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The joint processing of spectrometric, photometric and videometric data disclosed a high correlation (R ≥ 0.9985) between the integral and spectral changes of solar radiation with time as well as a concomitant correlation between the solar radiation intensity and the changes in the area and the brightness of the unshaded part of the solar disk in the time interval before and after the totality. The examination of the solar radiation dynamics revealed presence of fluctuations in the recorded spectral distributions before and after the eclipse totality expressed in a weak redistribution of the solar energy in the spectral range (480÷810 nm) in the limits of 1÷2%. Black and white images of the Sun's disk were taken using a television CCD-camera through a neutral filter. solar radiation was measured by means of a high-resolution multi-channel spectrometer and a photometer. The spectral distribution and integral changes in the solar radiation reaching the Earth's surface as well as images of the Sun's disk were registered from an observation post on the line of totality situated on the Black Sea coast. Results from videospectrometric investigations of the solar radiation during the total solar eclipse on 11 August 1999 in the territory of Bulgaria are presented. By analyzing the data on TEC gradient variations, one is led to conclude that the depression of TEC growth during the eclipse is essentially independent of the longitude and of the latitude (within the observation ranges 52☖° N and 104☑1° E). The delay of a minimum value of TEC with respect to the maximum phase of eclipse at 300 km altitude was about 10 min, and the depression depth of TEC growth varies from l÷3×1016m−2. indicative of profound changes in the ion production process in the ionosphere attendant on the solar eclipse, simultaneously in a large volume of space with a radius of at height 300 km at 300 km altitude. The interferometer consists of three receivers (one Turbo-Rogue SNR-8000, and two Ashtech Z-12) located at the vertices of a triangle and spaced by about 3–5 km.
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We do not guarantee that these techniques will work for you.This paper presents data from first measurements of total electron content (TEC) and its gradient during the solar eclipse of March 9, 1997, obtained with the GPS-radio interferometer at Irkutsk. Go to and click Book Samples, or go directly to the Quality Eclipse update site to download the. It worked your cooking skills have me soft as a marshmallow. I thought taking dinner off your hands would soften you up.
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