From golub@head.cfa.harvard.edu Thu May 31 12:12:36 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=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.1.8 Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by auriga.ta3.sk (8.13.6/8.13.1) with ESMTP id l4VCBhL0019715 for ; Thu, 31 May 2007 12:12:34 GMT Received: from corona.cfa.harvard.edu (corona [131.142.41.245]) by head.cfa.harvard.edu (w/d) with ESMTP id l4VCBgid008806 for ; Thu, 31 May 2007 08:11:43 -0400 (EDT) From: Leon Golub Received: (from golub@localhost) by corona.cfa.harvard.edu (8.13.6/8.13.6) id l4VCBgF2010147 for choc@ta3.sk; Thu, 31 May 2007 08:11:42 -0400 (EDT) Date: Thu, 31 May 2007 08:11:42 -0400 (EDT) Message-Id: <200705311211.l4VCBgF2010147@corona.cfa.harvard.edu> To: choc@ta3.sk Subject: Re: Rybak - Hinode proposal 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 Status: ROr Dear Dr. Rybak, I will print out your pdf file and look it over. If I have any comments or see any problems, I'll let you know. I will also sen this to the other relevant team members. Sincerely, Leon Golub From llundquist@cfa.harvard.edu Tue Jul 31 03:43:58 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,HTML_MESSAGE autolearn=ham version=3.2.1 Received: from sprg-asmtp.ssl.berkeley.edu (sprg-asmtp.SSL.Berkeley.EDU [128.32.147.163]) by auriga.ta3.sk (8.13.6/8.13.6) with SMTP id l6V3h5Ka028238 for ; Tue, 31 Jul 2007 03:43:56 GMT Received: (qmail 2721 invoked from network); 30 Jul 2007 20:42:59 -0700 Received: from unknown (HELO ?133.74.8.102?) (loraine@133.74.8.102) by sprg-asmtp.ssl.berkeley.edu with SMTP; 30 Jul 2007 20:42:59 -0700 In-Reply-To: <8ec266b80707302038r34b4f6dfs5dadca5dc3c6884c@mail.gmail.com> References: <8ec266b80707302038r34b4f6dfs5dadca5dc3c6884c@mail.gmail.com> Mime-Version: 1.0 (Apple Message framework v752.3) Content-Type: multipart/alternative; boundary=Apple-Mail-25--759783914 Message-Id: Cc: sot_co@solar.isas.jaxa.jp, eis_co@solar.isas.jaxa.jp, "Dick Shine" , "Dawn Myers" , "Jan Rybak" From: Loraine Lundquist Subject: Re: HOP 24 quiet Sun prominence target & plan sot_co:xrt_co:eis_co: Date: Tue, 31 Jul 2007 12:42:09 +0900 To: xrt_co@solar.isas.jaxa.jp X-Mailer: Apple Mail (2.752.3) 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: RO --Apple-Mail-25--759783914 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Dear Gary, I'm afraid XRT requires a week-long CCD bakeout and will not be able to participate. regards, Loraine ------------------------------------------------------------ Loraine Lundquist, Ph.D. Harvard Smithsonian Center for Astrophysics 60 Garden St., MS-58, Cambridge, MA 02138 (+1) 617-496-7964 (US) (+81) 090-6569-9964 (Japan) llundquist@cfa.harvard.edu ------------------------------------------------------------ On Jul 31, 2007, at 12:38 PM, Gary Kilper wrote: > Hello Hinode COs, > > There is a quiescent filament to the southwest of AR 10965 at about > [300", -500"] (on 7/31, 02:00) that has formed slowly and looks to > have stabilized in some sections, with some variability and possible > small eruptions in other sections. > > Assuming that it does not completely disappear, it will be targeted > via JOP 188 by SOHO & TRACE from 8/3 17:00 until 8/5 07:00 (excluding > 07:00-13:30 UT on 8/4, when JOP 189 will be running). > > For HOP 24 with Hinode, I would like to get observations when this > filament is still on the disk, and then when it is over the limb. > Those times would be: > > Disk: > 8/2, 17:00-24:00 > > Limb: > 8/4, 13:30-24:00 > 8/5, 00:00-07:00 > 8/5, 13:30-24:00 > > Previously I had talked with the COs in person about what I wanted > from their instruments, but here it is in writing (the HOP description > will be updated with this later): > > SOT: > disk: FG slot 12, H lc, CaH, G-b 2Kx2K 2x2, 30s (which is ROI2) > disk (if buffer is too full): FG slot 3, H lc 30sec, CaH and Gb > 120sec, 2Kx2K 2x2, ROI2 > limb: FG slot 14, H-a 2 wave for DG, CaH2Kx2K 2x2, 30s > > EIS: > Nothing too specific: Use a standard observing plan for quiet Sun > filament observations for the disk or limb. The wavelength list > should include Fe XII (195.12 A), Fe XIII (202.04 A), He II (256.32 > A), Fe XIV (264.78 A), and Fe XV (284.16 A). Depending on the > situation (i.e. raster size and data rate), more wavelengths would be > useful to fill out the temperature range -- especially on the lower > end. > > XRT: > Aluminum poly, 512"x512" field-of-view, 30 sec cadence. > > > I'm sending this a day early so I can field any questions there might > be. Also, note that JOP 188 will be finishing on August 5th, but the > observing window for HOP 24 is open-ended and should be listed as a > Target of Opportunity for quiet Sun prominences. > > > Thanks everyone! > Gary --Apple-Mail-25--759783914 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1 Dear Gary,=A0

I'm afraid XRT requires a = week-long CCD bakeout and will not be able to = participate.=A0

regards,=A0
Loraine=

Loraine Lundquist, Ph.D.
Harvard Smithsonian Center for = Astrophysics
60 Garden St., MS-58, Cambridge, = MA 02138
(+1) 617-496-7964 (US)
(+81) 090-6569-9964 (Japan)
llundquist@cfa.harvard.edu<= /DIV>
On Jul 31, = 2007, at 12:38 PM, Gary Kilper wrote:

Hello Hinode COs,

There is a = quiescent filament to the southwest of AR 10965 at about
[300", -500"] (on 7/31, 02:00) that has formed = slowly and looks to
have stabilized in some = sections, with some variability and possible
small eruptions in other sections.

Assuming = that it does not completely disappear, it will be targeted
via JOP 188 by SOHO & TRACE from 8/3 17:00 until = 8/5 07:00 (excluding
07:00-13:30 UT on 8/4, when = JOP 189 will be running).

For HOP 24 with Hinode, I would = like to get observations when this
filament is = still on the disk, and then when it is over the limb.
Those times would be:

8/2, 17:00-24:00

8/4, 13:30-24:00
8/5, 00:00-07:00
8/5, = 13:30-24:00

Previously I had talked with the COs in person about = what I wanted
from their instruments, but here = it is in writing (the HOP description
will be = updated with this later):

SOT:
disk: FG slot 12, H lc, CaH, G-b 2Kx2K 2x2, 30s = (which is ROI2)
disk (if buffer is too full): FG = slot 3, H lc 30sec, CaH and Gb
120sec, 2Kx2K = 2x2, ROI2
limb: FG slot 14, H-a 2 wave for = DG, CaH2Kx2K 2x2, 30s
EIS:
Nothing too specific: Use a standard observing plan = for quiet Sun
filament observations for the = disk or limb.=A0 The = wavelength list
should include Fe XII (195.12 = A), Fe XIII (202.04 A), He II (256.32
A), Fe = XIV (264.78 A), and Fe XV (284.16 A).=A0 Depending on the
situation (i.e. raster size and data rate), more = wavelengths would be
useful to fill out the = temperature range -- especially on the lower
end.

XRT:
Aluminum poly, 512"x512" field-of-view, 30 sec = cadence.


I'm = sending this a day early so I can field any questions there = might
be.=A0 Also, note that JOP 188 will = be finishing on August 5th, but the
observing = window for HOP 24 is open-ended and should be listed as a
Target of Opportunity for quiet Sun = prominences.


Thanks = everyone!
Gary
=





=

= --Apple-Mail-25--759783914--