Changes
On June 18, 2024 at 4:57:54 PM UTC,
-
Changed value of field
dataset_start_date
to2013-05-02
in 2013 MAY JICAMARCA PWR -
Changed value of field
dataset_end_date
to2013-05-02
in 2013 MAY JICAMARCA PWR -
Added resource JM91J_2013122154120_PWR.png to 2013 MAY JICAMARCA PWR
f | 1 | { | f | 1 | { |
2 | "creator_user_id": "770631d3-fc59-4c0b-a34e-8ec37ebe30ec", | 2 | "creator_user_id": "770631d3-fc59-4c0b-a34e-8ec37ebe30ec", | ||
3 | "data_type": "PWR", | 3 | "data_type": "PWR", | ||
n | 4 | "dataset_end_date": "2200-01-01", | n | 4 | "dataset_end_date": "2013-05-02", |
5 | "dataset_start_date": "1900-01-01", | 5 | "dataset_start_date": "2013-05-02", | ||
6 | "groups": [], | 6 | "groups": [], | ||
7 | "id": "7122098d-7a3a-40f8-9976-45a500039c1b", | 7 | "id": "7122098d-7a3a-40f8-9976-45a500039c1b", | ||
8 | "isopen": false, | 8 | "isopen": false, | ||
9 | "license_title": null, | 9 | "license_title": null, | ||
10 | "metadata_created": "2024-06-18T16:57:54.355843", | 10 | "metadata_created": "2024-06-18T16:57:54.355843", | ||
n | 11 | "metadata_modified": "2024-06-18T16:57:54.355849", | n | 11 | "metadata_modified": "2024-06-18T16:57:54.858595", |
12 | "name": "2013_may_pwr_jica", | 12 | "name": "2013_may_pwr_jica", | ||
13 | "notes": "Data of Ionosonde - PWR DATA", | 13 | "notes": "Data of Ionosonde - PWR DATA", | ||
n | 14 | "num_resources": 0, | n | 14 | "num_resources": 1, |
15 | "num_tags": 0, | 15 | "num_tags": 0, | ||
16 | "organization": { | 16 | "organization": { | ||
17 | "approval_status": "approved", | 17 | "approval_status": "approved", | ||
18 | "created": "2024-06-07T21:05:19.808275", | 18 | "created": "2024-06-07T21:05:19.808275", | ||
19 | "description": "The ionosondes provide virtual height information | 19 | "description": "The ionosondes provide virtual height information | ||
20 | and density profile estimates from the bottomside ionosphere (also by | 20 | and density profile estimates from the bottomside ionosphere (also by | ||
21 | bistatic soundings) with a cadence as small as 1 min, and follow the | 21 | bistatic soundings) with a cadence as small as 1 min, and follow the | ||
22 | twilight and nighttime E-region to sounding frequencies of less than | 22 | twilight and nighttime E-region to sounding frequencies of less than | ||
23 | 0.5 MHz when implemented with suitable antennas. They also provide | 23 | 0.5 MHz when implemented with suitable antennas. They also provide | ||
24 | information about drifts, ionospheric tilts, and the \u201crms\u201d | 24 | information about drifts, ionospheric tilts, and the \u201crms\u201d | ||
25 | amplitude and spectral index of density fluctuations by a phase | 25 | amplitude and spectral index of density fluctuations by a phase | ||
26 | structure function method. Five ionosondes with co-located flux-gate | 26 | structure function method. Five ionosondes with co-located flux-gate | ||
27 | magnetometers will be placed equidistantly and nearly aligned with the | 27 | magnetometers will be placed equidistantly and nearly aligned with the | ||
28 | magnetic flux tube intersecting the magnetic equator at 70\u00b0 W. In | 28 | magnetic flux tube intersecting the magnetic equator at 70\u00b0 W. In | ||
29 | our plan, one ionosonde will be installed at Tabatinga, Brazil located | 29 | our plan, one ionosonde will be installed at Tabatinga, Brazil located | ||
30 | near Leticia, Colombia and another near Antofagasta, Chile, to observe | 30 | near Leticia, Colombia and another near Antofagasta, Chile, to observe | ||
31 | the E- and F-region densities. Field lines intersecting 100 km | 31 | the E- and F-region densities. Field lines intersecting 100 km | ||
32 | altitude over these two stations map to the equator at 250 and 260 km | 32 | altitude over these two stations map to the equator at 250 and 260 km | ||
33 | respectively. A third ionosonde will be placed very close to the | 33 | respectively. A third ionosonde will be placed very close to the | ||
34 | magnetic equator in Puerto Maldonado. Two more ionosonde will be | 34 | magnetic equator in Puerto Maldonado. Two more ionosonde will be | ||
35 | located at 19-20\u00b0 away from the magnetic equator, near the crest | 35 | located at 19-20\u00b0 away from the magnetic equator, near the crest | ||
36 | caused by the equatorial \u2018fountain\u2019. Data from all 5 | 36 | caused by the equatorial \u2018fountain\u2019. Data from all 5 | ||
37 | ionosonde, magnetic fields from the co-located magnetometers, TEC | 37 | ionosonde, magnetic fields from the co-located magnetometers, TEC | ||
38 | values from the nearby GPS receivers, and the Kalman filter-based | 38 | values from the nearby GPS receivers, and the Kalman filter-based | ||
39 | assimilation will provide several geophysical parameters (winds, | 39 | assimilation will provide several geophysical parameters (winds, | ||
40 | electric fields and densities) from the E and F regions, and will also | 40 | electric fields and densities) from the E and F regions, and will also | ||
41 | fill in the regions between the sites. This will be the first time | 41 | fill in the regions between the sites. This will be the first time | ||
42 | that a numerical model of the equatorial ionosphere can be fully | 42 | that a numerical model of the equatorial ionosphere can be fully | ||
43 | constrained by data collected on both sides of the magnetic equator | 43 | constrained by data collected on both sides of the magnetic equator | ||
44 | and for a range of altitudes that includes the E region", | 44 | and for a range of altitudes that includes the E region", | ||
45 | "id": "6d5f18bf-4b25-4e58-bfcc-8b011418f417", | 45 | "id": "6d5f18bf-4b25-4e58-bfcc-8b011418f417", | ||
46 | "image_url": | 46 | "image_url": | ||
47 | "2024-06-11-201428.563392Screenshot-from-2024-06-11-15-14-08.png", | 47 | "2024-06-11-201428.563392Screenshot-from-2024-06-11-15-14-08.png", | ||
48 | "is_organization": true, | 48 | "is_organization": true, | ||
49 | "name": "ionosonde", | 49 | "name": "ionosonde", | ||
50 | "state": "active", | 50 | "state": "active", | ||
51 | "title": "IONOSONDE", | 51 | "title": "IONOSONDE", | ||
52 | "type": "project" | 52 | "type": "project" | ||
53 | }, | 53 | }, | ||
54 | "owner_org": "6d5f18bf-4b25-4e58-bfcc-8b011418f417", | 54 | "owner_org": "6d5f18bf-4b25-4e58-bfcc-8b011418f417", | ||
55 | "private": false, | 55 | "private": false, | ||
56 | "relationships_as_object": [], | 56 | "relationships_as_object": [], | ||
57 | "relationships_as_subject": [], | 57 | "relationships_as_subject": [], | ||
t | 58 | "resources": [], | t | 58 | "resources": [ |
59 | { | ||||
60 | "cache_last_updated": null, | ||||
61 | "cache_url": null, | ||||
62 | "created": "2024-06-18T16:57:54.871572", | ||||
63 | "datastore_active": false, | ||||
64 | "file_date": "2013-05-02", | ||||
65 | "format": "PNG", | ||||
66 | "hash": "", | ||||
67 | "id": "fc5d86b5-aad1-4b8a-bec0-b0fa8379cbbe", | ||||
68 | "last_modified": null, | ||||
69 | "metadata_modified": "2024-06-18T16:57:54.865528", | ||||
70 | "mimetype": "image/png", | ||||
71 | "mimetype_inner": null, | ||||
72 | "name": "JM91J_2013122154120_PWR.png", | ||||
73 | "others": [], | ||||
74 | "package_id": "7122098d-7a3a-40f8-9976-45a500039c1b", | ||||
75 | "position": 0, | ||||
76 | "private": false, | ||||
77 | "resource_type": null, | ||||
78 | "size": null, | ||||
79 | "state": "active", | ||||
80 | "url": | ||||
81 | ielo/base/ionosonde/JM91J/2013/05/02/PWR/JM91J_2013122154120_PWR.png", | ||||
82 | "url_type": null, | ||||
83 | "voc_file_type": "PWR" | ||||
84 | } | ||||
85 | ], | ||||
59 | "state": "active", | 86 | "state": "active", | ||
60 | "tags": [], | 87 | "tags": [], | ||
61 | "title": "2013 MAY JICAMARCA PWR", | 88 | "title": "2013 MAY JICAMARCA PWR", | ||
62 | "type": "dataset", | 89 | "type": "dataset", | ||
63 | "voc_instrument_type": "Ionosonde", | 90 | "voc_instrument_type": "Ionosonde", | ||
64 | "voc_station_name": "Jicamarca" | 91 | "voc_station_name": "Jicamarca" | ||
65 | } | 92 | } |