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  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1987
    In:  Journal of Geophysical Research: Space Physics Vol. 92, No. A11 ( 1987-11), p. 12352-12364
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 92, No. A11 ( 1987-11), p. 12352-12364
    Abstract: We present here a statistical study of signatures of the high‐latitude ionospheric convection pattern and the simultaneously observed energetic electron precipitation. We most often find convection cells in which the sunward flowing region contains auroral particle precipitation but the antisunward flowing region does not. However, our observations also show the frequent occurrence of convection cells in which neither the antisunward nor the sunward flowing plasma region contains auroral particle precipitation. These findings may appear within the dawnside or duskside convection pattern and strongly suggest that such convection cells may be associated with open magnetic field lines that thread the magnetotail lobes. Examination of the interplanetary magnetic field (IMF) data shows that this “lobe cell” convection signature is most likely to be accompanied by the signature of dayside merging when the IMF has a significant y component but is directed southward. A lobe convection cell has a location and sense of circulation that are dependent on the sign of B y . For the northern hemisphere, clockwise circulation displaced to the duskside appears roughly 35% of the time when B y is positive, and anticlockwise circulation displaced to the dawnside appears when B y is negative. The same circulation sense and location exist in the southern hemisphere for the opposite polarity of B y . At times of northward IMF, the circulation within the polar cap can be at least partially on closed field lines and cannot be easily reconciled with merely a distortion of the standard “two‐cell” convection pattern. The significance of these results to several models of the solar wind/magnetosphere interaction is discussed.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1987
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1988
    In:  Journal of Geophysical Research: Space Physics Vol. 93, No. A1 ( 1988-01), p. 115-136
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 93, No. A1 ( 1988-01), p. 115-136
    Abstract: Simultaneous satellite in situ measurements of density (Δ N/N ) and electric field fluctuation (Δ E ) spectra in the high‐latitude ionosphere are presented using two orbits of Dynamics Explorer 2 (DE 2) data traversing, respectively, the F region at 350 km altitude and the topside ionosphere at 900 km altitude. The spectral study was primarily confined to large structured velocity regions in the auroral oval. By means of the very complete set of energetic particle, dc and ac electric field, field‐aligned current, thermal plasma density, and temperature measurements available from DE 2, we were able to identify two categories of spectra associated with velocity shears irrespective of the height of the satellite. The first category was observed in very intense velocity shear regions of shear frequencies ∼10 Hz in conjunction with large field‐aligned current densities. Under these conditions the spatial spectra of Δ N/N and Δ E had identical power law indices of −1.8±0.2 between scale lengths of approximately 10 km and 300 m. At scale lengths shorter than 300 m the Δ E spectra steepened to an index of −3±0.5 while the spectral index of Δ N/N remained close to its original value of approximately −1.8±0.2, with large power spectral densities observed down to 10 m scale lengths. The second category was observed in more moderate velocity shear regions of shear frequencies ∼ 1 Hz in conjunction with weak field‐aligned currents. In this case the slopes of the density spectra were essentially unchanged, while the Δ E spectra had a much steeper slope of −3±0.5 between 10 km and a few hundred meters. Other factors identifying the two categories are as follows. The first category of spectra was characterized by the existence of upward flowing ions with conic distributions energized to 30 eV and possibly O + ion cyclotron waves and large electron temperature enhancements. The second category of spectra was associated with wave activity in the 4‐ to 16‐kHz range, most probably O + lower hybrid waves, and occasionally large ion temperature enhancements. The observations of Δ N/N and Δ E spectral behavior are compared to recent work on two‐dimensional plasma turbulence theory and nonlinear simulations of the collisional Kelvin‐Helmholtz (KH) instability. In particular, the spectral behavior associated with the moderate velocity shear category agrees well with some recent computations of the spatial power spectra of the KH instability (Keskinen et al., 1988).
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1988
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  • 3
    Online Resource
    Online Resource
    Mary Ann Liebert Inc ; 1987
    In:  Hybridoma Vol. 6, No. 6 ( 1987-12), p. 637-643
    In: Hybridoma, Mary Ann Liebert Inc, Vol. 6, No. 6 ( 1987-12), p. 637-643
    Type of Medium: Online Resource
    ISSN: 0272-457X , 0272-457X
    Language: English
    Publisher: Mary Ann Liebert Inc
    Publication Date: 1987
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  • 4
    In: Plant Pathology, Wiley, Vol. 35, No. 3 ( 1986-09), p. 390-395
    Type of Medium: Online Resource
    ISSN: 0032-0862 , 1365-3059
    URL: Issue
    Language: English
    Publisher: Wiley
    Publication Date: 1986
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  • 5
    Online Resource
    Online Resource
    Wiley ; 1986
    In:  Plant Pathology Vol. 35, No. 4 ( 1986-12), p. 427-433
    In: Plant Pathology, Wiley, Vol. 35, No. 4 ( 1986-12), p. 427-433
    Type of Medium: Online Resource
    ISSN: 0032-0862 , 1365-3059
    URL: Issue
    Language: English
    Publisher: Wiley
    Publication Date: 1986
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    SSG: 12
    Location Call Number Limitation Availability
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