DS/CSEF/06 May 3rd, 2004 Ladi3@H112 guide simulation: effect of a double curved guide From: E. Farhi to: R. Gaehler, P. Timmins, W. Press, C. Vettier cc: C. Carlile, M. Johnson, I. Sutton, D. Bazzoli On the request of C. Vettier and R. Gaehler, a model of the future H112 cold guide upper channel has been simulated. This project aims at positioning the LADI instrument on 'ILL7 2nd floor' , at one meter up from the present guide system, and in between the H22 and H23 thermal guides. The H112 model is curved both horizontally (Rh=1.5 km) and vertically (Rv=2 km), and fully coated with m=2 super mirror. Substantial flux gains (factor 2 to 4) will be obtained, compared to H142. Moreover, the beam will be naturally prefocussed, without loosing on divergence. Such prefocussing, resulting from the guide curvature, may also be envisaged for the horizontal reflectometer (which would require a vertically curved guide). The H112 Guide description The H112 guide project is still under design process. Anyway, the geometrical constrains are quite strong, as it has to fit in the middle of the H22 and H23 thermal guides, and be bent enough to come at a usable upper plane (say 1 meter up). Today, the envisaged geometry is a double bent guide (1.5 km horizontally, 2 km vertically), made of 1 meter elements, along about 80 meters [2]. The coating would be full m=2 super mirror (including inpile part). Section would be 12h x 6w (in cm2), splitted into 3h x 6w and 8h x 6w after 30 meters. The simulated guide model contains the elements listed in Table 1. Aluminium windows and gaps are in the model. The coating is assumed to produce a constant SM92 reflectivity curve (given by the mean value in the decreasing sloppy region, with Rm=1=0.99 and Rm=2=0.84). Actually, super mirrors in production today may reach much better specifications (Rm=2=0.92), which would bring even more flux as the current simulation results. Anyway, using a lower reflectivity is a way to take into account imperfections such as the guide misalignments, the coating and substrate inhomogeneities, the waviness, etc. The VCS specifications are taken from [1]. The Figure 1 shows a view of the model. The guide alignment is considered to be perfect. The simulation package is McStas [3] version 1.8. Similar simulations where carried out in 2001, and are reported in [4,6]. Element Detail of model Specifications Source Vertical Cold Source [1] 22h x 14w [cm2] Pink Carter Focusing, m=2 coating w=68>60 mm, h=12 cm, L=3.17 m Lead Shutter m=2 L=0.228 m H1122 Polygonal, 6 elements, m=2 L=6.1 m, w=60 mm, h=120 mm, ρ=1.5 km Vacuum space For the V.S L=0.2 m H1123, H1124, H1125 Polygonal, 20 elements, m=2 L= 20.5 m, w=60 mm, h=120 mm, ρ h=1.5 km, ρ v=2.0 km Vacuum space For the V.T.E. Guide splitting L=0.33 m H1126, H1127, H1128, H1129, H11210 Polygonal, 50 elements, m=2 End of guide: Ladi3 position (Sample is at 3 m) L=50 m, w=60 mm, h=30 mm, ρ h=1.5 km, ρ v=2.0 km Table 1: H112 guide geometry [2]. H112 Ladi3 Rv=2.0 Rh=1.5 m=2 135 elements 11 monitors includes gaps Source (VCS) 0 Ladi3 position y/[m] 20 40 Guide splitting 1 0.5 60 0 1.5 1 0.5 x/[m] z/[m] 0 80 Figure 1: Geometric view of the H112 guide model, as seen from the IN12 side of ILL7 building. Simulated neutron flux The H112 end of guide monitors provide flux estimates that may be compared with previous simulated results [4]. We find (see Table 2) about the same capture and integrated flux as in the previous H112 simulation carried out for the EDM experiment. Indeed, the main differences are in the total length (was 100 meters in previous simulation) and the curvature radius (was 2.7 km horizontal in previous simulation). The geometry is also slightly different. This is why the spectral distribution is a little different (see Figure 2), providing more cold neutrons for this project, as the curvature is more pronounced than any other cold guide. Φc [n/s/cm2] Guide Φ [n/s/cm2] dφ/dλ [n/s/cm2/Å] at λ ∼ 5 Å (gold foil) 28.1 109 6.3 109 8.9 108 H112 Rv=2 km 26.6 109 5.7 109 8.2 108 H113 (PF1b) 3.7 109 4.5 108 H112 (EDM) 28.1 109 (Rh=2.7 km) 7.3 109 1.1 109 H142 (LADI) 6.2 109 (Scurved) (Measured: 3 107 at λ ∼ 3.5 Å ±10 %) H112 Rv=0 15.2 109 (Measured: 16 109) 1.6 109 Table 2: Flux estimates for H112 guide model, as well as a few previous results [4] When looking at H113 (somewhat similar geometry as the current H112 project) and H142 (present LADI position), we estimate gain factors of about 1.7 and 4 in capture fluxes respectively. The flux measurement for H142 is given when using a 20% bandwidth filter, which transmission efficiency is not included in the simulation. Upgrading the inpile part to m=2 for both H112 and H113 will probably bring these two guide fluxes to similar values (increasing the H113 one). 12 x 10 8 H112 Ladi3 Rv=0 Rh=1.5 m=2 H112 Ladi3 Rv=2.0 Rh=1.5 m=2 H112 EDM Rv=0 Rh=2.7 m=2 H113 PF1b Rv=0 Rh=4.0 m=1.2/2 H142 Ladi3 Rv=0 Rh=+/2.7 m=1 Intensity Φ [n/s/cm 2 /Angs] 10 8 6 4 2 0 0 5 10 λ [Angs] 15 20 Figure 2: Flux as a function of the wavelength at the H112 Ladi3 position, compared with previous results [4]. The vertical Rv and horizontal Rh guide curvature, as well as the coating m are indicated. Monitors positioned along the guides provide an estimate of the flux as a function of the distance to the moderator (see Figure 3), which is related to the neutron losses. Close to the moderator, the H112 flux is higher than for the H113 and H142 guides, which use m=1.2 Ni58 coating at the beginning. The inpile part upgrade brings more neutrons. Then the H112 flux loss is comparable to the H15, which has quite a few gaps for the instruments, and H142, which is a long continuous Scurved guide without major gaps until IN12. In these latter guides, many neutrons are lost in the inpile part, and the remaining neutrons are kept efficiently to the end of the guide. The H113 guide has a ballistic shape (and no major gap), which reduces the flux loss. A few capture flux (gold foil) measurements are also presented in Figure 3 (at the end of the guides), and found in good agreement with simulations. inpile m=2 11 Capture flux Φc [n/s/cm 2] 10 10 H15 H15 measured H142 H142 measured H113 H113 measured H112 Rv=0 H112 Rv=2.0 km splitting m=2 ballistic guide m=1.2/2 10 m=1.2 20 40 60 Distance from VCS [m] 80 100 Figure 3: Flux along the H112 guide, compared with previous results [4]. For H112, the vertical Rv guide curvature is indicated. Rh is 1.5 km, and m=2. Simulated spatial and divergence distributions In order to estimate the beam distributions at the LADI instrument, we have positioned monitors just at the end of the guide. The instrument sample position itself should come after a 3 m beam tube, with filters, slits and shields. 0.015 [H112 Rv=0] PSD at the end of the guide [H112 Rv=2 km] PSD at the end of the guide 0.015 0.01 0.005 0.005 y [m] 0.01 0 0.005 0.005 0.01 0.01 0.015 0.03 0.02 0.01 0 x [m] 0.01 0.02 0 0.015 0.03 0.02 0.01 0 x [m] 0.01 0.02 Figure 4: Neutron beam spatial distribution (PSD) at the exit of the H112 curved guide, at λ=5 Å. For both plots, the horizontal curvature is Rh=1.5 km. The plot on the right has an additional Rv=2 km vertical curvature. Dimensions are in meters. Intensity scale goes from the white (low) to black (high). Coating is m=2. The analytical models [5,6] for curved guide do predict a shifting of the beam after a curved guide. This shift is removed when adding a long enough straight section downstream. Looking at the Figure 4 – left plot, this effect is indeed observed as expected: the beam intensity on the outer curvature side is 70 % higher than that of the inner side. In the case of a horizontal and vertical curved guide, the shift occurs in both directions as presented in Figure 4 – right plot, and finally the beam is gathered in one corner of the guide, producing a natural focusing which might be of great interest for Laue diffractometers such as LADI. The ratio of the maximum to the minimum intensity in the guide section is about 2. Other instruments such as horizontal reflectometers may also benefit from vertically curved guide which would produce well defined prefocussed horizontal beams. [H112] guide end divergence ( α on X, β on Y) 1.4 ∆α Rv=0 ∆β Rv=0 ∆α Rv=2 ∆β Rv=2 Divergence half width [deg] 1.2 1 0.8 0.6 0.4 0.2 0 0 5 10 λ [Angs] 15 20 Figure 5: Neutron beam divergence half width ∆α (on X) and ∆β (on Y) at the end of H112 as a function of the wavelength at the end of the H112 guide, with a vertical curvature Rv of 0 and 2 km. Coating is m=2. The divergence (see Figure 5) is close to the well known linear law for long guides. The vertical curvature has a small effect on the vertical divergence, which is lowered at small wavelengths (for λ < 5 Å ). Intensity ratio Min/Max on PSD [a.u.] 1 [H112] Spatial anisotropy at 80 m 0.8 0.6 Rv=0 Rv=2 km 0.4 0.2 5 10 λ [Angs] 15 20 Figure 6: Gravitation effect: spatial vertical anisotropy measured as the ratio of the top over the bottom intensity of the projection of the PSD over the vertical axis, at the end of the H112 guide with Rh=1.5 km, Rv=0 and 2 km, m=2. In order to estimate the effect of the gravitation at the end of the H112 guide, at 80 meters from the moderator, we have plotted on Figure 6 the ratio of the top over the bottom intensity extracted from the PSD projection on the vertical axis. When the vertical curvature Rv is zero (inplane), the anisotropy becomes sensible only for λ > 710 Å. For 20 Å cold neutrons, the gravitation stacks about 14 % more flux on the bottom part than on the upper part of the beam. Concerning the H112 model with vertical curvature, the effects are more pronounced. For low wavelengths, only garland reflections may occur in the guide, and the neutrons are stacked to the lower part. Then, reaching the guide critical wavelength (which is around 1.9 Å), the anisotropy is optimal (with still 10 % more neutrons on the bottom part), and becomes slowly worse for cold neutrons, reaching 25 % vertical anisotropy. This anisotropy will control the size and position of the slits for optimal beam flux. Conclusions It is clear that high flux gains (factor 2 to 4 compared to H142) will be reached with this new H112 guide. Moreover, the curved guide prefocusing will be useful to the LADI instrument. Anyway, as this is a super mirror guide, the divergence will be doubled compared to the actual H142 one, and the background level may be higher, even if the short curvature radius is expected to be very efficient for hot and thermal neutron filtering. Even if these flux gains might be overestimated (guide is perfectly aligned, glass quality is constant and reflectivity is high), we believe that the present H113 flux will be easily reached. References [1] P. Ageron, Nucl. Instr. Meth., A284 (1989) 197. [2] ILL Drawing AP0501002 IJ Sutton ' Guide H112 Avant projet Implantation Ladi III Option B' [3] McStas, <http://www.ill.fr/tas/mcstas> [4] ILL Internal Report DSCSEF/72/01 – October 26, 2001. <http://www.ill.fr/tas/mcstas/instruments/ill/h112/Report.pdf> [5] D.F.R. Mildner, Nucl. Inst. Meth. In Phys. Research, A 290 (1990) 189. [6] ILL Internal Report DSCSEF – February 16, 2001. <http://www.ill.fr/tas/mcstas/instruments/ill/h15/R010216.ps.gz>
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