analysis and comparison of awesome detected vlf perturbations
DESCRIPTION
Analysis and Comparison of AWESOME Detected VLF Perturbations. S. NAITAMOR 1 , M. A. ALABDOADAIM 2. 1 Centre de Recherche en Astronomie Astrophysique et Géophysique-Alegria . 2- Department of Physics, Sebha University-Libya. Outline. Analysis of Algeria AWESOME results - PowerPoint PPT PresentationTRANSCRIPT
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Analysis and Comparison of AWESOME Detected VLF Perturbations
S. NAITAMOR1, M. A. ALABDOADAIM2
1 Centre de Recherche en Astronomie Astrophysique et Géophysique-Alegria.2- Department of Physics, Sebha University-Libya
![Page 2: Analysis and Comparison of AWESOME Detected VLF Perturbations](https://reader036.vdocuments.us/reader036/viewer/2022062802/5681449c550346895db147d6/html5/thumbnails/2.jpg)
Outline
Analysis of Algeria AWESOME results
Association between TLEs and Early VLF signal perturbations Are TLEs the unique cause of early VLF perturbations?
Comparison between Algeria and Libya AWESOME results
Can we observe an Early event by distant receiver ?
Conclusions
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12-13 October EventsSprite at 22:51:35 (36.59N 3.32E)Sprite at 23:04:41 (38.06N 3.83E)
Elves at 00:32:00
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Direct Paths Scattered Path
Tons=198ms
Tons= 180
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Direct Paths
Scattered Paths
Circles Lightning near to the Elves time
Tons = 180ms
Tons = 120 ms
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October 17-18 eventsSprite at 21:28:27 (40.1N 4.55E) Sprite at 20:59:32 (39.98N 4.51E)
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Tons = 600ms
Tons = 330ms
Tons = 600ms
Tons = 300ms
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Sprite at 01:43:59
17-18 December events
Sprite at 23:09:48
The events were well situated for multi frequencies observations
17/12/200718/12/2007
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Sprite at 23:09:48
Tons = 48ms
Tons=258ms
Tons= 40ms
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Sprite at 01:43:59
Tons = 198ms
Tons = 138ms
Tons = 318ms
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Last TLE was at 03:54:25 234mn after 00:00
No TLE was observed during this time interval
Are TLEs the unique sources of VLF signal perturbations ?
What could be the sources of these perturbations ?
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No Signal perturbation was observed by the receiver at Sebha even though the CG locations were near the GCPs from HWU, GQD and NRK to Sebha
What about the distant receiver data ?
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• Near receiver results showed that Early VLF perturbation due to TLE may have different scattering process.
• The scattering process plays an important role in determining the onset time and the amplitude of the VLF signal perturbation.
• In absence of TLEs, supplementary ionization can occur due to Lightning discharges which can affect the VLF signal.
• Sebha (Libya) AWESOME receiver results showed clearly that not all the VLF perturbations survived the long distance to the receiver, event if the activity is close to the GCP.
Conclusion