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55 Fe Simulations under the divine guidance of Sauli’s “Bible”

55 Fe Simulations under the divine guidance of Sauli’s “Bible”. Jason for the SB Tent Crew. Mar 11, 2008. 55 Fe Simulation. Incidentals : Source sits 1 cm from mesh Drift Gap: 1.5 mm pad radius: 1.5 cm RB collection region: 150 μ. Simulation… γ is emitted from 55 Fe

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55 Fe Simulations under the divine guidance of Sauli’s “Bible”

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  1. 55Fe Simulations under the divine guidance of Sauli’s “Bible” Jason for the SB Tent Crew Mar 11, 2008

  2. 55Fe Simulation • Incidentals: • Source sits 1 cm from mesh • Drift Gap: 1.5 mm • pad radius: 1.5 cm • RB collection region: 150 μ • Simulation… • γ is emitted from 55Fe • determine γ angle φ top GEM mesh 55Fe γ 55Fe source readout pad φ Drift Gap note: not to scale 2

  3. conversion length 55Fe Simulation • Incidentals: • Source sits 1 cm from mesh • Drift Gap: 1.5 mm • pad radius: 1.5 cm • RB collection region: 150 μ • Simulation… • γ is emitted from 55Fe • determine γ angle φ • determine conversion length • where • for CF4, λ ~8.5cm conversion length top GEM mesh pe 55Fe γ 55Fe source readout pad φ Drift Gap note: not to scale 3

  4. 55Fe Simulation • Incidentals: • Source sits 1 cm from mesh • Drift Gap: 1.5 mm • pad radius: 1.5 cm • RB collection region: 150 μ • Simulation… • γ is emitted from 55Fe • determine γ angle φ • determine conversion length • where • for CF4, λ ~8.5cm • determine pe emission θ • follows a sin2 dist conversion length top GEM mesh pe 55Fe γ 55Fe source θ readout pad φ Drift Gap note: not to scale 4

  5. 55Fe Simulation • Incidentals: • Source sits 1 cm from mesh • Drift Gap: 1.5 mm • pad radius: 1.5 cm • RB collection region: 150 μ • Simulation… • γ is emitted from 55Fe • determine γ angle φ • determine conversion length • where • for CF4, λ ~8.5cm • determine pe emission θ • follows a sin2 dist • determine primary charge deposited by pe (poisson, 109) conversion length top GEM mesh pe 55Fe γ 55Fe source θ readout pad φ Drift Gap note: not to scale 5

  6. 55Fe Simulation • Incidentals: • Source sits 1 cm from mesh • Drift Gap: 1.5 mm • pad radius: 1.5 cm • RB collection region: 150 μ • Simulation… • γ is emitted from 55Fe • determine γ angle φ • determine conversion length • where • for CF4, λ ~8.5cm • determine pe emission θ • follows a sin2 dist • determine primary charge deposited by pe (poisson, 109) • dist traversed by e’s (E<300keV) Rp = 0.71xE1.72 (E in MeV, Rp in g/cm2) in CF4 at 5.9 keV, Rp ~286μ conversion length top GEM mesh pe 55Fe γ 55Fe source θ readout pad φ Rp Drift Gap note: not to scale 6

  7. 55Fe Simulation • Incidentals: • Source sits 1 cm from mesh • Drift Gap: 1.5 mm • pad radius: 1.5 cm • RB collection region: 150 μ • Simulation… • γ is emitted from 55Fe • determine γ angle φ • determine conversion length • where • for CF4, λ ~8.5cm • determine pe emission θ • follows a sin2 dist • determine primary charge deposited by pe (poisson, 109) • dist traversed by e’s (E<300keV) Rp = 0.71xE1.72 (E in MeV, Rp in g/cm2) in CF4 at 5.9 keV, Rp ~286μ • for each of 109 e’s, • determine position along track conversion length top GEM mesh pe 55Fe γ 55Fe source θ readout pad φ Rp Drift Gap note: not to scale 7

  8. 55Fe Simulation • Incidentals: • Source sits 1 cm from mesh • Drift Gap: 1.5 mm • pad radius: 1.5 cm • RB collection region: 150 μ • Simulation… • γ is emitted from 55Fe • determine γ angle φ • determine conversion length • where • for CF4, λ ~8.5cm • determine pe emission θ • follows a sin2 dist • determine primary charge deposited by pe (poisson, 109) • dist traversed by e’s (E<300keV) Rp = 0.71xE1.72 (E in MeV, Rp in g/cm2) in CF4 at 5.9 keV, Rp ~286μ • for each of 109 e’s, • determine position along track • If e is over our readout pad && • Forward Bias • if e is inside drift gap, avalanche it. • Reverse Bias • if e is within 150μ, avalanche it. conversion length top GEM mesh pe 55Fe γ 55Fe source θ readout pad φ Rp Drift Gap note: not to scale 8

  9. Actual Spectrum Simulated 55Fe Spectra • The FB bias spectrum is very similar to what we see in the gain test box. • After the 10th stack is installed, we’ll hook Maestro up to the “pre-CsI” box and measure RB spectra for comparison. 9

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