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  • Cation  (1)
  • magnetic network  (1)
  • Springer  (2)
  • Wiley-Blackwell
  • 1995-1999  (2)
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  • Springer  (2)
  • Wiley-Blackwell
Years
  • 1995-1999  (2)
Year
  • 1
    ISSN: 1432-0878
    Keywords: Key words Extraocular muscle ; Cation ; Muscular dystrophy ; Merosin ; dy Mouse
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Abstract Extraocular muscle is uniquely spared from damage in merosin-deficient congenital muscular dystrophy. Using a murine model, we have tested the hypothesis that the maintenance of calcium homeostasis is mechanistic in extraocular muscle protection. Atomic absorption spectroscopy has demonstrated a strong correlation between the perturbation of calcium homeostasis in hindlimb muscle that is severely damaged and the absence of changes in calcium in extraocular muscle. If, as in other skeletal muscles, extraocular muscle fibers are destabilized by merosin deficiency, we would expect an increase in total muscle calcium coupled with an adaptive response in the high capacity/speed of the sarcoplasmic reticulum of the eye muscle. However, we have not observed the expected increases in total muscle calcium content, Ca2+-ATPase activity, Na+/Ca2+ exchanger content, or smooth ER Ca2+-ATPase content that are predicted by this model. Instead, these results indicate that the increased membrane permeability that characterizes, and is potentially mechanistic in, myofiber degeneration in muscular dystrophy does not occur in merosin-deficient extraocular muscle. Thus, the high-capacity calcium-scavenging systems are not primarily responsible for extraocular muscle protection in muscular dystrophy.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1572-9672
    Keywords: coronal heating ; magnetic network ; coronal bright points
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract By combining quiet-region Fe XII coronal images from SOHO/EIT with magnetograms from NSO/Kitt Peak and from SOHO/MDI, we show that the population of network coronal bright points and the magnetic flux content of the network are both markedly greater under the bright half of the large-scale quiet corona than under the dim half. These results (1) support the view that the heating of the entire corona in quiet regions and coronal holes is driven by fine-scale magnetic activity (microflares, explosive events, spicules) seated low in the magnetic network, and (2) suggest that this large-scale modulation of the magnetic flux and coronal heating is a signature of giant convection cells.
    Type of Medium: Electronic Resource
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