Raw HRC Antico Rate v EPHIN Flux

Scatter plots for each of the PMT#2 HV step values of the raw HRC antico shield rate (MSID 2SHLDART) vs EPHIN fluxes in the three channels used in the RADMON process and Integral channel. Upper Left vs P4, Upper Right vs P41, Lower Left vs E1300, and Lower Right vs Integral. The red vertical line is the RADMON threshold level.

PMT#2 HV at Step 8

Antico rate at HV step 8 vs EPHIN P4 Flux Antico rate at HV step 8 vs EPHIN P41 Flux
Antico rate at HV step 8 vs EPHIN E1300 Flux Antico rate at HV step 8 vs EPHIN INT Flux

PMT#2 HV at Step 7

Antico rate at HV step 7 vs EPHIN P4 Flux Antico rate at HV step 7 vs EPHIN P41 Flux
Antico rate at HV step 7 vs EPHIN E1300 Flux Antico rate at HV step 7 vs EPHIN INT Flux

PMT#2 HV at Step 6

Antico rate at HV step 6 vs EPHIN P4 Flux Antico rate at HV step 6 vs EPHIN P41 Flux
Antico rate at HV step 6 vs EPHIN E1300 Flux Antico rate at HV step 6 vs EPHIN INT Flux

PMT#2 HV at Step 5

Antico rate at HV step 5 vs EPHIN P4 Flux Antico rate at HV step 5 vs EPHIN P41 Flux
Antico rate at HV step 5 vs EPHIN E1300 Flux Antico rate at HV step 5 vs EPHIN INT Flux

Last modified: Wed Dec 8 10:55:14 EST 2004

Dr. Michael Juda
Harvard-Smithsonian Center for Astrophysics
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Cambridge, MA 02138, USA
Ph.: (617) 495-7062
Fax: (617) 495-7356
E-mail: mjuda@cfa.harvard.edu