Changes
On March 10, 2025 at 8:27:33 PM UTC,
-
Changed value of field
dataset_start_date
to2024-11-01
in 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA -
Changed value of field
dataset_end_date
to2024-11-28
in 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA -
Added resource lsbr_241101.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241103.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241108.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241110.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241102.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241112.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241128.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241104.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241107.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241106.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241109.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241111.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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Added resource lsbr_241105.s4.gz to 2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA
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2 | "creator_user_id": "770631d3-fc59-4c0b-a34e-8ec37ebe30ec", | 2 | "creator_user_id": "770631d3-fc59-4c0b-a34e-8ec37ebe30ec", | ||
3 | "data_type": "Scintillation Data", | 3 | "data_type": "Scintillation Data", | ||
n | 4 | "dataset_end_date": "2200-01-01", | n | 4 | "dataset_end_date": "2024-11-28", |
5 | "dataset_start_date": "1900-01-01", | 5 | "dataset_start_date": "2024-11-01", | ||
6 | "groups": [], | 6 | "groups": [], | ||
7 | "id": "01e0dda9-5fcb-44a5-ada8-0474208b8cd4", | 7 | "id": "01e0dda9-5fcb-44a5-ada8-0474208b8cd4", | ||
8 | "isopen": false, | 8 | "isopen": false, | ||
9 | "license_title": null, | 9 | "license_title": null, | ||
10 | "metadata_created": "2025-03-10T20:27:32.825754", | 10 | "metadata_created": "2025-03-10T20:27:32.825754", | ||
n | 11 | "metadata_modified": "2025-03-10T20:27:32.825762", | n | 11 | "metadata_modified": "2025-03-10T20:27:33.549170", |
12 | "name": "2024_november_scint_data_lsbr", | 12 | "name": "2024_november_scint_data_lsbr", | ||
13 | "notes": "Data of GPS - SCINTILLATION DATA", | 13 | "notes": "Data of GPS - SCINTILLATION DATA", | ||
n | 14 | "num_resources": 0, | n | 14 | "num_resources": 13, |
15 | "num_tags": 0, | 15 | "num_tags": 0, | ||
16 | "organization": { | 16 | "organization": { | ||
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", | ||
31 | "id": "8ed10e33-fdf8-4b72-b5f0-4b7ead1a2fe2", | 31 | "id": "8ed10e33-fdf8-4b72-b5f0-4b7ead1a2fe2", | ||
32 | "image_url": | 32 | "image_url": | ||
33 | "2024-06-11-201248.169854Screenshot-from-2024-06-11-15-12-02.png", | 33 | "2024-06-11-201248.169854Screenshot-from-2024-06-11-15-12-02.png", | ||
34 | "is_organization": true, | 34 | "is_organization": true, | ||
35 | "name": "gnss", | 35 | "name": "gnss", | ||
36 | "state": "active", | 36 | "state": "active", | ||
37 | "title": "GNSS", | 37 | "title": "GNSS", | ||
38 | "type": "project" | 38 | "type": "project" | ||
39 | }, | 39 | }, | ||
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378 | "url": | ||||
379 | ca/database-cielo/base/gps/LISN/lsbr/2024/11/scint/lsbr_241128.s4.gz", | ||||
380 | "url_type": null, | ||||
381 | "voc_file_type": "Scintillation Data" | ||||
382 | } | ||||
383 | ], | ||||
45 | "state": "active", | 384 | "state": "active", | ||
46 | "tags": [], | 385 | "tags": [], | ||
47 | "title": "2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA", | 386 | "title": "2024 NOVEMBER SAN BARTOLOME SCINTILLATION DATA", | ||
48 | "type": "dataset", | 387 | "type": "dataset", | ||
49 | "voc_instrument_type": "Gnss", | 388 | "voc_instrument_type": "Gnss", | ||
50 | "voc_station_name": "San Bartolome" | 389 | "voc_station_name": "San Bartolome" | ||
51 | } | 390 | } |