5 th SECCHI Consortium Meeting Orsay, France March 5-8, 2007 SECCHI Planning and Scheduling Ed Esfandiari NRL/Interferometrics, Inc.

Slides:



Advertisements
Similar presentations
Medicaid Alternative Benefit Plans (ABP) Processing
Advertisements

SECCHI Flight Software Dennis Wang SECCHI Consortium Meeting July RAL CPU Utilization Memory Usage VxWorks H/W.
© 2010 MediaMind Technologies Inc. | All rights reserved Shelley Hen| Solution Specialist January Buying Module.
Commentary on Validating Resource Usage in Least Commitment Planning Authors: Nazma Ferdous and Mark Giuliano Commentary by Rob Sherwood October 2006.
Solar-B FPP 1 Ted Tarbell, TRACE Operations 3 February 2003 MODA Mtg, ISAS The TRACE Model for Operations Ted Tarbell
SECCI/COR2 Status Report SECCHI CONSORTIUM MEETING D. Socker, S. Plunkett, A. Vourlidas.
Package Engineering Container Design Request (CDR) Reference Guide
COR1 Science Overview Joseph M Davila Goddard Space Flight Center.
SECCHI_CDR_HW_Overview.1 Discussion of Synoptic Program and Use of SSR2 SECCHI Consortium SECCHI Consortium meeting 7 March 2007 Univ. Paris XI.
Flight Software Image Compression and Status Dennis Wang Interferometrics/NRL SECCHI Flight Software Lead Paris Mar 5-9, 2007.
2.0 Playing with SECCHI data. 6 Mar 2007FESTIVAL – SECCHI Consortium Meeting – Orsay Elie SoubriéProject manager / architect Franck LegallDeveloper Frédéric.
SECCHI – Sun-Earth Connections Coronal and Heliospheric Investigation SECCHI Synoptic and Special Observing Programs Simon Plunkett SECCHI Operations Lead.
Robin Colaninno March 6, th SECCHI Consortium Meeting Orsay, France Creating Calibrated Images with SECCHI_PREP 5 th SECCHI Consortium Meeting March.
2007 March 61 The SECCHI Campaign Jean-Pierre Wuelser SECCHI Consortium Meeting Orsay.
5 th SECCHI Tam Meeting.1 COR2 Status Angelos Vourlidas.
2007 March 51 EUVI Instrument and Calibration Status Jean-Pierre Wuelser James Lemen Markus Aschwanden Nariaki Nitta.
Page 1HMI Team Meeting – January 26, 2005 HMI Mission Operations Rock Bush HMI Stanford Program Manager Stanford University
EPOCH 1000 File Management Data Logging and Reporting
A Primer on Image Acquisition and Data Reduction Using TheSky6, CCDSoft V5 and Microsoft Excel Thomas C. Smith Dark Ridge Observatory (DRO)
Meghalaya Online Scholarship Portal Awareness program for VLEs.
7/12/20011 Observing Sequences in View of the SECCHI Science Goals From the EUVI Perspective J-P. Wülser.
OCAN College Access Program Data Submissions Vonetta Woods HEI Analyst, Ohio Board of Regents
IIS Home Screen (Teacher) Copyright © 2011 Pearson Education, Inc. or its affiliates. All rights reserved.1.
JTIMS Lesson Learned Initial Observation Capability LCDR Steven Jaureguizar JTIMS Program Manager.
Lead Management Tool Partner User Guide March 15, 2013
SECCHI Consortium Meeting, July 2001 SECCHI Ground Data Systems and Data Processing Nathan Rich NRL/Interferometrics
18-April-2006XRT Team1 Initial Science Observations Solar-B XRT Ed DeLuca for the XRT Team.
Heliospheric Imager – Scientific Operations  HI Operations Document – R. Harrison  HI Image Simulation – C. Davis & R. Harrison  HI Operations Scenarios.
SECCHI Status Russell A. Howard 27 MAR 2007 STEREO SWG.
Graphic material for HSC FAQ – March 23, Five things you should know about the Hubble Source Catalog (HSC) 1. Coverage can be very non-uniform,
WESS Application System PKI Login Registration Process.
1 EXT400 – Corporate Vendor Admin Activities. 2 1.Corporate Vendor Admin Process Overview 2.Complete Vendor Registration 3.Register Plants/Shipping Locations.
Heliospheric Imager – Scientific Operations  HI Operations Document – R. Harrison (presented by Dave Neudegg – SciOps for Cluster, Mars Express, Double.
Instructional Tools for Teachers: Creating & Sharing Instructional Materials Copyright © 2012 Schoolnet, Inc. All rights reserved.
000127STEREO_VGfigs.1 SECCHI Sun Earth Connection Coronal and Heliospheric Investigation R.A. Howard Presentation to Stereo SWG#1 27,28 January 2000 Web.
Feb 4, 20034th Solar-B Science Meeting1 SOT Scientific Observations & Operations T. Shimizu (National Astronomical Observatory of Japan)
2007 March 261 SECCHI-EUVI Status and First Observations Jean-Pierre Wuelser Lockheed Martin Solar and Astrophysics Lab And The SECCHI Team.
GLAST Science Support CenterNovember, 2005 GSSC User Committee Meeting Tools for Mission and Observation Planning Robin Corbet, GSSC
2007 March 51 EUVI Early Observations Jean-Pierre Wuelser James Lemen Markus Aschwanden Nariaki Nitta.
Human Resources 1 G-Top Global Workflow Employee View September 2014.
Operating Systems 1 K. Salah Module 1.2: Fundamental Concepts Interrupts System Calls.
STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG March 27-28, 2007.
STEREO - Solar Terrestrial Relations Observatory Mission SECCHI Calibration Activities Simon Plunkett SECCHI Operations Scientist Naval Research Laboratory.
Out of State Cigarette Importer’s Report. Log in with the User Id and Password provided through the EDS registration process and click on the Login button.
Improving your Audit Process Through Technology Christopher McDonald Director of Field Loss Prevention, Babies R’ Us Inc.
5 th SECCHI Consortium Meeting Orsay, France March 5-8, 2007 SECCHI Image and HouseKeeping Databases Ed Esfandiari NRL/Interferometrics, Inc.
Michael L. Kaiser STEREO Project Scientist NASA/Goddard Space Flight Center STEREO May 2, 2008 STEREO at 1.25 years.
When the program is first started a wizard will start to setup your Lemming App. Enter your company name and owner in the fields designated “Company Name”
Schoolwires Calendar App. Calendar Overview Calendar app uses the same color scheme and fonts as the rest of the IRHS site.
Advanced Website Training: June, 2010 Insert Images as Your Background Using Google Docs for Document Hosting Custom Contact Forms on Your Website.
SECCHI Status Russell A. Howard & The SECCHI Team March 2010 STEREO SWG – Trinity College, Dublin.
When the program is first started a wizard will start to setup your Lemming App. Enter your company name and owner in the fields designated “Company Name”
STEREO SWG 10/27/09 - GDS.1 NRL IDL Movie Tools STEREO SWG October 28, 2009 Meredith, NH Nathan Rich ( ) Lynn Simpson ( ) NRL/Interferometrics.
HEI/OCAN College Access Program Data Submissions.
Adding Events to Community. To add events to your group’s Community page click on Manage Events.
Company LOGO Sage CRM – Marketing Sage CRM 7.3 provides a new integration with MailChimp for marketing campaigns. In this.
COR1 Status William Thompson SECCHI Team Meeting, Dublin, Ireland, March 2010.
EIS Operation Planning H. Hara (NAOJ) 2007 Dec 10.
WESS Application System PKI Login Registration Process
Detlef Koschny Research and Scientific Support Department ESA/ESTEC
Software Testing With Testopia
FedEx Billing Online (FBO) Non-Revenue Quick Guide
WESS Application System PKI Login Registration Process
Launch and On-orbit Checkout
Instrument Performance Requirements
WESS Application System PKI Login Registration Process
WESS Application System PKI Login Registration Process
GLAST Large Area Telescope
WESS Application System PKI Login Registration Process
Presentation transcript:

5 th SECCHI Consortium Meeting Orsay, France March 5-8, 2007 SECCHI Planning and Scheduling Ed Esfandiari NRL/Interferometrics, Inc.

Planning and Scheduling Overview Scientist Has Observing Plan Idea Scientist Creates Detailed Plan Plan is ed to SECCHI Planner Plan Gets Converted to an Observing Schedule Schedule Gets Uploaded to SECCHI

Creating an Observing Plan ● Detail is essential! ● User needs to be aware of the various processing tables  Image category (Normal, Dark, Sequence, etc.)  Image Parameters ● Camera setup (7 entires per instrument) ● Exposure (7 entires per instrument) ● Image processing (100 entries for all instruments) ● ROI and Occulter Mask (1 of each per instrument) ● Be aware of telemetry constraints ● Be aware of instrument constraints ● All full-res images will be 2176x2048 ● Indicate if SC-A and SC-B images should be synced

Other Information... ● Tables can be obtained from the SECCHI wiki page under “Planning”  ● Observing plans should be submitted several days in advance ● Plans should be sent to the SECCHI Operations Scientist (Simon Plunkett)

Scheduling ● Observing plans, once approved, are entered into the IDL- based planning tool by the SECCHI planner (Ed Esfandiari) ● Planning tool is “ a set of IDL routines (of LASCO/EIT heritage) that generates daily-weekly command files and/or synoptic programs for commanding the 3 SCIP and 2 HI telescopes. It is a GUI tool that takes advantage of all available telescopes and on-board resources to maximize the use of the telemetry downlink. ” ● Planning tool monitors image sequences, buffer sizes, partition (SSR1, SSR2) sizes, downlink rates, etc

Typical Scheduling Steps ● Observing plan is scheduled through a series of IDL widgets ● Either a new observing sequence is created or an old existing sequence is imported. ● Reusing observing plans can save a great deal of time!

Verifying the Plan ● An “OS Num” (Observing Sequence Number) is generated for each unique observation ● Once all OS's are complete, the schedule is verified ● Schedule conflicts produce a warning

Schedule successfully created!

Summary ● Plan your observations carefully and be as detailed as you can ● If at all possible, use the table entry numbers ● Be aware of telemetry, buffer and instrument restrictions ● Try to reuse old observing plans ● Allow plenty of time ● Make use of the planning resources on the SECCHI wiki page

Jan-Feb 2007 Schedules ● Over 100 calibration, first light and commissioning schedules ● First draft of operations synoptics  Synced COR and HI observations  Different SC-A and SC-B EUVI observations

Operations Synoptics-First Draft  Synced COR and HI images  SC-A ● 5487 images (1442 EUVI, 861 COR1, 194 COR2, 1189 HI-1, 1801 HI-2) ● NRL EUVI version – less images, longer exposures ● 52KB upload file size (1157 commands)  SC-B (pushing the limits) ● 7476 images (3431 EUVI, same COR and HI images as SC-A) ● Lockheed EUVI version – more images, shorter exposures ● 98KB upload file size (2572 commands)

Required Details ● EUVI  Normal ● SC, FW, WL, FPS, IPT, ExpT, CamT  Double ● SC, FW, WL, WL, FPS, IPT, ExpT, CamT  Dark ● SC, FPS, IPT, CamT, ExpTime ( 0:99998ms )  LED ● SC, FW, WL, FPS, IPT, CamT, Pulse ( ), Color  Continuous ● SC, FW, WL, FPS, IPT, CamT  Sequence (n=2-4) ● SC, FW, WL*n, FPS, IPT, ExpT, CamT, Cadence ( 0=close-as-possible)

Required Details ● COR1 ad COR2  Normal ● SC, Polar, IPT, ExpT, CamT  Double ● SC, Polar, Polar, IPT, ExpT, CamT  Dark ● SC, IPT, CamT, ExpTime ( 0:99998ms )  LED ● SC, Polar, IPT, CamT, Pulse ( ), Color  Continuous ● SC, Polar, IPT, CamT  Sequence (n=2-4) ● SC, Polar*n, IPT, ExpT, CamT, Cadence ( 0=close-as-possible)

Required Details ● HI-1 and HI-2  Normal ● SC, IPT, ExpT, CamT  Dark ● SC, IPT, CamT, ExpTime ( 0:99998ms )  LED ● SC, IPT, CamT, Pulse ( ), Color  Continuous ● SC, IPT, CamT  Sequence (n=2-99) ● SC, IPT, ExpT, CamT, Cadence ( 0=close-as-possible)

An Example ● Scientist requests Full field EUVI images on SC-A every 2-hrs S1 FilterWheel, 284A, 1 sec exposure ● SECCHI planner requires SC-A, EUVI, Normal, FW=S1, Wave=284, FPS=Off, IPT=0, ExpT=6, CamT=1, Cadence=120min Where... ● IPTbl 0 >> SSR1, Rice Compressed ● EXPTbl 6 >> 1.0 Second exposure ● CamTbl 1 >> 2176x2048, no CCD summing, Hi gain