The Experts below are selected from a list of 246 Experts worldwide ranked by ideXlab platform

M S Shur - One of the best experts on this subject based on the ideXlab platform.

F Skiff - One of the best experts on this subject based on the ideXlab platform.

R Koch - One of the best experts on this subject based on the ideXlab platform.

  • radio frequency surface Plasma Oscillations electrical excitation and detection by ar ag 111
    Scientific Reports, 2017
    Co-Authors: Giulia Serrano, Stefano Tebi, Stefan Wiespointnerbaumgarthuber, Stefan Mullegger, R Koch
    Abstract:

    We electrically excite surface Plasma Oscillations on a Ag(111) single crystal by alternating electric charging at radio frequency. The radio frequency signal energy of 2.2 μeV, used to induce surface Plasma Oscillations, is about 5 to 6 orders of magnitude lower than the plasmon energies reachable by optical excitation or electron impact. The detection of the surface Plasma Oscillations is achieved by nano-fabricated 2D single-crystal sensor-islands of Ar atoms, which are shown by imaging with a scanning tunneling microscope to restructure in response to the radio frequency surface Plasma Oscillations, providing nanometer spatial resolution and a characteristic decay time of ≈150 ns.

  • Radio frequency surface Plasma Oscillations: electrical excitation and detection by Ar/Ag(111)
    Scientific Reports, 2017
    Co-Authors: Giulia Serrano, Stefano Tebi, Stefan Mullegger, Stefan Wiespointner-baumgarthuber, R Koch
    Abstract:

    We electrically excite surface Plasma Oscillations on a Ag(111) single crystal by alternating electric charging at radio frequency. The radio frequency signal energy of 2.2 μ eV, used to induce surface Plasma Oscillations, is about 5 to 6 orders of magnitude lower than the plasmon energies reachable by optical excitation or electron impact. The detection of the surface Plasma Oscillations is achieved by nano-fabricated 2D single-crystal sensor-islands of Ar atoms, which are shown by imaging with a scanning tunneling microscope to restructure in response to the radio frequency surface Plasma Oscillations, providing nanometer spatial resolution and a characteristic decay time of ≈150 ns.

William S. Kurth - One of the best experts on this subject based on the ideXlab platform.

  • Electron Plasma Oscillations Upstream of the Solar Wind Termination Shock
    2016
    Co-Authors: Donald A. Gurnett, William S. Kurth, Hz Where
    Abstract:

    Electron Plasma Oscillations have been detected upstream of the solar wind ter-mination shock by the Plasma wave instrument on the Voyager 1 spacecraft. These waves were first observed on 11 February 2004, at a heliocentric radial distance of 91.0 astronomical units, and continued sporadically with a gradually increasing occurrence rate for nearly a year. The last event occurred on 15 December 2004, at 94.1 astronomical units, just before the spacecraft crossed the termination shock. Since then, no further electron Plasma Oscillations have been observed, consistent with the spacecraft having crossed the termination shock into the heliosheath. Electron Plasma Oscillations, also known as Langmuir waves, are one of the oldest known and most widely studied of all Plasma wave phenomena (1). For many years it has been known that electron Plasma Oscillations are generated ahead of planetary bow shocks by energetic electrons escaping into the solar wind upstream of the shock (2–7). This close relationship led Kurth and Gurnett (8) to pre-dict that electron Plasma Oscillations would be present upstream of the solar wind termination shock. Here, we report the initial observations of these waves. Electron Plasma Oscillations are electro-static Oscillations that occur at a characteristic frequency of the Plasma known as the electron Plasma frequency. The electron Plasma fre-quency is given by fp 0 8980 ffiffiffiffi n

  • Evidence for a Shock in Interstellar Plasma: Voyager 1
    The Astrophysical Journal, 2013
    Co-Authors: Leonard F. Burlaga, Donald A. Gurnett, N. F. Ness, William S. Kurth
    Abstract:

    Voyager 1 (V1) observed electron Plasma Oscillations preceding a jump by a factor of 1.4 in the magnetic field intensity B near the end of 2012. The frequency of the electron Plasma Oscillations gives an electron density ne  = 0.05 cm–3, which implies that V1 was immersed in Plasma from the interstellar medium. The last day on which Plasma Oscillations were observed is day 332, 2012, and the jump in the B was centered on day 335, 2012 after a data gap in the wave data. The close association between the electron Plasma Oscillations and the jump in B suggests a causal connection, such as that frequently observed between electron Plasma Oscillations and interplanetary shocks at 1 AU. Based on the observed parameters and the smooth profile of B(t), the jump in B appears to be associated with a weak, subcritical, laminar, low beta, quasi-perpendicular, resistive, collisionless shock. However, the width of the jump is of the order of 104 times that expected for such a stationary shock at 1 AU. The large width of the jump in B might be the result of differences between the structure of shocks in the interstellar medium and the Plasma near 1 AU. Alternatively, the subcritical resistive shock might have decayed during a few days after producing the Plasma waves, leaving a broad profile in B(t) without significantly changing ambient parameters. Another possibility is that the jump in B is a pressure wave.

  • Electron Plasma Oscillations upstream of the solar wind termination shock.
    Science, 2005
    Co-Authors: Donald A. Gurnett, William S. Kurth
    Abstract:

    Electron Plasma Oscillations have been detected upstream of the solar wind termination shock by the Plasma wave instrument on the Voyager 1 spacecraft. These waves were first observed on 11 February 2004, at a heliocentric radial distance of 91.0 astronomical units, and continued sporadically with a gradually increasing occurrence rate for nearly a year. The last event occurred on 15 December 2004, at 94.1 astronomical units, just before the spacecraft crossed the termination shock. Since then, no further electron Plasma Oscillations have been observed, consistent with the spacecraft having crossed the termination shock into the heliosheath.

T E Cowan - One of the best experts on this subject based on the ideXlab platform.

  • two surface plasmon decay of Plasma Oscillations
    Physics of Plasmas, 2015
    Co-Authors: T Kluge, J Metzkes, K Zeil, M Bussmann, U Schramm, T E Cowan
    Abstract:

    The interaction of ultra-intense lasers with solid foils can be used to accelerate ions to high energies well exceeding 60 MeV [Gaillard et al., Phys. Plasmas 18, 056710 (2011)]. The non-linear relativistic motion of electrons in the intense laser radiation leads to their acceleration and later to the acceleration of ions. Ions can be accelerated from the front surface, the foil interior region, and the foil rear surface (target normal sheath acceleration (TNSA), most widely used), or the foil may be accelerated as a whole if sufficiently thin (radiation pressure acceleration). Here, we focus on the most widely used mechanism for laser ion-acceleration of TNSA. Starting from perfectly flat foils, we show by simulations how electron filamentation at or inside the solid leads to spatial modulations in the ions. The exact dynamics depend very sensitively on the chosen initial parameters which has a tremendous effect on electron dynamics. In the case of step-like density gradients, we find evidence that suggests a two-surface-plasmon decay of Plasma Oscillations triggering a Raileigh-Taylor-like instability.

  • two surface plasmon decay of Plasma Oscillations
    arXiv: Plasma Physics, 2015
    Co-Authors: T Kluge, J Metzkes, K Zeil, M Bussmann, U Schramm, T E Cowan
    Abstract:

    The interaction of ultra-intense lasers with solid foils can be used to accelerate ions to high energies well exceeding 60 MeV. The non-linear relativistic motion of electrons in the intense laser radiation leads to their acceleration and later to the acceleration of ions. Ions can be accelerated from the front surface, the foil interior region, and the foil rear surface (TNSA, most widely used), or the foil may be accelerated as a whole if sufficiently thin (RPA). Here, we focus on the most widely used mechanism for laser ion-acceleration of TNSA. Starting from perfectly flat foils we show by simulations how electron filamentation at or inside the solid leads to a spatial modulations in the ions. The exact dynamics depend very sensitively on the chosen initial parameters which has a tremendous effect on electron dynamics. In the case of step-like density gradients we find evidence that suggests a two-surface-plasmon decay of Plasma Oscillations triggering a Raileigh-Taylor-like instability.