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Electromagnetic design of superconducting dipoles based on sector coils

Electromagnetic design of superconducting dipoles based on sector coils Accelerator Technology Department, CERN, CH-1211 Geneva, Switzerland (Received 2 August 2007; published 30 November 2007) We study the coil layouts of superconducting dipoles for particle accelerators based on the sector geometry. We show that a simple model based on a sector coil with a wedge allows us to derive an equation giving the short sample field as a function of the aperture, coil width, cable properties, and superconducting material. The equation agrees well with the actual results of several dipole coils that have been built in the past 30 years. The improvements due to the grading technique and the iron yoke are also studied. The proposed equation can be used as a benchmark to judge the efficiency of the coil design, and to carry out a global optimization of an accelerator layout. DOI: 10.1103/PhysRevSTAB.10.112401 PACS numbers: 07.55.Db, 41.85.Lc, 84.71.Ba, 85.70.Ay I. INTRODUCTION Superconducting dipoles have been used for 30 years to bend particle beams in accelerator machines. Fields of 4 to 10 T have been reached with electromagnets based on NbTi cables [1–7], whose critical field at 1.9 K is around 13 T. A new generation based on the Nb3 Sn has allowed to break the 10 T barrier, such as the CERN-Elin [8], the MSUT [9] of the Twente University –CERN (11 T), and the D20 [10] made in Lawrence Berkeley Laboratory (13 T). Tests of a more recent Nb3 Sn conductor in a block configuration magnet [11,12] showed that the material can reach 16 T (LBNL HDI), and programs to obtain large fields in acceleratorlike magnets are ongoing [12 –14]. This technology would have the potential to double the energy of the Large Hadron Collider (LHC). The simplest way to create a pure dipolar field is to have an annulus where the current density is proportional to the cosine of the azimuth ( cos coil). In practical layouts, the current density has to be constant and conductors are piled up in blocks separated by spacers. This arrangement aims at approximating a cos coil with a finite number of blocks carrying the same constant current density. One defines a cos layout when the shape of the coil is still an annulus, thus providing a self-supporting structure, and the blocks are shaped as sectors. Most of the dipole coils have been based on this layout [15,16], with different number of layers and of spacers. Alternative layouts are based on rectangular blocks [12]. The aim of this paper is to find approximate equations that provide the field reachable in a given aperture with a given quantity of conductor, and to estimate what are the most effective design options among the ones that have been chosen in the past. The approach is analogous to what has been done for the quadrupoles [17]: we carry out an exhaustive analysis of the sector coil models (i.e., cos layouts), using semianalytical tools when the pure analytical approach is not viable. The sector coil models are slightly more representative than the cos coil (i.e. the ideal coil with current density 1098-4402=07=10(11)=112401(12) depending on the azimuth), which has been extensively studied in [18,19], since they include the difference between central field and peak field in the coil. This difference is not negligible when the ratio between the coil width and the aperture radius is small, such as in the RHIC dipoles [4]. The extension of this analysis to alternative layouts such as the block coil or the common coil will be presented separately. The final aim of the work is to have handy formulas to be able to carry out a global optimization of the parameters of an accelerator or of a part of it, and a dimension/cost estimate. In Sec. II we present the equations for the short sample field for the Nb-Ti and Nb3 Sn. The analysis of the sector layouts is given in Sec. III, including a comparison between different designs, dependence on coil width and magnet apertures, and grading techniques. The analysis of the actual design of 11 dipoles is done in Sec. IV, and the impact of the iron is analyzed in Sec. V. II. EQUATIONS DEFINING THE SHORT SAMPLE FIELD A. Critical current density A Nb-Ti or Nb3 Sn filament carrying a current density jsc in a magnetic field B is superconducting as long as the current density is less than the critical current density jsc;c , which for the Nb-Ti can be fit using the expression [20]   B jsc;c ˆ C…T†B ÿ1 1 ÿ  ; (1) Bc2 …T† where the constant C depends on the temperature,  0:5–1:0 and  1, and B c2 is the critical field at zero current density at the temperature T. This pretty complex parameter dependence can be very well approximated over a large domain by a simple linear function of the magnetic field (see Fig. 1): jsc;c ˆ c…b ÿ B†; B < b: (2) The fit is good for values of the magnetic field larger than © 2007 The American Physical Society 112401-1 L. ROSSI AND EZIO TODESCO 8000 6000 4000 2000 0 0 Nb-Ti at 1.9 K Nb-Ti at 4.2 K Nb3Sn at 1.9 K Nb3Sn at 4.2 K Phys. Rev. ST Accel. Beams 10, 112401 (2007) stabilizer and of the nonstabilizer (i.e. the sc and the passive material). For consistency, the critical current of the superconductor is defined as the critical current over the non-Cu cross section. In Table I we give Cu-sc for cables of 10 dipoles that have been built in the past 30 years, plus the NED design. Seven of them (Tevatron [1], HERA [2], the Superconducting Super Collider (SSC) 50 mm dipole [3], the Relativistic Heavy Ion Collider (RHIC) [4], the LHC dipole [5,6], and CERN FRESCA [7]) use Nb-Ti conductors. The remaining five (CERN-Elin [8], University of Twente MSUT [9], Berkeley D20 [10], Fermilab HFDA [13], and NED [14]) use Nb3 Sn conductors. The value of Cu-sc ranges from 1.2 to 2 for typical cases; RHIC dipoles have rather high Cu-sc (2.25), whereas very low values have been used for D20 (0.43 to 1). All the Nb3 Sn magnets plus Fresca are 1 m models, whereas the others are either long prototypes (SSC) or magnets belonging to a production of several hundreds units that have been used in an accelerator (Tevatron, HERA, RHIC, LHC). Wires are then assembled in cables, to obtain conductors with high operating currents, and finally insulated. These steps bring an additional dilution of the quantity of superconductor in the winding, which can be estimated in 10%– 20% for each step (see Table I). We define w-c as the compaction factor, i.e., the ratio between the area of the strands in the conductor and the area of the bare conductor. We define c-i as the ratio between the area of the bare conductor and of the insulated conductor. The current density j flowing in the insulated conductor (usually called engineering current density) is therefore given by j ˆ w-c c-i jsc  jsc ; 1 ‡ Cu-sc (5) jsc(A/mm ) B (T) FIG. 1. Critical surface for Nb-Ti: fit of Eq. (1) (empty markers), and linear fit (solid line) of Eq. (2). Critical surface for Nb3 Sn: fit of Eq. (3) (full markers), and hyperbolic fit (solid line) of Eq. (4). 5 T at 1.9 K, and 2 T at 4.2 K, with b  10 T at 4.2 K and 13 T at 1.9 K, and the slope c  6:00  108 A=…T m2 † is independent of the temperature. This corresponds to having 3000 A=mm2 at 8 T and 1.9 K, or at 5 T and 4.2 K. We will show that this is the relevant domain for our analysis. For the Nb3 Sn, the critical surface can be written according to Kramer [21]: 2  C…T; "† B jsc;c …B† ˆ p 1 ÿ  ; (3) Bc2 …T; "† B where the two constants depend on temperature T and strain ". In [17] we proposed an hyperbolic fit   b B < b; (4) jsc ˆ c ÿ 1 B where b is the value of the critical field at zero current density according to the fit. The parametrization (4) agrees well with (3) for typical parameters on a very wide domain, see Fig. 1. For the case of a very high density current Nb3 Sn giving 3000 A=mm2 at 12 T, 4.2 K, with a deformation of " ˆ 0:003, the agreement is within 5% from 5 to 17 T at 4.2 K (with c ˆ 3:9  109 ‰A=m2 Š and b ˆ 21:0 T). For the same case, at 1.9 K one has c ˆ 4:0  109 ‰A=m2 Š and b ˆ 23:1 T. These cable performances correspond to the original aim of the LHC Accelerator Research Program [22] and of the Next European Dipole [14] conductor programs. A practical superconductor wire is made of filaments in a copper matrix, and one defines Cu-sc as the ratio between the quantity of copper (stabilizer) and the superconductor in the strand cross section. For Nb-Ti this is a straightforward formulation. On the other hand, Nb3 Sn strands contain passive materials that are at the same time not superconductor and not used for stabilization: these elements are necessary to the formation of the superconductor itself. Since the critical current is referred to the surface of the nonstabilizer material (non-Cu), a consistent definition in this case is Cu-sc as the ratio between the quantity of TABLE I. Filling factors for cables used in some superconducting dipoles. Magnet Tevatron MB HERA MB SSC MB inner SSC MB outer RHIC MB LHC MB inner LHC MB outer FRESCA inner FRESCA outer CERN-Elin inner CERN-Elin outer MSUT inner MSUT outer LBNL D20 inner LBNL D20 outer FNAL HFDA02-03 NED Cu-Sc 1.85 1.88 1.50 1.78 2.25 1.65 1.95 1.60 1.87 1.63 1.78 1.25 1.25 0.43 1.00 1.25 1.25 w-c 0.82 0.89 0.84 0.88 0.87 0.87 0.86 0.87 0.88 0.88 0.87 0.85 0.91 0.83 0.88 0.86 0.83 c-i 0.81 0.85 0.89 0.84 0.84 0.87 0.83 0.88 0.85 0.88 0.84 0.88 0.85 0.84 0.77 0.76 0.84  0.23 0.26 0.30 0.27 0.23 0.29 0.24 0.29 0.26 0.29 0.26 0.33 0.34 0.48 0.34 0.29 0.31 Material Nb-Ti Nb-Ti Nb-Ti Nb-Ti Nb-Ti Nb-Ti Nb-Ti Nb-Ti Nb-Ti Nb3 Sn Nb3 Sn Nb3 Sn Nb3 Sn Nb3 Sn Nb3 Sn Nb3 Sn Nb3 Sn 112401-2 ELECTROMAGNETIC DESIGN OF SUPERCONDUCTING . . . where we defined the filling factor  which ranges from 1=3 to 1=4 in typical cases, reaching nearly 0.5 for the D20 inner layer conductor (see Table I). The fit for the critical surface for the engineering current density can then be written as jc ˆ c…b ÿ B† for Nb-Ti;   b jc ˆ c ÿ 1 for Nb3 Sn; B where in both cases B < b. B. Critical field, current, and peak field We now consider a dipole coil cross section, i.e., a layout of conductors that satisfies a twofold symmetry and where the current is flowing in opposite directions in each adjacent coil (see Fig. 2, where a 60 sector coil is shown). We assume that the magnetic field is entirely given by the current lines, that there is no contribution given by the iron, and that the current density j in the coil is uniform. The current density is defined as the conductor current divided by the cross-sectional surface of the insulated conductor. We then define: (i) the field B [T] at the center of the dipole; (ii) the peak field Bp [T], i.e., the highest value (in module) of the magnetic field in the coil. One can prove that, for uniform j, the maximum of the field is on the contour line of the coils. Because of the linearity of the Biot-Savart law, both B and Bp are proportional to the current density in the coil j: B ˆ j Bp ˆ j ; (7) (8) (6) Phys. Rev. ST Accel. Beams 10, 112401 (2007) For the Nb-Ti, substituting Eq. (6) in Eq. (8) we can solve for the critical peak field Bp;c , which is reached in the coil when the critical surface is hit (see Fig. 3): Bp;c ˆ cb  : 1 ‡ c (9) This corresponds to a point on the critical surface jp;c , jp;c ˆ cb ; 1 ‡ c (10) which gives the maximum obtainable field in the center of the dipole, Bss ˆ cb : 1 ‡ c (11) Bss means central field at the short sample limit (i.e. the experimental evaluation of the superconductor critical surface) and it is sometimes improperly called quench field. Indeed, the actual quench is also determined by the stability vs perturbation, i.e., by the induced disturbance, conductor design, and by the cooling conditions of the coil. Following the jargon currently in use, we denote the quantity defined in (11) by short sample field. The denomination ‘‘magnet critical field’’ would be more appropriate, but it would lead to ambiguity with the critical field of the superconducting material B c2 . For the Nb3 Sn, using the fit (6) and Eqs. (7) and (8), one can derive s  c 4b ‡1ÿ1 (12) jp;c ˆ 2 c c ˆ 2 s  4b ‡1ÿ1 c where we defined the following parameters that characterize the coil layout: (i) ‰T m2 =AŠ is the central field (in T) per unit of current density (in A=m2 ); (ii)  [adim] is the ratio between the peak field and the central field. Bp;c (13) c Bss ˆ 2 s  4b ‡1ÿ1 : c (14) j(A/mm ) j c= κ c(b-B) B p= λγ j [B p,c,j p,c] 0 0 5 B (T) 10 15 FIG. 2. Layout of a 60 sector coil for a dipole of aperture radius r and coil width w. FIG. 3. Example of critical surface, loadline, critical current, and critical peak field for the LHC main dipole (Nb-Ti at 1.9 K). 112401-3 L. ROSSI AND EZIO TODESCO C. Field limited and current limited regimes The previous formulas (9)–(11) suggest that for the NbTi there are two distinct regimes. (i) c  1.—The critical current at short sample field (10) is equal to cb, i.e., it depends only on the superconducting properties and it is independent of the coil layout. Moreover, the short sample field Bss is equal to c b and is independent of . When we add more cable, the corresponding increase of directly affects Bss . An increase of the filling ratio  also directly affects Bss . The magnetic field is low, and therefore superconducting coils are in general not used for these cases. Moreover, the linear approximation for the critical surface is not valid any more. Anyway, this regime (denoted as current limited) has some interest as a limiting case. (ii) c  1.—In this case the critical peak field tends to b, and the critical current tends to zero. All quantities become independent of . The short sample field is Bss  b  (15) Phys. Rev. ST Accel. Beams 10, 112401 (2007) 4), i.e. 10 T at 1.9 K. On the other hand, none of the designs are close to the field limited regime for the Nb3 Sn, i.e., thicker coils would give a sizable increase in the magnetic field. This means that Nb3 Sn magnets which have been built in the past are still relatively far from the ultimate limits of this material, i.e. 20 T. III. ANALYSIS OF THE CIRCULAR SHELL (SECTOR) LAYOUT A. Coil layout description We first consider a shell design composed by one sector of radial width w, of 60 azimuthal width, at a distance r from the aperture center (see Fig. 2). This well-known textbook example sets to zero the field harmonic b3 (see Appendix B). If we use a wedge in the sector, we have three parameters: the angle 1 of the upper edge of the first block, and the angles 2 and 3 of the lower and of the upper edge of the second block (see Fig. 4, left). We assume that there is no wedge in the midplane, i.e., that the angle of the lower edge of the first block is zero. One can prove that there is a one-parameter family of solutions that set b3 ˆ b5 ˆ 0 (see Appendix B). Among them we analyze … 1 ; 2 ; 3 † ˆ …48 ; 60 ; 72 † and the unique solution …43:2 ; 52:2 ; 67:3 † that sets b3 ˆ b5 ˆ b7 ˆ 0 (see Fig. 4, left). With two wedges (three blocks) one has five parameters, and one can prove that there is one solution … 1 ; 2 ; 3 ; 4 ; 5 †  …33:3 ; 37:1 ; 53:1 ; 63:4 ; 71:8 † that sets to zero all odd multipoles up to b11 (see Fig. 4, right). Summarizing, these are the four cases of the shell design we are going to study: (i) one block: the [0 –60 ] sector (one layer, no copper wedge, b3 ˆ 0); (ii) two blocks: the [0 – 48 , 60 –72 ] sectors (b3 ˆ b5 ˆ 0); (iii) two blocks: the [0 – 43.2 , 52.2 –67.3 ] sectors (b3 ˆ b5 ˆ b7 ˆ 0); (iv) three blocks: the [0 –33.3 , 37.1 –53.1 , 63.4 –71.8 ] sectors (b3 ˆ b5 ˆ b7 ˆ b9 ˆ b11 ˆ 0). For completeness, we also consider the case of a sector at 90 with a current density proportional to the cosine of the azimuthal position ( cos coil), providing a pure dipolar field. Its features have been analyzed in detail in [18,19]. and the behavior of  for large coils determines its maximum value. We denote this regime as field limited. For the Nb3 Sn, the relevant quantity is c =…4b†; when c =…4b†  1 one has a regime which is similar to the field limited case for the Nb-Ti, where the critical current density tends to zero and one obtains the same result as in Eq. (15). In Table II we give the aperture and the factors c and c =…4b† for 10 dipoles that have been built in the past 30 years, plus NED. For each layout we computed the factors for the conductor (Nb-Ti or Nb3 Sn) used in the magnet. Since the aim is to analyze the design and not the improvements of the cable performance, here we choose the same cable properties for magnets with the same material. Some layouts are close to the field limited regime for the Nb-Ti (in particular, Fresca has a c larger than TABLE II. Current/field limited factors for Nb-Ti and Nb3 Sn for some superconducting dipoles. Coil Nb-Ti Nb3 Sn Aperture width  c c =…4b† (mm) (mm) (adim) (adim) (adim) 38.05 37.50 25.00 40.00 28.00 43.90 27.50 24.95 25.00 21.75 44.00 16 21 26 10 31 34 34 39 53 29 53 0.232 0.262 0.298 0.226 0.286 0.293 0.293 0.330 0.484 0.288 0.309 1.5 2.1 3.1 1.0 3.5 4.2 0.35 0.47 0.89 0.22 0.44 Name Tevatron MB HERA MB SSC MB RHIC MB LHC MB FRESCA CERN-Elin MSUT LBNL D20 FNAL HFDA02-03 NED-II α3 α 2 α1 FIG. 4. Two sector layouts (one fourth shown in the plot), one with two blocks [0 – 43.2 , 52.2 –67. 3 ] (left) and one with three blocks [0 –33.3 , 37.1 –53. 1 , 63.4 –71.8 ] (right). 112401-4 ELECTROMAGNETIC DESIGN OF SUPERCONDUCTING . . . Phys. Rev. ST Accel. Beams 10, 112401 (2007) TABLE III. Values of parameter 0 defined in Eq. (17) for different sector coil layouts. Number of blocks 1 2 2 3 Block angles [0 –60 ] [0 – 48 , 60 –72 ] [0 – 43.2 , 53.2 –67.3 ] [0 –33.3 , 37.1 –53.1 , 63.4 –71.8 ] cos 0 [T m=A] 6:93  10ÿ7 6:63  10ÿ7 6:53  10ÿ7 6:48  10ÿ7 6:28  10ÿ7 B. Evaluation of the central field The computation of the central field for the sector layout is straightforward. For a sector of angular width , one has (see Appendix A) Z r‡w Z dd B/ / w sin… † (16) ÿi r 0 e and therefore in the case of one layer made of sectors of width w, one has B ˆ j 0 w ˆ 0 w; (17) D. Short sample field versus layouts and analytical fit The comparison of the short sample field versus the sector width (see Fig. 6) for the Nb-Ti shows that all the analyzed sector layouts give the same Bss within 1.5% for w > 6 mm. On the other hand, the cos coil gives a Bss larger by 10% for small w, that reduces to 3% for w ˆ 30 mm, and converges to the sector values for w > 30 mm. If Bss is expressed in terms of the coil cross-sectional area, the difference between the layouts is further reduced. This shows that for the four analyzed sector coils the presence of a copper wedge, its angular position, and the presence of one or two layers do not affect much Bss . A similar result holds for the Nb3 Sn case. We then propose a simple analytical approximation of the short sample field Bss as a function of the different parameters for the [0 – 48 , 60 –72 ] case. We use Eq. (11), replacing with its analytical expression (17), and we approximate  with (18), thus obtaining Bss  cB 0 w cB 0 w c2 c2 ar ˆ 1 ‡ c 0 w…1 ‡ w † 1 ‡ c 0 …w ‡ ar† (19) where the constant 0 depends on the layout (see Table III). C. Evaluation of the peak field The evaluation of the ratio between peak field and central field  is less straightforward than the previous case. The dependence of  on w for an aperture radius r of 30 mm has been evaluated using a numerical computation (see Fig. 5). The shapes of the curves are very similar in the four layouts: for increasing w,  decreases, tending to an asymptotic value close to 1. The difference between the layouts is 6% at w ˆ 20 mm, 4% at w ˆ 40 mm, and disappears for large w. One can prove that the parameter  is a function of w=r. A good fit is ar …w; r† ˆ 1 ‡ : (18) w For the [0 – 48 , 60 –72 ] case, the fit with a ˆ 0:06 is accurate within 2% for w > 8 mm, and within 0.5% for w > 14 mm. The cos coil has  ˆ 1. with 0 ˆ 0:663  10ÿ6 ‰T m=AŠ, a ˆ 0:06 and w, r expressed in meters. We then express w in terms of the conductor cross-sectional area: since for the [0 – 48 , 60 –72 ] case Aˆ one has r=30 mm 2 ‰…r ‡ w†2 ÿ r2 Š; 3 (20) Nb3Sn 4.2 K Bss (T) Nb-Ti 4.2 K 1 layer 60 1 layer 42.8-51.6-67 cos theta Cosθ 40 width (mm) 1 layer 48-60-72 1 layer three blocks FIG. 5. Numerical evaluation of  and fit defined in Eq. (18) versus sector width for different sector layouts, aperture radius of 30 mm. FIG. 6. (Color) Numerical evaluation of the short sample field versus sector width for different sector layouts, aperture radius of 30 mm. 112401-5 L. ROSSI AND EZIO TODESCO s  3A wˆr 1‡ ÿ1 2r2 and therefore we finally obtain q 3A cB 0 r… 1 ‡ 2r2 ÿ 1† c2 : Bss  q 3A 1 ‡ cr 0 ‰ 1 ‡ 2r2 ÿ 1 ‡ aŠ Phys. Rev. ST Accel. Beams 10, 112401 (2007) TABLE IV. Ratio between the short sample field evaluated through Eq. (22) and B c2 for Nb-Ti, different sector widths and aperture radii, for filling factor  ˆ 0:35. 15 30 0.80 0.79 0.77 0.74 0.68 w (mm) 45 0.86 0.85 0.83 0.81 0.76 60 0.89 0.89 0.87 0.85 0.81 90 0.92 0.92 0.91 0.89 0.86 (21) (22) The approximation agrees with the numerical values of the four considered layouts within 3% for w > 8 mm. Since the conductor area is a quantity which is not easy to appreciate, for a generic coil layout characterized by A and r we define an aspect ratio weq =r where weq is the width of a 60 sector coil with the same area s  3A weq  1 ‡ ÿ 1 r; (23) 2r2 and in the following sections we will express the results as a function of the aspect ratio weq =r rather than in terms of coil surface A. For the Nb3 Sn case, using Eq. (14) one obtains s  c 0 weq 4b ‡1ÿ1 : (24) Bss  2 c 0 …weq ‡ ar† E. Short sample field versus sector width The analytical approximations we derived for the short sample field Bss in a sector coil (22) and (24) have a strong dependence on the coil width w, and a weaker dependence on the aperture radius r. A smaller aperture gives a  closer to one [see Eq. (18)], and therefore a higher Bss . For small aperture radius, the sector results tend to the cos coil. For large aperture radius, the sector results are smaller than the cos coil (see Fig. 7). The ratio between the short sample field Bss and B c2 that can be obtained with a sector width w as a function of the aperture radius is given for the Nb-Ti in Tables IV and V for two typical values of the filling factor: for  ˆ 0:35, a coil width of 15 mm gives at most 2=3 of the critical field, 80% at w ˆ 30 mm and 90% at κ =0.35 15 Nb3Sn at 4.2 K cos theta r ˆ 10 mm r ˆ 30 mm r ˆ 60 mm r ˆ 120 mm TABLE V. Ratio between the short sample field evaluated through Eq. (22) and B c2 for Nb-Ti, different sector widths and aperture radii, for filling factor  ˆ 0:25. 15 cos theta r ˆ 10 mm r ˆ 30 mm r ˆ 60 mm r ˆ 120 mm 0.59 0.58 0.56 0.52 0.47 30 0.74 0.74 0.72 0.69 0.63 w (mm) 45 0.81 0.81 0.79 0.77 0.72 60 0.85 0.85 0.84 0.81 0.78 90 0.89 0.89 0.88 0.87 0.84 w ˆ 60 mm. These percentages are decreasing for increasing radii, and for smaller filling factors. F. The one-layer layout without field quality We then consider a sector of angular width ranging from 40 to 80. In this case we neglect all aspects related to field quality, which will be not optimum except in the case of 60 for b3 , i.e., we assume that the field harmonics can be compensated by corrector magnets. The aim of the simulation is to verify if relaxing the field quality constraint one can improve Bss . In Fig. 8 we show for an aperture of 30 mm and for Nb-Ti that a sector of 50 to 60 is the optimum solution, the other sectors providing a smaller critical field for the same conductor surface. A Bss (T) Nb-Ti at 4.2 K r=30 mm r=120 mm r=60 mm Cos theta cos θ 40 equivalent width (mm) FIG. 7. (Color) Short sample field versus equivalent width according to (22) and (24) for  ˆ 0:35. FIG. 8. (Color) Short sample field versus equivalent sector width for different angular widths of the sectors for an aperture radius of 30 mm, Nb-Ti case. Note that 50 and 60 curves are overlapping. 112401-6 ELECTROMAGNETIC DESIGN OF SUPERCONDUCTING . . . similar result holds for the Nb3 Sn. Unfortunately, no theoretical justification of this numerical result is available. G. Graded coils In the analyzed cases of sector coils, the peak field is located in the inner part of the coil, close to the pole. The outer part of the coil has a much lower field and therefore a higher current density could be used. The technique of using a higher current density in the coil regions that are far from the location of the peak field is called grading. It allows one to reach either a highest field for the same coil area, or the same field but with a smaller coil area. The equations for computing the short sample field in the case of grading are given in Appendix C. We carried out a simulation for a 30 mm aperture radius sector coil with a two blocks inner layer canceling b3 b5 , and b7 (i.e., the [0 – 43.2 , 52.2 –67.3 ] solution), and a 60 outer layer of the same width. We varied the layer width from 5 to 40 mm, we selected a filling factor of 0.35 for the inner and 0.25 for the outer layer, and for each case we varied the ratio between the current density in the outer and in the inner layer [2 in Eqs. (C1) and (C2)] to obtain the largest short sample field. Results for the Nb-Ti at 4.2 K are given in Fig. 9, where Bss is given as a function of the equivalent coil width defined in (23). If the comparison with a nongraded case is carried out for the same coil area, the gain in Bss given by grading is between 4% and 6%, with a mild dependence on the coil width. On the other hand, if we aim at a given Bss , the save in the equivalent width of a graded coil with respect to a nongraded one is relevant: for Nb-Ti at 4.2 K we have 20% at 7 T, 25% at 8 T, and 30% at 8.5 T. For instance, 8 T can be reached with an equivalent coil width of 40 mm without grading and of 30 mm with grading. We also varied the ratio between the width of the inner and the outer layer: beside the case of equal widths w2 ˆ w1 we considered thinner outer layers with w2 ˆ w1 =2 and w2 ˆ 3=4 w1 , finding similar results (see Fig. 9). We then selected the case with w2 ˆ w1 and we varied the aperture radius from 30 mm to 60 mm and 120 mm. 20 1 layer 60 2 graded layers w2=w1/2 2 graded layers w2=w1 2 graded layers w2=3/4 w1 Phys. Rev. ST Accel. Beams 10, 112401 (2007) The gain in the short sample field is rather similar, i.e., 4%–5%, becoming smaller for larger apertures. The optimal grading, providing the highest short sample field, strongly depends on the coil width and apertures. Results for the Nb-Ti and equal widths w2 ˆ w1 are given in Fig. 10. The optimal grading is a linear function of the coil width, and the slope decreases for larger apertures (se Figs. 10 and 11). For instance, a 30 mm aperture radius dipole with two layers of 15 mm (i.e., an equivalent width of 30 mm, similar to the main LHC dipoles) has an optimal grading of 1.6, i.e., the current density in the outer layer should be 60% larger than in the inner one. This must be considered as an upper limit, since the aspects related to the quench protection usually further reduce the applicable grading. For instance, the LHC main dipole has a grading of 23%, leading to a higher field of 3.8%. The different form of the equations between Nb-Ti and Nb3 Sn [see (C8) and (C10)] implies that both the gain in Bss and the optimal grading are different from the values found for the Nb-Ti. However, the gain in Bss for a given coil width is similar to the Nb-Ti case, being 4%–7% and getting slightly smaller for larger apertures. The saving in the coil width is 22%–23% at 14 –15 T, and 27% at 16 T (see Fig. 9). The optimal grading (see Fig. 11) is smaller than for Nb-Ti; for instance, a 30 mm aperture with two FIG. 10. Optimal grading, providing the highest short sample field, as a function of the sector width,  ˆ 0:35, Nb-Ti. B ss (T) Nb3Sn 4.2 K Nb-Ti 4.2 K 5 0 20 40 equivalent width (mm) 60 80 FIG. 9. (Color) Short sample field versus equivalent sector width for an aperture radius of 30 mm, Nb-Ti and Nb3 Sn case, graded versus nongraded coils. FIG. 11. Optimal grading as a function of the sector width, and  ˆ 0:35, Nb3 Sn. 112401-7 L. ROSSI AND EZIO TODESCO Phys. Rev. ST Accel. Beams 10, 112401 (2007) TABLE VI. Parameters of coil layouts of 11 superconducting dipoles. Aperture radius (mm) 38.05 37.50 25.00 40.00 28.00 43.90 27.50 24.95 25.00 21.75 44.00 Surface (mm2 ) 2700 3680 3224 1723 4657 7470 5551 6103 8998 3253 12 712 w equivalent (mm) 14.3 18.7 21.5 9.2 26.8 30.2 30.9 34.5 45.2 23.3 45.5 Grading (%) 0.0 0.0 29.9 0.0 23.0 23.5 42.4 65.1 80.5 0.0 0.0 Name Tevatron MB HERA MB SSC MB RHIC MB LHC MB FRESCA CERN-Elin MSUT D20 FNAL HFDA02-03 NED-II Layers 2 2 2 1 2 2 2 2 4 2 2 Blocks 2 [1,1] 4 [2,2] 6 [4,2] 4 6 [4,2] 7 [4,3] 6 [4,2] 5 [3,2] 13 [3,4,3,3] 6 [3,3] 7 [4,3] layers of 15 mm width has an optimal grading of 45% (60% for the Nb-Ti). H. Analysis of accelerator magnets (without iron) We finally compare the results of our analysis of simplified, uniform j sector layouts with actual designs that have been used in accelerator magnets. In Table VI we give the main parameters of the geometry of 10 dipoles actually built in the past 30 years, plus the NED design. For each one, we compute the equivalent width weq defined in Eq. (23). Apertures are ranging from 20 to 45 mm, equivalent widths from 10 to 45 mm, and the conductor area spans over 1 order of magnitude. All designs are based on sector coils, with one, two, or four layers, and 2 to 13 blocks. Several dipoles have grading, varying from 20% to 80%. Two typical layouts are shown in Fig. 12. The parameters [see Eq. (7)] of the dipoles of Table VI, evaluated without iron, are plotted in Fig. 13 versus the equivalent width we defined in Eq. (23): in the case of no current grading they all fit within 4% with the value computed for a [0 – 48 , 60 –72 ] sector coil (note that the agreement with the [0 ,60 ] sector coil is worse, the error being 8%). This shows that, for the analyzed cases, for a given quantity of cable one obtains within 4% the same field per unit of current density, independently of the layer or sector subdivisions. For the cases 80 60 y (mm) with current grading, we used the current density of the sector where the peak field is located (the inner layer in all cases) to define . The gain in is in most analyzed cases around 20%. Results for the parameter  are shown in Fig. 14, where we compare the actual values of the magnets given in Table VI without iron (markers) to the results for the [0 – 48 , 60 –72 ] sector coil (solid line). The agreement is within 1.5%. Magnet data confirm the trend that  increases for smaller aspect ratios weq =r and tends to one for the larger ones. Magnets designed with a current grading have a similar  to the single sector estimate. In Table VII we give a comparison between the estimated values for the short sample field with no grading as deduced theoretically using the analytical approximations (22) and (24) with 0 ˆ 0:663  10ÿ6 ‰T m=AŠ and a0 ˆ 0:06, and the actual ones for the 11 analyzed magnets without iron. The agreement in the case of no current grading is within 1.5%. One can conclude that in case of no grading Eqs. (22) and (24) model the short sample field with a high precision, neglecting the design details as the number of layers and the position of wedges. On the other -8 4E-08 4×10 -8 80 60 y (mm) 40 20 0 0 20 40 x (mm) 60 80 γ [T m /A] 3E-08 3×10 2E-08 2×10 10 1E-08 -8 -8 TEV MB SSC MB LHC MB CERN-Elin LBNL D20 NED HERA MB RHIC MB Fresca MSUT HFDA Grading 0 0E+00 0 10 20 30 equivalent width w (mm) 40 50 40 x (mm) FIG. 12. Coil layout of RHIC (left) and LHC (right) dipoles. FIG. 13. (Color) Parameter (central field per unit of current density) for 11 accelerator dipoles without iron (markers) and results for a 0 – 48 , 60 –72 sector (solid line) vs equivalent width defined in Eq. (23). 112401-8 ELECTROMAGNETIC DESIGN OF SUPERCONDUCTING . . . 1.3 TEV MB SSC MB LHC MB CERN-Elin LBNL D20 NED HERA MB RHIC MB Fresca MSUT HFDA Phys. Rev. ST Accel. Beams 10, 112401 (2007) 60 y (mm) 40 20 0 λ [adim] 1.2 λ [adim] 1.0 equivalent width w/r 40 x (mm) 0.5 equivalent width w/r FIG. 14. (Color) Ratio  between peak field and current density vs equivalent ratio width/aperture radius as defined in Eq. (23): analytical fit of Eq. (18) (solid line) and values for 11 dipoles evaluated without iron (markers). FIG. 15. Cross section of the INFN SIS-300 proposed model (left), and value of  (full marker) compared to the fit (18) and to numerical values (empty markers) of magnets shown in Fig. 14. hand, 6 magnets with current grading show a higher critical field with respect to our analytical benchmark of up to 4% for Nb-Ti and up to 7% for Nb3 Sn. The above analysis confirms that for small w=r the ratio peak field/central field  becomes less and less favorable: for instance RHIC and Tevatron magnets have a peak field 15%–18% larger than the central field, whereas MSUT and D20 have a peak field which is only 3%– 4% larger than the ¨ bore field (see Fig. 14). A layout for the Gesellschaft fur Schwerionenforschung (GSI) SIS-300 dipole recently proposed by the Istituto Nazionale Fisica Nucleare [23] features a rather small w=r  0:3 but a   1:08 well below the scaling (18). The cross section is shown in Fig. 15, left. The layout has been optimized to maximize the short sample field, given the cable width. The presence of a large wedge before the upper block, and the small number of cables of the last block on the pole, allows one to obtain a significantly lower , i.e., about 1.08 instead 1.16 as one would expect from the fit (18), see Fig. 15, right. This allows one to obtain (without grading) a short sample field which is 4% larger than that expected from our scaling law. One can conclude that, even though all the analyzed deTABLE VII. Actual and analytical estimates of critical field for 11 superconducting dipoles (no iron). Actual (T) 5.4 6.3 7.2 4.2 9.8 10.0 10.3 11.2 13.3 10.2 13.8 Critical field Analytical Error (T) (%) 5.3 6.2 6.9 4.2 9.5 9.6 9.5 10.4 12.5 10.4 13.9 1.2 1.0 4.0 0.5 3.9 3.4 7.1 7.4 6.2 ÿ1:6 ÿ0:6 Grading (%) 0.0 0.0 29.9 0.0 23.0 23.5 42.4 65.1 80.5 0.0 0.0 signs of built magnets agree well with the estimates based on the sector, it appears that there is still some space for further electromagnetic optimization of coil layouts with respect to what has been done in the past. IV. IRON EFFECT The presence of the iron yoke has the main function of providing a return flux path shielding the external side of the magnet from the inner magnetic field. The iron also induces a higher field in the aperture for the same current density, thus improving aspects related to stability and protection. However, it also induces a higher peak field and therefore the beneficial effect on the short sample field is not as large as it can be naively expected and strongly depends on the coil width. Finally, the iron yoke can also be used to transmit the retaining forces (mechanical function). Here we will focus on its impact on the short sample field for the Nb-Ti and Nb3 Sn. One has to clearly distinguish the increase of the central field for a given current density (i.e. the increase in ) from the increase of the maximum obtainable field, i.e., the short sample field. The first one can be large (20%–50%, see Table VIII), and helps coil protection by reducing the operational current. The second one is in general rather small: rarely the iron yoke makes an increase of 10% in the short sample field and it reduces to 5% for coils larger than 30 mm. In order to prove these statements, we first compute the relative increase of [see Eq. (7)], which is independent of the material, for the coil layouts analyzed in the previous section, see Table VIII. We then compute the gain in the short sample field. The increase is large (about 25%) only for the RHIC dipole, where both the coil and the collar are thin. It decreases for larger coil widths, being 3%–7% for widths larger than 30 mm, i.e., comparable to the effect of a strong grading. For the same layout, the increase is more relevant for Nb3 Sn due to the shape of the critical surface. V. CONCLUSIONS In this paper we aimed at finding explicit expressions for the short sample field in a superconducting dipole as a function of the material and cable parameters, of the op- Name Tevatron MB HERA MB SSC MB RHIC MB LHC MB FRESCA CERN-Elin MSUT D20 FNAL HFDA02-03 NED-II 112401-9 L. ROSSI AND EZIO TODESCO Phys. Rev. ST Accel. Beams 10, 112401 (2007) TABLE VIII. Increase of parameters and , and of the short sample field, due to the iron yoke for 7 Nb-Ti and 4 Nb3 Sn dipoles. Riron (mm) 90.0 86.5 69.0 59.7 98.0 114.4 115.0 107.0 92.5 60.0 130.0 Collar thickness (mm) 36.1 28.2 19.4 9.6 39.2 36.4 53.3 43.3 14.4 8.8 33.2  = (%) 25.2 29.6 30.9 56.7 21.2 29.5 16.6 19.8 39.9 37.4 31.7 … †=… † 22.0 27.1 29.3 47.9 20.4 27.8 16.1 19.2 39.0 35.0 30.4 Nb-Ti Nb3 Sn Bc =Bc (%) 10.4 9.4 7.2 26.7 3.8 5.7 4.1 4.3 5.5 10.6 6.8 Name Tevatron MB HERA MB SSC MB RHIC MB LHC MB FRESCA CERN-Elin MSUT D20 FNAL HFDA02-03 NED-II erating temperature, of the magnet aperture, and of the coil width. We derived semianalytical expressions for the cases of Nb-Ti [Eq. (22)] and Nb3 Sn [Eq. (24)] based on the analysis of a sector coil and making use of simple fits for the critical surfaces [Eqs. (2) and (4)]. The comparison with the numerical results relative to several nongraded dipoles built in the past 30 years show that using this method the short sample field can be estimated within a few percent. The equation can be used as a benchmark to judge the efficiency of the magnet design: we applied this method to work out the impact of grading and the effect of the iron on the short sample field. The equation can also provide plots as shown in Fig. 7, where, having the magnetic field and aperture requirements, one can quickly estimate the needed coil thickness, without the need of going through a detailed design. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Physical Review Special Topics - Accelerators and Beams American Physical Society (APS)

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