Description
The results of a comprehensive study of solar induced geophysical phenomena at pairs of stations linked by a magnetic field line are presented. Studies have established that magnetic variations (except Sq), telluric currents, ionospheric absorption, visual auroras, VLF and ELF emissions and auroral X-rays occur in similar manner in conjugate areas—in time, form and amplitude. The variations of the magnetic field were the most thoroughly studied phenomena. It was found that auroral zone electrojets occur in conjugate patterns, and that a conjugate area, elongated in geomagnetic latitude, can be defined by comparisons of magnetic records. This conjugate area appears to move in time, as the electrojets depart somewhat from conjugate patterns. The magnetic variations at mid and low latitude due to the return current paths of the electrojets are conjugate to approximately the same degree as the ‘primary’ auroral zone activity. At very high latitudes there is a diurnal variation in the degree of correlation at conjugate points—probably due to the distortion of the magnetic field by the solar wind. Some evidence is presented for two kinds of very high latitude magnetic disturbance. One occurring on the night side is probably due to the poleward expansion of auroral electrojet systems. The other occurs on the day side, even on very quiet days, and is possibly due to hydromagnetic waves, produced by the interaction of the magnetosphere surface and the solar wind. This dayside agitation shows inferior correlation. The Sq variation was investigated and found to be a non-conjugate phenomenon. The theoretical effects of field line linkage are found to skew rather than to equalize the variations from a conjugate pattern. The close relationship of telluric currents to magnetic variations, and the effects of local conductivity are considered. Comparison of records from paired stations confirm that telluric currents are conjugate. The mechanism of short period (~ 1 minute) oscillations may be found in modes of oscillation of the magnetosphere, as apart from ionospheric current systems. A pronounced diurnal variation was found in the power spectra and the polarization of short period oscillations at a mid-latitude pair. Comparisons of all-sky camera data from several conjugate pairs confirm that auroras occur in similar, simultaneous displays in conjugate areas. Occasional differences between the northern and southern displays were observed, similar to the anomalies in the magnetic variations. An attempt was made to study the conjugacy of radio auroras at 50-55 Mc/s but the results were inconclusive. Ionospheric absorption of cosmic radio noise—a phenomenon closely related to influx of charged particles and X-rays—has been shown in several studies to occur as a conjugate phenomenon. A conjugate area, similar in shape to that defined by correlation of magnetic variations was found for absorption events. Although no new work was carried out, the published results of conjugate studies of VLF (whistlers, etc.), ELF (micropulsations) and auroral zone balloon flights (auroral zone X-rays) are presented and discussed.
Publication Date
5-17-1964
Keywords
Geomagnetism
Recommended Citation
Wescott, Eugene M. and Mather, Keith Benson, "An investigation of solar induced phenomena at magnetically conjugate points" (1964). GI Reports. 196.
https://ualaska.researchcommons.org/uaf_gi_reports/196
Handle
http://hdl.handle.net/11122/15673