Changes
On February 8, 2025 at 1:06:17 AM UTC,
ckancielo:
-
Changed value of field
dataset_end_date
to2025-02-08
in 2025 FEBRUARY HUANCAYO SCINTILLATION -
Added resource lhyo_250208_s4.pdf to 2025 FEBRUARY HUANCAYO SCINTILLATION
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| 12 | "name": "2025_february_scint_figure_lhyo", | 12 | "name": "2025_february_scint_figure_lhyo", | ||
| 13 | "notes": "Data of GPS - SCINTILLATION FIGURES", | 13 | "notes": "Data of GPS - SCINTILLATION FIGURES", | ||
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| 17 | "approval_status": "approved", | 17 | "approval_status": "approved", | ||
| 18 | "created": "2024-06-07T20:42:27.841122", | 18 | "created": "2024-06-07T20:42:27.841122", | ||
| 19 | "description": "GPS receivers provide precise measurements of the | 19 | "description": "GPS receivers provide precise measurements of the | ||
| 20 | TEC of the ionosphere and plasma sphere, revealing depletions | 20 | TEC of the ionosphere and plasma sphere, revealing depletions | ||
| 21 | associated with plasma bubbles and AGW perturbations as traveling | 21 | associated with plasma bubbles and AGW perturbations as traveling | ||
| 22 | ionospheric disturbances (TIDs). They detect amplitude and phase | 22 | ionospheric disturbances (TIDs). They detect amplitude and phase | ||
| 23 | scintillations, and can also provide plasma density using inversion | 23 | scintillations, and can also provide plasma density using inversion | ||
| 24 | techniques. GPS receivers have proved to be a reliable, efficient, and | 24 | techniques. GPS receivers have proved to be a reliable, efficient, and | ||
| 25 | practical way to measure line-of-sight TEC in several points of the | 25 | practical way to measure line-of-sight TEC in several points of the | ||
| 26 | sky simultaneously. This is the reason why the number of GPS units | 26 | sky simultaneously. This is the reason why the number of GPS units | ||
| 27 | presently used for Aeronomy studies is 2000 or more on a worldwide | 27 | presently used for Aeronomy studies is 2000 or more on a worldwide | ||
| 28 | basis. The observatory will include a densely distributed array of 50 | 28 | basis. The observatory will include a densely distributed array of 50 | ||
| 29 | GPS receivers to be sited in 10 different countries of South | 29 | GPS receivers to be sited in 10 different countries of South | ||
| 30 | America.\r\n", | 30 | America.\r\n", | ||
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| 37 | "title": "GNSS", | 37 | "title": "GNSS", | ||
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| 178 | "title": "2025 FEBRUARY HUANCAYO SCINTILLATION", | 204 | "title": "2025 FEBRUARY HUANCAYO SCINTILLATION", | ||
| 179 | "type": "dataset", | 205 | "type": "dataset", | ||
| 180 | "voc_instrument_type": "Gnss", | 206 | "voc_instrument_type": "Gnss", | ||
| 181 | "voc_station_name": "Huancayo" | 207 | "voc_station_name": "Huancayo" | ||
| 182 | } | 208 | } |