Temperature and ion composition results obtained during the eclipse of 7 March 1970 at Millstone Hill are presented. The temperature variations appear to be controlled by the high degree of magnetic activity present on the eclipse day. Ion composition variations may be explained in terms of photochemical processes and the distribution of ionizing radiation across the solar disk. The data indicate the quality of ion composition determination by incoherent scatter radar, and it is concluded that these data are more useful when averaged in quantity to determine diurnal, seasonal, and solar cycle variations rather than short‐term temporal variations on a given day.
No takes yet. Share an insight, caveat, or question.
Oliver et al. (1974) studied this question.
Synapse has enriched 2 closely related papers on similar clinical questions. Consider them for comparative context: