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Laser production of highly charged ions

Abstract

A summary of ion generation experiments at both low (10(9) W=cm²) and high (10(16) W=cm²) laser intensities, using Nd:YAG and iodine lasers, as well as the properties of the ions produced, are presented. Different medium- and high-Z elements were tested as a target: Ag, Al, Au, Co, Cu, Nb, Ni, Pb, Pt, Sn, Ta, W. A maximum charge state 55+ and maximum energy 34 MeV were recorded for Ta ions at high laser intensities, while the charge states up to 10+ and energies lower than 10 keV are characteristic for the region of low limit intensities. At laser intensities above 2 × 10(14) W=cm² conditions for the presence of nonlinear processes are fulfilled and ion acceleration due to ponderomotive force appears, in addition to the thermal and hot electron guided ambipolar acceleration. The existence of two production mechanisms for highly charged ions with charge states above z = 50+ has been demonstrated by changing the minimum focus position with regard to the target surface (by changing the interaction length with pre-formed plasma for relativistic self-focusing). Various potential applications of LIS are mentioned.


Laser production of highly charged ions

L. LáskaI; J. BadziakII; F.P. BoodyIII; S. GamminoIV; K. JungwirthI; J. KrásaI; M. PfeiferI; K. RohlenaI; J. UllschmiedI; P. ParysII; J. WolowskiII; †E. WorynaII; L. TorrisiIV,V

IInstitute of Physics, A.S.C.R., Na Slovance 2, 182 21 Prague 8, Czech Republic

IIInstitute of Plasma Physics and Laser Microfusion, Hery St. 23, 00-908 Warsaw, Poland

IIIIon Light Technologies GmbH, 93077 Bad Abbach, Germany

IVINFN - Laboratori Nazionali del Sud, Via S. Sofia 44, 95123 Catania, Italy

VUniversita di Messina, Ctr. Papardo-Sperone, 31, 98166 S. Agata, Messina, Italy

ABSTRACT

A summary of ion generation experiments at both low (109 W=cm2) and high (1016 W=cm2) laser intensities, using Nd:YAG and iodine lasers, as well as the properties of the ions produced, are presented. Different medium- and high-Z elements were tested as a target: Ag, Al, Au, Co, Cu, Nb, Ni, Pb, Pt, Sn, Ta, W. A maximum charge state 55+ and maximum energy 34 MeV were recorded for Ta ions at high laser intensities, while the charge states up to 10+ and energies lower than 10 keV are characteristic for the region of low limit intensities. At laser intensities above 2 × 1014 W=cm2 conditions for the presence of nonlinear processes are fulfilled and ion acceleration due to ponderomotive force appears, in addition to the thermal and hot electron guided ambipolar acceleration. The existence of two production mechanisms for highly charged ions with charge states above z = 50+ has been demonstrated by changing the minimum focus position with regard to the target surface (by changing the interaction length with pre-formed plasma for relativistic self-focusing). Various potential applications of LIS are mentioned.

1 Introduction

There is no doubt at present that Laser Ion Sources (LIS) are the most efficient sources of highly charged ions. Depending on the type of laser used and its parameters, ions with charge states from 1+ up to more than 50+ can be produced, with ion energies ranging from hundreds of eV up to hundreds of MeV. The higher the laser intensity, the higher the charge states and the energy of the ions generated. The ion current density, j, may attain of mA/cm2 at a distance of 1 m from the target (j > 10 kA/cm2 near the target) [1]. Highly charged heavy ions (Pb25+) required for the preinjector of Large Hadron Collider (LHC) at CERN in Geneva (ions with charge state above 53+, considered for preinjectors of second generation, would save one stripper, where the lost of ions is about 80 %, at present) and Co25+ ions are needed for Terra Watt Accumulator (TWAC) at ITEP in Moscow [2-4]. Low charge state ions with energies of hundreds eV only are considered for the new hybrid ion source ECLISSE (ECR ion source Coupled to LIS for charge State Enhancement [5,6]) that should combine the best properties of LIS and ECRIS. On the contrary, ions with high energy (up to MeV without external acceleration) can be used for ion implantation [7-10] to modify surface properties of solid materials. Interest in Laser Space Propulsion, particularly using laser ablated plasmas, has been revived quite recently [11]. Most applications of LIS are based on production of a large number of ions. Thus, lasers with high repetition rate are preferred for applications, while single shot lasers are used mainly for fundamental studies.

Various lasers have been used for experiments in the authors' laboratories aimed at producing different kinds of ions. Maximum ion charge states z = 55+ have been recorded, as well as the maximum energy of emitted ions Ei = 34 MeV. The most important (typical) results and dependencies (both the older and the new ones) are summarized. All the presented experiments serve as a basis for wide discussions of various alternative, but not yet unambiguously determined, mechanisms of ion production and acceleration.

2 Experimental arrangement and ion diagnostics

To study ion production at low laser power densities, a Nd:YAG laser (LAB-190, Spectra Physics-Quanta Ray) with a nominal energy of 900 mJ in a 9 ns long pulse was used in our experiments at INFN LNS, Catania. The laser beam was focused using lenses of different focal length (mainly 500 mm) onto the target, which was located in an interaction chamber evacuated to about 6 × 10-7 mbar. The minimum focal spot was found to be smaller than 0.5 mm in diameter. Its area varied due to different distances of the lens from the target, different incidence angles of the beam on the target, and the dependence of the laser beam divergence on the laser pumping energy. A schematic view of the experimental arrangement is presented elsewhere [5].

Two high-power photodissociation iodine laser systems PERUN (l = 1.315 mm, EL ~ 50 J, t ~ 350 ps, IL ~ 1.5 ×1015 W/cm2) [12] and PALS (EL ~ 1 kJ, t ~ 400 ps, IL ~ 6 ×1016 W/cm2) [13], located at IP ASCR and at the PALS Research Center in Prague, were used to generate highly charged ions of several medium-Z and high-Z elements. After the frequency conversion in DKDP crystals, the lasers could be operated at the second (l/2 = 0.657 mm) and/or the third (l/3 = 0.438 mm) harmonic frequency with efficiency up to 50 %. Targets were irradiated obliquely (30° with respect to the target normal) or normally with regard to the incident laser beam. The 29-cm diameter beam of laser PALS was focused with an aspherical lens onto the targets with a minimum focal spot diameter of 70 mm. A sketch of the experimental arrangement is shown in Fig. 1.


The principal diagnostic techniques used for analysis of the properties of the laser-produced plasma were based on the time-of-flight method (ion collectors, IC) or on time of-flight combined with a superimposed electric and/or magnetic field (cylindrical electrostatic ion energy analyzer, IEA, and Thomson parabola spectrometer, TPS, [12,14]). Generally, the charge-integrated time-resolved IC signals show distinct, more or less pronounced, maxima, whose position and amplitude reflect not only the mechanisms of ion production and acceleration, but also variations of laser parameters: laser pulse divergence, radial inhomogeneities, spikes, prepulses, etc. From the IC signals, the peak and mean (and/or maximum) ion velocities and energies, as well as ion current densities can be evaluated (estimated).

The IEA makes it possible to identify the ion species produced, i.e. to determine their mass-to-charge ratios, energies and abundance. Charge-energy distribution is obtained by varying the voltage on the electrode plates of the analyzer from shot to shot at fixed experimental conditions. Using the TPS it is possible to distinguish different ions with the same m/z ratio, as well as to record their velocity (energy) distribution in a single laser shot. Although the TPS has a low dynamic range and a low mass-resolution for energetic and highly charged heavy ions, it can provide complete and quick information on the ion species and on the underlying physical processes in the plasma.

Quantitative results can be distorted by the kind of ion detector used (ion collector, windowless electron multiplier, microchannel plate). One of the problems is connected with the electron yield, g, of the electron emission induced by the impact of ions on the detector surface. The value of g depends on the ion charge state z, ion energy Ei, and the detectors surface quality. The g increases with the charge state of the impinging ions, for fixed ion kinetic energy, and, for fixed z, it has a minimum in its variation with Ei. Thus, the value of g/z (needed for evaluation of ion current) ranges from ~ 0.3 to ~ 3.5, depending on the charge state and kinetic energy of the ion; the lower the energy, the larger the spread of g/z [15,16].

3 Results and discussion

The yields and properties of Al, Au, Cu, Nb, Ni, Pb, Sn, Ta and W ions from plasma produced by the 0.9-J/9-ns Nd:YAG laser have been previously reported e.g. in [5,17,18]. By changing either the laser pulse energy or the focal spot size, the laser intensity on the target surface was varied from 1 × 109 to about 1 × 1011 W/cm2, i.e. from the threshold power density for ion generation up to the maximum laser intensities attainable with the setup used. The ion velocities (ion energies) ranged from about 2 × 106 to 2 × 107 cm/s (100 eV-10 keV) depending on the target element used and on the laser intensity. The ion emission was peaked along the normal to the target surface; the angular distribution of ions shows a strong anisotropy and it was not the same for all the elements studied. The relative steepness of the distribution with respect to the target normal is given by [19]

where bz is the charge state distribution, which depends on the plasma ion temperature (which, in turn, depends on the laser intensity), and nz depends strongly on the ion mass A, and less on the charge state z. From all the elements studied the narrowest distribution was recorded for W and the widest for Al and Ni (see Fig. 2). The recorded ion current densities ranged from 4 mA/cm2 (for Au) to 43 mA/cm2 (for Cu) at a distance of 44 cm from the target. Charge spectra of Au, Nb, Ta, Pb and W were measured at EL ~ 40 mJ and EL ~ 300 mJ, respectively, from which the charge-state distributions (CSD) and the charge-energy distributions (CED) were evaluated. The abundance of W ions produced at these two laser energies is compared in Fig. 3, as an example. The majority (about 70%) of emitted particles, at the laser intensities used, consisted of neutrals [17]. The proportion of ions (with respect to neutrals), as well as the presence of the highest charge state, increases with the increasing laser intensity. The maximum recorded charge state was 10+ at our experimental conditions. The charge state was lower than 4+ for more than 70 % of the ions for all elements tested.



Both the PERUN and the PALS iodine laser systems were used to generate highly charged ions of the following medium-Z and high-Z elements (Al, Co, Ni, Cu, Ag, Sn, Ta, W, Pt, Au, Pb, Bi) at their fundamental, as well as their 2nd and 3rd harmonic frequencies [1,12,20-23]. By changing either the laser pulse energy or the focal spot size (minimum focus spot position FP), the laser intensity on the target surface was varied from 1 × 1013 to about 3 × 1016 W/cm2. Ion charge states slightly above z = 50+ were recorded almost for all high-Z elements (Ta55+ was the maximum). The ion velocities (ion energies) ranged from about 2 × 106 up to 6 × 108 cm/s (about 100 eV - 34 MeV) depending on the target element used and the laser intensity. Ion current densities, recalculated to a distance of 1 m from the target, reached up to tens of mA/cm2 (tens of kA/cm2 near the target), depending on the group of ions produced. The characteristics of the ions produced are summarized in Table 1.

Charge spectra of Ta ions for both the 1w and 3w harmonic frequencies at various experimental conditions were measured, from which the charge-state distributions (CSD, Fig. 4) and the charge-energy distributions (CED) were evaluated. The major portion of the ions (50-65 %) is composed of ions with charge states up to 10+; the abundance of individual higher charge states is lower than 3 %. Increasing EL shifts zmax to higher values at the same laser frequency (3w) and also increases the amount of highly charged ions. Higher laser energy EL (laser intensity IL) generally means higher plasma temperature, which implies higher mean charge state zmean, higher zmax and higher Ei. An example of Ta ion charge-energy distributions for EL = 215 J at 1w is shown in Fig. 5.



Generation of ions with charge states above z = 45+ depends on the absorbed laser intensity and on the öptimum" focus setting, which has been proven to be in front of the target surface [23]. It is defined as the position of the minimum laser focal spot (caustic) with regard to the target surface FP, for which the highest charge states, zmax, are generated and consequently the highest amplitudes of the IC and IEA signals for the fastest Ta ion group are attained [12]. The convention used is that FP = 0 when the minimum focal spot is located on the target surface, while FP < 0 means that it is located in front of the target and FP > 0 means that it is inside the target. The variation of zmax with FP, for 1w and laser energy EL = 215 J, has a flat maximum at z ~ 50+ over a broad FP range of about 900 mm, but is not symmetric around FP = 0, where the nominal laser intensity is maximum (Fig. 6). The threshold laser intensity for Ta48+ ion production was IL ~ 5 × 1015 W/cm2 for FP ~ +70 mm, but only IL ~ 3 × 1014 W/cm2 for FP ~ + -850 mm (IL was calculated according the linear approximation of the shape of the laser caustic [23]). The variation of zmax with FP is narrower for 3w. Similar anomalous dependencies were recorded for the peak values of v, E and j of the fast ion group(s) - see Fig. 7, a-c. Surprisingly, similar asymmetrical dependence on the FP was also recorded for the diameter of the craters created on the target surfaces (which are not identical with the diameter of the laser spot at this location). The dependencies on FP for EL = 215 J and for EL = 500 J show both clear minima for FP < 0, as if the laser intensity minima were shifted [23].



This situation, with regard to the generation of highly charged ions, is similar to that where the conditions for the appearance of relativistic self-focusing are significantly improved by a short (ps) laser prepulse preceding the also short (ps) main pulse by about 100 ps [24]. A linear increase of the ion energy with increasing charge states represents, generally, the main ambipolar acceleration mechanism, which acts at different (low or high) plasma temperatures. The existence of an ''optimum focus position" for generation of highly charged ions, which is found to lying in front of the target surface, indicates that the interaction of a long (tL > 100 ps) laser pulse (whose intensity is above a threshold 2 × 1014 W/cm2 with the self-generated plasma creates the conditions for relativistic self-focusing of the high intensity laser radiation and for the ion acceleration by nonlinear (ponderomotive) forces. This seems to be an indirect confirmation of the existence of the mechanism suggested by Hora [2],[24],[25]. The existence of two groups of ions (with two mechanisms of their production) may be deduced from Fig. 5.

4 Conclusion

Highly charged ions of high-Z elements, with charge states above 50+ and with energies in MeV region, can be generated using the fundamental and lower harmonic frequencies of the iodine laser at high intensities above IL ~ 1 ×1016 W/cm2. Generally, the higher the laser energy (laser intensity) the higher the charge states and ion energies produced. Due to the convenient pulse length of the iodine laser (400 ps), a part of it may interact with the self-created expanding plasma. If the conditions for laser beam self-focusing are fulfilled, ions with maximum energies of MeV range and with charge states above 50+ can be generated, starting at laser intensities above only about 2 ×1014 W/cm2.

Acknowledgments

This work was supported by the Grant Agency of the ASCR (Grant A1010105), the European Union (Projects PALS/005 and PALS/006 under Contract HPRI-CT-1999-00053), the Ministry of Education of the Czech Republic (Project LN00A100), and the 5th National Committee of INFN (ECLISSE and PLAIA Projects).

References

[1] L. Láska, J. Badziak, F.P. Boody, S. Gammino, H. Hora, K. Jungwirth, J. Krása , P. Parys, M. Pfeifer, K. Rohlena, L. Torrisi, J. Ullschmied, J. Wolowski, and E. Woryna, Plasma Phys. Contr. Fusion 45, 585 (2003).

[2] H. Haseroth and H. Hora, Laser Part. Beams 14, 393 (1996).

[3] B. Yu. Sharkov, S. Kondrashev, I. Roudskoy, S. Savin, A. Shumshurov, H.Haseroth, H. Kugler, K. Langbein, N. Lisi, H. Magnusson, R. Scrivens, J.C. Schnuriger, J. Tambini, S. Homenko, K. Makarov, V. Roerich, A. Stepanov, and Yu. Satov, Rev. Sci. Instrum. 69, 1035 (1998).

[4] A. Balabaev, S. Kondrashev, K. Konukov, A. Lozhkin, B. Sharkov, A. Shumshurov, A. Charushin, K. Makarov, Yu. Satov, Yu. Smakovskii, O. Camut, J. Chamings, H. Kugler, and R. Scrivens, 10th ICIS 03, 2003, Dubna; Rev. Sci. Instrum. 75, 1572 (2004).

[5] S. Gammino, L. Torrisi, L. Ando L., G. Ciavola, L. Celona, L. Láska, J. Krása, M. Pfeifer, J. Wolowski, E. Woryna, P. Parys, and G.D. Shirkov, Rev. Sci. Instrum. 73, 650 (2002).

[6] S. Gammino, L. Torrisi, G. Ciavola, L. Ando, L. Celona, J. Krása, L. Láska, A.M. Mezzasalma, C. Gentile, A. Pizziotto, J. Wolowski, E. Woryna, D. Hitz, and G.A. Shirkov, J. Appl. Phys..

[7] V. Yu. Fominski, Vacuum 42, 73 (1991).

[8] F.P. Boody, R. Höpfl, H. Hora, and J.C. Kelly, Laser&Part.Beams 14, 443 (1996).

[9] L. Láska, J. Krása, K. Mašek, M. Pfeifer, K. Rohlena, B. Králiková, J. Skála, V. Perina, V. Hnatowitz, E. Woryna, P. Parys, J. Wolowski, F.P. Boody, R. Höpfl, and H, Hora, Czech. J. Phys. 50/S3, 81 (2000).

[10] L.Torrisi, S. Gammino S., A.M. Mezzasalma, J. Badziak, P. Parys, J. Wolowski, E. Woryna, J. Krása, L. Láska, M. Pfeifer, K. Rohlena, and F.P. Boody, Appl. Surface Sci. 217, 319 (2003).

[11] F.P. Boody, in Beamed Energy Propulsion, AIP Conf. Proc. 664, 634 (2003).

[12] L. Láska, J. Krása, K. Mašek, M. Pfeifer, B. Králiková, T. Mocek, J. Skála, P. Straka, P. Trenda, K. Rohlena, E. Woryna, J. Farny, P. Parys, J. Wolowski, W. Mróz, A. Shumshurov, B. Sharkov, J. Collier, K. Langbein, and H. Haseroth, Czech. J. Phys. 46, 1099 (1996).

[13] K. Jungwirth, A. Cejnarová, L. Juha, B. Králiková, J. Krása, E. Krouský, P. Krupicková, L. Láska, K. Mašek, T. Mocek, M. Pfeifer, A. Präg, O. Renner, K. Rohlena, B. Rus, J. Skála, P. Straka, and J. Ullschmied, Physics of Plasmas 8, 2495 (2001).

[14] E. Woryna, P. Parys, J. Wolowski, and W. Mróz, Laser&Part.Beams 14, 293 (1996).

[15] J. Krása, L. Láska, M.P. Stöckli, and D. Fry, Nucl. Instrum. Meth. B 173, 281 (2001).

[16] L. Láska, J. Krása, M.P. Stöckli and C.W. Fehrenbach, Rev. Sci. Instrum. 73, 776 (2002).

[17] L. Torrisi, L. Ando, S. Gammino, J. Krása, and L. Láska, Nucl.Instrum. and Methods B184, 327 (2001).

[18] L. Láska, J. Krása, M. Pfeifer, S. Gammino, L. Torrisi, L. Ando, and G. Ciavola, Rev. Sci. Instrum. 73, 654 (2002).

[19] A. Thum-Jäger and K. Rohr, J. Phys. D: Appl. Phys. 32, 2827 (1999).

[20] J. Krása, L. Láska, K. Mašek, M. Pfeifer, B. Králiková, J. Skála, P Straka, K. Rohlena, W. Mróz, E. Woryna, P. Parys, J. Wolowski, H. Haseroth, A.A. Golubev, and B. Yu. Sharkov, Laser&Part.Beams 16, 5 (1998).

[21] J. Wolowski, J. Badziak, F.P. Boody, H. Hora, V. Hnatowicz, K. Jungwirth, J. Krása, L. Láska, P. Parys, V. Perina, M. Pfeifer, K. Rohlena, L. Ryc, J. Ullschmied, and E. Woryna, Plasma Phys. Contr. Fusion 44, 1277 (2002).

[22] J. Wolowski, J. Badziak, F.P. Boody, S. Gammino, H. Hora, K. Jungwirth, J. Krása, L. Láska, P. Parys, M. Pfeifer, K. Rohlena, A. Szydlowski, L. Torrisi, J. Ullschmied, and E. Woryna, Plasma Phys.Control.Fusion 45, 1087 (2003).

[23] L. Láska, K. Jungwirth, B. Králiková, J. Krása J., M. Pfeifer, K. Rohlena, J. Skála, J. Ullschmied, J. Badziak, P. Parys, J. Wolowski, E. Woryna, L. Torrisi, S. Gammino, and F.P. Boody, 10th ICIS 03, 2003, Dubna; Rev. Sci. Instrum. 75, 1588 (2004).

[24] H. Hora, J. Badziak, F.P. Boody, R. Höpfl, K. Jungwirth, B. Králiková, J. Krása, L. Láska, P. Parys, V. Perina, M. Pfeifer, K. Rohlena, J. Skála, J. Ullschmied, J. Wolowski, and E. Woryna, Optics Communications 207, 333 (2002).

[25] T. Häuser, W. Scheid, and H. Hora., Phys Rev. A 45, 1278 (1991).

Received on 15 January, 2004; revised version received on 3 May, 2004

  • [1] L. Láska, J. Badziak, F.P. Boody, S. Gammino, H. Hora, K. Jungwirth, J. Krása , P. Parys, M. Pfeifer, K. Rohlena, L. Torrisi, J. Ullschmied, J. Wolowski, and E. Woryna, Plasma Phys. Contr. Fusion 45, 585 (2003).
  • [2] H. Haseroth and H. Hora, Laser Part. Beams 14, 393 (1996).
  • [3] B. Yu. Sharkov, S. Kondrashev, I. Roudskoy, S. Savin, A. Shumshurov, H.Haseroth, H. Kugler, K. Langbein, N. Lisi, H. Magnusson, R. Scrivens, J.C. Schnuriger, J. Tambini, S. Homenko, K. Makarov, V. Roerich, A. Stepanov, and Yu. Satov, Rev. Sci. Instrum. 69, 1035 (1998).
  • [4] A. Balabaev, S. Kondrashev, K. Konukov, A. Lozhkin, B. Sharkov, A. Shumshurov, A. Charushin, K. Makarov, Yu. Satov, Yu. Smakovskii, O. Camut, J. Chamings, H. Kugler, and R. Scrivens, 10th ICIS 03, 2003, Dubna; Rev. Sci. Instrum. 75, 1572 (2004).
  • [5] S. Gammino, L. Torrisi, L. Ando L., G. Ciavola, L. Celona, L. Láska, J. Krása, M. Pfeifer, J. Wolowski, E. Woryna, P. Parys, and G.D. Shirkov, Rev. Sci. Instrum. 73, 650 (2002).
  • [6] S. Gammino, L. Torrisi, G. Ciavola, L. Ando, L. Celona, J. Krása, L. Láska, A.M. Mezzasalma, C. Gentile, A. Pizziotto, J. Wolowski, E. Woryna, D. Hitz, and G.A. Shirkov, J. Appl. Phys..
  • [7] V. Yu. Fominski, Vacuum 42, 73 (1991).
  • [9] L. Láska, J. Krása, K. Maek, M. Pfeifer, K. Rohlena, B. Králiková, J. Skála, V. Perina, V. Hnatowitz, E. Woryna, P. Parys, J. Wolowski, F.P. Boody, R. Höpfl, and H, Hora, Czech. J. Phys. 50/S3, 81 (2000).
  • [10] L.Torrisi, S. Gammino S., A.M. Mezzasalma, J. Badziak, P. Parys, J. Wolowski, E. Woryna, J. Krása, L. Láska, M. Pfeifer, K. Rohlena, and F.P. Boody, Appl. Surface Sci. 217, 319 (2003).
  • [11] F.P. Boody, in Beamed Energy Propulsion, AIP Conf. Proc. 664, 634 (2003).
  • [12] L. Láska, J. Krása, K. Maek, M. Pfeifer, B. Králiková, T. Mocek, J. Skála, P. Straka, P. Trenda, K. Rohlena, E. Woryna, J. Farny, P. Parys, J. Wolowski, W. Mróz, A. Shumshurov, B. Sharkov, J. Collier, K. Langbein, and H. Haseroth, Czech. J. Phys. 46, 1099 (1996).
  • [13] K. Jungwirth, A. Cejnarová, L. Juha, B. Králiková, J. Krása, E. Krouský, P. Krupicková, L. Láska, K. Maek, T. Mocek, M. Pfeifer, A. Präg, O. Renner, K. Rohlena, B. Rus, J. Skála, P. Straka, and J. Ullschmied, Physics of Plasmas 8, 2495 (2001).
  • [15] J. Krása, L. Láska, M.P. Stöckli, and D. Fry, Nucl. Instrum. Meth. B 173, 281 (2001).
  • [16] L. Láska, J. Krása, M.P. Stöckli and C.W. Fehrenbach, Rev. Sci. Instrum. 73, 776 (2002).
  • [17] L. Torrisi, L. Ando, S. Gammino, J. Krása, and L. Láska, Nucl.Instrum. and Methods B184, 327 (2001).
  • [18] L. Láska, J. Krása, M. Pfeifer, S. Gammino, L. Torrisi, L. Ando, and G. Ciavola, Rev. Sci. Instrum. 73, 654 (2002).
  • [19] A. Thum-Jäger and K. Rohr, J. Phys. D: Appl. Phys. 32, 2827 (1999).
  • [21] J. Wolowski, J. Badziak, F.P. Boody, H. Hora, V. Hnatowicz, K. Jungwirth, J. Krása, L. Láska, P. Parys, V. Perina, M. Pfeifer, K. Rohlena, L. Ryc, J. Ullschmied, and E. Woryna, Plasma Phys. Contr. Fusion 44, 1277 (2002).
  • [22] J. Wolowski, J. Badziak, F.P. Boody, S. Gammino, H. Hora, K. Jungwirth, J. Krása, L. Láska, P. Parys, M. Pfeifer, K. Rohlena, A. Szydlowski, L. Torrisi, J. Ullschmied, and E. Woryna, Plasma Phys.Control.Fusion 45, 1087 (2003).
  • [23] L. Láska, K. Jungwirth, B. Králiková, J. Krása J., M. Pfeifer, K. Rohlena, J. Skála, J. Ullschmied, J. Badziak, P. Parys, J. Wolowski, E. Woryna, L. Torrisi, S. Gammino, and F.P. Boody, 10th ICIS 03, 2003, Dubna; Rev. Sci. Instrum. 75, 1588 (2004).
  • [24] H. Hora, J. Badziak, F.P. Boody, R. Höpfl, K. Jungwirth, B. Králiková, J. Krása, L. Láska, P. Parys, V. Perina, M. Pfeifer, K. Rohlena, J. Skála, J. Ullschmied, J. Wolowski, and E. Woryna, Optics Communications 207, 333 (2002).
  • [25] T. Häuser, W. Scheid, and H. Hora., Phys Rev. A 45, 1278 (1991).

Publication Dates

  • Publication in this collection
    26 Apr 2005
  • Date of issue
    Dec 2004

History

  • Accepted
    03 May 2004
  • Received
    15 Jan 2004
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