/******************************************************************************* * McXtrace instrument definition URL=http://www.mcxtrace.org * * Instrument: MAXIV_Bloch * * %Identification * Written by: Kristian Soerensen and Philip Smith (s154443@win.dtu.dk) * Date: June 2018 * Origin: DTU Physics * Version: 1.7 * %INSTRUMENT_SITE: MAXIV * * Bloch high resolution photoelectron spectroscopy beamline under development at the MAX IV synchrotron. * * %Description * This is a simple simulation of the BLOCH beamline at MAXIV. * * Two kinds of parameters are given, P and P2. * P Parameters are the ones used in the general simulation, i.e when the FOI is intensity ect. * P2 parameters are used when the strain of the beamline is the FOI, i.e what happens when the distances change. * * %Test: E0=0.03 dE=0 undK=0 Nper=187 zm_mirror1=14 theta_mirror1=3 R0_M1=1 zm_mirror2=2 R0_M2=1 grating_mode=0 zm_mirror3=1 theta_mirror3=3 R0_M3=1 zm_ExitSlit=9 xwidth_ExSlit=0.005 yheight_ExSlit=0.005 zm_mirror4=19 theta_mirror4=3 R0_M4=1 SourceChoice=0 cff=2.25 m=3 Exitslit_yshift=2 Detector: M4Before_e_monitor_I=5.64942e-20 * %Test: E0=0.6 Detector: M4Before_e_monitor_I=2.6528e-21 * * %Parameters: * E0: [keV] The central energy to sample from source model. * dE: [keV] Spectral width to sample from source model. * Wanted_energy: [keV] The grating reflection energy. Uses E0 when not set. * SourceChoice: [0/1] Choice of souce. For easy simulation do Flat souce [0],in nonzero, the undulator is used. * r_rho: [l/mm] Ruling density of the grating. * cff: [ ] Constant cff value for the grating. * xwidth_ExSlit: [m] xwidth of exit slit. * yheight_ExSlit: [m] yheight of exit slit. * Exitslit_yshift: [m] y-shift of the exit slit. * m: [ ] Diffraction order, used for Monochromator angle. (fungerer ikke). * display: [ ] If nonzero, different output will be printet, e.g PGM angle calculated. * undK: [ ] Undulator K parameter, overrides E0, only used if SourceChoice is non zero. * lu: [m] Magnetic period length of the undulator. * Nper: [ ] Number of magnetic periods in the undulator. * grating_mode: [0/1] If 1 the NIM mode will be used. If 0 cPGM. Otherwise, optimum will be calculated. * MCAngle: [deg] Monte Carlo variation of grating. If wanted energy is given, MCAngle is found automaticaly. * zm_mirror1: [m] distance(z) to first mirror from previous component. * theta_mirror1: [m] glancing angle of first mirror. * R0_M1: [ ] Constant relectivity of Mirror2 [0;1]. * zm_mirror2: [m] distance(z) to mirror2 from previous component. * R0_M2: [ ] Constant relectivity of Mirror2 [0;1]. * zm_mirror3: [m] distance(z) to mirror3 from previous component. * theta_mirror3: [deg] glancing angle of mirror3. * R0_M3: [ ] Constant relectivity of Mirror3 [0;1]. * zm_ExitSlit: [m] distance from Mirror4 to exit slit. * zm_mirror4: [m] distance(z) to mirror4 from previous component. * theta_mirror4: [deg] glancing angle of mirror4. * R0_M4: [ ] Constant relectivity of Mirror4 [0;1] * verbose: [] Flag to print more information * perfectMirrors: [] When 0, a toroidal mirros is used, otherwise a plane mirror is used. * Error: [] When 1, alignment errors are applied randomly on the optics (from R. Sankari) * angle_grating: [deg] Additional tilt on the grating angle. * mirror2_angle: [deg] M2 angle used when grating_mode is 0, otherwise it is computed. * * %Link * Bloch_MAX IV description: https://www.maxiv.lu.se/accelerators-beamlines/beamlines/bloch/ * %Link * McXtrace komponent definition: http://www.mcxtrace.org * * %End *******************************************************************************/ DEFINE INSTRUMENT MAXIV_Bloch( Wanted_energy=0.378,m=3,cff=0, r_rho=800, SourceChoice=0,E0=0.6, dE=0.4, undK=5.6,Nper=187, grating_mode=-1, zm_mirror2=2,R0_M2=1, zm_mirror1=14,theta_mirror1=3,R0_M1=1, zm_mirror3=1,theta_mirror3=3,R0_M3=1, zm_mirror4=19,theta_mirror4=3,R0_M4=1, zm_ExitSlit=9,xwidth_ExSlit=1e-2,yheight_ExSlit=1e-2,Exitslit_yshift=0.005, int verbose=0,perfectMirrors=0,Error=0, angle_grating=6, mirror2_angle=6) /****************************************************** * *The DECLARE section is used to define parameters or small functions than can be used within the entire instrument. * *******************************************************/ DECLARE %{ /* values for the undulator */ int h; double E1st; /*For monitor energies*/ double monitor_wl_min,monitor_wl_max, monitor_Emin, monitor_Emax; /*Parameters for the slits*/ double slit_yshit; /* Angles used in the beamline */ double theta_cPGM, theta_PG_NIM, theta_NIM,theta_mirror2, PGM_theta; /*Parameters to find grating angle theta_cPGM.*/ double m, PGM_alpha, PGM_r_rho,PGM_beta,PGM_wl; /* Distances for monochromtor, for motivation see (R. Sabkari: "ARPES beamline at MAX IV: Detailed optical design report", 2014) */ double A,B,C,D,E,F,G,X; /* Parameters for errors */ double M2_theta_error,theta_PG1_error; double M2_theta_error,theta_PG1_error,X_error,y_error ,pitch_error ,yaw_error ,roll_error ,X_error_PGM ,Y_error_PGM ,Z_error_PGM, pitch_error_PGM ,yaw_error_PGM ,roll_error_PGM ,Z_error_exitSlit, Opening_error_exitslit; /* MISC*/ double R0_cPGM, R0_NIM,d; double MCAngleVariation; double d,a,bb,c,vinkel,beta_wl,beta_rho; //double angle_grating; double alpha,beta; //double mirror2_angle; %} /****************************************************** * *The INITIALIZE section is used to caculate/define/run jobs once. *You may use them as component parameter values. * *The INITIALIZE section is devided into several sub-secions. This is purly done for readability. * *******************************************************/ INITIALIZE %{ /* Description of initialize section: 1) Error section. 2) Undulator section. 3) Distances in monochromator section. 4) Calculate wanted energy and corresponding grating order. 5) Calculating angles used in the monochromator as defined from input parameters. 6) Monitor definitions. 7) Error messages. */ #include /****************************************************** 1) Errors: If Error=1, the error in accuracy will be implemented as a random error in the beamline. The errors are found from R. Sankari. These can easily be implemented. *******************************************************/ M2_theta_error=0;theta_PG1_error=0;X_error=0;y_error=0;pitch_error=0;yaw_error =0;roll_error=0;X_error_PGM =0;Y_error_PGM =0;Z_error_PGM=0; pitch_error_PGM =0;yaw_error_PGM =0;roll_error_PGM =0; Z_error_exitSlit=0;Opening_error_exitslit=0; if(Error) { M2_theta_error=rand01()*(0.01*(1/3600)); theta_PG1_error=rand01()*(0.02*(1/3600)); X_error = 5e-6*rand01(); y_error = 5e-6*rand01(); pitch_error =0.5e-6*rand01()*RAD2DEG; yaw_error = 0.5e-6*rand01()*RAD2DEG; roll_error = 5e-6*rand01()*RAD2DEG; X_error_PGM = 1e-4*rand01(); Y_error_PGM = 1e-4*rand01(); Z_error_PGM = 1e-4*rand01(); pitch_error_PGM =2e-6*rand01()*RAD2DEG; yaw_error_PGM = 2e-6*rand01()*RAD2DEG; roll_error_PGM = 2e-6*rand01()*RAD2DEG; Z_error_exitSlit = 1e-5*rand01(); Opening_error_exitslit = 1e-6*rand01(); } /****************************************************** 2) Calculate harmonic order(h) and fundamental harmonic(E1st) of the undulator If SourceChoice!=0 and undulator will be used. *******************************************************/ h=5; if (E0>15.757){ h=7; } else if (E0>20.253){ h=9; } else if (E0>24.753){ h=11; }else if (E0>29.254){ h=13; }else if (E0>33.755){ h=15; } E1st=1.0018*E0/h; /******************************************************* 3) Distances used in the Monochromator: *******************************************************/ A = 0.064819; B = -0.000125; C = 0.043821; D = 0.020; E = 0.620; F = 0.042; G = 0.140; X = 0.072746; theta_NIM = (M_PI_2-atan(F/X))*RAD2DEG; /******************************************************* 4) Finding wanted energy if none is given Finding grating mode if none is given *******************************************************/ if (!Wanted_energy){ /* If no wanted energy is given, it is assumed the wanted energy is E0. */ printf("Warning: No wanted energy is given. Default is E0=%f keV \n",E0); Wanted_energy = E0; } if(grating_mode!=1 && grating_mode!=0){ // If no grating mode is given, the grating mode will be found using the incoming energy. if(E0>=0.01 && E0<0.025){ grating_mode=1; printf("Exception: Cannot set range [nan, nan]No grating mode is given. The NIM mode will be used. \n"); } else if (E0>=0.025){ printf("No grating mode is given. The cPGM mode will be used.\n"); grating_mode=0; } else { printf("Warning:Energy below 1 keV (%f keV), NIM mode is used. \n", E0); grating_mode=0; } } /******************************************************* 5) Calculating the angle for the monochromator. For motivation, see Urpelainen, Samuli 2014. *******************************************************/ MCAngleVariation=5; /*If grating_mode=0, the cPGM will be used.*/ if (cff && !grating_mode){ beta_wl = (12.398/Wanted_energy)*pow(10,-10); beta_rho = 1/(r_rho*1000); a = (1-pow(cff,2)); bb = 2*pow(cff,2)*(m*beta_wl/beta_rho); c = pow(cff,2)-1-pow(cff,2)*((pow(m,2)*pow(beta_wl,2))/pow(beta_rho,2)); beta = asin((-bb+sqrt(pow(bb,2)-4*a*c))/(2*a)); alpha =acos(cos(beta)/cff); beta = (beta*RAD2DEG); alpha = alpha*RAD2DEG; angle_grating = (beta+90); mirror2_angle = ((180+beta-alpha)); mirror2_angle= mirror2_angle/2; // mirror2_angle = (90-blazed_angle+beta); mirror2_angle = (90+beta); } /*if(blazed && blazed_angle){*/ /* angle_grating = angle_grating-blazed_angle;*/ /*}*/ if(verbose){ fprintf(stdout,"INFO(%s):Monochromator specs: \n Angle of pre-mirror=%f deg. \n Angle of grating=%f deg.\n",instrument_name,mirror2_angle,angle_grating); } MCAngleVariation=angle_grating*0.99; /******************************************************* 6) Monitor definitions: *******************************************************/ if(E0 && dE){ monitor_Emin = E0-2*dE; monitor_Emax = E0+2*dE; } else if(E0 && !dE){ monitor_Emin = E0-3e-3; monitor_Emax = E0+3e-2; } else if (!E0){ printf("\n Error: No Energy is given! \n"); exit(-1); } monitor_wl_max = 12.3984/monitor_Emin; monitor_wl_min = 12.3984/monitor_Emax; /******************************************************* 7) Error messages: *******************************************************/ if (angle_grating>30 || angle_grating<0) { fprintf(stderr,"ERROR: cPGM grating angle is out of bounds(%f DEG). Simulation ended.\n",angle_grating); exit(-1); } if (mirror2_angle>21 || mirror2_angle<0) { fprintf(stderr,"ERROR: M2 angle is out of bounds(%f DEG). Simulation ended.\n",mirror2_angle); exit(-1); } if (theta_PG_NIM>30 || theta_PG_NIM<0) { fprintf(stderr,"ERROR: NIM grating angle is out of bounds(%f DEG). Simulation ended.\n",theta_PG_NIM); exit(-1); } %} /************************************************************** * *Trace section: *The TRACE section is where the actual components are placed. * **************************************************************/ TRACE COMPONENT origin = Progress_bar() AT (0, 1.3, 0) RELATIVE ABSOLUTE /************************************************************** Sources: 1) When SourceChoice=0 the flat source is used. 2) When SourceChoice=1 the undulator is used. The TRACE option in the McXtrace GUI IS NOT possible when using the undulator. using the Undulator: Harmonics are found in initialize. Find general info on the undulator at: https://www.maxiv.lu.se/accelerators-beamlines/technology/insertion-devices/ Find general info on the 1.5 GeV storage ring at: https://www.maxiv.lu.se/accelerators-beamlines/accelerators/accelerator-documentation/1-5-gev-storage-ring/ Find live info on the 1.5 storage ring at: **************************************************************/ COMPONENT source_flat = Source_flat( yheight=0.001e-5,xwidth=0.001,dist=zm_mirror1,focus_xw=0.02e-6,focus_yh=0.02,E0=E0,dE=dE) WHEN (!SourceChoice) AT (0, 0, 0) RELATIVE origin EXTEND %{ do { double k=sqrt(kx*kx+ky*ky+kz*kz); kx=ky=0;kz=k; }while(0); %} /*COMPONENT dmu = Undulator(verbose=1,E0=E0,dE=dE,Ee=1.5,dEe=((6e-9)*(60e-12))/1.5,Ie=0.5,tbunch=43,K=undK,gap=14e-3,Nper=Nper, */ /* lu=84e-3,sigey=1.3e-5,sigex=185e-5,sigepx=32e-6,sigepy=4.6e-6,focus_xw=1.1e-3,focus_yh=1.1e-3,dist=zm_mirror1,E1st=E1st)*/ /*WHEN (SourceChoice)*/ /*AT(0,0,0) RELATIVE origin*/ /**************************************** Monitors After source: ****************************************/ COMPONENT Source_E_monitor = E_monitor(nE=101,filename="source_E_monitor",xwidth=5e-3,yheight=5e-3,Emin=monitor_Emin,Emax=monitor_Emax,restore_xray=1) AT (0, 0, 1) RELATIVE PREVIOUS /*COMPONENT Source_wl_monitor = L_monitor(nL=101,filename="source_wl_monitor",xwidth=5e-3,yheight=5e-3,Lmin=monitor_wl_min,Lmax=monitor_wl_max,restore_xray=1)*/ /*AT (0, 0, 0) RELATIVE PREVIOUS*/ COMPONENT Source_psd_monitor = PSD_monitor(filename="Source_psd_monitor",restore_xray=1,nx = 271,ny = 271,xwidth=0.06,yheight=0.06) AT (0, 0, 0.0) RELATIVE PREVIOUS /************************************************************** M1: toroidial mirror 1) When perfectMirrors=0, a toroidal mirros is used: - collimates vertically - focuses horizontally 2) When perfectMirrors=1, a plane mirror is used. **************************************************************/ COMPONENT M1_arm= Arm() AT(0,0,zm_mirror1) RELATIVE origin ROTATED (0,0,90) RELATIVE origin COMPONENT Mirror_toroid = Mirror_toroid(zdepth=0.340,xwidth=0.020,radius=246.9254,radius_o=246.9254,R0=R0_M1) WHEN (!perfectMirrors) AT (0, 0, 0) RELATIVE M1_arm ROTATED (-theta_mirror1, 0, 0) RELATIVE M1_arm COMPONENT M1_perfect_mirror = Mirror(zdepth=0.34,xwidth=0.02,R0=R0_M1) WHEN (perfectMirrors) AT (0, 0, 0) RELATIVE M1_arm ROTATED (-theta_mirror1,0, 0) RELATIVE M1_arm /**************************************** Monitors After Toroidal Mirror: ****************************************/ COMPONENT Toroidal_Monitor_arm1= Arm() AT(0,0,zm_mirror1) RELATIVE origin ROTATED (0,-2*theta_mirror1,0) RELATIVE origin COMPONENT Toroidal_Monitor_arm2= Arm() AT(0,0,1) RELATIVE Toroidal_Monitor_arm1 ROTATED (0,90,90) RELATIVE Toroidal_Monitor_arm1 COMPONENT M1_E_monitor = E_monitor(nE=101,filename="M1_E_monitor", xwidth=0.06,yheight=0.06,Emin=monitor_Emin,Emax=monitor_Emax,restore_xray=1) AT (0, 0, 0) RELATIVE PREVIOUS ROTATED (90,0,90) RELATIVE PREVIOUS /*COMPONENT M1_wl_monitor = L_monitor(nL=101,filename="M1_wl_monitor",xwidth=0.06,yheight=0.06,Lmin=monitor_wl_min,Lmax=monitor_wl_max,restore_xray=1)*/ /*AT (0, 0, 0) RELATIVE PREVIOUS*/ COMPONENT M1_psd_monitor = PSD_monitor(filename="M1_psd_monitor",nx = 21,ny = 21,xwidth=0.06,yheight=0.06,restore_xray=1) AT (0, 0, 0) RELATIVE PREVIOUS /************************************************************** cPGM mode: 1) Arms are placed to define rotation axis. 2) If perfect mirrors are used, grating will be removed, orherwise, blazed should be used. **************************************************************/ /*Rotation arms*/ COMPONENT cPGM_arm= Arm() AT(0,0,zm_mirror1) RELATIVE origin ROTATED (0,-2*theta_mirror1,0) RELATIVE origin COMPONENT PG1_arm= Arm() AT(0,F,2) RELATIVE cPGM_arm ROTATED (0,0,0) RELATIVE cPGM_arm COMPONENT M2_rotation_arm1= Arm() AT(0,A-F,B) RELATIVE PG1_arm ROTATED (-mirror2_angle+M2_theta_error,0,0) RELATIVE PG1_arm COMPONENT M2_rotation_arm2= Arm() AT(0,0,-D-(E/2)) RELATIVE M2_rotation_arm1 ROTATED (0,0,0) RELATIVE M2_rotation_arm1 COMPONENT M2_rotation_arm3= Arm() AT(0,-C,0) RELATIVE M2_rotation_arm2 ROTATED (0,0,0) RELATIVE M2_rotation_arm2 /*Mirror and grating*/ COMPONENT mirror2 = Mirror( zdepth=0.57,xwidth=0.015,R0=R0_M2) WHEN (!grating_mode) AT (0, 0, 0) RELATIVE M2_rotation_arm3 ROTATED (0,0, 0) RELATIVE M2_rotation_arm3 COMPONENT pg_a = Arm() AT (0, 0, 0) RELATIVE PG1_arm ROTATED (-angle_grating,0, 0) RELATIVE PG1_arm COMPONENT Plane_grating2 = Grating_reflect( d_phi=MCAngleVariation/100, rho_l=r_rho, zdepth=0.136,xwidth=0.015) WHEN(grating_mode==0) AT(0,0,0) RELATIVE PG1_arm ROTATED(-angle_grating,0,180) RELATIVE PG1_arm COMPONENT postPgmfpi=PSD_monitor_4PI(filename="postpgm",radius=1, restore_xray=1) AT(0,0,0) RELATIVE PREVIOUS COMPONENT psd2ma = Arm() AT(0,0,0) RELATIVE pg_a ROTATED (angle_grating,0,0) RELATIVE pg_a COMPONENT vbanana = Monitor_nD(xwidth=1,yheight=0.1,options="banana theta limits -6 6 energy limits 0.1 1.1", bins=1001, filename="vbanana",restore_xray=1) AT(0,0,0) RELATIVE psd2ma ROTATED (0,0,90) RELATIVE psd2ma COMPONENT psd2m = PSD_monitor(nx=1,ny=501, yheight=0.5, xwidth=0.1, filename="psd2m", restore_xray=1) AT(0,0,2) RELATIVE psd2ma /**/ /*COMPONENT Plane_grating_perfect_mirror = Mirror(*/ /* zdepth=0.136,xwidth=0.015,R0=R0_PG)*/ /*WHEN (!grating_mode && perfectMirrors)*/ /*AT (0, 0, 0) RELATIVE PG1_arm*/ /*ROTATED (-angle_grating,0, 0) RELATIVE PG1_arm*/ /**/ /************************************************************** NIM mode: 1) Arm for the NIM mirror is placed 2) lamellar grating is used There is no reason for a perfect mirror in the NIM case. **************************************************************/ /*COMPONENT NIM_arm1= Arm()*/ /*AT(0,-A,X) RELATIVE M2_rotation_arm1*/ /*ROTATED (0,0,0) RELATIVE M2_rotation_arm1*/ /**/ /*COMPONENT NIM = Mirror(*/ /* zdepth=0.02,xwidth=0.02,R0=0) */ /*WHEN (!grating_mode)*/ /*AT (0, 0, 0) RELATIVE PREVIOUS*/ /*ROTATED (-theta_NIM,-2*theta_mirror1, 0) RELATIVE origin*/ /**/ /*COMPONENT Laminar_Grating = Reflective_grating(*/ /* d_phi=4,blazed=0,cff=0,display=0,blazed_angle=0,zdepth=0.136,xwidth=0.015,R0=R0_PG,r_rho=r_rho,b=0,N_slits=0,d=0)*/ /*WHEN (grating_mode)*/ /*AT (0, 0, 0) RELATIVE PG1_arm*/ /*ROTATED (-theta_PG_NIM,0, 0) RELATIVE PG1_arm*/ /**************************************** Monitors After Monochromator ****************************************/ COMPONENT Monochromator_Monitor_arm= Arm() AT(0,F,2.7) RELATIVE PG1_arm ROTATED (0,0,0) RELATIVE PG1_arm COMPONENT Monochromator_E_monitor = E_monitor(nE=101,filename="AfterMonochromator_E_monitor", xwidth=0.06,yheight=0.06+(F/8),Emin=monitor_Emin,Emax=monitor_Emax,restore_xray=1) AT (0, 0, 0) RELATIVE PREVIOUS ROTATED (0,0,0) RELATIVE PREVIOUS /*COMPONENT Monochromator_wl_monitor = L_monitor(nL=101,filename="AfterMonochromator_wl_monitor",xwidth=0.06,yheight=0.06+(F/8),Lmin=monitor_wl_min,Lmax=monitor_wl_max,restore_xray=1)*/ /*AT (0, 0, 0) RELATIVE PREVIOUS*/ COMPONENT Monochromator_psd_monitor = PSD_monitor(filename="AfterMonochromator_psd_monitor",nx = 40,ny = 100,xwidth=0.06,yheight=0.06+(F/8),restore_xray=1) AT (0, 0, 0) RELATIVE PREVIOUS /************************************************************** Mirror 3: 1) M3_Arm to point in M3 location: -Even though the monochromator is rotating, the cylindrical mirror has to stay stationary relative to M2 2) Plane mirror in place of the true cylindrical mirror (which isnt developed in McXtrace) - Deflect horizontally **************************************************************/ COMPONENT M3_arm= Arm() AT(0,F,3) RELATIVE cPGM_arm ROTATED (0,theta_mirror3,0) RELATIVE cPGM_arm COMPONENT m3Psd=PSD_monitor(xwidth=0.5, yheight=0.5, filename="m3psd", restore_xray=1) AT(0,0,0) RELATIVE M3_arm COMPONENT mirror3 = Mirror_curved( R0=1, radius=0.94205, length=0.06, width=0.2) AT (0, 0, 0) RELATIVE M3_arm ROTATED (90, 0, 0) RELATIVE M3_arm EXTEND %{ /* if(!SCATTERED){*/ /* ABSORB;*/ /* }*/ %} /* else{*/ /* printf("through\n");*/ /* }*/ /*%}*/ /**/ /*COMPONENT mirror3_perfect_mirror = Mirror(*/ /* zdepth=0.2, */ /* xwidth=0.06, */ /* R0=1)*/ /*WHEN(perfectMirrors)*/ /*AT (0, 0, 0) RELATIVE M3_arm*/ /*ROTATED (0, 0, 90) RELATIVE M3_arm*/ /**/ COMPONENT Exit_slit_arm0= Arm() AT(0,0,0) RELATIVE M3_arm ROTATED (0,0,0) RELATIVE M3_arm COMPONENT M4_arm1= Arm() AT(0,0,0) RELATIVE Exit_slit_arm0 ROTATED (0,theta_mirror3,0) RELATIVE Exit_slit_arm0 /**************************************** Monitors After Mirror 3 ****************************************/ COMPONENT M3_Monitor_arm= Arm() AT(0,0,0.5) RELATIVE M4_arm1 ROTATED (0,0,0) RELATIVE M4_arm1 COMPONENT M3_E_monitor = E_monitor(nE=101,filename="M3_E_monitor", xwidth=0.04,yheight=0.03,Emin=monitor_Emin,Emax=monitor_Emax,restore_xray=1) AT (0, 0, 0) RELATIVE PREVIOUS ROTATED (0,0,0) RELATIVE PREVIOUS /*COMPONENT M3_wl_monitor = L_monitor(nL=101,filename="M3_wl_monitor",xwidth=0.04,yheight=0.03,Lmin=monitor_wl_min,Lmax=monitor_wl_max,restore_xray=1)*/ /*AT (0, 0, 0) RELATIVE PREVIOUS*/ COMPONENT M3_psd_monitor = PSD_monitor(filename="M3_psd_monitor",nx = 171,ny = 171,xwidth=0.04,yheight=0.03,restore_xray=1) AT (0, 0, 0) RELATIVE PREVIOUS /************************************************************** EXIT SLIT: 1)Exit slit placed in front of mirror 4 2) based on input parameters, different photons will be let through, i.e different wavelengths. *************************************************************/ COMPONENT ExT_arm2= Arm() AT(0,0,zm_ExitSlit) RELATIVE M4_arm1 ROTATED (0,0,0) RELATIVE M4_arm1 COMPONENT bef_slit = PSD_monitor(xwidth=3*xwidth_ExSlit, yheight=3*yheight_ExSlit, filename="bef_slit") AT(0,0,-1e-3) RELATIVE ExT_arm2 COMPONENT Exitslit = Slit( xwidth=xwidth_ExSlit, yheight=yheight_ExSlit) AT (0, 0,0) RELATIVE ExT_arm2 ROTATED (0,0,0) RELATIVE ExT_arm2 COMPONENT aft_slit = COPY(bef_slit)(filename="aft_slit") AT(0,0,1e-3) RELATIVE ExT_arm2 /**************************************** Monitors Before Mirror 4 ****************************************/ COMPONENT M4Before_psd_monitor = PSD_monitor(filename="M4Before_psd_monitor",restore_xray=1,nx = 271,ny = 271,xwidth=0.2,yheight=0.2) AT (0, 0, 1) RELATIVE Exitslit COMPONENT M4Before_e_monitor = E_monitor(nE=101,filename="M4Before_e_monitor",xwidth=0.2,yheight=0.2,Emin=0,Emax=2,restore_xray=1) AT (0, 0, 1) RELATIVE Exitslit /*COMPONENT M4Before_wl_monitor = L_monitor(nL=101,filename="M4Before_wl_monitor",xwidth=0.2,yheight=0.2,Lmin=monitor_wl_min,Lmax=monitor_wl_max,restore_xray=1)*/ /*AT (0, 0, 1) RELATIVE Exitslit*/ /************************************************************** Mirror 4 1) Placing an arm 2) Placing a plane mirror instead of a ellipsoidal mirror for simplicity. - deflect horizontally. **************************************************************/ COMPONENT M4_arm2= Arm() AT(0,0,zm_mirror4) RELATIVE M4_arm1 ROTATED (0,theta_mirror4,0) RELATIVE M4_arm1 COMPONENT mirror4 = Mirror( zdepth=0.2,yheight=0.06,R0=R0_M4) AT (0, 0, 0) RELATIVE M4_arm2 ROTATED (0, 0, 0) RELATIVE M4_arm2 /**************************************** Monitors After Mirror 4 ****************************************/ COMPONENT M4_Monitor_Arm= Arm() AT(0,0,0) RELATIVE mirror4 ROTATED (0,theta_mirror4,0) RELATIVE mirror4 COMPONENT M4_psd_monitor = PSD_monitor(filename="M4_psd_monitor",restore_xray=1,nx = 271,ny = 271,xwidth=0.06,yheight=0.06) AT (0, 0, 0.3) RELATIVE PREVIOUS ROTATED (0,0,0) RELATIVE PREVIOUS COMPONENT M4_e_monitor = E_monitor(nE=101,filename="M4_e_monitor",xwidth=0.06,yheight=0.06,Emin=0,Emax=2,restore_xray=1) AT (0, 0, 0) RELATIVE PREVIOUS /*COMPONENT M4_wl_monitor = L_monitor(nL=101,filename="M4_wl_monitor",xwidth=0.06,yheight=0.06,Lmin=monitor_wl_min,Lmax=monitor_wl_max,restore_xray=1)*/ /*AT (0, 0, 0) RELATIVE PREVIOUS*/ /* COMPONENT Filter_Argon = Filter( material_datafile="Ar.txt", xwidth=0.2, yheight=0.2, zdepth=0.2) WHEN(E0>0.0015759) AT (0, 0, 0.5) RELATIVE M4_Monitor_Arm COMPONENT Filter_Neon = Filter( material_datafile="Ne.txt", xwidth=0.2, yheight=0.2, zdepth=0.2) WHEN(E0>0.0021565) AT (0, 0, 0.4) RELATIVE PREVIOUS COMPONENT Filter_Helium = Filter( material_datafile="He.txt", xwidth=0.2, yheight=0.2, zdepth=0.2) WHEN(E0>0.0024587) AT (0, 0, 0.4) RELATIVE PREVIOUS COMPONENT Filter_psd_monitor = PSD_monitor(filename="Filter_psd_monitor",restore_xray=0,nx = 271,ny = 271,xwidth=0.06,yheight=0.06) AT (0, 0, 1) RELATIVE PREVIOUS ROTATED (0,0,90) RELATIVE M4_Monitor_Arm COMPONENT Filter_e_monitor = E_monitor(nE=101,filename="Filter_e_monitor",xwidth=0.06,yheight=0.06,Emin=0,Emax=50,restore_xray=0) AT (0, 0, 0) RELATIVE M4_Monitor_Arm COMPONENT Filter_wl_monitor = L_monitor(nL=101,filename="Filter_wl_monitor",xwidth=0.06,yheight=0.06,Lmin=monitor_wl_min,Lmax=monitor_wl_max,restore_xray=0) AT (0, 0, 0) RELATIVE M4_Monitor_Arm */ /************************************************************** Experiment hutch: - sample station - monitor - detector - sample ect.. **************************************************************/ FINALLY %{ %} END