Strongly anisotropic layered superconductors hold Josephson vortices across layers in parallel magnetic fields1. Josephson vortices have no core, because the phase winding occurs in the non-superconducting region between the layers. When the magnetic field is applied perpendicular to the layers, Abrikosov vortices with a core nucleate within each layer. Abrikosov vortices in layered superconductors are composed by columns of disk-like pancake vortices and their shear modulus is significantly smaller than the shear modulus of Abrikosov vortices in isotropic superconductors. In the absence of Josephson vortices or pinning the pancake vortices form straight lines along the c-axis. But in tilted magnetic fields, there is a finite in-plane magnetic field component and Josephson vortices appear. The mutual interaction between the columns of pancake vortices and the Josephson vortices leads to deformed combined lattices consisting of tilted vortex lines having kinks and different arrangements composed by layers with alternating pancake and Josephson vortices2,3. Buzdin et al.4 showed that the pancake vortices in such composite vortex lattices in tilted magnetic fields attract each other at large distances when located on top of a Josephson vortex. This long range attraction shapes the structure of combined lattices and leads to the formation of chains of pancake vortices along Josephson vortices. The chains decorate Josephson vortices, because pancake vortices sit rather close to each other along the lines of Josephson vortices. This occurs even at small perpendicular magnetic fields.

The vortex attraction in tilted magnetic fields is quite a general phenomenon and is also expected in superconductors that are not extremely anisotropic, such as YBa2Cu3O7 and 2H-NbSe2. It is caused by the current distribution produced by tilted magnetic fields when superconducting properties are anisotropic. Supercurrents then circulate on complex paths, which consist of ellipsoids whose shape depends on the tilt of the magnetic field with respect to the crystalline direction and this easily leads to the appearance of a minimum in the interaction potential between vortices5,6,7,8,9,10,11,12.

The phase diagrams with intertwined Josephson and pancake lattices in highly anisotropic layered superconductors have been intensively studied as a function of the magnetic field and temperature1,2,13,14,15,16,17,18,19,20,21,22. Josephson vortices have circulating currents on an area defined by the interlayer separation s and the in-plane length λJ (Fig. 1a, b). Pancake vortices have currents circulating on a disk of size of order of the in-plane penetration depth λab. Pancake vortices lie in each layer. Thus, there are pancake vortices in the two layers forming the Josephson vortex. The mutual interaction between the two kinds of vortices leads to a shift of the pancake vortices lying in each layer along the Josephson vortex. Thus, pancake vortices are not exactly on top of each other, as usual in an Abrikosov lattice in perpendicular fields, but are slightly displaced along the length of the Josephson vortex. This is due to the Lorentz force from the intralayer currents, which are directed opposite to each other in each layer. There is a phase change of 2π across each vortex, once across layers for a Josephson vortex and once within each layer for a pancake vortex. But when pancake vortices are not exactly on top of each other in two adjacent layers, the π phase slip across the two layers vanishes in between displaced pancake vortices. Thus there is no Josephson vortex in between two pancake vortices at two different locations on two different layers (Fig. 1c, d). This results in an energy gain, which is of order of the Josephson coupling energy of the section of the Josephson vortex that disappears in between pancake vortices. When repeating along the whole sample, the presence of pancake vortices on top of the Josephson vortex can thus significantly decrease the overall energy cost of tilted magnetic fields. The interaction between neighboring pancake vortices in the same layer provides a balance and there is an equilibrium distance for pancake vortices along the Josephson vortex. The variation of this distance with tilt and value of the magnetic field and with temperature leads to the equilibrium phase diagrams discussed in literature1,2,21.

Fig. 1
figure 1

Crossing lattices of pancake and Josephson vortices. In a we show superconducting layers by gray planes. Josephson vortices are represented by tubes of elliptical cross-section with axis γs and s where γ is the anisotropy parameter and s the interlayer distance. Yellow disks represent pancake vortices, whose size in the schematic picture is of the order of the circulating current distribution, i.e., of order λab. The pancake vortices are located along the Josephson vortex in the top and bottom planes. In b we show a lateral cross-section through a Josephson vortex (at a position along x free of pancake vortices). Josephson current is shown by black arrows between layers. The phase difference Δφ between layers as a function of the position is also given. The current in each layer is shown by black arrows within each layer. The lateral size of the Josephson vortex is approximately of λJ = γs. In c we show the phase difference between consecutive layers along a line through the center of a Josephson vortex (y = 0), taking into account the presence of pancake vortices (yellow disks). In the white areas Δφ = 2π = 0 and in the green areas Δφ = π, because pancake vortices are displaced to each other. The currents circulating across a Josephson vortex lead to oppositely oriented Lorentz forces in each layer. The displacement u is induced by the Lorentz force and provides an energy gain thanks to the disappearance of the phase difference Δφ = 2π = 0 between pancake vortices. In d we show a view of a Josephson vortex with pancake vortices from the top. This is highly schematical, detailed calculations provide intricate patterns depending on pancake vortex density and relative sizes of pancake and Josephson vortices, see e.g., refs. 1,2,13,14,15,16,17,18,19,20,21

Here we study slightly underdoped Bi2Sr2CaCu2O8 (BSCCO), which is a highly anisotropic superconductor consisting in CuO2 bilayers separated by a distance s = 1.5 nm, with Ca, SrO, and BiO layers in between. We find an anisotropy factor γ ≈ 1000 (γ = λc/λab = ξab/ξc with λab and ξab the in plane and λc and ξc the out-of-plane penetration depths and coherence lengths respectively). We mostly study Josephson vortices with an in-plane magnetic field. We decorate the Josephson vortices by pancake vortices and work in a strongly out-of-equilibrium situation. We obtain vortex patterns by modifying the amount of pancake vortices on top of the Josephson vortices through repeated heating and cooling. We show that, under such out-of-equilibrium situation, pancake vortices can be displaced in between Josephson vortices and Josephson vortices can be manipulated by changing the in-plane direction of the magnetic field.


Invasive action of the Magnetic Force Microscope (MFM) tip

We start by discussing briefly the decoration of Josephson vortices with pancake vortices and the invasive action of the MFM tip. In Fig. 2a we show a MFM image of a crossing lattice of Josephson and pancake vortices obtained at 5 K. To obtain this image we first apply a magnetic field of 50 G perpendicular to the layers. This introduces pancake vortices in the sample. We then apply 200 G parallel to the layers and ramp the perpendicular component down to zero. We briefly heat the sample to above 50 K and cool down again. This leads to a re-arrangement of pancake vortices that position themselves along the Josephson vortices, creating the vertical rows shown in Fig. 2a.

Fig. 2
figure 2

Tip induced vortex motion far below the depinning temperature. Magnetic Force Microscope (MFM) images taken at 5 K (a) 12 K (b), and 15 K (c) at a magnetic field of 200 G applied along the y-axis of the images. Prior to the application of the parallel magnetic field, we have induced pancake vortices to decorate Josephson vortices, by applying a perpendicular magnetic field, removing it and heating repeatedly to decrease the density of pancake vortices lying in between Josephson vortices, see the Supplementary Fig. 1. The field of view is the same for all images. The contrast is given by the color bars on the right in changes in degrees of the phase of the cantilever oscillation and white bars in the images are of 2.4 μm size

By heating above 50 K again, we can reduce the amount of pancakes in between Josephson vortices (see also Supplementary Fig. 1) until we reach a non-equilibrium situation with an in-plane magnetic field and pancake vortices lying on top of Josephson vortices, discussed below.

It is quite convenient to discuss the invasive action of the MFM tip using the location shown in Fig. 2a, which was obtained before repeated heating and has quite a large amount of interstitial vortices. When we increase the temperature from 5 to 15 K (Fig. 2b, c), we observe that the size of pancake vortices in the images is considerably increased when reaching 15 K (see also Supplementary Figs. 2 and 3 and Supplementary Notes 1 and 2). At higher temperatures, we do not resolve pancake vortices anymore. This increase in apparent size is due to thermal motion. Thermal motion is activated by the wiggling action produced by the MFM tip when scanning on pancake vortices, in a similar way that vortex lattice melting is favored by a dithering magnetic field. To complete a square image, the tip scans along a line (say, the x-axis, as in Fig. 2) and then moves to the next. Thus, it moves fast along one direction (say, x-axis) and slow along the other direction (say, y-axis). The tip scans several times over each pancake vortex when moving along the fast scan direction. Avraham et al.23 showed that a dithering magnetic field considerably reduces vortex pinning. It has been shown previously that scanning a magnetic tip produces such a dithering field locally and enough vortex shaking to eliminate pinning24,25,26,27,28,29,30. This allows to manipulate pancake vortices thanks to the dithering magnetic field produced by the tip motion during scanning. It is interesting to note that the temperature where we observe depinning, which is of 15 K, is far below the depinning temperature of BSCCO (a few K below Tc = 88 K)1,31. The depinning temperature was reduced down to about 30 K in a similar sample by dithering magnetic fields23. In our experiment, we reach temperatures about half that value, suggesting that the spatial gradient of the magnetic field plays a role and increases the force on vortices during this process. By increasing and decreasing the temperature in a relatively small interval, we can thus trigger pancake vortex motion using our MFM tip.

Moving pancake vortices between Josephson vortices

We now study a situation where we have built a decorated Josephson vortex lattice with only a few interstitial pancake vortices and show that we can move pancake vortices across Josephson vortices using the MFM tip. In the Fig. 3a, the tilt is along the x-axis of the image and most pancake vortices are aligned and pinned at the Josephson vortices. The in plane component of the magnetic field in this image is aligned with the slow axis of the scan direction. We then increase the temperature to 12 K and exchange slow and fast scanning directions. We observe the images shown in Fig. 3b, c. Pancake vortices move across Josephson vortices. Note that vortex motion is perpendicular to the slow scan direction. This corresponds to the view that the dithering magnetic field reduces or eliminates vortex pinning. The fast scanning acts to reduce the pinning and the vortices are slowly pushed along the slow scan direction when the tip moves from one line to the next. Correspondingly, vortex motion is not exactly perpendicular to the Josephson vortices, but with a small angle (see also Supplementary Fig. 2). The angle depends on the direction of the fast scan, from right to left (Fig. 3b) or viceversa (Fig. 3c).

Fig. 3
figure 3

Pancake vortex motion across Josephson vortices. Magnetic Force Microscope (MFM) images at a magnetic field of 200 G parallel to the layers. The in-plane direction of the magnetic field is shown by the white arrows. The scanning procedure is detailed in the Methods section. The direction at which the tip scans fast is given by the black arrows. Image a is taken at 5.5 K and b, c at 12 K. White bars in the images are of 2.6 μm size. In b, c we observe pancake vortex motion along the slow scanning direction (towards the top of the image) across Josephson vortices. This provides traces of pancake vortices that are slightly to the left in b and slightly to the right in c. We mark two of these traces by black dashed lines with arrows. The contrast is given by the color bars on the right in changes in degree of the phase of the cantilever oscillation (see Methods section)

Approaching and crossing Josephson vortices

We now produce crossing Josephson vortices using the combined action of pinning and changing the direction of the in-plane magnetic field. We start by nucleating a single decorated Josephson vortex in a field of view that has a linear defect. The linear defect is actually a large circular wrinkle (details shown and discussed in the Supplementary Note 3). We apply the in-plane magnetic field exactly along the defect and observe that we nucleate a Josephson vortex along the defect (Fig. 4a). We then turn the in-plane magnetic field by about 10 degrees and heat and cool several times. We observe further Josephson vortices in the field of view. These are Josephson vortices that are oriented along the tilt of the magnetic field and are thus at an angle with respect to the Josephson vortex pinned at the wrinkle (Fig. 4b, c). Heating and cooling from Fig. 4b, c leads to motion of the decorated Josephson vortex lines. As we can see in the left part of the Fig. 4c, the Josephson vortices do not repel. The leftmost Josephson vortex has approached the pinned Josephson vortex and the Josephson vortex in the middle of the image Fig. 4c results from the motion of a Josephson vortex from the lower left corner to the middle of the image. In this process, the latter vortex has joined to pancakes that were previously located in between Josephson vortices in the middle of the image in Fig. 4b. The observed lines of Josephson vortices, lying in different layers (as discussed below), clearly cross each other. The density of pancake vortices along the crossing Josephson vortices changes when they are close to each other. For instance, the upper part of the leftmost Josephson vortex in Fig. 4c has a smaller density than the lower part.

Fig. 4
figure 4

Attraction between crossing Josephson vortices. In a we apply a magnetic field of 200 G tilted 5 degrees with respect to the y-axis of the image (white arrow). In b we show the same field of view after modifying the in-plane tilt of the magnetic field by 10° (white arrow) and heating once up to 20 K. In c we show the same image, after heating anew to 20 K. Images are taken at 5.3 K. Fast scanning direction is given by the black arrow. The contrast is given by the color bars on the right in changes in degree of the phase of the cantilever oscillation (see Methods section) and white bars in the images are of 2.6 μm size. In d we show a schematical view of Josephson vortices (green tubes), layers (gray planes), and pancake vortices (yellow disks). Josephson vortices cross in different layers. When they join, they share the same pancake vortex columns (view from the top, e), leading to a decrease in energy that produces an effective attractive interaction between Josephson vortices decorated by pancake vortices


Most previous experiments dealing with crossing Josephson and pancake vortex lattices were made close to liquid nitrogen temperatures using non-invasive imaging such as scanning Hall microscopy. Modifications in the Josephson vortex structure can then be made by changing the direction of the magnetic field2,21.

In our experiments, we take advantage of dithering field produced by the moving MFM tip. The magnetic field due to the scanning MFM tip oscillates with a frequency of the order of several tens or hundreds of Hz (see Methods section for details). Previous experiments used the same effect to move vortices in other cuprates with less in-plane vs out-of-plane anisotropy and in thin films of low temperature superconductors24,25,26,27. Macroscopic experiments have shown vortex shaking at frequencies ranging from tens of Hz to hundreds of kHz also in both low temperature and in cuprate superconductors, including BSCCO23,29,32. This provides the opportunity to manipulate vortices and show their vortex motion and mutual interaction at low temperatures, even in presence of strong pinning and interacting Josephson and pancake vortex lattices in BSCCO.

When the magnetic field is parallel to the layers, say of 200 G, the distance between Josephson vortices along the c-axis az ≈ 10 nm, which is nearly an order of magnitude larger the distance s between superconducting CuO2 bilayers (s = 1.5 nm). The pancakes decorate two adjacent rows of Josephson vortices. These occupy different interlayer spaces, shifted by az/2 ≈ 6 nm33. Therefore, when we drag the row of pancake vortices toward the pancake vortices decorating another Josephson vortex in the experiment shown in (Fig. 4b, c), the approach and crossing occurs between different layers. When two Josephson vortices cross (Fig. 4) the rows of pancakes are additionally distorted by the flux from the pancakes in the Josephson vortex immediately below (Fig. 4c, d). The resulting decrease of the vortex energy provides a mechanism of a short range attraction between rows of Josephson vortices.

The energy per unit area of the Josephson interaction between superconducting layers is given by EJ(1 − cosΔφ), where \(E_{\mathrm{J}} = \frac{{s{\mathrm{\Phi }}_0^2}}{{16\pi ^3\lambda _{ab}^2\lambda _{\mathrm{J}}^2}}\) and Δφ is the phase difference between layers33. By contrast, the energy due to the mutual attraction between two pancakes to lie on top of each other is \(E_{\mathrm{M}} = u^2{\mathrm{\Phi }}_0^2\left( {\frac{1}{{32\pi ^2\lambda _{ab}^4}}\mathrm{ln}\left( {\frac{{\lambda _{ab}}}{u}} \right)} \right)\) where u is the displacement of pancake vortices between layers (Fig. 1b). When pancake vortices are displaced along the Josephson vortex, the total energy is of order of EJλJu + EM. The crossing of the pancake stack with a Josephson vortex produces stack’s deformation and leads to the energy decrease \(\delta E \approx - E_{\mathrm{J}}\lambda _{ab}^2 \approx - \frac{{{\mathrm{\Phi }}_0^2}}{{\gamma ^2s}}\)33.

When two Josephson vortices are one under the other, the same pancake stacks cross them, which doubles the energy gain due to the crossing. This leads to the attraction between these Josephson vortices. The corresponding attractive force (per one stack crossing) can be estimated as \(F_{{\rm{att}}} \approx \frac{{\delta E}}{{\lambda _{\mathrm{J}}}} \approx \frac{{{\mathrm{\Phi }}_0^2}}{{\gamma ^3s^2}}\), where we took into account that the effective mutualisation of the pancake stacks occurs when the distance between Josephson vortices is less than λJ. The equilibrium distance between pancake stacks decorating Josephson vortex is ≈ 4λab and the attraction force Fatt (per unit length) between Josephson vortices can be estimated as \(F_{{\rm{att}}} \approx \frac{{{\mathrm{\Phi }}_0^2}}{{\gamma ^3s^2\lambda _{ab}}} \approx 5 \times 10^{ - 6}\,{\mathrm{Nm}}^{ - 1}\). This force is comparable to the repulsive force Frep between Josephson vortices \(F_{{\rm{rep}}} \approx \frac{{{\mathrm{\Phi }}_0H_{c1}}}{{\lambda _{ab}}} \approx \frac{{{\mathrm{\Phi }}_0^2}}{{\gamma \lambda _{ab}^3}}\). This makes it possible to obtain the metastable configuration of Josephson vortices with crossing and branching as observed in the experiments and shows that Josephson vortices lying in different planes have a tendency to share pancakes.

Grigorenko et al.17 have extensively discussed the interaction between linear defects in the CuO2 bilayers and crossing lattices using Scanning Hall Microscopy and tilted magnetic fields at liquid nitrogen temperatures. It has been shown that pancake vortices can be preferentially pinned at linear defects, favoring that Josephson vortices are located along these lines. Usually, linear defects lie perpendicular to each other and are of a finite length. This can lead to kinks in the pancake vortex distribution when abruptly modifying the in-plane magnetic field, because some vortex sections remain pinned whereas others free themselves. Images then show Josephson vortices that fork, similar to those we see in our experiment. Experiments in ref. 17 were made close to liquid nitrogen temperatures, whereas we work at much lower temperatures. Furthermore, they abruptly modified the magnetic field, whereas we use a superconducting coil which is slow. Finally, the phenomenon of forking appears here in a true wrinkle that leads to a considerable modification of the surface (see Supplementary Note 3), suggesting that the strongly pinned Josephson vortex is at the surface. Linear defects might be related to small steps at the surface of finite size. We did not manage to pin and cross vortices with such defects, in spite of trying. This shows that the temperature is playing a relevant role in vortex manipulation. Manipulating vortices at low temperature requires very well defined pinning centers. Nevertheless, it is clear that our results are also influenced by quenched disorder. For instance, our images show pancake vortex lines that are not completely straight and there are often pancake vortices in between lines.

We can now discuss the observed drag of pancake vortices across Josephson vortices by the tip (Fig. 3). The force needed to move pancakes can be of order of Fatt, which gives about 5 pN if we consider a length of the pancake column of order of a micron. This suggests that it is relatively simple to move pancakes across the Josephson vortices, as made in Fig. 3b, c. Note that in that experiment, the temperature is close to the depinning threshold, which explains the decrease in the depinning force with respect to experiments made at lower temperatures. Furthermore, the pancake vortices can be also pushed into the neighboring Josephson vortices (arrows in Fig. 3b, c), showing again that the effective attractive interaction of pancake vortices inside a Josephson vortex strongly influences vortex dynamics.

It is also worth to discuss the lateral motion of pancake vortices in between Josephson vortices (dashed lines in Fig. 3b, c). The crystal is aligned in such a way that the nodes of the d-wave superconducting order parameter are located along the diagonals in Fig. 3a–c. Macroscopic critical current experiments in the flux flow regime show indications for enhanced mobility along these directions34. It thus is tempting to think that the additional quasiparticles present along nodes favor, together with the lateral push of the tip, the direction of motion in these experiments.

Vortex entanglement, which is a usual situation in superfluids, is more difficult to find experimentally in superconductors35,36. Using manipulation with MFM, it is in principle possible to entangle vortices in layered superconductors. The entangled state consists of interacting groups of vortices, forming, for instance, helices or disordered tangles and is different from the situation where vortices cut each other37,38. The entangled state results in strongly reduced vortex mobility due to the interaction among vortices, whereas cutting increases vortex mobility and reduces pinning39,40,41,42. The low coupling between pancake vortices lying in different planes makes it difficult to produce vortex entanglement (instead of flux cutting) in layered two-dimensional systems as BSCCO37. Previous pancake vortex manipulation experiments using a MFM in YBa2Cu3O6.4 show that, even in perpendicular fields, it is possible to produce kinks in lines of pancake vortices43. Here we have shown that, in parallel magnetic fields, Josephson vortices lying in different planes can move to be one on top of the other thanks to the attractive interaction among pancake vortices. The modifications in the interaction between vortices produced by tilted magnetic fields have been previously considered and depend on the anisotropy of the superconducting properties40,44. However, the strongly non-equilibrium situation we unveil here in tilted magnetic fields has not been treated until now and significantly adds to the previous observation of kinks in Abrikosov pancake vortex lines43. In particular, the effective attraction between Josephson vortices that we unveil here shows that crossing lattices of Josephson and pancake vortices can have strong interactions among them. If this leads to increased pinning and avoids flux cutting is not fully clear from our data. We also see that crossing Josephson vortices are quite stable and remain when rotating the magnetic field (see Supplementary Fig. 3). This suggests that pinning instead of flux cutting is indeed dominating the behavior at very low magnetic fields.

In summary, we have shown how to manipulate pancake and Josephson vortices by combining a MFM tip and rotating magnetic fields well below the critical temperature. We find that pancake vortices can be dragged in between Josephson vortices and unveil an effective attractive interaction between pancake vortices lying inside Josephson vortices.


Sample and Magnetic Force Microscope (MFM) setup

We have measured a BSCCO single crystal with onset Tc of 88 K, i.e., on the slightly underdoped regime45,46. We mounted a sample in the sample holder of a low temperature MFM and inserted the microscope in a three axis vector magnet. The setup is described by Galvis et al.47. The crystal is a millimeter sized rectangular plate with a thickness of about 0.3 mm. We cleaved the crystal and aligned it with the main axis of our coil system, to apply the z-component of the magnetic field along the c-axis and align x and y components of the magnetic field with the in-plane crystalline axis and the x and y directions of the scanning field of view. We prepared our tip by leaving a coercive magnetic field on the tip that is parallel to the z-component of the applied magnetic field. We always applied magnetic fields well below the switching or saturating fields of the tip47.

MFM images

The color scale of the images provides the change in the phase of the oscillation of the cantilever with respect to the excitation as a function of the position. The interaction between tip and sample can be influenced by the local magnetic field, but also by a variety of other interactions, such as electrostatic interactions, stray magnetic fields coming from close-by areas of the sample, or small changes in the magnetic properties of the tip. Thus, the color scale cannot be easily transformed into a magnetic field. When the tip is far enough, however, magnetic force is expected to dominate other effects. Thus, we can consider, given the mentioned caveats, that, in each image, the color scale provides relative measure of the changes in the magnetic field as a function of the position. As a matter of fact, it is quite clear from the images that, when vortices wiggle and their apparent size increases, the corresponding contrast in the MFM images (difference in phase across the whole image) is also reduced. Furthermore, tests such as the density of pancake vortices with respect to the tilt of the magnetic field (see Supplementary Note 4), provide results in good agreement with expectations from simple geometrical constructions giving the z-component of the applied magnetic field. Images are rendered using WSXM software48 and software developed by some of the authors that will be described in another publication.

Scanning process and dithering field

The scanning process is optimized to make fast images. We make lines by going forth and back with the tip, and then advance one further step in the other direction. The direction for back and forth scanning is the fast scanning direction, and the direction perpendicular to it is the slow scanning direction. We scan close to the sample to record topographic information in AFM (Atomic Force Microscopy) mode when we go forth and retrace the tip about 50 nm and scan back the same line to record the magnetic image (MFM mode), or viceversa. The left to right and right to left motion of vortices in Fig. 3b, c is produced by the scan close to the sample in AFM mode. The scanning speed is of about a second per scanning line and we usually make images of 256 × 256 points. The tip needs between between 0.01 and 0.05 seconds to scan across a vortex, which gives an oscillating magnetic field of between several tens and a hundred Hz.

Calculations of distances between vortices and sample parameters

Following Buzdin et al.4, we can calculate the equilibrium distance between pancake vortices and find d ~ 4λab ~ 1 μm for B|| = 200 G. Using the distance between the pancake rows drows and the value of the magnetic field B we can calculate the anisotropy factor of our BSCCO crystals γ and the distance between Josephson vortices along the c-axis, az1,49,50. We obtain \(\gamma = 2d_{{\rm{rows}}}^2B{\mathrm{/}}\left( {\sqrt 3 {\mathrm{\Phi }}_0} \right) \approx 1000\) and az ≈ 10 nm. The lateral size of the Josephson vortex is given by γs where s is the distance between CuO2 bilayers and we find approximately a μm (s being 1.5 nm).