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  • 1
    Monograph available for loan
    Monograph available for loan
    Washington : American Geophysical Union
    Associated volumes
    Call number: 5/M 97.0367
    In: Geophysical monograph
    Type of Medium: Monograph available for loan
    Pages: x, 266 S.
    ISBN: 0875900801
    Series Statement: Geophysical monograph 98
    Classification:
    Geomagnetism, Geoelectromagnetism
    Language: English
    Location: Reading room
    Branch Library: GFZ Library
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  • 2
    Unknown
    Washington : American Geophysical Union
    Associated volumes
    Call number: 98.0136
    In: Geophysical monograph
    Pages: x, 266 S.
    ISBN: 0875900801
    Series Statement: Geophysical monograph 98
    Classification:
    Geomagnetism, Geoelectromagnetism
    Language: English
    Branch Library: GFZ Library
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  • 3
    Monograph available for loan
    Monograph available for loan
    Washington, DC : American Geophysical Union
    Associated volumes
    Call number: 5/M 92.1329(35)
    In: Geophysical monograph
    Type of Medium: Monograph available for loan
    Pages: viii, 303 S.
    ISBN: 0875900615
    Series Statement: Geophysical monograph 35
    Classification:
    Astronomy and Astrophysics
    Language: English
    Location: Reading room
    Branch Library: GFZ Library
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  • 4
    Publication Date: 2023-09-06
    Description: Learning from successful applications of methods originating in statistical mechanics, com- plex systems science, or information theory in one scientific field (e.g., atmospheric physics or climatology) can provide important insights or conceptual ideas for other areas (e.g., space sciences) or even stimulate new research questions and approaches. For instance, quantification and attribution of dynamical complexity in output time series of nonlinear dynamical systems is a key challenge across scientific disciplines. Especially in the field of space physics, an early and accurate detection of characteristic dissimilarity between nor- mal and abnormal states (e.g., pre-storm activity vs. magnetic storms) has the potential to vastly improve space weather diagnosis and, consequently, the mitigation of space weather hazards. This review provides a systematic overview on existing nonlinear dynamical systems- based methodologies along with key results of their previous applications in a space physics context, which particularly illustrates how complementary modern complex systems ap- proaches have recently shaped our understanding of nonlinear magnetospheric variability. The rising number of corresponding studies demonstrates that the multiplicity of nonlin- ear time series analysis methods developed during the last decades offers great potentials for uncovering relevant yet complex processes interlinking different geospace subsystems, variables and spatiotemporal scales.
    Description: Published
    Description: 38
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 5
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 5 (1993), S. 2623-2630 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: This article reviews some of the physical properties of geomagnetic storms and the solar and interplanetary causes of these sporadic events. To give the reader an overview of the whole system, the focus will be on the primary plasma processes. References will be provided for those who wish to obtain further information.
    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. 3691-3695 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: This paper extends the results of Gary et al. [Phys. Fluids 27, 1852 (1984)]. That paper examined the linear theory of electromagnetic instabilities driven by an ion beam streaming along a magnetic field in a homogeneous Vlasov plasma, emphasizing the parametric dependence of the instability growth rates. This paper considers the parametric dependence of the real frequency at maximum growth of two such instabilities with right-hand polarization. It is shown that the right-hand resonant ion beam instability can have maximum growth at frequencies near the ion-cyclotron frequency if the beam–main component relative drift speed is about twice the Alfvén speed and at least one of the following conditions holds: the ion beta or the beam–main component relative temperature are sufficiently small, or the perpendicular-to-parallel beam temperature ratio is sufficiently large. These results support the identification of the right-hand resonant instability as the source of the large amplitude magnetic fluctuations observed upstream of slow shocks in the Earth's magnetotail.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 321 (1986), S. 307-310 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The plasma-wave probe (PWP) system carried by the Sakigake spacecraft used two detectors: a 10-m tip-to-tip dipole antenna and a search coil-type magnetic field detector. The receivers of the PWP system comprised a swept frequency receiver and a 16-channel frequency analyser, referred to as the ...
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 358 (1992), S. 26-26 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] SIR - Kurth's News and Views article1 captures much of the excitement of the phenomenon of solar coronal mass ejec-tions (CMEs) and their role in triggering terrestrial magnetic storms. But we wish to correct the impression that we do not yet know why some CMEs cause storms and others do not. The ...
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 222 (1994), S. 113-125 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Weakly nonlinear MHD stability of the Halley cometosheath determined by the balance between the outward ion-neutral drag force and the inward Lorentz force is investigated including the transverse plasma motion as observed in the flanks with the help of the method of multiple scales. The eigenvalues and the eigenfunctions are obtained for the linear problem and the time evolution of the amplitude is obtained using the solvability condition for the solution of the second order problem. The diamagnetic cavity boundary and the adjacent layer of about 100 km thickness is found unstable for the travelling waves of certain wave numbers. Halley ionopause has been observed to have strong ripples with a wavelength of several hundred kilometers. It is found that nonlinear effects have stabilizing effect.
    Type of Medium: Electronic Resource
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  • 10
    ISSN: 1572-9672
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The rate of occurrence of interplanetary discontinuities (ROID) is examined using Ulysses magnetic field and plasma data from 1 to 5 AU radial distance from the Sun and at high heliospheric latitudes. It is found that there are two regions in interplanetary space where the ROID is high: in stream-stream interaction regions and in Alfvén wave trains. This latter feature is particularly obvious at high heliographic latitudes when Ulysses enters a high speed stream associated with a polar coronal hole. These streams are characterized by the presence of continuous, large-amplitude ( $$\Delta \bar B/l BI - 1 - 2$$ ,) Alfvén waves and an extraordinarily high ROID value (∼150 discontinuities/day). In a number of intervals examined, it is found that (rotational) discontinuities are an integral part of the Alfvén wave: they represent ∼ 90° phase rotation of the wave out of the full 360° rotation of the wave. These large amplitude nonlinear Alfvén waves thus appear to be phase steepened. The nonlinear Alfvén waves are spherically polarized, i.e., the tip of the perturbation vector resides on the surface of a sphere (a consequence of constant |B|). The best description of this wave plus discontinuity is a “spherical arc polarization”.
    Type of Medium: Electronic Resource
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