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  • 1
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 4 (1992), S. 1372-1372 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 1 (1989), S. 2340-2344 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A general form of the derivative nonlinear Schrödinger (DNLS) equation, describing the nonlinear evolution of Alfvén waves propagating parallel to the magnetic field, is derived by using two-fluid equations with electron and ion pressure tensors obtained from Braginskii [in Reviews of Plasma Physics (Consultants Bureau, New York, 1965), Vol. 1, p. 218]. This equation is a mixed version of the nonlinear Schrödinger (NLS) equation and the DNLS, as it contains an additional cubic nonlinear term that is of the same order as the derivative of the nonlinear terms, a term containing the product of a quadratic term, and a first-order derivative. It incorporates the effects of finite beta, which is an important characteristic of space and laboratory plasmas.
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  • 3
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 28 (1985), S. 763-766 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A gyrating electron beam supports negative energy modes near the harmonics of electron-cyclotron frequency. An electromagnetic wave passing through such a beam parametrically up-converts into high-frequency electromagnetic modes separated from the pump frequency by the electron-cyclotron harmonics. The growth rate for this process varies directly as the oscillatory velocity of beam electrons caused by the pump and as square root of the beam density. It has a maximum at values of scattering angle close to 180° and is also implicitly dependent on the beam velocity and the cyclotron frequency of electrons. The effect of a cold electron component is to reduce the growth rate.
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  • 4
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 28 (1985), S. 3292-3301 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A study is made of the linear stability of finite-thickness, anisotropic compressible shear layers v=zˆvz(x), with a parallel uniform magnetic field, B=zˆB0. The stability of such sheared flows, described by the double adiabatic equations of Chew, Goldberger, and Low [Proc. R. Soc. London Ser. A 236, 112 (1956)], and involving the nonlocal coupling of the firehose and mirror modes caused by the velocity shear, is relevant in a number of astrophysical, geophysical, and space plasma configurations. The scalar perturbation quantities have the form f (x) exp[i(kzz −ωt)]. The dimensionless variables characterizing a shear layer with a given velocity profile, assumed to be a linear profile in the present work, are the sonic Mach number, M ≡ (2vzm/S⊥), the ratio of the magnetic field energy density to the perpendicular thermal energy density, q2 ≡ (vA/S⊥)2, and the anisotropy parameter, r2 ≡ (S(parallel)/S⊥)2. Here, vz(x=±∞)=±vzm, S(parallel), and S⊥ are the sound speeds parallel and perpendicular to the magnetic field, and vA is the Alfvén speed. The dimensionless variable characterizing the perturbation is the wavenumber B ≡ kzL, where L is the shear layer thickness. It is shown that the resonance of the sound and firehose modes drives unstable standing and traveling waves for a shear layer having a vortex sheet profile [where vz(x) is a step function]. For the vortex sheet, the unstable standing wave modes first appear at M=2(3)1/2r for r〉(1+q2)1/2/2, and the unstable traveling wave modes first appear at M=0 for r〈((1+q2)1/2/2). Numerical methods are used to generate values of ωr and ωi〉0 (corresponding to unstable wave motion) for the "linear'' shear layer in the (B, M) plane for various values of q and r.The coverage of the (B, M) plane is for B≤5, M≤10, and for discrete values of q≤0.5 and r≤2. Two regimes of instability are found to occur in the (B, M) plane with the structure of the unstable modes of the "linear'' layer being very different from that for the anisotropic vortex sheet. The unstable modes are standing waves with ωr=0, and traveling waves with ωr≠0.
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  • 5
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 29 (1986), S. 3486-3488 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A high amplitude whistler wave propagating along the magnetic field lines (k0(parallel)Bs) in a plasma is unstable to a transverse electromagnetic perturbation (k⊥k0), having a perturbed magnetic field B(parallel)Bs(parallel)zˆ, where Bs is the static magnetic field. The instability grows on an Alfvén time scale and is relevant when vo/vA(approximately-greater-than)ω0/ωc, where vo is the oscillatory velocity of electrons caused by the pump and vA is the Alfvén speed, ω0 is the frequency of the whistler pump, and ωc is the electron cyclotron frequency.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 28 (1985), S. 3328-3332 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A gyrating ion beam, with ring shape distribution in velocity space, supports negative energy modes near the harmonics of beam gyrofrequency. An investigation of the nonlinear interaction of high-frequency lower-hybrid waves with the negative energy beam cyclotron mode is made. A nonlinear dispersion relation is derived for the coupled modes. It is shown that a gyrating ion beam frequency upconverts the lower-hybrid waves separated by harmonics of the beam gyrofrequency. This process of upconversion may thus provide a tool for the diagnostics of the gyrating ion beams. The process may also be important in the saturation of lower-hybrid waves observed in the auroral zone S3-3 satellite data.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 29 (1986), S. 1339-1339 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 313 (1985), S. 559-560 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The Jicamarca Radar Observatory near the geomagnetic equator (magnetic dip 2) at 75 W longitude provides observations of ionospheric electron drift velocities through the incoherent scatter technique5. The electric field is determined from the electron drift velocity, Vc = ExB/B2 (where E and B are ...
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  • 9
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 218 (1968), S. 857-858 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Micropulsations with periods longer than 30 min have been found in the geomagnetic field6'7, however. I suggest that their origin can also be explained by certain models of the tail. Ness et al.8 have observed that, even though the tail field appears steady for several hours, occasional ...
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  • 10
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 20 (1973), S. 431-437 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The interplanetary magnetic field has been shown to influence the ring current field represented by Dst. Explorer 28 hourly magnetic field observations have been used with the hourly Dst values. The moderate geomagnetic storms of 60 γ and quiet-time fluctuations of 10–30 γ are correlated with the North to South change of the interplanetary field component perpendicular to the ecliptic. This change in the interplanetary field occurs one to three hours earlier than the corresponding change in the Dst field.
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