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  • 1
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    Magnetic storms (1997)
    Washington : American Geophysical Union
    Associated volumes
    Details Availability
    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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  • 2
    Monograph available for loan
    Monograph available for loan
    Magnetic storms (1997)
    Washington : American Geophysical Union
    Associated volumes
    Details Availability
    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
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  • 3
    Monograph available for loan
    Monograph available for loan
    Collisionless shocks in the heliosphere : reviews of current research (1985)
    Washington, DC : American Geophysical Union
    Associated volumes
    Details Availability
    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
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  • 4
    Electronic Resource
    Electronic Resource
    On the solar and interplanetary causes of geomagnetic stormsf| (1993)
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 5 (1993), S. 2623-2630 
    Details
    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
    URL: http://dx.doi.org/10.1063/1.860700
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  • 5
    Electronic Resource
    Electronic Resource
    Electromagnetic ion beam instabilities: II (1985)
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 28 (1985), S. 3691-3695 
    Details
    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
    URL: http://dx.doi.org/10.1063/1.865101
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  • 6
    Electronic Resource
    Electronic Resource
    Discovery of cometary kilometric radiations and plasma waves at comet Halley (1986)
    [s.l.] : Nature Publishing Group
    Nature 321 (1986), S. 307-310 
    Details
    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
    URL: http://dx.doi.org/10.1038/321307a0
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  • 7
    Electronic Resource
    Electronic Resource
    Tweaking the magnetosphere (1992)
    [s.l.] : Nature Publishing Group
    Nature 358 (1992), S. 26-26 
    Details
    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
    URL: http://dx.doi.org/10.1038/358026a0
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  • 8
    Electronic Resource
    Electronic Resource
    Nonlinear stability of Halley cometosheath with transverse plasma motion (1994)
    Springer
    Astrophysics and space science 222 (1994), S. 113-125 
    Details
    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
    URL: http://dx.doi.org/10.1007/BF00627087
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  • 9
    Electronic Resource
    Electronic Resource
    Interplanetary discontinuities and Alfvén waves (1995)
    Springer
    Space science reviews 72 (1995), S. 205-210 
    Details
    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
    URL: http://dx.doi.org/10.1007/BF00768781
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  • 10
    Electronic Resource
    Electronic Resource
    Magnetic storms (1997)
    Springer
    Surveys in geophysics 18 (1997), S. 363-383 
    Details
    ISSN: 1573-0956
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract This talk provides a brief summary of the first conference devoted entirely to magnetic storms. The conference was held in Pasadena, California, at the Jet Propulsion Laboratory, 12-16 February 1996. Topics covered the relevant time-varying phenomena at the sun/corona, propagation of these structures through interplanetary space, the response of the magnetosphere from its interaction with these interplanetary structures, the formation of the storm- time ring-current (in particular the oxygen content of the ring-current), and storm ionospheric effects and ground based effects. A complementary summary is provided by Gonzalez et al. in EOS, 1996. The full set of review articles will be published in an AGU monograph and many of the contributed articles will appear in a special section of the Journal of Geophysical Research, Space Physics.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1023/A:1006555215463
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