The Effects of Solar Eclipse of August 1, 2008 on Earth’s Atmospheric Parameters
01 Oct 2010-Pure and Applied Geophysics (SP Birkhäuser Verlag Basel)-Vol. 167, Iss: 10, pp 1273-1279
TL;DR: In this paper, the effects of the solar eclipse on Fair Weather Field (FWF) and VLF amplitude and phase were investigated at Kolkata (latitude: 22°34′N, longitude: 88°30′E).
Abstract: Several experiments were undertaken at Kolkata (latitude: 22°34′N, longitude: 88°30′E) on the solar eclipse day of August 1, 2008 to observe the effects of the solar eclipse on Fair Weather Field (FWF) and VLF amplitude and phase. The experimental results presented here show significant deviations of the observed parameters from their normal values, as they are determined by the average of the records obtained on 5 days adjacent to the day of the solar eclipse.
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TL;DR: Atmospheric effects of solar eclipses stimulated by the 2015 UK eclipse are reviewed, with particular attention to events providing important early insights into the ionization of the upper atmosphere.
Abstract: This article reviews atmospheric changes associated with 44 solar eclipses, beginning with the first quantitative results available, from 1834 (earlier qualitative, accounts also exist). Eclipse meteorology attracted relatively few publications until the total solar eclipse of 16 February 1980, with the 11 August 1999 eclipse producing the most papers. Eclipses passing over populated areas such as Europe, China and India now regularly attract scientific attention, whereas atmospheric measurements of eclipses at remote locations remain rare. Many measurements and models have been used to exploit the uniquely predictable solar forcing provided by an eclipse. In this paper we compile the available publications and review a sub-set of them chosen on the basis of importance and novelty. Beyond the obvious reduction in incoming solar radiation, atmospheric cooling from eclipses can induce dynamical changes. Observations and meteorological modelling provide evidence for the generation of a local eclipse circulation which may be the origin of the "eclipse wind". Gravity waves set up by the eclipse can, in principle, be detected as atmospheric pressure fluctuations, though theoretical predictions are limited, and many of the data are inconclusive. Eclipse events providing important early insights into the ionisation of the upper atmosphere are also briefly reviewed.
42 citations
TL;DR: This article reviewed atmospheric changes associated with 44 solar eclipses, beginning with the first quantitative results available, from 1834, and reviewed a subset of them chosen on the basis of importance and novelty.
Abstract: This article reviews atmospheric changes associated with 44 solar eclipses, beginning with the first quantitative results available, from 1834 (earlier qualitative accounts also exist). Eclipse meteorology attracted relatively few publications until the total solar eclipse of 16 February 1980, with the 11 August 1999 eclipse producing the most papers. Eclipses passing over populated areas such as Europe, China and India now regularly attract scientific attention, whereas atmospheric measurements of eclipses at remote locations remain rare. Many measurements and models have been used to exploit the uniquely predictable solar forcing provided by an eclipse. In this paper, we compile the available publications and review a subset of them chosen on the basis of importance and novelty. Beyond the obvious reduction in incoming solar radiation, atmospheric cooling from eclipses can induce dynamical changes. Observations and meteorological modelling provide evidence for the generation of a local eclipse circulation that may be the origin of the ‘eclipse wind’. Gravity waves set up by the eclipse can, in principle, be detected as atmospheric pressure fluctuations, though theoretical predictions are limited, and many of the data are inconclusive. Eclipse events providing important early insights into the ionization of the upper atmosphere are also briefly reviewed. This article is part of the themed issue ‘Atmospheric effects of solar eclipses stimulated by the 2015 UK eclipse’.
35 citations
TL;DR: In this article, the effects of the total solar eclipse on the dynamics of the equatorial lower ionosphere during ionospheric sunrise transition period were studied using subionospherically propagating VLF signal at 18.2 kHz over a distance of 2200 km.
Abstract: [1] Changes in equatorial D-region electron density are studied using subionospherically propagating VLF signal at 18.2 kHz over a distance of 2200 km during the total solar eclipse of 22 July 2009. There are very few studies about the eclipse's effects on the equatorial lower ionosphere in the scientific literature. In the light of that, the objective of the present work is to study the effects of the eclipse on the dynamics of the equatorial lower ionosphere during ionospheric sunrise transition period. In the present case, great circle path between VLF transmitter and receiver falls totally in partial eclipse zone, having a maximum solar obscuration of 90% and an average obscuration of 74%. Results show an average decrease of 3.2 dB in signal strength compared to control days during peak solar obscuration over the path. A comparison with previous studies shows an increase both in lower ionosphere virtual reflection height (H′) and Wait inverse scale height parameter (β); the values estimated are 74.5 km and 0.46 km−1 compared to unperturbed ionosphere values of 71 km and 0.43 km−1, respectively. During maximum eclipse over the path, the model profile shows an average 80% drop in electron density at a height of 71 km at equatorial lower ionosphere. A nonlinear variation of lower ionosphere electron density with solar radiation is found as opposed to the model study proposed by previous workers.
35 citations
Cites background from "The Effects of Solar Eclipse of Aug..."
...[14] Previous studies involving VLF signal during eclipse period showed both increases and decreases in their amplitude on different occasions [De and Sarkar, 1997; Fleury and Duchesne, 2000; Clilverd et al., 2001; De et al., 2009 ]....
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TL;DR: In this paper, the effects of two solar eclipses on the propagation characteristics of VLF sferics in the Earth-ionosphere waveguide were investigated at a fixed receiver location (23.75°N, 91.25°E).
Abstract: [1] Effects of solar eclipses on the propagation characteristics of worldwide VLF sferics from lightning activity require more investigation. An attempt was made on the occasion of two solar eclipses during 22nd July, 2009 and 15th January, 2010 to study the effects of the two eclipses on the propagation characteristics of VLF sferics in the Earth-ionosphere waveguide. Identical experimental setups were used to study the VLF sferics during the two eclipse events. The spectral character of VLF sferics propagating inside the waveguide is studied at a fixed receiver location (23.75°N, 91.25°E) at six discrete frequencies in between 3 and 20 kHz. During both the eclipse events, it is observed that VLF sferics at all the six discrete frequencies is increased from the mean normal average ambient level. The increment peaks around 10–12 kHz with an overall increment of 6.4 dB with respect to its ambient level. The VLF spectral character of enhancement of sferics show similar characters in two eclipses. The percentage decrease in electron density using standard modeling equations is found to be 90% at the height of 71 km for both the eclipses, supporting linear variation of electron density with solar radiation at the D-region of the ionosphere. The results are explained qualitatively on the basis of a decrease in electron density at the lower ionosphere modifying the reflection coefficient which affected the propagation of VLF sferics in Earth-ionosphere waveguide during eclipsed condition.
14 citations
TL;DR: In this article, the phase and amplitude changes of the VLF signals transmitted by the NDK station at 25.2 kHz in North Dakota, USA during the August 21, 2017 solar eclipse were detected.
7 citations
References
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06 Oct 2018
483 citations
TL;DR: In this paper, the fair-weather global electric circuit has been studied and it has been shown that lightning and thunderstorms must occur continually to maintain the fair weather electric field, and the time constant of the circuit, ∼>2 min, demonstrates that thunderstorms are necessary and sufficient for maintaining the electric field.
319 citations
TL;DR: In this article, the authors used measured field strengths from VLF transmitters to determine improved day-time values of ionospheric parameters to enable improved VlF propagation predictions.
165 citations
"The Effects of Solar Eclipse of Aug..." refers background in this paper
...43 km and H0 = 72 km, since these are appropriate (THOMSON, 1993)....
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...…T ¼ d k 1 2a þ k 2 16h3 Dh: ð6Þ Using the experimental value of Dt as observed in the case of 25 kHz transmitted signal and taking h = 72 km, it is found that Dh % 3.75 km. xr can be expressed as xr ¼ 2:5 105 exp b h H 0 n o ; ð7Þ (WAIT and SPICE, 1964; THOMSON, 1993; CLILVERD et al., 2001)....
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...For normal ionosphere, b = 0.43 km-1 and H0 = 72 km, since these are appropriate (THOMSON, 1993)....
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TL;DR: On a clear day, there is a downward electric field of 100 to 300 volts/meter at Earth's surface, although this field is not noticeable in daily life as discussed by the authors. But the field is there.
Abstract: On a clear day, there is a downward electric field of 100 to 300 volts/meter at Earth's surface, although this field is not noticeable in daily life. That is, one does not encounter a 1 kV potential difference when getting into a car on an upper floor in a parking garage, and electrocution is not the major hazard associated with jumping out of trees. The major reason why we don't notice the fair‐weather field is that virtually everything is a good conductor compared to air. Objects such as tree trunks and our bodies are excellent ionic conductors that short out the field and keep us from noticing it. But the field is there.
154 citations
"The Effects of Solar Eclipse of Aug..." refers background in this paper
...Introduction The quasi-static electric fields near the Earth’s surface, i.e., Fair Weather Field (FWF), are governed by global thunderstorm and lightning activities (BERING et al., 1998; RYCROFT and PRICE, 2000)....
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..., Fair Weather Field (FWF), are governed by global thunderstorm and lightning activities (BERING et al., 1998; RYCROFT and PRICE, 2000)....
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TL;DR: In this paper, the amplitude and phase of the ionospheric potential and Carnegie curve of atmospheric electricity are considered to distinguish causes for the negatively charged earth in fair weather, and the results suggest that conduction current other than lightning is the dominant charging agent for the Earth's surface.
Abstract: Both the amplitude and the phase of the ionospheric potential and Carnegie curve of atmospheric electricity are considered to distinguish causes for the negatively charged earth in fair weather. Satellite-observed longitudinal distributions of electrical activity are convolved with local diurnal variations of cloud-to-ground lightning and point discharge current to produce universal diurnal variations which are compared with the Carnegie curve. The amplitude ratio (maximum-minimum)/mean) for the predicted universal diurnal variation of point discharge shows good agreement with the Carnegie curve, whereas the predicted amplitude ratio for lightning is 2–3 times greater. These comparisons suggest that conduction current other than lightning is the dominant charging agent for the Earth's surface.
153 citations
"The Effects of Solar Eclipse of Aug..." refers background in this paper
...It can reach several thousand kilometers from its source (WILLIAMS and HECKMAN, 1993), therefore thunderstorm activities at long distances can be monitored by studying the intensity of the sferics....
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