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MARS Simulation Progress

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Preliminary Results from MARS Calculations: FNAL Technical Memo 2221 Mokhov, ... close to the nominal design.I did this by halving the density of the molybdenum. ... – PowerPoint PPT presentation

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Title: MARS Simulation Progress


1
MARS Simulation Progress
  • Tweaking the geometry
  • Dose vs. Shield thickness
  • Dose w/ vs. w/o a satellite
  • Next steps

Tom Diehl 01/21/2004
2
Recent History
  • Igor Rakhno Co. wrote
  • Preliminary Results from MARS Calculations FNAL
    Technical Memo 2221 Mokhov, Rakhno, Striganov,
    Peterson Radiation Load to the SNAP CCD
    09/15/03.
  • Modeling the Cosmic Rays
  • SNAP Satellite Model
  • Preliminary Dose Calculations
  • We know we have some things to improve.
  • We know we have some systematic tests to carry
    out.
  • Igor sent me his code.

3
Shielding and Detector Model (Rakhno)
4
The Rakhno Model
  • The total mass included amounts to 276 kg.
  • Shield is 2 cm thick, 35 to 41 kg aluminum.
  • Cold Plate is 99 kg moly.
  • Silicon substrate is 5 kg mixture.
  • Silicon itself is 200 m thick amounting to 107 g.
  • Radiator is 69 kg aluminum.
  • The rest is deck, optical bench, supports, etc
    amounting to 61 kg.
  • I modified the cold plate to 49 kg, close to the
    nominal design.I did this by halving the density
    of the molybdenum.

5
Progress Dec. 10th to Dec 31st.
  • I learned MARS 14 tricks, pictures, plots.
  • Reran Igors code
  • Same Orbit (solar minimum) 10M galactic protons
    gt 6.8 R/y. Igor had 7.9 R/y.
  • Same orbit (solar minimum) 100M trapped protons
    gt 34 kR/y. Igor had 21 kR/y.
  • The program is functioning properly when I run
    it. Well I get approx. the same results as Igor
    does using that geometry.

6
Dose vs. Shield Thickness (AL)
  • The shield in the nominal geometry is 2 cm thick
    aluminum cone. Is there an optimal thickness?
  • Test dose in the silicon as change thickness (AL
    density) of the shield.
  • A much thicker shield will block these protons
    effectively.
  • No apparent reason to make the shield 35 kg.

2.7 g/cc
7
Material vs. No Material
  • Jodi L. has a fast cosmic ray simulation using 4
    charged particles/cm2/s. Thats the textbook
    unprotected rate. I can calculate a scale
    factor that accounts for the material.
  • I set all the material to vacuum, except the
    silicon, and reran MARS, 10 M galactic protons
    10M galactic electrons, elliptical orbit.
  • Dose (silicon) 4.7 R/y, less than with the
    material around the detector.
  • Ratio (satellite vs. no satellite) 1.5 - 0.1
    from galactic protons.
  • R 2.0- 0.2 from galactic electrons. But the
    electrons are 100 x less than the protons,
    anyway.

8
More Progress since Dec. 10th
  • Nibble File (Cease, Page, Lanfranco)
  • Solidworks Model -gt IDEAS CAD Program
  • Step through the satellite volume in small cubes
  • Report the material in each cube, its position,
    density, name, mass, and volume.
  • I can turn this into a table suitable for MARS.
    Maybe it will be suitable for GEANT, as well.

9
Summary Immediate Plan
  • Change to L2 Orbit.
  • The galactic spectrum will be similar to the
    elliptical orbit spectrum.
  • Trapped radiation goes away
  • Verify the shield thickness calculation
  • Test some different materials
  • Dose vs. Z at constant mass
  • Polyethylene Lithiated polyethylene (may not be
    wise to use poly, but want to check that anyway)
  • 2 material sandwich
  • Start importing simple nibbled Solidworks parts.

10
Buffer slide
  • Stuff here on isnt part of this talk.

11
Shielding and Detector Model (1)
  • The trick with MARS is to select the appropriate
    level of detail.
  • Include the most important shielding components.
    Consideration is given to proximity to detector
    and components mass.
  • Put a lot of effort into detailing the detector.

12
Microsoft Project Stuff
Done x
  • I sketched this up Nov. 2003 _at_ Collaboration
    Meeting.
  • I only show details for MARS stuff.
  • I rolled up the rest.
  • This isnt up to code
  • it could already stand to be updated.

x
x
x
12/30/2003
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