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=========================================
UNITOV Catalogue of geoeffective CMEs
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
UNITOV Catalogue of geoeffective CMEs
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
A database associating L1 Time of Arrival and Speed of an interplanetary CME to the kinematic characteristics of the corresponding CME, covering the period 1996-2020.
Data Description
----------------
| **Data type**: tableset
| **Data formats**: - csv
| **Version**: v2.1
Data Provider
---------------
Data are collected by the following instruments:
- **SDO** - source:
- AIA
- **SOHO** - source:
- LASCO
- **Richardson & Cane CME List**
- **ACE**
Data Relationships
-----------------
- type: related-to
- description: P-DBM model can ingest part of the table to simulate the ICME propagation
- relatedproduct: UNITOV-PDBM
- relatedproductid: aspis:/unitov/p-dbm
.
Data are ND with - type: related-to
- description: P-DBM model can ingest part of the table to simulate the ICME propagation
- relatedproduct: UNITOV-PDBM
- relatedproductid: aspis:/unitov/p-dbm
marked as id: - type: related-to
- description: P-DBM model can ingest part of the table to simulate the ICME propagation
- relatedproduct: UNITOV-PDBM
- relatedproductid: aspis:/unitov/p-dbm
- :ref:`- type: related-to
- description: P-DBM model can ingest part of the table to simulate the ICME propagation
- relatedproduct: UNITOV-PDBM
- relatedproductid: aspis:/unitov/p-dbm
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Corona
- Interplanetary Space (not L1 and Planets)
- Sun-Earth L1
| **Temporal** - time_start: 1997-01-01T00:00:00+01:00
- time_stop: 2019-12-31T23:59:00+01:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-08T11:24:13+02:00
| **Last Update**: 2022-04-08T11:25:24+02:00
Data Policy
--------------
This product contains public data. Other.
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
IAPS Test Particle Simulation on Magnetic Clouds
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
IAPS Test Particle Simulation on Magnetic Clouds
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Galactic cosmic ray intensity variations associated to the passage of magnetic clouds. The particle intensity variation is estimated through a dedicated full-orbit test-particle simulation.
Data Description
----------------
| **Data type**: spectral-cubes
| **Data formats**: - mat
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
- **Solar Modulation Parameter Table Oulu NM** - source:
- https://cosmicrays.oulu.fi/phi/phi.html
- **Grad-Shafranov reconstruction maps** - source:
- in ASPIS
Data Relationships
-----------------
- type: related-to
- description: Test-Particle Simulation on magnetic clouds
.
Data are ND with - type: related-to
- description: Test-Particle Simulation on magnetic clouds
marked as id: - type: related-to
- description: Test-Particle Simulation on magnetic clouds
- :ref:`- type: related-to
- description: Test-Particle Simulation on magnetic clouds
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Interplanetary Space (not L1 and Planets)
- Sun-Earth L1
| **Temporal** - time_start: 1997-01-01T00:00:00+01:00
- time_stop: 2022-01-01T00:00:00+01:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-26T12:00:39+02:00
| **Last Update**: 2022-04-26T12:00:50+02:00
Data Policy
--------------
This product contains public data. Other.
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
IAPS Test Particle Simulation on Magnetic Clouds
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
IAPS Test Particle Simulation on Magnetic Clouds
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Visualization of the galactic cosmic ray intensity variations associated to the passage of magnetic clouds.
Data Description
----------------
| **Data type**: image
| **Data formats**: - m
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
- **Particle intensity variation maps** - source:
- in ASPIS
Data Relationships
-----------------
- type: related-to
- description: Test-Particle Simulation on magnetic clouds
.
Data are ND with - type: related-to
- description: Test-Particle Simulation on magnetic clouds
marked as id: - type: related-to
- description: Test-Particle Simulation on magnetic clouds
- :ref:`- type: related-to
- description: Test-Particle Simulation on magnetic clouds
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Interplanetary Space (not L1 and Planets)
- Sun-Earth L1
| **Temporal** - time_start: 1997-01-01T00:00:00+01:00
- time_stop: 2022-01-01T00:00:00+01:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-26T12:00:39+02:00
| **Last Update**: 2022-04-26T12:00:50+02:00
Data Policy
--------------
This product contains public data. Other.
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
INAF-bidimensional maps of Mercury Na exosphere
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
INAF-bidimensional maps of Mercury Na exosphere
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Dataset of observations of Mercury's exosphere in the sodium D lines. Data are taken from the ground-based solar telescope THEMIS (years 2009-2013). They have been produced in both D1 and D2 lines (when both available) and converted into bi-dimensional maps of Rayleigh emission. Estimation of the “seeing” parameter is included in the jpeg files. Here the original fits files are given too for the whole database (2007-2014), and it may be expanded to the most recent data from 2021 and 2022 (TBC). Data can be provided both uncalibrated and/or calibrated (TBD).
Data Description
----------------
| **Data type**: spectral-cubes
| **Data formats**: - fts
| **Version**: v1.1
Data Provider
---------------
Data are collected by the following instruments:
- **THEMIS solar telescope **
Data Relationships
-----------------
- type: related-to
- relatedproductid: aspis://inaf/mercna
- description: bi-dimensional maps
.
Data are ND with - type: related-to
- relatedproductid: aspis://inaf/mercna
- description: bi-dimensional maps
marked as id: - type: related-to
- relatedproductid: aspis://inaf/mercna
- description: bi-dimensional maps
- :ref:`- type: related-to
- relatedproductid: aspis://inaf/mercna
- description: bi-dimensional maps
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Mercury
| **Temporal** - time_start: 2009-04-17T12:10:42+02:00
- time_stop: 2013-05-25T19:00:33+02:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-29T17:15:42+02:00
| **Last Update**: 2022-05-06T17:47:07+02:00
Data Policy
--------------
This product contains mixed data. TBD (this point needs to be decided together with the THEMIS telescope and the CNRS that should own the orignal data).
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
INAF-bidimensional maps of Mercury Na exosphere
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
INAF-bidimensional maps of Mercury Na exosphere
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Dataset of observations of Mercury's exosphere in the sodium D lines. Data are taken from the ground-based solar telescope THEMIS (years 2009-2013). They have been analyzed in both D1 and D2 lines (when both available) and converted into bi-dimensional maps of Rayleigh emission. Estimation of the “seeing” parameter is included in the jpeg files..
Data Description
----------------
| **Data type**: image
| **Data formats**: - jpg
| **Version**: v1.1
Data Provider
---------------
Data are collected by the following instruments:
- **THEMIS solar telescope **
Data Relationships
-----------------
- type: related-to
- relatedproductid: aspis://inaf/mercnafts
- description: original data-cube with the spectra
.
Data are ND with - type: related-to
- relatedproductid: aspis://inaf/mercnafts
- description: original data-cube with the spectra
marked as id: - type: related-to
- relatedproductid: aspis://inaf/mercnafts
- description: original data-cube with the spectra
- :ref:`- type: related-to
- relatedproductid: aspis://inaf/mercnafts
- description: original data-cube with the spectra
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Mercury
| **Temporal** - time_start: 2009-04-17T12:10:42+02:00
- time_stop: 2013-05-25T19:00:33+02:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-29T17:15:42+02:00
| **Last Update**: ND
Data Policy
--------------
This product contains mixed data. TBD.
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
Simulated Maps of SW Flux at the Surface of Mercury
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
Simulated Maps of SW Flux at the Surface of Mercury
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Simulated flux maps of SW precipitating onto the surface of Mercury for a subset of IMF condition, with surface resolution of 1° (LAT/LON) and IMF binning of 5 nT (from -20 to 20 nT)
Data Description
----------------
| **Data type**: image
| **Data formats**: - PNG
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
Missing providers
Data Relationships
-----------------
ND.
Data are ND with ND marked as id: ND - :ref:`ND`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Mercury
| **Temporal** - time_start: 2008-12-01T00:00:57+01:00
- time_stop: 2021-12-01T00:00:42+01:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-05-04T16:00:00+02:00
| **Last Update**: 2022-05-04T16:00:00+02:00
Data Policy
--------------
This product contains public data. Results will be publicly available.
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
IAPS > M2 SXR Flare Catalogue
~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
IAPS > M2 SXR Flare Catalogue
~~~~~~~~~~~~~~~~~~~~~~~~~~~~
The catalogue will contain the > M2 Soft X- Ray (SXR) flares from 1995 to 2017. The columns in the table are defined as follows: (1) event number; (2) date of the SXR flare; (3) peak time of SXR flare; (4) peak SXR classification (saturated events flagged with an S in which case (3) refers to the onset of saturation); (5) flare location; (6) time-integrated SXR intensity (nominally between the 1/3 power points on rise and fall); (7) time-integrated 1 MHz Wind/WAVES intensity from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak; (8) Waves frequency used.
Data Description
----------------
| **Data type**: tableset
| **Data formats**: - xlsx
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
- **GOES** - sources:
- 1-8 Å soft X-ray flux
- http://www.ngdc.noaa.gov/stp/satellite/goes/dataaccess.html
- **Wind** - sources:
- Waves 1 MHz radio flux
- ftp://solar-radio.gsfc.nasa.gov/
Data Relationships
-----------------
- type: related-to
- description: > M2 SXR Flare Catalogue
.
Data are ND with - type: related-to
- description: > M2 SXR Flare Catalogue
marked as id: - type: related-to
- description: > M2 SXR Flare Catalogue
- :ref:`- type: related-to
- description: > M2 SXR Flare Catalogue
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Interplanetary Space (not L1 and Planets)
- Sun-Earth L1
| **Temporal** - time_start: 1995-01-01T00:00:00+01:00
- time_stop: 2017-07-01T00:00:00+02:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-26T12:00:39+02:00
| **Last Update**: 2022-04-26T12:00:50+02:00
Data Policy
--------------
This product contains public data. Other.
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
Preliminary L'Aquila magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
Preliminary L'Aquila magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at L'Aquila magnetic observatory (IAGA code: AQU; Latitude: 42.383000°; Longitude: 13.316000°; Altitude: 682.000 m). In detail, preliminary "pseudo" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies.
Data Description
----------------
| **Data type**: timeseries
| **Data formats**: - json
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
- **INGV** - source:
- Magnetometer
Data Relationships
-----------------
- type: related-to
- relatedproduct: L'Aquila GIC index
- relatedproductid: AQUGIC
- description: GIC index is calculated for both X and Y components
.
Data are ND with - type: related-to
- relatedproduct: L'Aquila GIC index
- relatedproductid: AQUGIC
- description: GIC index is calculated for both X and Y components
marked as id: - type: related-to
- relatedproduct: L'Aquila GIC index
- relatedproductid: AQUGIC
- description: GIC index is calculated for both X and Y components
- :ref:`- type: related-to
- relatedproduct: L'Aquila GIC index
- relatedproductid: AQUGIC
- description: GIC index is calculated for both X and Y components
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Earth's Ground
| **Temporal** - time_start: 2017-01-01T00:00:00+01:00
- time_stop: 2022-04-21T00:00:00+02:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-21T18:15:32+02:00
| **Last Update**: 2022-04-21T18:15:00+02:00
Data Policy
--------------
This product contains public data. Access to the preliminary data, consisting of one-minute averaged values, is provided for general purposes. Acknowledgement of the INGV Geomagnetism Program in all published documents which make use of our data is requested. .
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
Preliminary Castello Tesino magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
Preliminary Castello Tesino magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino (TN) magnetic observatory (IAGA code: CTS; Latitude: 46.047000°; Longitude: 11.649000°; Altitude: 1175.000 m). In detail, preliminary \"pseudo\" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available.
Data Description
----------------
| **Data type**: timeseries
| **Data formats**: - json
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
- **INGV** - source:
- Magnetometer
Data Relationships
-----------------
- type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
.
Data are ND with - type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
marked as id: - type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
- :ref:`- type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Earth's Ground
| **Temporal** - time_start: 2017-01-01T00:00:00+01:00
- time_stop: 2022-04-21T00:00:00+02:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-21T18:15:32+02:00
| **Last Update**: 2022-04-21T18:15:00+02:00
Data Policy
--------------
This product contains public data. Access to the preliminary data, consisting of one-minute averaged values, is provided for general purposes. Acknowledgement of the INGV Geomagnetism Program in all published documents which make use of our data is requested..
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
Definitive Castello Tesino magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
Definitive Castello Tesino magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino magnetic observatory (IAGA code: CTS; Latitude: 46.047000°; Longitude: 11.649000°; Altitude: 1175.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly.
They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies.
Data Description
----------------
| **Data type**: timeseries
| **Data formats**: - json
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
- **INGV** - source:
- Magnetometer
Data Relationships
-----------------
- type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
.
Data are ND with - type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
marked as id: - type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
- :ref:`- type: related-to
- description: GIC index is calculated for both X and Y components
- relatedproduct: Castello Tesino GIC index
- relatedproductid: CTSGIC
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Earth's Ground
| **Temporal** - time_start: 2017-01-01T00:00:00+01:00
- time_stop: 2020-12-31T00:00:00+01:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-21T18:15:32+02:00
| **Last Update**: 2022-04-21T18:15:00+02:00
Data Policy
--------------
This product contains public data. Access to the preliminary data, consisting of one-minute averaged values, is provided for general purposes. Acknowledgement of the INGV Geomagnetism Program in all published documents which make use of our data is requested. .
Example
------------
Example is not yet provided .
\ No newline at end of file
=========================================
Preliminary Dome C magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
=========================================
.. sectnum::
.. contents:: The tiny table of contents
Preliminary Dome C magnetic data
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Dome C magnetic observatory(AGA code: DMC; Latitude: -75.250000°; Longitude: 124.167000°; Altitude: 3250.000 m). In detail, preliminary "pseudo" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies.
Data Description
----------------
| **Data type**: timeseries
| **Data formats**: - json
| **Version**: ND
Data Provider
---------------
Data are collected by the following instruments:
- **INGV** - source:
- Magnetometer
Data Relationships
-----------------
.
Data are ND with marked as id: - :ref:``
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Earth's Ground
| **Temporal** - time_start: 2011-11-05T00:00:00+01:00
- time_stop: 2019-06-13T00:00:00+02:00
| **Spectral** range: ND ND - ND ND
Product Status
---------------
| **Status**: Active
| **Creation date**: 2022-04-21T18:45:00+02:00
| **Last Update**: 2022-04-21T18:45:00+02:00
Data Policy
--------------
This product contains public data. Access to the preliminary data, consisting of one-minute averaged values, is provided for general purposes. Acknowledgement of the INGV Geomagnetism Program in all published documents which make use of our data is requested. .
Example
------------
Example is not yet provided .
\ No newline at end of file
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