Changes
On September 5, 2024 at 1:06:35 PM UTC,
ckancielo:
-
Changed value of field
dataset_end_date
to2015-11-17
in 2015 NOVEMBER TUPIZA OX -
Changed value of field
dataset_start_date
to2015-11-17
in 2015 NOVEMBER TUPIZA OX -
Added resource TZJ2J_2015321134411_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321134627_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321134718_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321135133_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321140332_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321135210_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321135037_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321140223_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321140302_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321135950_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321140153_OX.png to 2015 NOVEMBER TUPIZA OX
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Added resource TZJ2J_2015321140108_OX.png to 2015 NOVEMBER TUPIZA OX
| 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": "OX", | 3 | "data_type": "OX", | ||
| n | 4 | "dataset_end_date": "2200-01-01", | n | 4 | "dataset_end_date": "2015-11-17", |
| 5 | "dataset_start_date": "1900-01-01", | 5 | "dataset_start_date": "2015-11-17", | ||
| 6 | "groups": [], | 6 | "groups": [], | ||
| 7 | "id": "1e8b8204-5b9f-4d36-9817-4c4c348f7dda", | 7 | "id": "1e8b8204-5b9f-4d36-9817-4c4c348f7dda", | ||
| 8 | "isopen": false, | 8 | "isopen": false, | ||
| 9 | "license_title": null, | 9 | "license_title": null, | ||
| 10 | "metadata_created": "2024-09-05T13:06:34.342370", | 10 | "metadata_created": "2024-09-05T13:06:34.342370", | ||
| n | 11 | "metadata_modified": "2024-09-05T13:06:34.342398", | n | 11 | "metadata_modified": "2024-09-05T13:06:35.433988", |
| 12 | "name": "2015_november_ox_tupi", | 12 | "name": "2015_november_ox_tupi", | ||
| 13 | "notes": "Data of Ionosonde OX", | 13 | "notes": "Data of Ionosonde OX", | ||
| n | 14 | "num_resources": 0, | n | 14 | "num_resources": 12, |
| 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", | ||
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| 59 | "state": "active", | 372 | "state": "active", | ||
| 60 | "tags": [], | 373 | "tags": [], | ||
| 61 | "title": "2015 NOVEMBER TUPIZA OX", | 374 | "title": "2015 NOVEMBER TUPIZA OX", | ||
| 62 | "type": "dataset", | 375 | "type": "dataset", | ||
| 63 | "voc_instrument_type": "Ionosonde", | 376 | "voc_instrument_type": "Ionosonde", | ||
| 64 | "voc_station_name": "Tupiza" | 377 | "voc_station_name": "Tupiza" | ||
| 65 | } | 378 | } |