Solar-B EIS - PowerPoint PPT Presentation

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Solar-B EIS

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effort in UK slow or stalled. science goals not well ... magnification - short spectrometer section. add telescope length - improve spatial resolution ... – PowerPoint PPT presentation

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Title: Solar-B EIS


1
Solar-B EIS
  • Steering Committee meeting
  • 27th May 1999

2
The position last February
  • Design dichotomy
  • effort in UK slow or stalled
  • science goals not well articulated e.g.
    wavelength range choice
  • Interface management unclear
  • Schedule and costs unclear

3
Kick-off MeetingISAS, March 8-13 1999
  • Mission Philosophy
  • Organisation
  • Master Schedule
  • Spacecraft Overview

4
Design of EIS
  • Cassegrain or OAP?
  • Technical drivers - feasibility, costphysical
    resourcesdisturbance torque- for Structure,
    Optics, Detectors, Elec.
  • Line lists
  • Effective areas - useful lines in QS, AR, Fl.

5
Management Plan
  • Decision making
  • Science - PIs Project Scientist Consortium
  • Program - PM (MSP) PIs
  • Engineering - SDT
  • Decision dissemination
  • Science Technical email lists (points of
    contact)

6
Design of EIS (2)
  • Value of Spatial Resolution
  • Value of Throughput
  • Decision-making panel ISAS, NAOJ, NASA, NRL,
    PPARC/MSSL
  • Throughput (OAP) given priority

7
on from there
  • NRL asked to propose an OAP concept
  • with two wavelength ranges170-206 Å250-290 Å
  • on the same detector, non-overlapped, if
    possible (implies two grating surfaces)
  • keep high throughput,improve spatial resolution
    if possible

8
The new NRL/GSFC designs
  • NRL/MSSL series of teleconferences- discuss
    progress and direction of optical design-
    also an opportunity to learn lessons from
    SOHO/LASCO
  • became clear that engineer-level round-table
    interaction needed Þ NRL opto-mechanical
    engineering meet.

9
preferred design EIS-7T
  • one of a series of optimisations
  • small grating - low risk
  • toroidal grating - more vendor choice
  • magnification - short spectrometer section
  • add telescope length - improve spatial
    resolution
  • details published by FTP 7 May 99

10
Optical properties
  • Nyquist-limited - spot sizes closer to detector
    pixel size
  • effective detector pixels governed by charge
    spreading (R. Stern investigations)
  • large effective field-of-view - 1000

11
UK response
  • BU - structural concepts
  • MSSL - camera head concepts
  • swift drawing interchange
  • mechanisms - mass? power? placement?

12
Opto-mechanical engineeringmeeting, NRL 17-18
May 99
  • US, UK, J involvement
  • review NRL/GSFC work to date
  • approve the criteria and results
  • review subsystem technology designsitems
    connected with main instrument
  • suggest ideal placement
  • iterate before BU consortium meeting

13
The main Actions
  • NRL/GSFC- reduce lengthby 10 cm- issue new
    optical layout- denote volumes which must be
    separate
  • 1st June
  • BU/MSSL- iterate structural concept, use
    sectional construction- include radiator
    placement- camera update
  • 14th June

14
Interface Management
  • System engineering - an MSSL responsibility to
    lead, but need help/experience from team
  • Timetables () - e.g. mechanical thermal models
    - aiming for Phase B !!
  • Interface list - ()
  • Spacecraft Interfaces ()

15
Panels - Meetings - Minutes
  • Consortium
  • Science
  • Oversight of technical progress
  • archive EIS-meet-cons-YYMMmins -YYMMagen
  • System Design Team - includes NRL telecon
  • Technical
  • Sys Engineering, Budget, Schedule
  • EIS-meet-sdt-minutesX EIS-meet-sdt-tcXXXX

16
The position now ...
  • Major design decision made
  • UK work going ahead
  • Science goals getting clearer
  • Wavelength ranges selected
  • Interfaces clearer - need more work
  • Planning (schedule /costs) - improving
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