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  • 2020-2023  (2)
  • 1935-1939  (2)
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  • 1
    Publication Date: 2022-04-01
    Description: Observations by the Magnetospheric Multiscale spacecraft (MMS) of an unusual layer, located between the dayside magnetosheath and the magnetosphere, alternating with encounters with the magnetosheath during an extended time period between December 31, 2015 and January 01, 2016, when the interplanetary magnetic field was strongly southward and the Earth's dipole tilt large and negative, are presented. It appears to have been magnetically connected to both magnetosphere and magnetosheath. The layer appears to be located mostly on closed field lines and was bounded by a rotational discontinuity (RD) at its magnetosheath edge and by the magnetosphere on its earthward side. A separatrix layer, with heated magnetosheath electrons streaming unidirectionally along the field lines, was present sunward of the RD. We infer that the layer was started by a dominant reconnection site well north of the spacecraft and that it may have gained additional width, from a large drop in solar wind density and ram pressure, which preceded the beginning of the event by more than an hour. Relative to the magnetosheath, in which the magnetic field was strongly southward, this unusual layer was characterized by a less southward, more dawnward magnetic field of lower magnitude. The plasma density and flow speed in the region were lower than in the magnetosheath, albeit with Alfvénic jetting occurring at the magnetosheath edge as well as at the magnetospheric edge of the layer. The closing of the magnetic field lines requires the existence of another reconnection site, located southward/tailward of MMS.
    Description: Key Points: Magnetopause encounter for strongly southward interplanetary magnetic field, low solar wind Alfvén Mach number, and large dipole tilt. Persistent and broad magnetopause layer with magnetospheric O+ and heated magnetosheath plasma. Inferred dominant reconnection site near northern cusp, far from the Magnetospheric Multiscale spacecraft location.
    Description: MPE
    Description: NASA http://dx.doi.org/10.13039/100000104
    Description: Norwegian Research Council http://dx.doi.org/10.13039/501100005416
    Keywords: ddc:538.7
    Language: English
    Type: doc-type:article
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  • 2
    Electronic Resource
    Electronic Resource
    s.l. : American Chemical Society
    Journal of the American Chemical Society 59 (1937), S. 1387-1388 
    ISSN: 1520-5126
    Source: ACS Legacy Archives
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 3
    Publication Date: 1937-07-01
    Print ISSN: 0002-7863
    Electronic ISSN: 1520-5126
    Topics: Chemistry and Pharmacology
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  • 4
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    In:  Code4Lib Journal
    Publication Date: 2021
    Description: There are many ways to look at electronic resource use, individually or aggregated. I propose two new metrics to help give a better understanding of comparative use across an online collection. 〈em〉Users per mille〈/em〉 is a relative annual measure of how many users a platform had for every thousand potential users: this tells us how many people used a given platform. 〈em〉Interest factor〈/em〉 is the average number of uses of a platform by people who used it more than once: this tells us how much people used a given platform. These two metrics are enough to give us good insight into collection use. Dividing each into quartiles allows a quadrant comparison of lows and highs on each metric, giving a quick view of platforms many people use a lot (the big expensive ones), many people use very little (a curious subset), a few people use a lot (very specific to a narrow subject) and a few people use very little (deserves attention). This helps understand collection use and informs collection management.
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