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1.
Phys Rev E ; 94(3-1): 033206, 2016 Sep.
Article in English | MEDLINE | ID: mdl-27739720

ABSTRACT

Radially polarized intense terahertz (THz) radiation behind a thin foil irradiated by ultrahigh-contrast ultrashort relativistic laser pulse is recorded by a single-shot THz time-domain spectroscopy system. As the thickness of the target is reduced from 30 to 2 µm, the duration of the THz emission increases from 5 to over 20 ps and the radiation energy increases dramatically, reaching ∼10.5mJ per pulse, corresponding to a laser-to-THz radiation energy conversion efficiency of 1.7%. The efficient THz emission can be attributed to reflection (deceleration and acceleration) of the laser-driven hot electrons by the target-rear sheath electric field. The experimental results are consistent with that of a simple model as well as particle-in-cell simulation.

2.
Rev Sci Instrum ; 87(6): 066101, 2016 Jun.
Article in English | MEDLINE | ID: mdl-27370502

ABSTRACT

Single-shot terahertz time-domain spectroscopy is presented with directly encoded spatial resolution. A single reflective echelon and multiple semi-cylindrical lenses are used to obtain both the temporal waveform and the spatial distribution of the terahertz field. This system can be used to rapidly characterize terahertz pulses generated by high power pulsed laser systems, which themselves suffer from large pulse energy and spectrum fluctuations.

3.
Rev Sci Instrum ; 83(4): 045104, 2012 Apr.
Article in English | MEDLINE | ID: mdl-22559573

ABSTRACT

A tapered parallel plate waveguide was developed for frequency up-conversion experiments in the terahertz (THz) region by flash ionization. The element at the plasma-source-wave interaction area determines the conversion efficiency. It causes THz pulses to converge to a narrow plate separation, which is smaller than the wavelength. The waveguide exhibited good performance for transmitting p-polarized THz pulses in a 50 µm separation, making it suitable for flash ionization experiments.


Subject(s)
Radiation Equipment and Supplies , Lasers , Models, Theoretical , Plasma Gases
4.
Phys Rev E Stat Nonlin Soft Matter Phys ; 69(6 Pt 2): 066406, 2004 Jun.
Article in English | MEDLINE | ID: mdl-15244744

ABSTRACT

The propagation characteristics of a high-power microwave [electromagnetic (em) wave] in a plasma waveguide are reported. The plasma waveguide is formed by expanding plasmas via the ponderomotive force of the high-power microwave and the microwave pulse remains trapped within the plasma waveguide and is guided in it. With the increase of the incident microwave power, the width of the plasma waveguide increases and the half width of the radial electric field distribution decreases. This shows that the em wave modifies the refractive index of the plasma waveguide area. For a plasma waveguide with narrower width, the microwave propagates along the plasma waveguide at the fundamental TE mode, while as the waveguide width increases the higher mode component starts appearing. Analytical treatment to the propagation of the electromagnetic wave in a dielectric waveguide having a step-index profile and the numerical calculations for the radial distribution of the electric field show fairly good agreement with the results observed in the present experiments.

5.
Phys Rev E Stat Nonlin Soft Matter Phys ; 66(2 Pt 2): 026404, 2002 Aug.
Article in English | MEDLINE | ID: mdl-12241294

ABSTRACT

The theory of the interaction of an electromagnetic wave with a uniformly moving ionization front in a gas is extended to include the case when the front suddenly stops. This nonstationary character of the wave/front interaction, which is typical for experiments carried out in a finite-size gas tube, gives rise to fresh physical effects. First, currents induced near the plasma boundary after the front stops produce a static magnetic field not only in the plasma behind the front but also in the vacuum ahead of the front. Second, in the regime where the transmitted wave falls off behind the front, the skinning field leaks through the stopped front and produces a burst of highly frequency up-shifted radiation.

6.
Phys Rev Lett ; 89(6): 065003, 2002 Aug 05.
Article in English | MEDLINE | ID: mdl-12190591

ABSTRACT

A proof-of-principle experiment demonstrates the generation of radiation from the Cherenkov wake excited by an ultrashort- and ultrahigh-power pulse laser in a perpendicularly magnetized plasma. The frequency of the radiation is in the millimeter range (up to 200 GHz). The intensity of the radiation is proportional to the magnetic field intensity as expected by theory. Polarization of the emitted radiation is also detected. The difference in the frequency of the emitted radiation between these experiments and previous theory can be explained by the electrons' oscillation in the electric field of a narrow column of ions in the focal region.

7.
Phys Rev E Stat Nonlin Soft Matter Phys ; 65(5 Pt 2): 056407, 2002 May.
Article in English | MEDLINE | ID: mdl-12059715

ABSTRACT

The guided laser pulse propagation and wake-field generation are studied in a wide (in comparison with the laser spot size) gas-filled capillary with an on-axis gas density depletion, which can be produced by a rapid spin of the capillary around its axis or by radially propagating shock waves generated in a piezoceramic tube. A single equation for the wake-field potential, which describes the fully relativistic plasma response in the presence of optical field ionization (OFI) of a gas, is derived and used to demonstrate a guided propagation of a short intense laser pulse over many Rayleigh lengths in a leaky plasma channel produced by the pulse due to OFI in the capillary filled with a radially inhomogeneous gas. The efficient generation of a regular wake field over long distances suitable for the laser wake-field accelerators is shown.

8.
Phys Rev E Stat Nonlin Soft Matter Phys ; 64(1 Pt 2): 016403, 2001 Jul.
Article in English | MEDLINE | ID: mdl-11461406

ABSTRACT

The interaction of high power microwave with collisionless unmagnetized plasma is studied. Investigation on the generation of superthermal electrons near the critical layer, by the resonance absorption phenomenon, is extended to very high microwave power levels (eta=E(2)(0)/4 pi n(e)kT(e) approximately 0.3). Here E0, n(e), and T(e) are the vacuum electric field, electron density, and electron temperature, respectively. Successive generation of electron bunches having maximum energy of about 2 keV, due to nonlinear wave breaking, is observed. The electron energy epsilon scales as a function of the incident microwave power P, according to epsilon proportional to P0.5 up to 250 kW. The two-dimensional spatial distribution of high energy electrons reveals that they are generated near the critical layer. However, the lower energy component is again produced in the subcritical density region indicating the possibility of other electron heating mechanisms.

9.
Article in English | MEDLINE | ID: mdl-11102082

ABSTRACT

The asymmetric spatial distribution of electron density perturbation is observed by using a frequency-domain interferometry technique. The wake amplitude of the outside bump is enhanced by the elliptical distribution of the pump laser pulse. This asymmetry can be explained with a two-dimensional analytical model expanded from cylindrically symmetric linear theory.

10.
Phys Rev Lett ; 85(21): 4542-5, 2000 Nov 20.
Article in English | MEDLINE | ID: mdl-11082591

ABSTRACT

A frequency upshift of a short microwave pulse is generated by the interaction between a relativistic underdense ionization front and a periodic electrostatic field with a perpendicular dc magnetic field. When the dc magnetic field is applied, further frequency upshift of 3 GHz is observed with respect to an unmagnetized case which has typically a GHz range. The radiation frequency depends on both the plasma density and the strength of the dc magnetic field, i.e., the plasma frequency and the cyclotron frequency. The frequency of the emitted radiation is in reasonable agreement with the theoretical values.

11.
Phys Rev Lett ; 76(24): 4540-4543, 1996 Jun 10.
Article in English | MEDLINE | ID: mdl-10061317
12.
Phys Rev Lett ; 76(22): 4171-4174, 1996 May 27.
Article in English | MEDLINE | ID: mdl-10061219
16.
Phys Rev Lett ; 66(18): 2328-2331, 1991 May 06.
Article in English | MEDLINE | ID: mdl-10043457
17.
Phys Rev Lett ; 66(14): 1854-1857, 1991 Apr 08.
Article in English | MEDLINE | ID: mdl-10043327
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