> Zoe Frank >> Lockheed Martin ATC, O/ADBS, Bldg 252 >> 3251 Hanover St., Palo Alto, CA 94304 >> ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com >> =========================================================== >> > > > > (IGAM/UG) > ------------------------------------------------- > This mail sent through IMP: http://horde.org/imp/ =========================================================== Zoe Frank Lockheed Martin ATC, O/ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com =========================================================== From zoe@lmsal.com Fri Aug 17 09:32:45 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=AWL,BAYES_00 autolearn=ham version=3.2.1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7H9VkkN021219 for ; Fri, 17 Aug 2007 09:32:37 GMT Received: from [133.74.8.198] (account zoe@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7389816; Fri, 17 Aug 2007 02:31:45 -0700 From: "Zoe Frank" Subject: sot_co: HOP 20 coordination To: asv@IGAM06WS.uni-graz.at Cc: dot_jop189_hop020@astro.sk, sot_co@solar.isas.jaxa.jp X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Fri, 17 Aug 2007 02:31:45 -0700 Message-ID: In-Reply-To: <1187252280.46c408381e791@igam01ws.kfunigraz.ac.at> References: <46C19426.8030007@stud.uni-graz.at> <46C2D39B.9090006@stud.uni-graz.at> <1187252280.46c408381e791@igam01ws.kfunigraz.ac.at> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 177 Status: RO Hi Astrid, I have one more request. Please email targeting to the sot_co@solar.isas.jaxa.jp address (adding sot_co: in the subject line, as well) during the HOP 20 campaign. Also, note that the field of view for your data will be centered 10 arcsec west of disk center and the best cadence we could get in our telemetry was 35 seconds. I hope this will work for your team. Yours, Zoe =========================================================== Zoe Frank Lockheed Martin ATC, O/ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com =========================================================== From zoe@lmsal.com Fri Aug 17 23:14:44 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7HNDiJa003569 for ; Fri, 17 Aug 2007 23:14:34 GMT Received: from [133.74.8.198] (account zoe@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7394835; Fri, 17 Aug 2007 16:13:42 -0700 From: "Zoe Frank" Subject: Re: [sot_co:01800] sot_co: To: sot_co@solar.isas.jaxa.jp, asv@IGAM06WS.uni-graz Cc: dot_jop189_hop020@astro.sk X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Fri, 17 Aug 2007 16:13:42 -0700 Message-ID: In-Reply-To: <1187361557.46c5b3150bbe2@igam01ws.kfunigraz.ac.at> References: <46C19426.8030007@stud.uni-graz.at> <46C2D39B.9090006@stud.uni-graz.at> <1187252280.46c408381e791@igam01ws.kfunigraz.ac.at> <1187346914.46c579e2735b9@igam01ws.kfunigraz.ac.at> <1187361557.46c5b3150bbe2@igam01ws.kfunigraz.ac.at> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 201 Status: RO Hi Astrid, See comments below: On Fri, 17 Aug 2007 16:39:17 +0200 asv@IGAM06WS.uni-graz.at wrote: > Hi Zoe, > > here is our HOP20 pointing for Monday and Tuesday, where we would >like to follow > first QS at disk center and then the decaying AR/magnetic flux >concentration for > our microflare study. > > Monday 20/8, 7:00-10:40 UT: (x,y) = (0, 0) , no tracking > Monday 20/8, 10:40-13:30 UT: (x,y) = (+70, -240) , no tracking > Tuesday 21/8, 7:00-10:40 UT: (x,y) = (+260, -240) , no tracking Understood. > > These pointings are the same ones we sent to the EIS team. The >"10:40" time > refers to the beginning of a new Hinode observing day, and should be >adjusted to > its exact time (I think it's exact time is changing a bit from day >to day?) Yes, and the chief planner can adjust for it. > > The pointing for the Tuesday 21/8 10:40-13:30 and Wednesday 22/8 >07:00-10:40 > period I will send to you by Monday 20/8, 1 UT. As I understood from >your email, > this will be early enough. > > Please let me know if this is all ok. This is perfect. Thanks for your patience and good luck with your observing. Yours, Zoe ======================================================== Zoe Frank Lockheed Martin ATC, O/ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com ======================================================== From zoe@lmsal.com Fri Aug 17 23:46:16 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=AWL,BAYES_00 autolearn=ham version=3.2.1 Received: from lmsal.com (mail.lmsal.com [198.116.7.6]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7HNjGpG005158 for ; Fri, 17 Aug 2007 23:46:07 GMT Received: from [133.74.8.198] (account zoe@lmsal.com) by lmsal.com (CommuniGate Pro WEBUSER 5.1.10) with HTTP id 7395040; Fri, 17 Aug 2007 16:45:16 -0700 From: "Zoe Frank" Subject: Re: [sot_co:01799] Re: sot_co: HOP 20 coordination To: sot_co@solar.isas.jaxa.jp, asv@IGAM06WS.uni-graz.at Cc: dot_jop189_hop020@astro.sk X-Mailer: CommuniGate Pro WebUser v5.1.10 Date: Fri, 17 Aug 2007 16:45:16 -0700 Message-ID: In-Reply-To: <1187346914.46c579e2735b9@igam01ws.kfunigraz.ac.at> References: <46C19426.8030007@stud.uni-graz.at> <46C2D39B.9090006@stud.uni-graz.at> <1187252280.46c408381e791@igam01ws.kfunigraz.ac.at> <1187346914.46c579e2735b9@igam01ws.kfunigraz.ac.at> MIME-Version: 1.0 Content-Type: text/plain;charset=utf-8;format="flowed" Content-Transfer-Encoding: 8bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 202 Status: RO Hi Astrid, Regarding your question below, yes, all three Hinode instruments plan observations on the same schedule. In the observations we have running over the weekend, EIS and SOT are co-pointed but the the center of the 109"x109" SOT images will be 10" west of the EIS FOV center. The *.gif files at https://sot.lmsal.com/operations/timeline/ is a good graphical representation of our daily plans, including pointing. There are other details about the observations there, too. Hope this helps, Zoe On Fri, 17 Aug 2007 12:35:14 +0200 asv@IGAM06WS.uni-graz.at wrote: > I have another question regarding the planning: The Hinode/EIS team >splits the > plannning/pointing for our campaign since our obs. period spans over >2 Hinode > obs. days. Of course we want to combine EIS and SOT in our campaign, >so the > question is whether it is possible to split the SOT >planning/pointing > accordingly into > a) 7:00 until approx 11 UT, and > b) approx 11 UT until 13:30 UT. =========================================================== Zoe Frank Lockheed Martin ATC, O/ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 ph:(650)424-4009, fx:(650)424-3994, em: zoe@lmsal.com ===========================================================