Extent Of Visibility Research Articles

Multinuclear NMR studies of the Langendorff perfused rat heart

The quantitation of intracellular sodium ion concentration [Na+]in perfused organs using NMR spectroscopy requires a knowledge of the extent of visibility of the 23Na resonance and of the intracellular volume of the organ. We have used a multinuclear NMR approach, in combination with the extracellular shift reagent dysprosium (III) tripolyphosphate, to determine the NMR visibility of intra- and extracellular 23Na and 35Cl ions, intracellular volume, and [Na+]in in the isolated Langendorff perfused rat heart. Based on a comparison of the extracellular volumes calculated using 2H and 23Na, 35Cl, or 59Co NMR of the perfused heart we conclude that resonances of extracellular sodium and chloride ions (including ions in interstitial spaces) are fully visible, contrary to assumptions in the literature. Furthermore, prolonged hypoxia or ischemia caused a dramatic increase in intracellular Na+ and [Na+] in rose to approach that in the external medium indicating full visibility of the intracellular 23Na resonance. Resonance intensities of intra- and extracellular 23Na ions, along with a knowledge of the extracellular space as a fraction of the total organ water space, yielded an average [Na+] in of about 10 mM (10 +/- 1.5 mM) for the rat heart at 37 degrees C. Double-quantum filtered 23Na NMR of the perfused rat heart in the absence and presence of paramagnetic reagents revealed, contrary to assumptions in the literature, that both intra- and extracellular sodium ions contribute to the detected signal.

Directivity of Saturn electrostatic discharges and ionospheric implications

From a detailed analysis of the intensity distribution of Saturn electrostatic discharges (SED) as a function of time during the Voyager 1 encounter with Saturn, the total beaming pattern of the SED source, which is found to be isotropic, is fetermined. This result allows for the derivation of the diurnal variations of the peak electron density over the dayside equatorial ionosphere of Saturn, and thus explains the puzzling features observed during the Voyager 1 encounter with Saturn—the longer extent of the SED visibility after closest approach and the existence of double-humped SED episodes before the encounter—by ionospheric absorption of the SED radio emission.