Skip to main content
  • Research article
  • Open access
  • Published:

Straightening of superconducting HERA dipoles for the any-light-particle-search experiment ALPS II

This article has been updated


At DESY the ALPS II experiment is being installed in the HERA tunnel to search for axion like particles. A laser beam will be injected into the magnetic field of a string of superconducting (s.c.) dipole magnets, available from the HERA proton storage ring, to produce axion like particles. After passing a light tight wall, the ALPs can reconvert into photons in a second string of HERA s.c. dipoles. The sensitivity of the experiment will be increased by two mode-matched optical cavities before and behind the wall. The dipoles for the HERA storage ring are curved, suited for stored proton beam. However, the curvature of the magnets limits the aperture and hence the performance of the optical resonators beyond a certain length. As the sensitivity of the search scales with the length of the magnetic field, the aperture for the optical resonators inside the HERA dipoles was increased by straightening the curved magnet yoke. The procedure of straightening the s.c. HERA dipoles is described in this report.


One of the most important open questions in physics is the nature of dark matter. Among the candidates from particle physics are axions [1] and other very weakly interacting slim particles (WISPs), e.g. axion-like particles (ALPs) (see [2] for an overview). Light-shining-through-a-wall experiments [3] allow searches for these particles in the laboratory.

More than 10 years ago an experiment of this kind was performed at DESY (ALPS I) [4] making use of a single spare superconducting HERA dipole. This experiment could not prove the existence of ALPs, but only establish limits on the coupling of photons to ALPs with masses below a few meV. These limits could be tightened by the OSQAR light-shining-through-a-wall experiment at CERN using two spare LHC dipoles [5].

Now the ALPS IIFootnote 1 experiment [6] is being set up in a straight section of the HERA tunnel with substantially increased sensitivity compared to the previous experiments, using 24 superconducting HERA dipoles. The magnetsFootnote 2, almost 10 m long with a magnetic field of 5.3 Tesla [7, 8], are available from the HERA proton storage ring [9], which has not been in operation since 2007. In addition to a straight section of the HERA tunnel, infrastructure like cryogenics [10], and power supplies needed to operate superconducting magnets are available.

The principal concept of the experiment

Axions and axion like particles (called ALPs in the following) can be produced by photons traveling in a section of magnetic field, transverse to the flight direction. Similarly ALPs can convert into photons again in another section of the transversal magnetic field. To separate these photons from the photons which produce the ALPs, a light tight wall is inserted between the two sections of the magnetic field. ALPs penetrate the wall practically without any attenuation (see Fig. 1).

Fig. 1
figure 1

Physics principle of the experiment. Laser photons interact with the magnetic field B to create an axion like particle. The ALP penetrates the material wall and occasionally reconverts to a photon in the magnetic field behind the wall, to be detected by a photon detector

Laser light is injected into the first section of the magnetic field. To increase the production probability of ALPs, the light is reflected back and forth many times in an optical resonator. The conversion probability of ALPs to light in the second magnetic field section is enhanced also by an optical resonator (enhanced ‘spontaneous emission’) [1113] (see Fig. 2). For details of the optics layout of the ALPS II experiment see [14] and [15].

Fig. 2
figure 2

Schematic layout of the experiment. The probability for the generation of an ALP by a photon gets increased in an optical resonator. Behind the light tight wall a second optical resonator increases the probability of re-conversion to a photon in the magnetic field. (Figure from Aaron Spector)

The sensitivity, in measuring the coupling of photons to ALPs, scales with the strength of the magnetic field B in the two sections and their length L, i.e. with B·L (for details see [16]). At DESY strong superconducting dipoles are available from the 6.3 km long lepton-proton-collider ring HERA. Some of these dipoles will be used to set up two long straight strings of magnets for the ALPS II experiment in a straight section of the HERA tunnel. The geometry of the tunnel limits the number of dipoles to be installed as straight strings to 2·12, i.e. to a length of ≈2·120 m.

To obtain high quality factors in the optical resonators, leading to high production and regeneration probabilities, the total loss of photons on the wall of the vacuum pipe, within the dipoles of each string, must remain below 2·10−6 [17]. This requires that the aperture of the vacuum pipe must be larger than the envelope of the photon beam within each string of dipoles. The loss of photons caused by scattering from gas molecules is negligible as the optical resonators are located in the high vacuum of the beam pipe.

Unfortunately, the vacuum pipes within the HERA dipoles [18, 19] are curved, suited for the storage of protons. For light however, moving on a straight line, the horizontal aperture in the optical resonators is reduced from 55.3 mm (inner diameter of the beam pipe) to about 35 mm only. This aperture allows only for 2·40m of magnetic length, i.e. 2 strings of 4 HERA dipoles each, without limiting the performance of the optical resonators.

The aperture can be increased by straightening the HERA dipoles leading to a practically loss free length of about 120 m for each resonator, which matches the above mentioned maximum length, given by the tunnel geometry, for installing straight strings of dipoles. The ALPS II setup with 2·12 straightened dipoles in the HERA tunnel is shown schematically in Fig. 3.

Fig. 3
figure 3

Schematics of the experimental setup of ALPS II in a straight section of the HERA tunnel. The two strings of 12 straightened dipoles each are connected by a vacuum insulated bypass line for cold Helium and the magnet current, leaving sufficient space for the setup of the optics in the middle of the experiment. The Helium and the current for the magnet strings are supplied at the box closest to the DESY site

The superconducting HERA dipole

The ‘cold mass’ of the HERA dipole, i.e. the superconducting coil and the magnet iron, is supported from the vacuum vessel at three planes along the cryostat (see Fig. 4). The suspensions (6 in total) also support the radiation shield.

Fig. 4
figure 4

Schematic view of the HERA dipole. 1 Helium vessel containing cold mass, 2 Suspension, 3 Radiation shield, 4 Vacuum vessel, 5 Helium pipes

As indicated in Fig. 4, the cold mass is contained in a stainless steel vessel (Helium vessel) welded from two half cylinders. The beam pipe in the middle of the cold mass is surrounded by the magnet coil wound from superconducting cable (‘Rutherford’ cable). The coil is held by strong clamps counteracting the magnetic forces. The magnetic field outside the coil is concentrated in slices of magnet iron surrounding the clamps.

Some of the properties of the HERA dipole are compiled in Table 1, including results from measurements of the magnetic field [20, 21].

Table 1 HERA dipole properties

Figure 5 shows the ends of a HERA dipole with the pipes for 1- and 2-phase Helium emerging from the Helium vessel. The s.c. cables to and from the coils in the magnet are routed through the 1-phase tubes at the ends of the Helium vessel. The radiation shield is cooled by Helium gas at 40-70K from a single pipe.

Fig. 5
figure 5

View of the two ends of a HERA dipole. 1: Beam tube, 2: One phase Helium pipe with superconducting cables for the magnet coil, 3: Two phase Helium pipe, 4: Helium gas pipe for the cooling of the radiation shield, 5: Helium vessel containing the cold mass, 6: Radiation shield, 7: Vacuum vessel

Originally the cold mass was fabricated as a straight unit. By a strong press the two half cylinders of the Helium vessel were forced around the magnet iron and bent to the required radius before joining the half cylinders by weldingFootnote 3. The beam pipe (see Fig. 6) was forced to follow the curvature by spacers, glued to the outside of the pipe. The outer vacuum vessel forms a polygon, roughly following the curvature of the cold mass (see Fig. 13 right).

Fig. 6
figure 6

The beam tube of the HERA dipole. Indicated are (right) the Vespel spacers which keep the pipe centered in the coil and force the pipe to follow the deformation of the yoke

The cold mass could, in principle, be straightened again by cutting the welds on the Helium vessel. However this would require a complete disassembly of the cryostat and the proper tooling, which mostly would have to be rebuilt.

As this would be a very costly procedure, we chose a cheaper method to increase the aperture of the beam pipe without disassembly of the cryostat: bending the cold mass inside the vacuum vessel by ‘brute force’Footnote 4(see “The straightening procedure” section).

There was serious concern, that the superconducting coils might be damaged by this way of straightening. To ensure that the magnets could still be operated at the design current for ALPS II of 5693 A, all magnets were tested after straightening up to their respective quench currents on a test bench available at DESY.

The test bench

One dipole test benchFootnote 5 is still available from the magnet test facility on the DESY site [22] for the lepton-proton-collider HERA (see Fig. 7), with all the cryogenics tubing, current leads, valves, sensors, safety systems, and so on. Helium, liquid and gas, can be supplied by the existing vacuum insulated transfer line from the central DESY cryogenics plant.

Fig. 7
figure 7

Remaining bench for cryogenic tests of HERA dipoles with a dipole on the bench. Note the open sliding sleeve connection of the vacuum vessel to the cryogenics end box

The original power supply of the test facility, capable to supply up to 7000 A at 20 Volts, is available. The old quench detection and protection system [23] for magnet operation was updated. A turbo pump station and a roughing pump for the insulating vacuum are available. So, everything required for a test of HERA dipoles is operational.

After a dipole was positioned on the test bench, the electrical connection between the coil and the power supply was established by soldering the superconducting cables emerging from the dipole cryostat (see Fig. 5) with the ones from the feed box of the test bench [24].

When the survey of the beam pipe during the straightening of the magnet (see “The survey of the vacuum pipe” section) was completed, the Helium lines between the boxes and the magnet were sealed by special Aluminium seals. Copper half shells were connected around the bellows in the Helium pipes, to prevent them from buckling when pressurized. The Helium pipes, and the magnet at the flanges were shielded from thermal radiation with super insulation (see “The new suspensions” section) after leak checking the connections of the Helium pipes. Then the open flanges and the sliding sleeves on the vacuum tank (see Fig. 7) were closed, to evacuate the vacuum vessel. At about 10−4 mbar in the vacuum vessel, the cool down of the cold mass to 4K proceeded.

It should be noted, that the beam tube was open within the cryostat on the test bench, being evacuated together with the vacuum vessel. This will be different for the magnet strings in ALPS II, where the vacuum pipes of adjacent dipoles will be connected, and the beam tube vacuum will be separated from the insulating vacuum.

Experimental/ methods

The straightening procedure

The straightening of the magnet and the vacuum pipe, to increase the horizontal aperture of the beam tube for the optical resonators, was performed on the test bench. It was achieved by fixing the position of the ‘cold mass’ at the outer suspensions of the magnet and pushing (and thus deforming) the cold mass in the middle (see Fig. 8). The cold mass was fixed in position by inserting and tightening Titanium pressure props (see Figs. 9 and 16) between the cold mass and the vacuum vesselFootnote 6. By a transportation fixture (see Fig. 10) on the opposite side of the cryostat, the cold mass was prevented from moving, while tightening a pressure propFootnote 7.

Fig. 8
figure 8

Schematics of straightening. Left: Before applying the deforming force, Right: The deformation forces the pipe to develop two ‘camel humps,’ exaggerated in the figure for better illustration. This deformation yields the largest achievable horizontal aperture

Fig. 9
figure 9

Outer pressure prop parts (left) and prop inserted into the cryostat (right)

Fig. 10
figure 10

Left: Cross section of the cryostat with an inserted outer pressure prop (blue) and a transportation fixture (red). A transportation fixture mounted into the vacuum vessel (right)

The deformation in the middle was achieved by a steel screw (‘pressure screw’) (see Fig. 11) exerting a force of about 40 kN, inserted between the vacuum tank and the Helium vessel at the lower flange of the vacuum vessel.

Fig. 11
figure 11

Pressure screw mounted into the vacuum vessel in the middle of the cryostat for the deformation of the cold mass (left), Pressure screws (right)

When the aimed for deformation was achieved, another Titanium pressure prop was inserted (see Fig. 12) from the upper flange above the pressure screw. After tightening the pressure prop, the pressure screw and the transportation fixtures were removed. With all three pressure props installed and tightened, the deformation of the yoke is maintained by the tension of the yoke, counteracted by the vacuum tank via the pressure props. Figure 13 shows the cryostat with three Titanium pressure props inserted before the removal of the transportation fixtures.

Fig. 12
figure 12

Left: Middle pressure prop, Middle: Inserting the prop, Right: Inserted pressure prop in the middle of the cryostat

Fig. 13
figure 13

Schematic view of the cryostat after the straightening. 1: Outer pressure prop, 2: Middle pressure prop, 3: Transportation fixture, 4: Suspension

The ends of the beam tube cannot be straightened independently, as no force can be applied beyond the outer suspension planes. The ends just rotate around the fix points, given by the outer pressure props, due to the bending of the beam tube in the middle (see Fig. 8). The middle of the cold mass was bent in a way, to force the beam tube to develop two ‘camel humps’ (see Fig. 8 and also Fig. 15). This deformation yields the largest achievable horizontal apertureFootnote 8. In the figure the deformation is exaggerated for better illustration.

The pressure prop in the middle (see “The pressure props” section) of the cryostat constitutes a fix point for the thermal shrinkage/expansion during cool down/warm up of the cold mass.

Finite element calculations, determining the additional stress on the Helium vessel by the straightening procedure, were performed [25] and presented to the agency for pressure vessel safety (TUEV). The calculations showed that all stresses are well below the limits set by pressure vessel regulations.

There is a detailed report on the work required for the straightening [26], partially presented on the PATRAS workshop 2018 [27].

The survey of the vacuum pipe

The position of the center of the beam pipe before, during, and after the deformation was measured by the DESY survey group with a laser tracker and a so-called mouse with a reflector attached. The mouse was pulled by a string through the vacuum pipe along the length of the magnet, while the laser tracker continuously measured the position of the reflector (see Fig. 14) through an open flange in the middle of the end box of the test bench.

Fig. 14
figure 14

The laser tracker to measure the position of a reflector in the vacuum pipe of the dipole through an open flange in the end box. Middle: Mouse with attached reflector inserted into the beam pipe; Right: Before insertion. The string connected to the mouse is used to pull it through the beam pipe

Fig. 15
figure 15

The result of straightening a dipole. Shown is the measured center of the vacuum pipe before and after straightening. The positions of the outer pressure props are indicated by arrows. The maximum achievable aperture by the deformation is about 50 mm. The inner diameter of the beam tube is 55.3mm

Fig. 16
figure 16

Schematic view of the pressure prop at an outer suspension in the cryostat with the thin walled Titanium tube. Note the spherical sections at both ends (marked by *) from ball bearing steel. The full sphere for the roll of the pressure prop is indicated on the right. The support cup at the vacuum vessel stays fixed, while the cup on the Helium vessel moves with the shrinkage/expansion of the Helium vessel. The support cups are marked by +

A typical result of straightening a dipole vacuum tube is shown in Fig. 15, in comparison with the original curved shape of the vacuum pipe. The success of the deformation was judged by the horizontal aperture achieved.

The result of the survey of the beam pipe, i.e. the position of the beam pipe center line after straightening, was transferred to marks, welded to the outside of the vacuum vessel. When setting up the straight magnet strings for ALPS II in the HERA tunnel, these survey marks will allow alignment of the dipoles to yield the largest possible overall horizontal aperture within the strings.

The curvature of the beam pipe before the straightening slightly varied among the dipoles. The maximum deviation from the straight line connecting the ends of the beam tube (17.9 mm in the example shown in Fig. 15) varied by ±2.5 mm between the extremes of 16 and 21 mm. The average was 18.4 mm. There is a correlation between this maximum deviation and the achieved aperture after the straightening procedure. In general, the larger the achieved final aperture, the smaller is the deviation from a straight line connecting the ends of the original beam tube.

The beam tubes also showed deviations from the horizontal plane, i.e. in the vertical direction by ±1 to 2 mm, both before and after straightening. These deviations reduce the vertical aperture from 55.3 mm (diameter of the beam tube) to 51.3 mm at most. This value equals the largest horizontal aperture obtained by the straightening procedure (see “Results” section) and does therefore not deteriorate the performance of the optical resonators.

During one cryogenic test, the mouse with reflector was installed into the vacuum pipe in the middle of a dipole, which was on the test bench at the time, to monitor the position of the vacuum pipe after cool down of the dipole. The position of the reflector in the cold vacuum pipe could be measured with the laser tracker through a quartz window on a flange in the end box of the test bench.

The measurement showed that the horizontal aperture increase, achieved by the deformation of the cold mass, is reduced by the cool down of the magnet by about 0.5 millimeter, caused by the thermal shrinkage of the pressure props and the cold mass. The impact on the performance of the two 120 m long optical resonators for ALPS II is tolerable (see “Results” section).

To check whether the straightening of the dipole would suffer from transportation between DESY and the HERA hall East for installation into the tunnel, a straightened dipole (BR 221) was put on a transport trailer and driven from the DESY site on public roads to the HERA hall East and back. Then the center line of the beam tube was measured again. It was identical to the one measured before the transportation.

The pressure props

As the deformation of the yoke is elastic, the deforming force by the pressure props must be maintained, also at cryogenic temperatures. However, the pressure props constitute a thermal short between the Helium vessel at 4K and the vacuum vessel at room temperature. To keep the additional heat flow to the 4K level of the cryogenics supply as low as possible, the props were made from a thin walled (1.5 mm) Titanium tube (see Figs. 9, 10, 12, and 16), a material with low thermal conductivity, comparably low thermal expansion, and large mechanical strength. In addition, the contact area at both temperature levels is small for the props at the outer suspensions, as the ends of the props form sections of a sphere. The thermal flux from room temperature to the yoke at liquid Helium temperature was estimated to about 1 Watt per prop from the thermal conductivity of the thin walled Titanium tube (see “Results” section).

The props near the ends of the dipole must allow for the length change of the yoke with respect to the vacuum vessel (≈ 30 mm total) during cool down and warm up and yet maintain the deforming force. Shaping the ends of the props as sections of a sphere, allows for a tilt of the props during cool down or warm up (see Fig. 16), without changing the distance between the vacuum vessel and the cold massFootnote 9 except for the thermal shrinkage of the props and the cold mass (see above).

The deforming forces are always perpendicular to the surfaces of the support cups, (see Figs. 16 and 9) resting on the Helium and the vacuum vessel, thus reducing the momentum on the prop and the danger of it tipping over. The support cups of the outer pressure props at the vacuum vessel stay fixed, while the cups on the Helium vessel move with the shrinkage/expansion of the Helium vessel.

The Titanium tube of the pressure prop in the middle was screwed into a stainless steel strip (5 mm thick and 50 mm wide), which matches the inner surface of the vacuum vessel (see Fig. 12). The steel strip remained in the cryostat after straightening the yoke. The middle pressure prop has a flat contact area to the Helium vessel and does not tilt during thermal cycles. It thus constitutes a fix point for the thermal shrinkage/expansion during cool down/warm up of the cold mass.

To place the pressure props at the right position and angle within the cryostat, special mounting tools were developed (see Fig. 17 and also Fig. 12). After positioning the prop, the assembly tool was removed. It should be noted, that all props are finally held in position inside the cryostat only by the spring pressure between the vacuum vessel and the Helium vessel.

Fig. 17
figure 17

Tool for proper placing of the outer pressure props. Left: 1: Plate to fasten the tool to the flange of the vacuum vessel, 2: Cradle to hold the pressure prop, 3: Pins to connect to the outer pressure plate. Middle: Complete prop in the assembly tool. Right: Outer pressure plate with support cup

The proper choice of materials and the concept were validated by a test of an outer pressure prop in vacuum at liquid Nitrogen temperature. A force of 40 kN was exerted on the prop in a test device while moving one side back and forth by ±15 mm several hundred times. No problem with the prop was encountered.

The new suspensions

The insertion of pressure props at any of the three positions, foreseen in the midplane of the magnet, was impossible with the original suspensions in place. The radiation shield box, connected to the suspension, was blocking the insertion of a prop (see Figs. 18 and 10). Therefore the original suspensions of the cold mass with the radiation shield box had to be removed from the cryostat for the insertion of a pressure prop.

Fig. 18
figure 18

Left: Original suspension of the cold mass removed from the cryostat. The suspension with the radiation shield box (1) prevented the installation of a pressure prop into the cryostat (see text). Middle: The new suspension, with a slit machined into the radiation shield box and Titanium strips replacing the G10 loop, allowed to slide the suspension over the installed pressure prop. 1: Radiation shield box, 2: G10 supporting loop, 3: Suspension screw, 4: Titanium support strips. Right: Suspension screw at top of the suspension

In the beginnings of the straightening studies, which were performed on a defective dipole used as an exhibit, all three suspensions were removed at the same time. The cold mass was still safely suspended by the remaining three suspensions. However, the yoke bent vertically by several millimeters, causing concerns over an undesirable reduction of aperture.

Therefore, in the final procedure, applied to all straightened dipoles, only one suspension was removed at a time, according to the following sequence: First, one of the outer suspensions was removed, then the corresponding pressure prop was installed. After a modification of the suspension (see below) it was reinstalled, now carrying again the weight of the cold mass. Then followed the same steps for the other outer suspension. Finally, the suspension in the middle was removed and modified. After the straightening of the magnet, the middle suspension was reinstalled in the same way as the other suspensions. The vertical deformation was small for this procedure (a few tenth of a millimeter) and could easily be restored by the new suspensions (see below).

Obviously, an installed pressure prop prevented the re-installation of the original suspension. Therefore a slit was machined into the radiation shield box, to allow for the re-installation of the suspension, when the pressure prop was in place. Also the G10 loops, supporting the cold mass, were replaced by an open structure, realized by Titanium strips (10 mm wide and 1 mm thick) to pass by the inserted pressure prop (see Fig. 18). The thermal flow to 4K due to the modified suspension was increased by 0.3 Watt per suspension i.e. 0.9 Watt per dipole (see “Results” section).

The free length of the support screws (see Fig. 18 right) at the top of the suspensions were measured before their removal from the cryostat. Before removing the shield box from an original suspension, the positions of the ears – for the fastening screws to the radiation shield – were marked on a special tool, while the upper part of the G10 loop had tight contact with the transfer pivot of the tool (see Fig. 19 left). After machining, the shield box was aligned in the device to the marks, before fastening it to the new suspension, positioned by the transfer pivot of the tool. These measures ensured, that the ears of the radiation shield box were at the same position on the new suspension as on the original one with respect to the support screw.

Fig. 19
figure 19

Left: Original suspension of cold mass mounted to the transfer tool. 1: Radiation shield box, 2: G10 supporting loop, 3: Fastening ears, 4: Transfer pivot. Right: Steel bracket fastened to the lower end of the new suspension replacing the support by the G10 loop. 1: Bracket, 2: Support pivot, 3: Lower end of new suspension

After the new suspension was inserted into the cryostat, the shield box was screwed to the radiation shield. An especially tailored package of super insulation foils, sliding over the pressure prop, was attached to the shield box. Then the length of the support screw on top of the suspension was adjusted to its original – before measured – value, ensuring that the new suspension – and thus the radiation shield – was at the same position as the original one. Finally a support bracket was fastened by nuts to the suspension. The bracket, now carrying the cold mass (see Fig. 19 right), was pushed up by nuts with only little force against the support pivot of the cold mass. The nuts were secured by a counter nut.

Finally the lower end of the suspension and the support pivot were shielded against thermal radiation by an Aluminium cap, covered with super insulation foil and attached to the radiation shield by two screws.


There were 23 spare magnets from the HERA proton ring available for straightening and subsequent cryogenic operation on the test bench. It should be noted, that these magnets were stored in a heated hall on the DESY site for about 25 years after their original test. All tested dipoles belong to the large contribution from Italy (50% of all superconducting dipoles) to the HERA project, built by the companies Ansaldo and Zanon.

Two magnets from the spares showed a missing or bad electrical connection, either at 4K or at room temperature, between voltage tabs on the superconducting coils – needed for quench detection – and the corresponding feed-through at the vacuum vessel. These magnets were rejected. During the test of one magnet, the power supply tripped for unknown reasons (no quench). As a precaution, this magnet was also rejected from installation into the ALPS II setup. Thus, 20 of the spare dipoles remained for the setup of the ALPS II experiment, designed for a total number of 24 dipoles.

The ALPS II experiment requires space for optics clean rooms at the ends of the magnet strings (see Fig. 3). To gain this space and, at the same time, yielding additional magnets for the ALPS II setup, several dipoles of the HERA ring were removed from the tunnel. These dipoles, which also belong to the above mentioned Italian HERA contribution, were also straightened and operated at the test bench.

Figure 20 shows the obtained horizontal apertures in mm on the vertical axis versus the identification name of the dipoles according to the chronicle order of the measurements. For total photon losses below 2·10−6 in the optical resonators, for infrared light at a wavelength of 1064 nm, an aperture of 45.5 mm is required at the outer ends of the experiment. The aperture values shown in the figure have to be reduced by 0.5 mm, due to the shrinkage of the pressure props and the Helium vessel during cool down (see “The survey of the vacuum pipe” section). For comparison the average horizontal aperture before the straightening of about 37 mm is shown.

Fig. 20
figure 20

Achieved horizontal apertures after the straightening of HERA dipoles in mm on the vertical axis versus the identification name of the dipoles according to the chronicle order of the measurements. For comparison the average horizontal aperture before the straightening is shown. For total photon losses below 2·10−6 an aperture of 45.5 mm is required at the outer ends of the experiment, for infrared light with 1064 nm wavelength used in ALPS II

The cross section of the stored photon beam in the optical cavities is larger at both ends of the experiment than in the middle (see Fig. 2). Therefore, in order to minimize clipping of the stored photon beam in the optical resonator, dipoles with larger apertures were selected to be positioned near the outer ends of the experiment and magnets with smaller aperture near the middle of the experiment. Figure 21 shows the apertures of the dipoles vs. their selected positions in the ALPS II setup. This selection leaves about ±2mm free space for adjustment uncertainties, without limiting the performance of the optical resonators.

Fig. 21
figure 21

Horizontal apertures of the dipoles installed in the HERA tunnel. Large apertures are at the outer ends of the magnet strings, smaller apertures close to the middle of the experimental setup. Near the ends of the strings for ALPS II, magnets with large quench currents (>6400 A) were selected, to compensate for potential additional heat loads from the neighboring boxes or the cryogenic bypass in the middle of the experimental setup. The positions of dipoles with a pumping port are marked by red circles. The vertical bar in the middle of the experiment indicates the position of the light tight wall

All dipoles were operated on the test bench up to their quench current twice. In addition all dipoles were operated continuously at the nominal operating current of the ALPS II experiment for about 8 hours. Figure 22 shows that all dipoles have quench currents well above the nominal operating current of 5693 A.

Fig. 22
figure 22

Measured quench currents of straightened dipoles at the test bench versus the identification number of the dipoles according to the chronicle order of the measurements

Near the ends of the strings for ALPS II, magnets with large quench currents (>6400 A) were selected, to compensate for potential additional heat loads from the neighboring boxes or the cryogenic bypass in the middle of the experimental setup (see Fig. 3).

The concern, that the performance of the dipoles would be deteriorated by the straightening, was not substantiated by the data (see Fig. 23). The differences between the dipole quench currents, before and after straightening, are below 3%.

Fig. 23
figure 23

Quench currents of dipoles before straightening vs. after straightening

Finally, we succeeded in obtaining dipoles with sufficiently large horizontal apertures and sufficiently large quench currents for two strings of 12 dipoles each, plus two spares.

The slight polygon shape of the outer vacuum vessel does not pose any problem in connecting adjacent magnets in the straight magnet strings, as verified in a test with two dipoles.

Among the selected dipoles for the experiment are 6 dipoles with a pumping connection from the outer vacuum vessel to the beam tube (see [19]). These will be evenly distributed along the strings, allowing adequate pumping of the beam tube at room temperature. The selected positions of the magnets with pumping ports are compatible with the selection of the dipole positions concerning the aperture (see Fig. 21).

A measurement of the additional heat loads on the 4K and 70K level, caused by the new suspensions and the pressure props, was performed. For this, the heat loads of a dipole were measured on the test bench before and after the modifications made during the straightening procedure. However, the heat loads from the adjacent cryogenic boxes dominated the measurements and their uncertainties, preventing a determination of the additional heat load of the magnet by the modifications. The measured heat loads were the same in both cases within the uncertainties, with the heat loads of the straightened dipole being even slightly lower than that of the original dipole.

The magnetic stray field was measured, as it might interfere with the electronics used in the detection of regenerated photons in the ALPS II experiment. The measurement was performed on the test bench with a pickup coil at the end of a dipole about 1 m away laterally from the axis and 0.5 m below the middle of the magnet. The stray field rises with the magnet current and amounts to 0.5 Gauss at the nominal operating current of 5693 A for ALPS II.

At the time of writing this report the installation of the dipole strings in the HERA tunnel is progressing.


The geometry of the HERA tunnel allows to install 2·12 HERA dipoles, at most, as straight strings, due to the curvature of the tunnel. Optical resonators for infrared light at a wavelength of 1064 nm, corresponding to this length, require a horizontal aperture at the outer ends of the experiment of 45.5 mm, for losses below 2·10−6 in the beam pipe.

This requirement was clearly met, as straightened dipoles with larger apertures were selected to be positioned near the outer ends of the experiment and magnets with smaller aperture near the middle of the experiment, following the envelope of the photon beam in the optical resonators. There is about ±2mm free space for adjustment uncertainties, without limiting the performance of the optical resonators.

By the ‘brute force’ straightening procedure we succeeded in obtaining dipoles with sufficiently large horizontal apertures and sufficiently large quench currents for two strings of 12 dipoles each for the ALPS II experiment, plus two spares.

Availability of data and materials

The data sets generated and analysed for this article are available at the DESY Engineering Data Management System (DESY EDMS)

Change history

  • 04 July 2022

    The License was not not correctly tagged in the HTML of the original publication, this article has been updated.


  1. The ALPS II Collaboration: Albert-Einstein-Institute, Hannover, Germany; Cardiff University, UK; DESY Hamburg, Germany; Johannes Gutenberg-University Mainz, Germany; University of Florida, Gainesville, USA

  2. Key people in the development of the HERA dipole were H. Kaiser, K. H. Meß, P. Schmüser, and S. Wolff.

  3. The dipoles were fabricated by companies in Italy (Ansaldo and Zanon) and Germany (ABB).

  4. A similar method was considered independently at CERN by P.Pugnat for LHC dipoles.

  5. The test bench was used already for the ALPS I experiment.

  6. Proposal by Gerhard Meyer, DESY

  7. Normally, the transportation fixtures prevent the cold mass from moving with respect to the vacuum vessel during transportation of the magnet.

  8. Unpublished study by Gerhard Meyer, DESY

  9. Proposal by Gerhard Meyer, DESY



Axion like particle




Hadron electron ring anlage


Large hadron collider


Technischer Überachungs Verein


Weakly interacting slim particle


  1. Peccei RD, Quinn HR. CP conservation in the presence of instatons. Phys Rev Lett. 1977; 38:1440.

    Article  ADS  Google Scholar 

  2. Irastorzi I, Redondo X. New experimental approaches in the search for axion-like particles. 2018.

  3. von Bibber K, Dagdeviren NR, Koonin SE, Kerman AK, Nelson HN. Proposed experiment to produce and detect light pseudo-scalars. Phys Ref Lett. 1987; 59:759.

    Article  ADS  Google Scholar 

  4. Ehret K, Frede M, Ghazarayan S, Hildebrandt M, Knabbe EA, Kracht D, Lindner A, List J, Meier T, Meyer N, Notz D, Redondo J, Ringwald A, Wiedemann G, Willke B. Resonant laser power build-up in ALPS. A ‘Light-shining-through-walls’ experiment. Nucl Instrum Meth. 2009; A612:83–96.

    Article  ADS  Google Scholar 

  5. Ballou R, Deferne J, Finger Jr. M, Finger M, Flekova L, Hosek J, Kunc S, Macuchova K, Meissner KA, Pugnat P, Siemko A, Slunecka M, Sulc M, Weinsheimer C, Zicha J (OSQAR Collaboration). New exclusion limits on scalar and pseudoscalar axionlike particles from light shining through a wall. Phys. Rev. 2015; D 92:092002.

    ADS  Google Scholar 

  6. Bähre R, Döbrich B, Dreyling-Eschweiler J, Ghazaryan S, Hodajerdi R, Horns D, Januschek F, Knabbe EA, Lindner A, Notz D, Ringwald A, von Seggern JR, Stromhagen R, Trines D, Willke B. Any Light Particle Search II, Technical Design Report JINST-001T-0313. 2009.

  7. Wolff S. The Superconducting Magnet System for HERA. In: Proceedings of the International Conference on Magnet Technology. Zürich: 1985. p. 62–67. DESY-HERA 85-21,

  8. Kaiser H. Design of Superconducting Dipole for HERA. In: Proceedings of the 13th International Conference on High Energy Accelerators (HEACC 1986), Vol 2. Novosibirsk: 1986. DESY-HERA 1986-14,

  9. HERA-A proposal for a large electron-proton colliding beam facility at DESY. 1981.

  10. Horlitz G. A central refrigeration system for the superconducting HERA proton magnet ring, DESY-HERA 84-02. 1984.

  11. Hoogeveen F, Ziegenhagen T. Production and detection of light bosons using optical resonators. Nucl Phys. 1991; B358:3–26.

    Article  ADS  Google Scholar 

  12. Sikivie P, Tanner DB, van Bibber K. Resonantly enhanced Axion-photon regeneration. 2007.

  13. Fukuda Y, Kohmoto T, Nakajima S, Kunitomo M. Production and detection of axions by using optical resonators. Prog Cryst Growth Charact Mater. 1996; 33:363–6.

    Article  Google Scholar 

  14. Põld JH, Spector AD. Demonstration of the length stability requirements for ALPS II with a high finesse 9.2m cavity. EPJ Tech Instrum. 2020; 7(1):1.

    Article  Google Scholar 

  15. Spector AD, Põld JH, Bähre R, Lindner A, Willke B. Characterization of optical systems for the ALPS II experiment. Opt Express. 2016; 24:9237.

    Article  Google Scholar 

  16. Arias P, Jäckel J, Redondo J, Ringwald A. Optimizing light-shining-through-a-wall experiments for axion and other WISP searches. Phys Rev. 2010; D82:115018.

    ADS  Google Scholar 

  17. Põld JH. Analyzing the option for longer magnet strings for the ALPS II experiment from the optics point of view, ALPS internal report. 2019.

  18. Trines D. The HERA Cold Bore Vacuum System, DESY-HERA 85-22. 1985.

  19. Böhnert M, Brauer D, Hensler R, Hoppe D, Hubert D, Rehlich K, Sanok Z, Trines D, Wyszogrodzki A. The cold bore beam pipe vacuum system of the HERA proton storage ring, DESY-HERA 92-02. In: Proceedings of the 15th International Conference on High-Energy Accelerators, HEACC 1992: 1992.

  20. Meinke R. Superconducting magnet system for HERA. IEEE Trans Magn. 1991; 27(2):1728–34.

    Article  ADS  Google Scholar 

  21. Schmüser P. Field quality issues in superconducting magnets. PAC 1991 proceedings: IEEE; 1991, p. 37.

  22. Barton Jr. HR, Clausen M, Kessler G, Rettig S. Cryogenic Experience at the HERA Magnet Measurement Facility, DESY-HERA 87-14, Contribution to the Cryogenic Engineering Conference CEC87. St. Charles; 1987.

  23. Meß KH. Quench Protection at HERA, DESY-HERA 87-10, Contribution to the 12th IEEE Particle Accelerator Conference (PAC1987), Washington, USA, Conf. Proc. C 870316. 1987:1474–6.

  24. Eschke J, Sawlanski O, Stolper M. Soldering the connection between the dipole on the test bench and the power supply, Internal report. 2016.

  25. Meissner D. Elastische Rückbiegung eines HERA Dipolmagneten, Ergebnisse der FEM-Berechnung, Internal report, DESY ZM1. 2015.

  26. Hintz H. Anleitung zum Umbau der HERA Dipole, Internal report. 2016.

  27. Albrecht C, Barbanotti S, Fuhr O, Hagedorn C, Hintz H, Jensch K, Klos R, Maschmann W, Paschold O, Tödten T, Trines D. Using long strings of s.c. HERA dipoles in search for axion like particles (ALP’s), PATRAS Workshop 2018, DESY, Germany.

  28. Albrecht C, Barbanotti S, Hintz H, Jensch K, Klos R, Maschmann W, Sawlanski O, Stolper M, Trines D. Straightening of superconducting HERA dipoles for the any-light-particle-search experiment ALPS II, DESY Report 20-070.

Download references


Special thanks go to Gerhard Meyer for most of the detailed layout of the straightening procedures. He supplied many ideas and designed f.e. the pressure screws, the pressure props, and the assembly tools.

The idea for a brute force straightening was stimulated by Rüdiger Bandelmann, when proposing the G10 transverse stabilization rods in the middle of the HERA dipole for a deformation of the cold mass.

The DESY survey group MEA2 with Wolf Benecke, Yvonne Imbschweiler, Nicolai Lass, and Hans Peter Lohmann made the survey of the beam pipe during the straightening of the dipoles.

Daniel Meissner from the DESY design office ZM1 performed the FEM calculations, necessary for the approval of the straightening procedure by the agency for pressure vessel safety (TUEV).

Babette Döbrich and Martin Berg were of great help during the assembly of the first dipoles and the functional test of the pressure props.

The DESY group MEA with Philipp Altmann, Clemens Bösch, Stefan Baark, and Henrik Weitkämper were a great support during the assembly of the first dipoles. Clemens Bösch designed and fabricated the tool to transfer the position of the shield box from the original to the new suspensions. Henrik Weitkämper did the modifications of the shield box for the first dipoles.

Members of the DESY cryogenics group MKS were of great support during the straightening of the HERA dipoles: Christian Hagedorn was strongly involved in the straightening work and in machining of parts, Olaf Fuhr also helped in the straightening work, Oliver Paschold was involved in magnet installation and the welding of survey marks on the vacuum vessel, Thomas Tödten organized the magnet storage and the repainting of the dipole vacuum vessels.

Martin Schäfer and Frank Wien were very cooperative in modifying most of the shield boxes without any delay.

Jürgen Eschke made the electrical connections of the magnet to the cryogenic boxes with Matthias Stolper in the beginning, later with Olaf Sawlanski.

The measurements of the quench currents were performed by Heiner Brück with Matthias Stolper for the first dipoles.

Lothar Steffen installed a prototype quench detection system in parallel, later to be used for the ALPS II experiment.

Wolfgang Ratuschni from the DESY group MKK made sure that the power supply operated properly.

Thanks go to the operators of the central DESY cryogenics plant for the cryogenic operation of the dipoles on the test bench.

Bernd Petersen as group leader of the cryogenics group MKS at DESY and Detlef Sellmann as his deputy followed the work on the test bench and supported the activities.

Dennis Lenz and the DESY transportation group of Uwe Eggerts managed the transportation of the dipoles and the positioning on the test bench.

The DESY vacuum group MVS with Thomas Kurps, Rene Ritter, Matthias Schwalger, Antonio Wagner and Sven Lederer were very supportive on the insulating vacuum system of the dipoles.

Jan Kuhlman made the new CAD drawings for the HERA dipole and the modifications.

Björn Hager and the central DESY Workshop supplied the parts for the pressure props and the new suspensions. The first pressure props were fabricated by Uwe Packheiser.

Daniela Käfer managed the storage of the data from the magnet straightening and quench current measurements in the EDMS data base.

Martin Köhler helped in formating the manuscript for submission to the preprint server and to EPJTI.

We want to thank the DESY directorate for allowing, that personnel engaged in the preparation of the work and the necessary tests.

Finally we want to especially thank Axel Lindner– the spokesperson of the ALPS II experiment– for his encouragement and continuous support of this work, and careful reading of the draft.


The work described in this article was funded by DESY. Open Access funding enabled and organized by Projekt DEAL.

Author information

Authors and Affiliations



C.A. worked on the straightening of the magnets, prepared tools and materials, and worked on the preparation of the tests, S.B. prepared pictures and graphs and coedited the text, H.H. accumulated a detailed instructions manual of the working steps, worked on straightening and the preparation of magnets for the cryogenic tests, K.J. coordinated the work for the magnet straightening, the installation on the test bench and the cryogenic test, R.K. worked on the magnet straightening and the preparation of the cryogenic tests, W.M. worked on the magnet straightening and the preparation of the cryogenic tests, O.S. worked on the electrical connections of the magnets to the power supply and the operation with current, M.S. worked on the electrical connections of the magnets to the power supply, the operation with current, updated the quench detection electronics, and performed the stray field measurement, D.T. supervised the work connected with the straightening, the optical survey, the tests and wrote the text of the article. The author(s) read and approved the final manuscript.

Corresponding author

Correspondence to Dieter Trines.

Ethics declarations

Competing interests

The authors declare that they have no competing interests.

Additional information

Publisher’s Note

Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Additional information

Rights and permissions

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Albrecht, C., Barbanotti, S., Hintz, H. et al. Straightening of superconducting HERA dipoles for the any-light-particle-search experiment ALPS II. EPJ Techn Instrum 8, 5 (2021).

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI: