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168 18-Apr-2021 19:22 9 KB inetryconydot to previous
167 30-Oct-2016 22:20 9 KB JianSun to previous | to last
166 25-Jan-2010 14:11 9 KB JianSun to previous | to last
165 25-Jan-2010 14:10 9 KB JianSun to previous | to last
164 03-Dec-2008 11:25 9 KB JianSun to previous | to last
163 17-Nov-2008 19:50 9 KB Ignacio Ugarte-Urra to previous | to last Comment by Ignacio Ugarte-Urra
162 16-Jul-2008 06:14 8 KB David R Williams to previous | to last
161 16-Jul-2008 06:12 8 KB David R Williams to previous | to last

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At line 1 removed 2 lines
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
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This page lists several typical examples of EIS studies created for use under the new Hinode data-volume management scheme.
This page lists several typical examples of EIS studies created for use under %%(color:#cc0000;)the new Hinode data-volume management scheme%%, as well as information about %%(color:#cc0000;)operational restrictions%% and %%(color:#cc0000;)regular activities%% performed by EIS.
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If you want more general guidance about operational restrictions on observing with EIS using the new antenna, then just go over to our Wiki page on [Observing with EIS and the S-band Antenna|SbandObservingInfo].
For %%{color:#cc0000;)general information on observing with EIS using the new antenna%% go over to our Wiki page on [Observing with EIS and the S-band Antenna|SbandObservingInfo].
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There are now (* as of 2008 Jun 25) almost %%(color:green;)325%% pre-defined studies (including both science and so-called ''engineering'' studies) already available if you want to make observations with EIS.%% \\ \\
The details of each study, such as line list, window size, exposure time,
etc. can be accessed online at the [Hinode/EIS website|http://solarb.mssl.ucl.ac.uk/SolarB/] (MSSL). This is a very powerful tool where you can not only look up a Study by its ID number, but also immediately access all the FITS files created by that study. That way you can take a look at the real data and see whether it's appropriate to what you want to do!
\\ \\ Alternatively you can use the [EIS planning tool|http://sohowww.nascom.nasa.gov/solarsoft/hinode/eis/idl/planning/], which is distributed within [Solarsoft|http://www.mssl.ucl.ac.uk/surf/surfsolarsoft.html].
\\
\\
There are now[1] almost %%(color:green;)290%% stuies (including science & engineering task) available to EIS observation.%% \\ \\
The details of each study such as line list, winodw size, exposure time etc. can be accessed online at [Hinode/EIS website|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/] (MSSL), or \\ \\ alternatively you can use [EIS planning tool|http://sohowww.nascom.nasa.gov/solarsoft/hinode/eis/idl/planning/], which is distributed within [Solarsoft|http://www.mssl.ucl.ac.uk/surf/surfsolarsoft.html].
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To run the EIS Planning Tool, first ensure that you've followed the [guidelines for its set-up|http://solarb.mssl.ucl.ac.uk/SolarB/PlanningTool_v3.0.jsp].
To make sure that you're pointing at the official studies database (OSDB), first type
\\
{{{print,fix_zdbase(/eis)}}}
\\
The easiest thing to do is to look up a study the website. But to look up a study in SolarSoft just to use the command \\
{{{eis_xstudy}}}
\\
There, you can look at the details of the rasters (i.e. component parts that make up a study).
Go to [EisXstudy] for a walk-through on how to use this interface.
\\
=>  Checking EIS planning tool [user guides|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/docs/EISPlanningToolGuide_Draft.pdf].
%%  
[#1] as of 2008 Jun 25
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[Studies Available for EIS|http://solarb.mssl.ucl.ac.uk/SolarB/EisStudyList.jsp]\\
[{Image src='images/study/1227_d.png' link='http://solarb.mssl.ucl.ac.uk/SolarB/EisStudyList.jsp' width=180px height=180px}]
[Studies Available for EIS|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/EisStudyList.jsp]\\
[{Image src='images/study/1227_d.png' link='http://msslxr.mssl.ucl.ac.uk:8080/SolarB/EisStudyList.jsp' width=180px height=180px}]
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[EIS Study Use Summary|http://solarb.mssl.ucl.ac.uk/SolarB/studysummary.jsp]
[{Image src='images/study/1228_d.png' link='http://solarb.mssl.ucl.ac.uk/SolarB/studysummary.jsp' width=180px height=180px}]
[EIS Study Use Summary|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/studysummary.jsp]
[{Image src='images/study/1228_d.png' link='http://msslxr.mssl.ucl.ac.uk:8080/SolarB/studysummary.jsp' width=180px height=180px}]
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%%roundedCorners-yynn-F0F0E7-C0C0C0
__EIS Weekly Observing Summary__ is a guidance of EIS science observation, decided by EIS team. EIS planner will make observing plan based on this guidance for the incoming week. \\ \\ It is very usful if you'd like to check whether your proposal is on the schedule and when your observation will be run by EIS (roughly).
%%information
=>  You can click to access [EIS weekly observing summary|http://msslxr.mssl.ucl.ac.uk:8080/eiswiki/Wiki.jsp?page=EISWeeklyObservingSummary]
%%  
%%
%%roundedCorners-nnyy-dcdcdc-C0C0C0
 
%%
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This will give you a rough idea of the allocated EIS volume for a __three-day__ plan.
This will give you a roughly idea of EIS daily data volume.
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For FITS files obtained using this study, please visit [Studies Available for EIS|http://solarb.mssl.ucl.ac.uk/SolarB/EisStudyList.jsp] page and click the button on the right for #241
For obtained fits files by this study, please visit [Studies Available for EIS|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/EisStudyList.jsp] page and click right button for study #241
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For FITS files obtained using this study, please visit [Studies Available for EIS|http://solarb.mssl.ucl.ac.uk/SolarB/EisStudyList.jsp] page and click the button on the right for #251
For obtained fits files by this study, please visit [Studies Available for EIS|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/EisStudyList.jsp] page and click right button for study #251
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For FITS files obtained using this study, please visit [Studies Available for EIS|http://solarb.mssl.ucl.ac.uk/SolarB/EisStudyList.jsp] page and click the button on the right for study #286
For obtained fits files by this study, please visit [Studies Available for EIS|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/EisStudyList.jsp] page and click right button for study #286
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----
Here is a recommendation for a low telemetry slot imaging study.
As of today, the estimated data rate is 13 KBits/s. Notice that compression is Q65.
{{{
Study 000292:
ACRONYM: IUU_SLOT_136x400_Q65
Slot imaging. Low data rate. Four 15s exposures at adjacent pointing
positions sampling a 136"x400" FOV in around 90s (there's a 5 second
delay after each exposure). 8" overlapping scan (40" Slot, 32" FMIR step size).
Spectral windows are selected for their spectral purity, diagnosed from
previous 40" observations. JPEG65 compression.
TARGET : Active Region (AR)
EXPOSURE TIME : 15s (+5s exposure delay)
SLIT : 40"
FOV : 136"x400"
SPECTRAL WIND. : 9
COMPRESSION : JPEG65
ESTIMATED CADENCE : ~90s
ESTIMATED DURATION : ~15m 41s (10 repeats)
Data rate : 10.39 kBits/s
Data Volume (per hour) : 37.4 MBits/h
WARNING:
None
}}}
Here are two examples of expected performance for Active Region (on top) and Quiet Sun (bottom) targets. These are animated GIFs of just a few frames. Reload page if movies are not running. The Fe XXIII spectral window is a blend of several lines. That line in particular is only significant at very high temperatures.
[{Image src='Study4LowDataVolume/20081103_slotmovie.gif' align='left' }]
\\
[{Image src='Study4LowDataVolume/20081028_slotmovie.gif' align='left' }]
--[Ignacio Ugarte-Urra|http://null], 17-Nov-2008