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dc.contributor.authorFlock, Warren L.
dc.date.accessioned2024-11-09T01:08:51Z
dc.date.available2024-11-09T01:08:51Z
dc.date.issued1962-10
dc.identifier.urihttp://hdl.handle.net/11122/15608
dc.descriptionUAG R-130en_US
dc.description.abstractThe relations between VHF and UHF radio aurora and geomagnetic activity, as indicated by telluric current records, have been investigated. (VHF and UHF radio aurora are considered in Parts I and II, respectively, of this report.) VHF radio aurora, observed over Barrow, Alaska by a 41 Mc/s radar at Kotzebue, Alaska, and telluric current activity at Barrow show a high correlation, particularly with respect to onsets of major activity. Slight or moderate activity usually gives some forewarning of intense activity, but some disturbances have extremely abrupt onsets of intense activity. The correlation is clearly highest for overhead and nearly overhead radio aurora and drops off for separations of 300 km and more. Incoherent scatter from ionosphere has been recorded by the BMEWS UHF radar at Clear, Alaska by use of two different techniques. A generally applicable procedure is to record radar return for a period of time in analog form on magnetic tape for subsequent processing by a digital computer. The BMEWS radar is also capable of detecting incoherent scatter by the use of “DTO” reports accumulated over a period of time. Conventional ionospheric electron density profiles showing E, F1, and F2 layers, with the highest electron densities in the F2 layer, have been obtained at times. On other occasions the peak in electron density occurs at F1 layer heights. The technique is capable of providing profiles under conditions causing “blackout” of conventional ionosonde recorders.en_US
dc.description.sponsorshipPrepared for Radio Corporation of America; Moorestown, New Jersey; Final Report, Contract No. AF 04(647)179.en_US
dc.description.tableofcontentsAbstract -- 1. Introduction -- 2. Radio aurora and geomagnetic activity -- 2.1. Introduction -- 2.2. VHF radio aurora and geomagnetic activity – 2.2.1. High correlation between radio aurora ad telluric currents – 2.2.2. Distance from echoing region to recorder – 2.2.3. Diurnal variations – 2.2.4. Seasonal characteristics – 2.2.5. Fast fluctuations in telluric currents – 2.2.6. Rapidity of onsets – 2.2.7. Discontinuous scattered radio echoes – 2.2.8. Relative sensitivities and onset times – 2.2.9. Amplitude of radio echoes -- 3. The auroral ionosphere -- 3.1. Introduction -- 3.2. The aurora polaris – 3.2.1. The northern auroral zone – 3.2.2. Prediction of auroral activity – 3.2.3. Certain characteristics of radio aurora – Introduction – Interpretation of data of section 2 -- 3.3. Polar-cap absorption -- 3.4. The ionospheric layers and incoherent scatter – 3.4.1. Application of incoherent scatter to ionospheric sounding – 3.4.2. Incoherent scatter measurements -- 4. Recording facilities and procedures -- 4.1. The 41 Mc/s auroral radar -- 4.2. Telluric current equipment -- 4.3. Recording equipment at site II – 4.3.1. Photographic recording – 4.3.2. Magnetic-tape recording -- 4.4. Processing of radar return for incoherent scatter – 4.4.1. Reduction of magnetic-tape data – 4.4.2. Future plans for analysis of magnetic-tape data -- 5. Conclusions and recommendations -- Acknowledgments -- References -- List of illustrations -- Appendix.en_US
dc.language.isoen_USen_US
dc.publisherGeophysical Institute at the University of Alaska Fairbanksen_US
dc.subjectRadar meteorologyen_US
dc.subjectAurorasen_US
dc.subjectIonospheric radio wave propagationen_US
dc.titleEnvironmental studies for radar operations in the auroral zoneen_US
dc.typeReporten_US
refterms.dateFOA2024-11-09T01:08:53Z


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