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https://apps.dtic.mil/dtic/tr/fulltext/u2/a104149.pdf
ties, or scintillations, have been variously described as bubbles, plumes, patches, irregu-larities, disturbances and plasma (electron) density depletions. 3.1.2.1.1 Equatorial scintillation is predominantly a night time phenomena, usually occurring one to two hours after local sunset.
https://www.sciencedirect.com/science/article/pii/S1674984717302173
Mar 01, 2019 · It is observed that scintillations are prone to occur during the entire day, but the scintillation intensity tends to be higher during post–sunset period and early morning hours. This analysis shows that the intense scintillation activity begins after sunset. Download : Download high-res image (502KB) Download : Download full-size image; Fig. 2.Cited by: 8
https://agupubs.onlinelibrary.wiley.com/doi/10.1002/2015RS005807
Nov 17, 2015 · Observations of scintillations by COSMIC during early evening hours (13:00–15:00 UT) at locations around the magnetic equator (~10–12°N geographic latitude in the Indian longitude sector) are noted only on 8 March 2015 (13:47 UT, 12.56°N geographic latitude, 95.75°E geographic longitude).Cited by: 2
https://ieeexplore.ieee.org/abstract/document/4812009
Apr 07, 2009 · Scintillations are momentarily local breakdowns in tantalum capacitors, which are often considered as nuisances rather than failures. However, this paper shows that scintillations are damaging for more than 30% of part types and up to 100% for some lots. Scintillations can be observed after many hours of operation, and the probability of repeat scintillations is higher than of the initial ...Cited by: 6
https://angeo.copernicus.org/articles/23/2457/2005/angeo-23-2457-2005.pdf
gest that the occurrence of scintillations is mainly due to two types, namely the Plasma Bubble Induced (PBI), which max-imizes during the post sunset hours of winter and equinoctial months, and the Bottom Side Sinusoidal (BSS) type, which maximizes during the post-midnight hours of the summer solstice months. A detailed study on the spectral ...Cited by: 48
https://link.springer.com/article/10.1007/s10509-015-2292-9
Apr 10, 2015 · Scintillations exhibit daily trend of occurrences during the hours of 1900 LT–0200 LT, with higher occurrence levels being localized within the hours of 2000–2300 LT. Generally, highest scintillation occurrences were recorded during equinoxes and the least during June solstice. Intriguingly, over equatorial Africa, January was observed to ...
https://www.sciencedirect.com/science/article/pii/S0273117712005789
Feb 01, 2013 · More GPS scintillations were observed in pre-midnight hours than in post-midnight hours in all months . During quiet solar activity period (July 2008 to December 2010), most of the scintillations were observed in equinox months, and there was almost no scintillation observed in summer and winter.
https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2006SW000260
scintillations at higher frequencies and more irregular plasmas produce stronger amplitude scintillations. The temporal behavior of diffractive scintillations depends on the Fresnel length of the scintillations (see section 2.2), the drift speed of the ionosphere, and the relative velocities of the satellites and receivers [Kintner et al., 2004].
https://www.youtube.com/watch?v=Oz8X2FF3fd4
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