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  • 74.20. Fg  (1)
  • LUNAR AND PLANETARY EXPLORATION  (1)
  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Applied physics 59 (1994), S. 41-48 
    ISSN: 1432-0630
    Keywords: 61.16. Di ; 74.20. Fg ; 74.50. +r ; 74.60. Ec
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Physics
    Notes: Abstract The current status of scanning probe microscopy on superconductors is briefly reviewed. Both tunneling and force microscopy have clearly become valuable tools for topographic surface characterization of superconductors. They have especially contributed to our understanding of growth mechanisms, morphology and surface properties of high-temperature superconductors. Furthermore, scanning tunneling spectroscopy on some special model-type conventional superconductors has provided completely new insight into fundamentals of superconductivity. In the latter respect only moderate success has yet been met for all technically relevant materials and especially for the ceramic materials due to surface quality problems. Very recent results show that magnetic force microscopy may be capable of imaging flux lines in superconductors, even if the surface is non-ideal. Flux-line imaging has already been achieved by employing scanning field probes. Some concrete future challenges concerning the application of scanning probe techniques to the study of superconducting materials and superconductivity are discussed.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-07-13
    Description: The Pioneer 10 and 11 Jupiter probes have provided several opportunities for observation of the Jovian satellites J I through J V. From these data, a tenuous atmosphere of hydrogen for Io has been identified. In the present work, an additional short-wavelength (less than 800 A) emission associated with an extended cloud centered on Io is reported and interpreted as arising from the radiative decay of excited atomic ions. Characteristic X-rays produced by electron bombardment of Io's surface may also contribute to the signal. Emission features associated with Amalthea (J V) and Europa (J II) are also observed. Signals apparently associated with J V occur in the long-wavelength channel, while emissions were observed in the short-wavelength channel during J II observations. The data of the long-wavelength channel are interpreted as arising from atomic hydrogen Lyman-alpha emission in all cases. The source species for the short-wavelength emissions cannot at this time be unambiguously determined, but the wavelength range of the signals is well established.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Colloquium on Jupiter: Studies of the interior, atmosphere, magnetosphere and satellites; May 19, 1975 - May 21, 1975; Tucson, AZ
    Format: text
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