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  "creator_user_id": "770631d3-fc59-4c0b-a34e-8ec37ebe30ec",
            
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  "data_type": "Scintillation Figure",
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  "data_type": "Scintillation Figure",
            
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  "dataset_end_date": "2200-01-01",
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  "dataset_end_date": "2025-04-08",
            
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  "dataset_start_date": "1900-01-01",
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  "dataset_start_date": "2025-04-01",
            
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  "groups": [],
            
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  "id": "260fee64-7f18-4c03-9fc4-ea1c40301ce2",
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  "id": "260fee64-7f18-4c03-9fc4-ea1c40301ce2",
            
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  "isopen": false,
            
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  "license_title": null,
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  "license_title": null,
            
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  "metadata_created": "2025-05-20T20:22:13.776895",
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  "metadata_created": "2025-05-20T20:22:13.776895",
            
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  "metadata_modified": "2025-05-20T20:22:13.776902",
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  "metadata_modified": "2025-05-20T20:22:14.518911",
            
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  "name": "2025_april_scint_figure_lsbr",
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  "name": "2025_april_scint_figure_lsbr",
            
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  "notes": "Data of GPS - SCINTILLATION FIGURES",
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  "notes": "Data of GPS - SCINTILLATION FIGURES",
            
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  "organization": {
            
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    "approval_status": "approved",
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    "approval_status": "approved",
            
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    "created": "2024-06-07T20:42:27.841122",
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    "created": "2024-06-07T20:42:27.841122",
            
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    "description": "GPS receivers provide precise measurements of the 
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    "description": "GPS receivers provide precise measurements of the 
            
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TEC of the ionosphere and plasma sphere, revealing depletions 
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TEC of the ionosphere and plasma sphere, revealing depletions 
            
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associated with plasma bubbles and AGW perturbations as traveling 
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associated with plasma bubbles and AGW perturbations as traveling 
            
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ionospheric disturbances (TIDs). They detect amplitude and phase 
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ionospheric disturbances (TIDs). They detect amplitude and phase 
            
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scintillations, and can also provide plasma density using inversion 
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scintillations, and can also provide plasma density using inversion 
            
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techniques. GPS receivers have proved to be a reliable, efficient, and 
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techniques. GPS receivers have proved to be a reliable, efficient, and 
            
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practical way to measure line-of-sight TEC in several points of the 
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practical way to measure line-of-sight TEC in several points of the 
            
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sky simultaneously. This is the reason why the number of GPS units 
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sky simultaneously. This is the reason why the number of GPS units 
            
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presently used for Aeronomy studies is 2000 or more on a worldwide 
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presently used for Aeronomy studies is 2000 or more on a worldwide 
            
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basis. The observatory will include a densely distributed array of 50 
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basis. The observatory will include a densely distributed array of 50 
            
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GPS receivers to be sited in 10 different countries of South 
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GPS receivers to be sited in 10 different countries of South 
            
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America.\r\n",
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America.\r\n",
            
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    "id": "8ed10e33-fdf8-4b72-b5f0-4b7ead1a2fe2",
            
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    "image_url": 
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"2024-06-11-201248.169854Screenshot-from-2024-06-11-15-12-02.png",
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"2024-06-11-201248.169854Screenshot-from-2024-06-11-15-12-02.png",
            
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    "is_organization": true,
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    "is_organization": true,
            
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    "name": "gnss",
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    "name": "gnss",
            
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    "state": "active",
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    "state": "active",
            
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    "title": "GNSS",
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    "title": "GNSS",
            
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    "type": "project"
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    "type": "project"
            
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  },
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  "state": "active",
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  "state": "active",
            
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  "tags": [],
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  "tags": [],
            
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  "title": "2025 APRIL SAN BARTOLOME SCINTILLATION",
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  "title": "2025 APRIL SAN BARTOLOME SCINTILLATION",
            
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  "type": "dataset",
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  "type": "dataset",
            
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  "voc_instrument_type": "Gnss",
            
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  "voc_station_name": "Piura"
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  "voc_station_name": "Piura"
            
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}
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}