Scintillations Hours

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Characteristics of postmidnight L band scintillation in ...

    https://agupubs.onlinelibrary.wiley.com/doi/10.1002/2015RS005807#:~:text=Intense%20amplitude%20scintillations%20at%20VHF%20and%20L%20band,and%20extend%20in%20both%20horizontal%20and%20vertical%20directions.
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Scintillating Scotoma - an overview | ScienceDirect Topics

    https://www.sciencedirect.com/topics/veterinary-science-and-veterinary-medicine/scintillating-scotoma
    A 47-year-old woman with a history of migraine with aura had her typical scintillations lasting 25 minutes and followed by a headache for 4 hours 10 minutes after an injection of lauromacrogol 400 foam (0.15%) 2 …

Characteristics of postmidnight L band scintillation in ...

    https://agupubs.onlinelibrary.wiley.com/doi/10.1002/2015RS005807
    During the postmidnight hours (19:00–23:00 UT), nine cases of intense scintillations (S 4 ≥ 0.6) were found between the latitudes of 20 and 40°N, of which seven occurred at latitudes greater than 30°N as seen from Figure 3. On further analyzing these seven cases, it was found that they occurred between 19:00 and 20:00 UT and were confined to heights of 234–341 km.

SWS - Section Information - About Ionospheric Scintillation

    https://www.sws.bom.gov.au/Satellite/6/3
    Each division on the X axis (15°) corresponds to 1 hour. Again, two strong scintillation bands can be seen roughly corresponding to ±15° geomagnetic latitude (as indicated by the dashed lines). The equatorial scintillation is present at decreasing intensity levels throughout most of …

(PDF) Statistics of Night time Ionospheric Scintillation ...

    https://www.researchgate.net/publication/230639488_Statistics_of_Night_time_Ionospheric_Scintillation_Using_GPS_data_at_lowlatitude_ground_station_Varanasi
    The diurnal variation of scintillations shows a nighttime maximum. This occurs before midnight in summer and about 3 hours postmidnight the rest of the year.

Ionospheric Scintillations: Indices and Modeling ...

    https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2018RS006655
    The slope decreases with time from an average value equal to 2.3 to a value of 1.8 at the end of the time period of scintillation occurrence. As the scintillations disappear after a few hours, this may correspond to a decrease of the turbulences inside the medium.

Geostationary L-band signal scintillation observations ...

    https://www.sciencedirect.com/science/article/abs/pii/S1364682606002239
    Considering individual hours, a maximum percentage occurrence of 37 was recorded in the interval 19–20 LT. Although the percentage occurrence appears to be low, scintillations with Scintillation Index (SI)>20 dB were recorded on 23 out of 31 nights during the same month, indicating that scintillations do not occur continuously over a long interval of time, but in small patches with clear gaps in between.

Geophysicae VHF and L-band scintillation characteristics ...

    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 charac-

Scintillating scotoma - Wikipedia

    https://en.wikipedia.org/wiki/Scintillating_scotoma
    Scintillating scotoma is a common visual aura that was first described by 19th-century physician Hubert Airy (1838–1903). Originating from the brain, it may precede a migraine headache, but can also occur acephalgically (without headache).It is often confused with retinal migraine, which originates in the eyeball or socket.

VHF and L-band scintillation characteristics over an ...

    https://ui.adsabs.harvard.edu/abs/2005AnGeo..23.2457R/abstract
    Using the onset times of several similar scintillation patches across the two satellite (FLEETSAT 73° E, INMARSAT 65° E) ray paths (sub-ionospheric points are separated by 82 km), the East ward movement of the irregularity patches is found to vary from 150 to 250 m/s during the post sunset hours and decrease slowly during the post midnight hours.

Ionospheric S4 Scintillations from GNSS Radio …

    https://www.mdpi.com/2072-4292/12/15/2373/htm
    Figure 4 shows such a wide spread of the scintillations from ESF and EPBs with an impact on the entire RO scan in the post–evening hours in March COSMIC–1 S4. At 20° N the S4 amplitude from ESF and EPBs remains approximately same above ( h t = 120 km) and below ( h t = 30 km) the Es layer, suggesting little impact form the RO path ...

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