IDS120j WITHOUT RESISTIVE MAGNETS: NEW Hg MODULE

Slides:



Advertisements
Similar presentations
SUPERCONDUCTING SOLENOIDS - SHIELDING STUDIES 1. N. Souchlas BNL (Oct. 5, 2010)
Advertisements

Beam-plug and shielding studies related to HCAL and M2 Robert Paluch, Burkhard Schmidt November 25,
Mercury Chamber Update V. Graves NF-IDS Meeting October 4, 2011.
IDS120j WITH/WITHOUT GAPS SH#4 AZIMUTHAL DPD DISTRIBUTION ANALYSIS Nicholas Souchlas, PBL (3/14/2012) 1.
Neutrino Factory Target Cryostat Review Van Graves Cale Caldwell IDS-NF Phone Meeting August 10, 2010.
Meson Production Comparison between Hg and Ga at 8 GeV X. Ding, UCLA Target Studies, Oct. 04, 2011.
Meson Production Comparison between HG and GA at 8 GeV (Update) X. Ding, UCLA Target Studies, Oct. 18, 2011.
Particle Production of a Carbon/Mercury Target System for the Intensity Frontier X. Ding, UCLA H.G. Kirk, BNL K.T. McDonald, Princeton Univ MAP Spring.
1Managed by UT-Battelle for the U.S. Department of Energy MERIT Videoconference 11 Mar 2009 Neutrino Factory Cryostat 1 Concept V.B. Graves MERIT Videoconference.
Operated by Brookhaven Science Associates for the U.S. Department of Energy A Pion Production and Capture System for a 4 MW Target Station X. Ding, D.
1Managed by UT-Battelle for the U.S. Department of Energy NF/IDS Hg Vessel Layout 30 Jun 09 Cryostat 2 Front Drain Mercury Vessel Concept Matthew F. Glisson.
IDS120h: Be WINDOW DETAILED CALCULATION, SHIELDING VESSELS, RESULTS FOR DIFFERENT GLOBAL STEPS Nicholas Souchlas (9/20/2011) 1.
MC/NF TARGET SHIELDING STUDIES. NICHOLAS SOUCHLAS (10/29/2010)‏ 1.
SHIELDING STUDIES FOR THE MUON COLLIDER TARGET NICHOLAS SOUCHLAS BNL Nov 30, 2010 ‏ 1.
Preliminary Analysis of the Target System Magnets 1.Version with a 6-T copper magnet insert 2.Version with a 6-T high-temperature superconductor insert.
Harold G. Kirk Brookhaven National Laboratory Target System Update IDS-NF Plenary Meeting Arlington, VA October 18, 2011.
Harold G. Kirk Brookhaven National Laboratory Target Baseline IDS-NF Plenary CERN March 23-24, 2009.
IDS-NF Target Studies H. Kirk (BNL) July 8, 2009.
1 Comparison of Power Depositions X. Ding, D. B. Cline, UCLA H. Kirk, J. S. Berg, BNL Collaboration Meeting July 2, 2010.
Comparison of Power Deposition in SC1 Coil Xiaoping Ding UCLA Target Studies Jun. 29, 2010.
Power Deposition in SC1 Coil Xiaoping Ding UCLA Target Studies Apr. 20, 2010.
SUPERCONDUCTING SOLENOIDS - SHIELDING STUDIES 3. NICHOLAS SOUCHLAS (10/28/2010)‏
IDS120h POWER DEPOSITION AND Hg POOL STUDIES Nicholas Souchlas (7/26/2011) 1.
STUDY II: m1507 vs. m1510 IDS120f: m1507/MCNP vs. M1510/MCNP vs. FLUKA IDS120f vs. IDS20g GEOMETRY IDS90f: B10/B11 SHIELDING RING(S) STUDIES Nicholas Souchlas.
SUPERCONDUCTING SOLENOIDS - SHIELDING STUDIES 1..
Meson Productions for Target System with GA/HG Jet and IDS120h Configuration X. Ding (Presenter), D. Cline, UCLA H. Kirk, J.S. Berg, BNL Muon Accelerator.
Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,
Study of Pion Capture Solenoids for PRISM H.Ohnishi AB M. Aoki C, Y. Ajima A, N. Fukasawa AD, K. Ishibashi B, Y. Kuno C, T. Miura A, K. Nakahara C, T.
Review of Recent IDS120 Target Concepts Van Graves October 31, 2013.
IDS120j WITHOUT GAPS AND WITH MAXIMUM SIZE GAPS ( aka ''NIGHTMARE'' CASE SCENARIO ) SC#4, SC#7 AZIMUTHAL DPD DISTRIBUTION ANALYSIS. Nicholas Souchlas,
20to2T5m100cm Images Van Graves February 13, 2014.
IDS120h GEOMETRY WITH MODIFIED Hg POOL VESSEL. SIMULATIONS FOR 60%W+40%He SHIELDING (P12 'POINT') WITH STST SHIELDING VESSELS EFFECTS OF Be WINDOW WATER.
SHIELDING STUDIES FOR THE MUON COLLIDER TARGET. (From STUDY II to IDS120f geometries) NICHOLAS SOUCHLAS (BNL)‏ ‏ 1.
KT McDonald MAP Tech Board Meeting Oct 20, The MAP Targetry Program in FY11 and FY12 K. McDonald Princeton U. (Oct 20, 2011) MAP Technical Board.
DEPOSITED POWER STUDIES FOR THE MC/NF TARGET STATION. Nicholas Souchlas (PBL) (MAP CONFERENCE SLAC 2012) 1 DEPOSITED POWER STUDIES FOR THE MC/NF TARGET.
1 Energy Deposition of 4MW Beam Power in a Mercury Jet Target X. Ding, D. B. Cline UCLA H. Kirk, J. S. Berg BNL The International Design Study for the.
Simulations on “Energy plus Transmutation” setup, 1.5 GeV Mitja Majerle
IDS120j WITH GAPS SC#3 AZIMUTHAL DPD DISTRIBUTION ANALYSIS WITH MAX GAPS SC#3, SC#4 AZIMUTHAL DPD DISTRIBUTION ANALYSIS, DP AND SC TOTAL DP WITH VARYING.
IDS120h GEOMETRY WITH MODIFIED Hg POOL VESSEL. SIMULATIONS FOR 60%W+40%He SHIELDING (P12 'POINT') WITH STST SHIELDING VESSELS. BP#1(STST/W), SH#1, BeWindow,SC#8.
Particle Production at 3 GeV (update) X. Ding, UCLA Target Studies Sept. 23, /23/13.
Target Magnets & Shielding Bob Weggel Particle Beam Lasers, Inc. Magnet Optimization Research Engineering, LLC. March 5,
IDS120j WITHOUT RESISTIVE MAGNETS: NEW Hg MODULE mars1510 ( DESKTOP ) vs. mars1512 ( PRINCETON CLUSTER ) Nicholas Souchlas, PBL (3/28/2012) 1.
Collimator and beamline heating External Review of the LHC Collimation Project CERN Wed 30/6/2004.
Kinetic Energy Spectra of pi +, pi -, mu +, mu - and sum of all from the 20to4T5m Configuration X. Ding Front End Meeting June 23,
Meson Production of Carbon Target at 3 GeV X. Ding, UCLA Target Studies 17/18/13.
Carbon Target Design and Optimization for an Intense Muon Source X. Ding, UCLA H.G. Kirk, BNL K.T. McDonald, Princeton Univ MAP Winter Collaboration.
Chicane shielding and energy deposition (IPAC’13 follow-up) Pavel Snopok IDS-NF phone meeting June 4, 2013.
IDS120j WITHOUT RESISTIVE MAGNETS ( 20 cm GAPS AND 15.8 g/cc W BEADS ) AZIMUTHAL DPD DISTRIBUTION STUDIES FOR: BP#1, SH#1, SHVS#1/LFL, SC#1+SC#2, BeWind.
Multiprocessing/MARS15(2012)/Princeton Cluster (IDS120j w/t Resistive Magnets: New Hg Module) X. Ding UCLA (4/11/2013)
IDS120j WITHOUT RESISTIVE MAGNETS MODIFYING Hg MODULE Nicholas Souchlas, PBL (11/1/2012) 1.
IDS120j WITH AND WITHOUT RESISTIVE MAGNETS PION AND MUON STUDIES WITHIN TAPER REGION, III ( 20 cm GAPS BETWEEN CRYOSTATS ) Nicholas Souchlas, PBL (9/4/2012)
Meson Production at Low Proton Beam Energy (Update) X. Ding, UCLA Target Studies May 9, /9/113.
IDS120i GEOMETRY. SIMULATIONS FOR 60%W+40%He SHIELDING WITH STST SHIELDING VESSELS. Hg vs. Ga DEPOSITED POWER DISTRIBUTION. (using Ding's optimized parameters)
IDS120j WITHOUT RESISTIVE MAGNETS SEMGENTATION STUDIES FOR BEAM PIPE BEYOND FIRST CRYOSTAT ( 20 cm GAPS AND 15.8 g/cc W BEADS ) Nicholas Souchlas, PBL.
IDS120j WITHOUT RESISTIVE MAGNETS SEMGENTATION STUDIES FOR BP#2 WITHIN FIRST CRYOSTAT AND RIGHT FLANGE OF Hg POOL INNER VESSEL ( 20 cm GAPS AND 15.8 g/cc.
Neutrino Factory Target Vessel Concept Update V. Graves Target Studies EVO June 12, 2012.
Neutrino Factory Target Cryostat Review (Update Aug 12) Van Graves Cale Caldwell IDS-NF Phone Meeting August 10, 2010.
SHIELDING STUDIES FOR IDS80 (NO IRON PLUG/YOKE), ADDING SHIELDING IN 75 TO 80 cm (WC/H 2 O, B, Cd). NICHOLAS SOUCHLAS (BNL) Dec. 14, 2010‏ ‏ 1.
ENERGY FLOW AND DEPOSITION IN A 4-MW MUON-COLLIDER TARGET SYSTEM
Francesco Cerutti, Andrea Tsinganis WP10 Energy deposition & R2E
IDS120h: PROTON P0-P14 TRAJECTORY FOOTPRINT
X. Ding, UCLA MAP Spring 2014 Meeting May 2014 Fermilab
PROGRESS REPORT OF A NLNS-FFAG ADS MAGNET
1 Nicholas Souchlas, PBL (11/15/2011)
1 Nicholas Souchlas (PBL) (MAP CONFERENCE SLAC 2012)
Energy deposition studies in IR7 for HL-LHC
Detector Configuration for Simulation (i)
Interaction Region Design Options e+e- Factories Workshop
Higgs Factory Backgrounds
Revised estimates of heat loads and radiation damage in the IT and D1
Presentation transcript:

IDS120j WITHOUT RESISTIVE MAGNETS: NEW Hg MODULE SC#7, SC#8, SC#9 ( IN CRYOSTAT #3 ) AZIMUTHAL TDPD DISTRIBUTION Nicholas Souchlas ( PBL ) [ 10/24/2013 ] 1

*********************************************************** IDS120j GEOMETRY, NO RESISTIVE MAGNETS: WITH 20 cm GAPS BETWEEN CRYOSTATS *********************************************************** # MODIFIED Hg MODULE SIMULATES VAN GRAVE'S DESIGN. AZIMUTHAL POWER DISTRIBUTION IN SC#7, SC#8, SC#9 IN CRYOSTAT#3. COMPARISON WITH FLUKA STUDIES. ➡ SIMULATIONS CODE: mars15 (2010) [ USING MCNPDATA x-SECTION LIBRARIES FOR NEUTRON INTERACTIONS WITH KE < 14 MeV ] ➡ NEUTRON ENERGY CUTOFF: 10-12 GeV ➡ SHIELDING: 60% W + 40% He [ WITH STST VESSELS ] ➡ Bz ( r = 0, z ) : 15 T [ z = -37.5 cm ] ---➜ 1.5 T [ z = 1470.0 cm ] ➡ Hg JET RADIUS / ANGLE: 0.4 cm / 0.09667 deg. ➡ PROTON BEAM POWER: 4 MW ➡ PROTON ENERGY: E = 8 GeV ➡ PROTON BEAM PROFILE : GAUSSIAN, σx = σy = 0.12 cm [ P12 OBTAINED USING DING'S STUDY II OPTIMIZED DATA ] ➡ EVENTS IN SIMULATIONS : Np = 5,000,000 [ AVERAGE FROM 4 x 5E4 EVENTS ] 2 IDS120j GEOMETRY, NO RESISTIVE MAGNETS: WITH 20 cm GAPS BETWEEN CRYOSTATS *********************************************************** # MODIFIED Hg MODULE SIMULATES VAN GRAVE'S DESIGN. AZIMUTHAL POWER DISTRIBUTION IN SC#7, SC#9 IN CRYOSTAT#3. COMPARISON WITH FLUKA STUDIES. ➡ SIMULATIONS CODE: mars15 (2010) [ USING MCNP CROSS SECTION LIBRARIES ] ➡ NEUTRON ENERGY CUTOFF: 10-12 GeV ➡ SHIELDING: 60% W + 40% He ( WITH STST VESSELS) PROTON BEAM POWER: 4 MW >PROTON ENERGY: E = 8 GeV >PROTON BEAM PROFILE: GAUSSIAN, σx = σy = 0.12 cm ( P12 ) >EVENTS IN SIMULATIONS : Np = 5,000,000 ( AVERAGE FROM 4 x 5E4 EVENTS ) IDS120j GEOMETRY, NO RESISTIVE MAGNETS: WITH 20 cm GAPS BETWEEN CRYOSTATS *********************************************************** # MODIFIED Hg MODULE SIMULATES VAN GRAVE'S DESIGN. AZIMUTHAL POWER DISTRIBUTION IN SC#7, SC#9 IN CRYOSTAT#3. COMPARISON WITH FLUKA STUDIES. ➡ SIMULATIONS CODE: mars15 (2010) [ USING MCNP CROSS SECTION LIBRARIES ] ➡ NEUTRON ENERGY CUTOFF: 10-12 GeV ➡ SHIELDING: 60% W + 40% He ( WITH STST VESSELS) >PROTON BEAM POWER: 4 MW >PROTON ENERGY: E = 8 GeV >PROTON BEAM PROFILE: GAUSSIAN, σx = σy = 0.12 cm ( P12 ) >EVENTS IN SIMULATIONS : Np = 5,000,000 ( AVERAGE FROM 4 x 5E4 EVENTS ) IDS120j GEOMETRY, NO RESISTIVE MAGNETS: WITH 20 cm GAPS BETWEEN CRYOSTATS *********************************************************** # MODIFIED Hg MODULE SIMULATES VAN GRAVE'S DESIGN. AZIMUTHAL POWER DISTRIBUTION IN SC#7, SC#9 IN CRYOSTAT#3. COMPARISON WITH FLUKA STUDIES. ➡ SIMULATIONS CODE: mars15 (2010) [ USING MCNP CROSS SECTION LIBRARIES ] ➡ NEUTRON ENERGY CUTOFF: 10-12 GeV ➡ SHIELDING: 60% W + 40% He ( WITH STST VESSELS) ➡ Bz ( r = 0, z ) : 15 T [ z = -37.5 cm ] ➡ PROTON BEAM POWER: 4 MW ➡ PROTON ENERGY: E = 8 GeV ➡ PROTON BEAM PROFILE: GAUSSIAN, σx = σy = 0.12 cm ( P12 ) ➡ EVENTS IN SIMULATIONS : Np = 5,000,000 ( AVERAGE FROM 4 x 5E4 EVENTS ) IDS120j GEOMETRY, NO RESISTIVE COILS: WITH 20 cm GAPS *********************************************************** # SIMULATIONS USING LOWEST GRADE W BEADS IN SHIELDING ( OF 15.8 g/cc ) # BP#2 SEGMENTATION STUDIES WITHIN THE FIRST CRYOSTAT AND RIGHT FLANGE OF Hg POOL INNER VESSEL. >SIMULATIONS CODE: mars1512 ( USING MCNP CROSS SECTION LIBRARIES ) >NEUTRON ENERGY CUTOFF: 10-11 MeV >SHIELDING: 60% W + 40% He ( WITH STST VESSELS) >PROTON BEAM POWER: 4 MW >PROTON ENERGY: E = 8 GeV >PROTON BEAM PROFILE: GAUSSIAN, σx = σy = 0.12 cm

IDS120j: yz CROSS SECTIONS WITH DETAILS OF Hg POOL MODULE FROM VAN GRAVE'S PRESENTATION ( 8 / 9 / 2012 ). He FOR COOLING VACUUM THE DESIGN REQUIRES A 2.5 cm ! GAP BETWEEN SH#1 INNER VESSEL AND Hg POOL MODULE OUTER VESSEL. AN EVEN LARGER SPACE APPEARS TO BE BETWEEN INNER AND OUTER VESSEL OF THE Hg POOL MODULE FOR THE FLOW OF He GAS FOR COOLING THE POOL WALLS. THE RADIUS OF THE UPPER HALF ( ~ SEMICIRCULAR ) SECTION OF INNER Hg POOL VESSEL WILL BE 26.5 cm, MUCH LARGER THAN THE BEAM PIPE APERTURE AT THE END OF CRYO#1 ( ~ 17.7 cm ). 3

IDS120j: yx CROSS SECTION WITH DETAILS OF Hg POOL MODULE FROM VAN's PLOTS ( LEFT ) AND ADAPTED DESIGN FOR MARS SIMULATIONS ( RIGHT ) [ AT z = 100 m ]. IDS120j: yx CROSS SECTION WITH DETAILS OF Hg POOL MODULE FROM VAN's PLOTS ( LEFT ) AND ADDAPTED DESIGN FOR MARS SIMULATIONS ( AT z = 100 cm ). φ = 0O 2.5 cm VACUUM GAP BETWEEN SHVS#1 INNER AND Hg MODULE OUTER TUBE φ = 90O y SH#1 HU = 15 cm VACUUM φ = 30O φ = 0O HgPL = - 15 cm HL = - 26 cm Hg 1.0 cm STST INNER / OUTER Hg MODULE TUBE SHVS#1: 2.0 cm STST INNER TUBE x 2.0 cm He GAP BETWEEN INNER AND OUTER MODULE TUBES FOR COOLING. EVERYTHING HAS BEEN PARAMETRIZED FOR FUTURE CONVINIENCE. THE HEIGHTS OF THE END POINTS OF THE STRAIGHT SECTIONS ARE HL = - 26 cm AND HU = 15 cm. THE FREE Hg POOL SURFACE IS AT y = - 15 cm. THE RADIUS OF THE LOWER HALF OF THE INNER VESSEL OF THE Hg MODULE IS NOW SMALLER THAN BEFORE : FROM ~ 45 cm ----> ~ 39 cm. THE REST OF THE SPACE BETWEEN SHVS#1 INNER AND OUTER TUBE ( AT R ~ 115 cm ) IS FILLED WITH SHIELDING. 4 φ = 90O φ = 0O EVERYTHING HAS BEEN PARAMETRIZED FOR FUTURE CONVINIENCE. THE HEIGHTS OF THE END POINTS OF THE STRAIGHT SECTIONS ARE HL = - 26 cm AND HU = 15 cm. THE FREE Hg POOL SURFACE IS AT y = - 15 cm. THE RADIUS OF THE LOWER HALF OF THE INNER VESSEL OF THE Hg MODULE IS NOW SMALLER THAN BEFORE : FROM ~ 45 cm ----> ~ 42 cm. THE REST OF THE SPACE BETWEEN SHVS#1 INNER AND OUTER TUBE IS FILLED WITH SHIELDING. 7 y SHVS#1 2.0 cm STST OUTER TUBE SHVS#4 2.0 cm STST INNER TUBE IDS120j: yx CROSS SECTION WITH DETAILS OF Hg POOL MODULE FROM VAN PLOTS ( LEFT ) AND ADDAPTED DESIGN FOR MARS SIMULATIONS ( AT z = 100 cm ). 1.0 cm He GAPS BETWEEN VESSELS AND SHIELDING 0.5 cm GAP BETWEEN INNER SHVS#4 AND SHVS#1 OUTER TUBE

IDS120j: yz ( LEFT ) AND yx AT z = 10 cm ( RIGHT ) CROSS SECTION WITH DETAILS OF THE NEW Hg MODULE AND THE LOWER HALF OF THE UPSTREAM REGION. φ = 90O y y z = - 100 cm z = 372.9 cm RU1 φ = 0O 5.0 cm STST RL1 z 10 cm THICK STST FOR THE UPSTREAM AND DOWNSTREAM FLANGE OF Hg MODULE x THE RADIUS OF THE TOP SEMICIRCULAR SECTION OF THE Hg INNER TUBE IS SUCH THAT WILL NOT INTERFERE WITH THE Hg JET AND THE BEAM PROTONS AT THE BEGINNING OF CRYO#1 ( z ~ - 240 cm ) [ RU1 = 28.0 cm AND RL1 = 45.0 cm ] #> ACCORDING TO VAN'S DESIGN THE VOLUME FROM THE BEGINNING OF CRYO#1 ( z ~ - 240 cm ) TO THE BEGINNING OF THE Hg POOL ( z ~ - 100 cm ) AND FROM y ~ -15 cm TO THE BOTTOM OF THE Hg MODULE INNER VESSEL ( R ~ 39 cm ) WILL BE EMPTY TO ACCOMODATE THE He PIPES AND OTHER COMPONENTS OF THE Hg POOL MODULE. #> SOME IMPROVEMENT IN SHIELDING IS ACHIEVED BY UNIFYING SH#1 AND SH#4. THERE WILL BE SIGNIFICANT INCREASE IN THE SHIELDING MASS ( > 200 tons ) TO BE CONTAINED IN THE NEW VESSEL (SHVS#1) ==> GREATER ASSYMETRY IN THE WEIGHT DISTRIBUTION. He COOLING OF SUCH A LARGE VOLUME ( > 22 m3 ) OF SHIELDING CAN BE CHALLENGING. 5 # ACCORDING TO VAN'S DESIGN THE VOLUME FROM THE BEGINNING OF CRYO#1 ( z ~ - 240 cm )TO THE BEGINNING OF THE Hg POOL ( z ~ - 100 cm ) AND FROM y ~ -15 cm TO THE BOTTOM OF THE Hg MODULE INNER VESSEL ( R ~ 39 cm ) WILL BE EMPTY TO ACCOMODATE THE PIPES AND OTHER COMPONENTS OF THE Hg POOL MODULE. # SOME IMPROVEMENT IN SHIELDING IS ACHIEVED BY UNIFYING SH#1 AND SH#4. THERE WILL BE SIGNIFICANT INCREASE IN THE SHIELDING MASS ( > 200 tons ) TO BE CONTAINED IN THE NEW VESSEL (SHVS#1) ==> GREATER ASSYMETRY IN THE WEIGHT DISTRIBUTION. He COOLING OF SUCH A LARGE VOLUME ( > 22 m3 ) OF SHIELDING CAN BE CHALENGING. 5 IDS120j: yz ( LEFT ) AND yx AT z = 10 cm ( RIGHT ) CROSS SECTION WITH DETAILS OF THE NEW Hg MODULE AND THE LOWER HALF OF THE UPSTREAM REGION.

--- SEGMENTATION DATA --- IDS120j: yz AT x = 0.0 cm [ LEFT ] AND yx AT z = 1040.0 cm [ RIGHT ] CROSS SECTION WITH DETAILS OF SC#7 SEGMENTATION. IN LEFT PLOT ONE CAN ALSO SEE DETAILS OF THE 20.0 cm GAP BETWEEN CRYOSTAT#2 AND CRYOSTAT#3. . φ = 90O y y φ = 0O z x --- SEGMENTATION DATA --- 70.0 < r < 89.97 cm dr = 9.985 cm Nr = 2 bins 1036.0 < z < 1046.67 cm dz = 5.335 cm Nz = 2 bins 0.0 < φ < 360.0 deg. dφ = 30 deg. Nφ= 12 bins Ntot = 48 ''pieces'' IDS120j: yz ( LEFT ) AND yx ( RIGHT ) CROSS SECTION WITH DETAILS OF THE BP#1 SEGMENTATION. X CROSS SECTION WITH DETAILS OF THE BP#2 SEGMENTATION. 6 18 6 120.0 < r < 150.0 cm dr = 10.0 cm Nr = 3 bins - 55.0 < z < 185.0 cm dz = 20.0 cm Nz = 12 bins 0.0 < φ < 360.0 deg. dφ = 30 deg. Nφ= 12 bins Ntot = 432 ''pieces'' ONLY THE AREA WITH HIGHEST AVERAGE AZIMUTHAL DPD ( DETERMINED FROM MARS PLOTS ) WAS STUDIED. IDS120j: yz ( LEFT ) AND yx ( RIGHT ) CROSS SECTION WITH DETAILS OF THE SC#1+2 SEGMENTATION. 70.0 < r < 89.97 cm dr = 9.985 cm Nr = 2 bins 1036.0 < z < 1046.67 cm dz = 5.335 cm Nz = 2 bins 0.0 < φ < 360.0 deg. dφ = 30 deg. Nφ= 12 bins Ntot = 48 ''pieces''

Mars1510 (DESKTP) 5 E05 PEAK TDPD ~ 0.040 mW / g AT ABOUT 200 deg ( BOTTOM OF THE COIL NEAR -x AXIS ) . THIS IS FOR z1 AND FOR BOTH r1, r2 RADIUS. THESE AREAS FACE UPSTREAM TOWARDS THE TARGET REGION. THE REASON FOR THE RELATIVE INCREASE IN THE TDP IN THE LOWER HALF OF THE COIL AND FOR THE UPSTREAM SIDE IS THE INCREASE OF THE Hg POOL LENGTH ALL THE WAY TO THE END OF THE FIRST CRYOSTAT AT THE EXPANCE OF W SHIELDING THERE. SC#7 : 48 “PIECES” TDP = 0.0086 kW VS. ONE VOLUME COIL TDP = 0.0078 kW FLUKA SC#7 TDP = 0.008 ± 0.007 kW SC#7 PEAK TDPD = 0.03 mW/g RADIAL / 0.15 mW/g AZIMUTHAL ( ± ??? ) ( FROM JOHN BACK / JUNE 10 2012 ) . 7 PEAK TDPD mars1510 < 0.06 mW / g IN SC#1 mars1512 < 0.19 mW / g IN SC#2. BOTH CODES SHOW MOST OF THE DP TO BE BETWEEN ~ - 40 < z < 40 cm AND IN THE LOWER HALF OF SC#1+2, TOWARDS THE + x DIRECTION. NEW MARS CODE GIVES TDPD ~ 0.1 mW / g IN THE SAME REGION mars1510 GIVES PEAK TDPD. BUT THE PEAK TDPD ACCORDING TO mars1512 IS FURTHER DOWNSTREAM. 7 PEAK TDPD < 0.06 mW / g. MOST OF THE DP IS BETWEEN -20 < z < 40 cm, AND THE LOWER HALF OF SC#1+2, TOWARDS THE + x DIRECTION . THIS IS THE RESULT OF REMOVING SHIELDING IN THE LOWER PART OF THE Hg MODULE AND REPLACING IT WITH LIQUID Hg. THE NEGATIVE IMPACT OF THE NEW Hg MODULE IN SH#1 IS GREATELY MITIGATED BY THE INTRODUCTION OF ~ 8 cm THICK CYLIDRICAL SHIELDING VOLUME AT R ~ 50 cm WHEN SH#1 AND SH#4 ARE UNIFIED INTO ONE VOLUME.

--- SEGMENTATION DATA --- IDS120j: yz AT x = 0.0 cm [ LEFT ] AND yx AT z = 1090.0 cm [ RIGHT ] CROSS SECTION WITH DETAILS OF SC#8 SEGMENTATION. DUE TO THE COIL RADIAL THIKNESS UNAVOIDABLY THE RADIAL BIN SIZE IN THE SEGMENTATION IS SMALL. . φ = 90O φ = 90O y y y φ = 0O z z x --- SEGMENTATION DATA --- 70.0 < r < 72.54 cm dr = 2.54 cm Nr = 1 bins 1081.70 < z < 1421.20 cm dz = 19.971 cm Nz = 17 bins 0.0 < φ < 360.0 deg. dφ = 30 deg. Nφ= 12 bins Ntot = 204 ''pieces'' IDS120j: yz ( LEFT ) AND yx ( RIGHT ) CROSS SECTION WITH DETAILS OF THE SC#1+2 SEGMENTATION. 8 18 X CROSS SECTION WITH DETAILS OF THE BP#2 SEGMENTATION. 6 6 --- SEGMENTATION DATA --- 70.0 < r < 89.97 cm dr = 9.985 cm Nr = 2 bins 1036.0 < z < 1046.67 cm dz = 5.335 cm Nz = 2 bins 0.0 < φ < 360.0 deg. dφ = 30 deg. Nφ= 12 bins Ntot = 48 ''pieces'' IDS120j: yz ( LEFT ) AND yx ( RIGHT ) CROSS SECTION WITH DETAILS OF THE BP#1 SEGMENTATION. IDS120j: yz AT x = 0.0 cm [ LEFT ] AND yx AT z = 1040.0 cm [ RIGHT ] CROSS SECTION WITH DETAILS OF SC#7 SEGMENTATION. IN LEFT PLOT ONE CAN ALSO SEE DETAILS OF THE 20.0 cm GAP BETWEEN CRYOSTAT#2 AND CRYOSTAT#3. .

PEAK TDPD ~ 0.015 mW / g AT ABOUT 220, 285 deg AROUND THE -y AXIS AND AT z ~ 1225 cm . THERE IS LOT OF STATISTICAL FLUCTUATIONS DUE TO THE SMALL RADIAL BIN SIZE. SC#8 : SEGMENTATION TDP = 0.0102 kW VS. ONE VOLUME COIL TDP = 0.0106 kW FLUKA SC#8 TDP = 0.014 ± 0.006 kW SC#8 PEAK TDPD = 0.02 mW/g RADIAL / 0.02 mW/g AZIMUTHAL ( ± ??? ) ( JOHN BACK / JUNE 10 2012 ) . 9 7 Mars1510 (DESKTP) 5 E05 PEAK TDPD ~ 0.018 mW / g AT ABOUT 90 deg ( + y AXIS ) AT r2, z1 AND LITTLE AFTER THAT WE HAVE A SECOND PEAK ~ 0.0013 mW/g AT r1,z1. BOTH PEAKS ARE FOR “PIECES” FACING THE TARGET BUT AS ONE MAY EXPECT WE HAVE MORE STATISTICAL UNCERTAINTY. SINCE THE TWO PEAK VALUES ARE NOT MUCH DIFFERENT THOUGH ONE SHOULD NOT EXPECT A BIG CHANGE IN THE RESULT IF HIGHER STATISTICS IS USED. IT IS ALSO IMPORTANT TO NOTICE THAT TDP ~ 4.6 Watts AND IT WILL BE RATHER UNUSUAL A LOT OF THIS ENERGY TO BE FOCUSED IN A SMALL AREA IN A BIG COIL LIKE SC#9 LOCATED ~ 15 m DOWNSTREAM THE TARGET. SC#9: SEGMENTATION TDP = 0.0046 kW VS. ONE VOLUME COIL TDP = 0.0042 kW FLUKA SC#9 TDP = 0.005 ± 0.004 kW SC#7 PEAK TDPD = 0.03 mW/g RADIAL / 0.10 mW/g AZIMUTHAL ( ± ??? ) ( FROM JOHN BACK / JUNE 10 2012 ) . 7 PEAK TDPD < 0.06 mW / g. MOST OF THE DP IS BETWEEN -20 < z < 40 cm, AND THE LOWER HALF OF SC#1+2, TOWARDS THE + x DIRECTION . THIS IS THE RESULT OF REMOVING SHIELDING IN THE LOWER PART OF THE Hg MODULE AND REPLACING IT WITH LIQUID Hg. THE NEGATIVE IMPACT OF THE NEW Hg MODULE IN SH#1 IS GREATELY MITIGATED BY THE INTRODUCTION OF ~ 8 cm THICK CYLIDRICAL SHIELDING VOLUME AT R ~ 50 cm WHEN SH#1 AND SH#4 ARE UNIFIED INTO ONE VOLUME.

--- SEGMENTATION DATA --- IDS120j: yz AT x = 0.0 cm [ LEFT ] AND yx AT z = 1455.0 cm [ RIGHT ] CROSS SECTION WITH DETAILS OF SC#9 SEGMENTATION. COILS SC#7 AND SC#9 HAVE ABOUT THE SAME DIMENSIONS. IN LEFT PLOT ONE CAN ALSO SEE DETAILS OF THE 20.0 cm GAP BETWEEN CRYOSTAT#3 AND CRYOSTAT#4. . φ = 90O y y φ = 0O z x --- SEGMENTATION DATA --- 70.0 < r < 89.97 cm dr = 9.985 cm Nr = 2 bins 1453.0 < z < 1464.04 cm dz = 5.335 cm Nz = 2 bins 0.0 < φ < 360.0 deg. dφ = 30 deg. Nφ= 12 bins Ntot = 48 ''pieces'' IDS120j: yz ( LEFT ) AND yx ( RIGHT ) CROSS SECTION WITH DETAILS OF THE SC#1+2 SEGMENTATION. 18 10 9 X CROSS SECTION WITH DETAILS OF THE BP#2 SEGMENTATION. 6 6 --- SEGMENTATION DATA --- 70.0 < r < 89.97 cm dr = 9.985 cm Nr = 2 bins 1036.0 < z < 1046.67 cm dz = 5.335 cm Nz = 2 bins 0.0 < φ < 360.0 deg. dφ = 30 deg. Nφ= 12 bins Ntot = 48 ''pieces'' IDS120j: yz ( LEFT ) AND yx ( RIGHT ) CROSS SECTION WITH DETAILS OF THE BP#1 SEGMENTATION. IDS120j: yz AT x = 0.0 cm [ LEFT ] AND yx AT z = 1040.0 cm [ RIGHT ] CROSS SECTION WITH DETAILS OF SC#7 SEGMENTATION. IN LEFT PLOT ONE CAN ALSO SEE DETAILS OF THE 20.0 cm GAP BETWEEN DIPOLE#2 AND DIPOLE#3. .

PEAK TDPD ~ 0.018 mW / g AT ABOUT 90 deg ( + y AXIS ) AT r2, z1 AND LITTLE AFTER THAT WE HAVE A SECOND PEAK ~ 0.0013 mW/g AT r1,z1. BOTH PEAKS ARE FOR “PIECES” FACING THE TARGET BUT AS ONE MAY EXPECT WE HAVE MORE STATISTICAL UNCERTAINTY THAN IN SC#7 . SINCE THE TWO PEAK VALUES ARE NOT MUCH DIFFERENT ONE SHOULD NOT EXPECT A BIG CHANGE IN THE RESULT IF HIGHER STATISTICS IS USED. IT IS ALSO IMPORTANT TO NOTICE THAT TDP ~ 4.6 Watts AND IT WILL BE RATHER UNUSUAL A LOT OF THIS ENERGY TO BE FOCUSED IN A SMALL AREA IN A BIG COIL LIKE SC#9 LOCATED ~ 15 m DOWNSTREAM THE TARGET. SC#9: SEGMENTATION TDP = 0.0046 kW VS. ONE VOLUME COIL TDP = 0.0042 kW FLUKA SC#9 TDP = 0.005 ± 0.004 kW SC#7 PEAK TDPD = 0.03 mW/g RADIAL / 0.10 mW/g AZIMUTHAL ( ± ??? ) ( FROM JOHN BACK / JUNE 10 2012 ) . PEAK TDPD < 0.06 mW / g. MOST OF THE DP IS BETWEEN -20 < z < 40 cm, AND THE LOWER HALF OF SC#1+2, TOWARDS THE + x DIRECTION . THIS IS THE RESULT OF REMOVING SHIELDING IN THE LOWER PART OF THE Hg MODULE AND REPLACING IT WITH LIQUID Hg. THE NEGATIVE IMPACT OF THE NEW Hg MODULE IN SH#1 IS GREATELY MITIGATED BY THE INTRODUCTION OF ~ 8 cm THICK CYLIDRICAL SHIELDING VOLUME AT R ~ 50 cm WHEN SH#1 AND SH#4 ARE UNIFIED INTO ONE VOLUME. 12 7 7 Mars1510 (DESKTP) 5 E05 PEAK TDPD < 0.040 mW / g AT ABOUT 200 deg AT THE BOTTOM OF THE COIL (NEAR -x AXIS ) . THIS IS FOR z1 AND FOR BOTH r1, r2. THESE AREAS FACE UPSTREAM TOWARDS THE TARGET REGION. THE REASON FOR THE RELATIVE INCREASE IN THE TDP IN THE LOWER HALF OF THE COIL AND FOR THE UPSTREAM SIDE IS THE INCREASE OF THE Hg POOL LENGTH ALL THE WAY TO THE END OF THE FIRST CRYOSTAT AT THE EXPANCE OF W SHIELDING THERE. SC#7 : SEGMENTATION TDP = 0.0086 kW VS. ONE VOLUME COIL TDP = 0.0078 kW FLUKA SC#7 TDP = 0.008 ± 0.007 kW SC#7 PEAK TDPD = 0.03 mW/g RADIAL / 0.15 mW/g AZIMUTHAL ( ± ??? ) ( JOHN BACK / JUNE 10 2012 ) .

**** COMMENTS ON MARS AND FLUKA PEAK TDPD [ USING SC#7 CASE FOR EXAMPLE ] **** # SC#7 : VOLUME = 1.07 10^5 cc, Dens (NbTi ) =7.0 g/cc ==> Mass ~ 7.49 10^5 gr. # MARS: PEAK TDPD FROM SEGMENTATION ~ 0.04 mW / g. # FLUKA: PEAK TDPD AVERAGE(?) RADIAL ~ 0.03 mW / g AVERAGE(?) AZIMUTHAL ~ 0.15 mW / g -->??. # MARS: TDP ~ 7.8 Watts ( NO SEGMENT. ) ==> AVERAGE TDPD ( SC#7 VOLUME ) ~ 0.0104 mW/ g . FROM 48 SEGMENTATION “PIECES” ==> AVERAGE TDPD ~ 0.0139 mW/ g. THESE TWO NUMBER ARE IN GOOD AGREEMENT. # FLUKA: TDP ~ 8.0±7.0 Watts ==> AVERAGE TDPD FOR ALL VOLUME ~ FROM 0.0013 TO 0.02 mW/ g . IF WE CONSIDER THE MAXIMUM AVERAGE DENSITY OF 0.02 mW/g THERE IS STILL A HUGE GAP WITH THE AZIMUTHAL PEAK TDPD 0.15 mW/g ( EVEN WORSE IF THIS IS THE AVERAGE AZIMUTHAL TDPD ) # THERE IS SOMETHING STRANGE WITH FLUKA RESULTS ... >> ALSO P12 USED FOR SO FAR STUDIES IS EXTRACTED BY USING STUDY II OPTIMIZED P12 POINT BY BACTRACKING PROTONS ( OR TRAKING ANTIPROTONS ) FROM STUDY II P12 COORDINATES AT z = -37.5 cm. DING HAS NEVER WORKED OUT A SET OF OPTIMIZED POINTS FOR THE LATEST IDS120j. 13