id | product | Short description | category * (data/software/documents/etc.) | scientific cases ** | functionalities *** |
1 | Full-disk LoS magnetic and velocity maps | Full-disk LoS magnetic and velocity data from TSST (Tor Vergata Synoptic Solar Telescope) TSST is managed by UNITOV. | Calibrated data – Lev3
Visualization codes
Documentation and Metadata
| I. (WP1110, WP1130) | Internal: int2130.1 I. int2320.2 I. External: ext2220.1 I. ext2220.2 I. ext2220.3 I. ext2220.4 I. ext2230.1 I. ext2230.2 I. ext2230.3 I. ext2330.1 I. |
2 | H-alpha images from the TSST | Full-disk images of the Sun (656.300 +- 0.04 nm) | Calibrated data – Lev1
Visualization codes
Documentation and Metadata | I. (WP1120, WP1130) | Internal: int2130.1 I. int2320.2 I. External: ext2220.1 I. ext2220.2 I. ext2220.3 I,. ext2230.1 I. ext2230.2 I. ext2230.3 I. ext2330.1 I. |
3 | R and D parameters and flare (M- and X-class) probability | Morphological and topological describers of Active Region PIL. These feature can be used to estimate the M- and X-class flare probability 24h in advance | Derived Data
Visualization codes
Documentation and Metadata | I., II. (WP1120, WP1130) | Internal: int2130.1 I., II. int2320.2 I., II. External: ext2220.1 I., II. ext2220.2 I., II. ext2220.3 I., II. ext2230.1 I., II. ext2230.2 I., II. ext2230.3 I., II. ext2330.1 I., II. |
4 | Sunspots Zurich and McIntosh class | Automated determination of the sunspots Zurich and McIntosh class, using real-time and archival (last 3 years) OACT continuum images with a spatial resolution of 2 arcsec and a cadence of 1 image per day. | Derived data
data analysis codes
Visualization codes
Documentation and Metadata | I. (WP1120) | Internal: int2130.1 I. int2130.4 I. int2320.1 I. int2320.2 I. External: ext2220.1 I. ext2220.2 I. ext2220.3 I. ext2230.1 I. ext2230.2 I. ext2230.3 I. ext2330.1 I.
|
5 | Facular area in chromosphere and geometrical characteristics of filaments on the disk | Automated determination of the facular area and of the filaments geometrical characteristics using OACT H-alpha real-time and archival (last 3 years) images with a spatial resolution of 2 arcsec and a cadence of 10 min for the archival data and 1 min for real-time data. | Derived data
data analysis codes
Visualization codes
Documentation and Metadata | I. (WP1120) | Internal: int2130.1 I. int2130.4 I. int2320.1 I. int2320.2 I. External: ext2220.1 I. ext2220.2 I. ext2220.3 I. ext2230.1 I. ext2230.2 I. ext2230.3 I. ext2330.1 I.
|
6 | Geometry and location of prominences on the solar limb
| Automated determination of the geometry and location of prominences on the solar limb using real-time OACT H-alpha images with a spatial resolution of 2 arcsec and a cadence of 1 image/day. | Derived data data analysis codes
Visualization codes
Documentation and Metadata | I. (WP1120) | Internal: int2130.1 I. int2320.1 I. int2130.4 I. int2320.2 I. External: ext2220.1 I. ext2220.2 I. ext2220.3 I. ext2230.1 I. ext2230.2 I. ext2230.3 I. ext2330.1 I. |
7 | ≥M2 SXR flare catalogue | The catalogue will contain the ≥M2 SXR flares from 1995 including occurrence date and time, flare features, SXR fluence and radio fluence | Derived data
Visualization codes
Documentation and Metadata | I., II. (WP1130, WP1210) | Internal: int2130.1 I.,II. int2320.2 I.,II. External: ext2220.1 I.,II. ext2220.2 I.,II. ext2220.3 I.,II. ext2230.1 I.,II. ext2230.2 I.,II. ext2230.3 I.,II. ext2330.1 I.,II. |
8 | Geomagnetic field data from ground-based observatories | 1-minute averages of the magnetic field variations at the geomagnetic ground observatories in Italy (Castello Tesino from May 2017; L’Aquila from January 2017; Duronia from January 2017; Lampedusa from April 2017) and Antarctica (Baia di Terranova from January 201; Dome C from December 2020), managed by INGV. | Calibrated data – Lev2
data analysis code
Visualization codes
Documentation and Metadata | II., III. (WP1330, WP1710) | Internal: int2130.1 II., III. int2130.2 II., III. int2130.4 II., III. int2320.2 II., III. External: ext2220.1 II., III. ext2220.2 II., III. ext2220.3 II., III. ext2220.4 II., III. ext2230.1 II., III. ext2230.2 II., III. ext2230.3 II., III. ext2330.1 II., III. |
9 | Geomagnetic field data from ground-based observatories | 1-minute averages of the magnetic field variations at the geomagnetic ground observatories in the INTERMAGNET network and World Data Center for Geomagnetism | Calibrated data – Lev2
Visualization codes
Documentation and Metadata | II., III. (WP1330, WP1710) | Internal: int2130.1 II., III. int2130.2 II., III. int2320.1 II., III. int2320.2 II., III. External: ext2220.1 II., III. ext2220.2 II., III. ext2220.3 II., III. ext2230.1 II., III. ext2230.2 II., III. ext2230.3 II., III. ext2330.1 II., III. |
10 | Geomagnetic field data from EMMA ground-based observatories | 1-minute averages of the magnetic field variations recorded at 27 ground stations located in Italy and Europe along a meridional chain covering a large range in geographical latitude (from 70o to 42o). The data are automatically collected in near real-time and updated every 15 minutes. | Calibrated data
Visualization codes
Documentation and Metadata | II., III. (WP1330) | Internal: int2130.1 II., III. int2130.2 II., III. int2130.4 II., III. int2320.1 II., III. int2320.2 II., III. External: ext2220.1 II., III. ext2220.2 II., III. ext2220.3 II., III. ext2220.4 II., III. ext2230.1 II., III. ext2230.2 II., III. ext2230.3 II., III. ext2330.1 II., III. |
11 | 5-minutes forecasting model of the SYM-H geomagnetic index | Forecasting of the geomagnetic SYM-H index 1 hour in advance and with a cadence of 5 minutes by using an Artificial Neural Networks model | Model output
Visualization codes
Documentation and Metadata | II., III. (WP1330) | Internal: int2130.1 II., III. int2130.4 II., III. int2320.1 II., III. int2320.2 II., III. External: ext2220.1 II., III. ext2220.2 II., III. ext2220.3 II., III. ext2220.4 II., III. ext2230.1 II., III. ext2230.2 II., III. ext2230.3 II., III. ext2330.1 II., III. |
12 | Ionospheric ionosonde data | 15-minutes ionospheric physical parameters from ionosondes in Italy (Rome from 2005; Gibilmanna from 2003) and Argentina (Tucuman from 2007; Bahia Blanca from 2016), managed by INGV. | Calibrated data – Lev2
Visualization codes
Documentation and Metadata | IV. (WP1410) | Internal: int2130.1 IV. int2130.2 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2220.4 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
13 | Ionospheric ionosonde data | 1-hour validated ionospheric physical parameters from ionosondes in Italy (Rome from 1976, and Gibilmanna from 1976), managed by INGV | Calibrated data – Lev2.5
Visualization codes
Documentation and Metadata | IV. (WP1410) | Internal: int2130.1 IV. int2130.2 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
14 | SWA data | Density, velocity and temperature of protons in solar wind. Resolution: between 0.25 s and 4 s. Source: Solar Orbiter Archive
| Calibrated data Visualization codes
Documentation and Metadata | II. (WP1220) | Internal: int2130.1 II. int2130.3 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II. |
15 | 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. | Derived data
Visualization codes
Documentation and Metadata | II. (WP1220) | Internal: int2130.1 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II. |
16 | SEP catalogue | The catalogue will contain SEP events observed at the Earth with flux ≥ 10 pfu at > 10 MeV from 1995, including features of the associated flare | Derived data Visualization codes
Documentation and Metadata | II., VII. (WP1210, WP1720) | Internal: int2130.1 II., VII. int2320.1 II., VII. int2320.2 II., VII. External: ext2220.1 II., VII. ext2220.2 II., VII. ext2220.3 II., VII. ext2230.1 II., VII. ext2230.2 II., VII. ext2230.3 II., VII. ext2330.1 II., VII. |
17 | GLE catalogue | The catalogue will contain GLEs from 1995 observed by neutron monitors | Derived data Visualization codes
Documentation and Metadata | II., VI., VII. (WP1210, WP1610, WP1720) | Internal: int2130.1 II., VI., VII. int2320.1 II., VI., VII. int2320.2 II., VI., VII. External: ext2220.1 II., VI., VII. ext2220.2 II., VI., VII. ext2220.3 II., VI., VII. ext2230.1 II., VI., VII. ext2230.2 II., VI., VII. ext2230.3 II, VI, VII ext2330.1 II, VI, VII |
18 | LOFAR radio flux | It is derived after merging the LOFAR radio data to cover most part of a day at frequencies of 30 MHz | Derived data Visualization codes
Documentation and Metadata | I., II. (WP1130, 1210) | Internal: int2130.1 I., II. int2130.2 I., II. int2320.1 I., II. int2320.2 I., II. External: ext2220.1 I., II. ext2220.2 I., II. ext2220.3 I., II. ext2230.1 I., II. ext2230.2 I., II. ext2230.3 I., II. ext2330.1 I., II.
|
19 | SEP\GLE primary spectrum | The GLE spectrum at the top of the atmosphere is obtained by modelling the neutron monitor response to an anisotropic SEP flux, registered during a GLE event, and solving the inverse problem | Model output Visualization codes
Documentation and Metadata | II.,VI. (WP1210, WP1610) | Internal: int2130.1 II. VI. int2320.1 II. VI. int2320.2 II. VI. External: ext2220.1 II. VI. ext2220.2 II. VI. ext2220.3 II. VI. ext2220.5 II. VI. ext2230.1 II. VI. ext2230.2 II. VI. ext2230.3 II. VI. ext2330.1 II. VI. |
20 | SEP spectra | Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft) | Derived data Visualization codes
Documentation and Metadata | II. (WP1210) | Internal: int2130.1 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II. |
21 | ESP spectra | Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft); 3) from 2009 for STEREO A data. | Derived data Visualization codes
Documentation and Metadata | II. (WP1210) | Internal: int2130.1 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II. |
22 | Parameters of shocks associated with SEP and ESP events
| Magnetosonic Mach number, angle between the magnetic field and the normal to the shock surface, plasma beta for: 1) geoeffective target events (at L1) and; 2) widespread target events (at different heliographic locations from multiple spacecraft); 3) from 2009 for STEREO A data.
| Derived data Visualization codes
Documentation and Metadata | II. (WP1220) | Internal: int2130.1 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II.
|
23 | Turbulence and intermittency data nearby IP shocks
| Power spectral densities of the magnetic field, magnetic field structure functions exponents. These data will be obtained from WIND and ACE spacecraft measurements for geoeffective target SWE events; from STEREO, PSP, SolO, and Bepicolombo spacecraft measurements for widespread target SWE events.
| Derived data Visualization codes
Documentation and Metadata | II. (WP1220) | Internal: int2130.1 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II. |
24 | Velocity-magnetic field correlation coefficient data of solar wind streams
| Computed at tenth of min scale from plasma and magnetic field data of STEREO, WIND, ACE, PSP SolO, Bepicolombo spacecraft | Derived data Visualization codes
Documentation and Metadata | II. (WP1220) | Internal: int2130.1 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II. |
25 | Grad-Shafranov reconstruction of magnetic clouds
| Quasi 3-d magnetic field maps of magnetic field configuration within magnetic clouds for geoeffective target SWE events. Such maps will be estimated through the Grad-Shafranov reconstruction from single-spacecraft plasma and magnetic field data | Derived data Visualization codes
Documentation and Metadata | II. (WP1220) | Internal: int2130.1 II. int2320.1 II. int2320.2 II. External: ext2220.1 II. ext2220.2 II. ext2220.3 II. ext2230.1 II. ext2230.2 II. ext2230.3 II. ext2330.1 II. |
26 | Quality index of the Walèn test for reconnection at the magnetopause
| The Walén test quality index is derived from the density, velocities and magnetic field measurements of Cluster, MMS and Themis during magnetopause crossings | Derived data
Data Analysis code
Visualization codes
Documentation and Metadata | III. (WP1310) | Internal: int2130.1 III. int2130.4 III. int2320.1 III. int2320.2 III. External: ext2220.1 III. ext2220.2 III. ext2220.3 III ext2220.4 III. ext2230.1 III. ext2230.2 III. ext2230.3 III. ext2230.4 III. ext2330.1 III. |
27 | Magnetosheath parameters | Ratio of the local velocity, density, and temperature with respect to the unperturbed upstream SW values at the magnetospheric nose and flanks
| Model Output
Visualization codes
Documentation and Metadata | III. V. (WP1310, WP1510) | Internal: int2130.1 III. V. int2320.1 III. V. int2320.2 III. V. External: ext2220.1 III. V. ext2220.2 III. V. ext2220.3 III. V. ext2230.1 III. V. ext2230.2 III. V. ext2230.3 III. V. ext2330.1 III. V. |
28 | Maps of maximum usable frequency (MUF) and skip distance | MUF and skip distance will be derived from ionosonde data centred over Milan, Rome, Catania and Cagliari with 1°x1° spatial resolution. Long-term maps will be generated with 1-hour resolution, while nowcasting maps will be generated with 15-minutes resolution. | Derived data
Data Analysis code
Visualization codes
Documentation and Metadata | IV. (WP1410) | Internal: int2130.1 IV. int2130.4 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2220.4 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2230.4 IV. ext2330.1 IV. |
29 | Equatorial plasma mass density estimates in plasmasphere (2 < L < 6)
| Equatorial plasma mass density estimates in plasmasphere (2 < L < 6) are derived from the the EMMA magnetometers network, updated every 15 minutes. | Derived data
Visualization codes
Documentation and Metadata | III. (WP1330) | Internal: int2130.1 III. int2130.4 III. int2320.1 III. int2320.2 III. External: ext2220.1 III. ext2220.2 III. ext2220.3 III. ext2220.4 III. ext2230.1 III. ext2230.2 III. ext2230.3 III. ext2330.1 III. |
30 | SuperDARN convection maps
| Ionospheric convection maps at high latitudes in both hemispheres derived from the raw SuperDARN data retrieved from the BAS repository or from models based on historical series of SuperDARN observations | Derived data
Visualization codes
Documentation and Metadata | IV. (WP1410) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
31 | Cross Polar Cap Potential | maximum potential difference measured through the polar caps
| Derived data
Visualization codes
Documentation and Metadata | IV. (WP1410) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
32 | Global maps of ionospheric indices | RODI, ROTEI and ROTI ionospheric indices derived from the Swarm constellation from 2014 | Derived data
Visualization codes
Documentation and Metadata
| IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
33 | 1 Hz on track values and global maps of electron density | In situ electron density derived from the Swarm constellation from 2014 to 2020
| Derived data
Visualization codes
Documentation and Metadata
| IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
34 | 1 Hz on track values and global maps of electron temperature | In situ electron temperature derived from the Swarm constellation from 2014 to 2020
| Derived data
Visualization codes
Documentation and Metadata
| IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
35 | 1 Hz on track values and global maps of vector geomagnetic field | In situ vector geomagnetic field derived from the Swarm constellation from 2014 to 2020
| Derived data
Visualization codes
Documentation and Metadata
| IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
36 | 1 Hz on track values and global maps of external vector geomagnetic field | In situ external vector geomagnetic field derived from the Swarm constellation from 2014 to 2020
| Derived data
Visualization codes
Documentation and Metadata | IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
37 | 1 Hz on track values and global maps of external parallel and perpendicular geomagnetic field components | In situ external vector geomagnetic field decomposed in directions parallel and perpendicular to the main field derived from the Swarm constellation from 2014 to 2020
| Derived data
Visualization codes
Documentation and Metadata
| IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
38 | 1 Hz on track values and global maps of parallel electrical conductivity | In situ parallel electrical conductivity derived from the Swarm constellation from 2014 to 2020 Available in full cadence, seasonal and yearly averages, and grouped by different geomagnetic activity levels | Derived data
Visualization codes
Documentation and Metadata | IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
39 | P-DBM model
| The CME propagation is modeled by using probability distribution functions. This allows us to evaluate the ICME arrival times and velocities along with the uncertainties on the forecast.
| Model codes Visualization codes
Documentation and Metadata | II., III., V. (WP1220, WP1310,WP1510) | Internal: int2130.1 II., III., V. int2130.4 II., III., V. int2320.2 II., III., V. External: ext2220.1 II., III., V. ext2220.3 II., III., V. ext2220.5 II., III., V. ext2230.1 II., III., V. ext2230.3 II., III., V. ext2230.4 II., III., V. ext2330.1 II., III., V. |
40 | MA.I.GIC. model: time series and maps of current intensity | Evaluation of the ionospheric and magnetospheric current system via the application of the MA.I.GIC. model from geomagnetic observations | Model output
Visualization codes
Documentation and Metadata | III., IV. (WP1330, WP 1420) | Internal: int2130.1 III., IV. int2320.1 III., IV. int2320.2 III., IV. External: ext2220.1 III., IV. ext2220.2 III., IV. ext2220.3 III., IV. ext2220.5 III., IV. ext2230.1 III., IV. ext2230.2 III, IV. ext2230.3 III., IV. ext2330.1 III., IV. |
41 | MA.I.GIC. model: time series and maps of geoelectric field | Evaluation of the Geoelectric field for the correct calculation of the geomagnetically induced current via the application of the MA.I.GIC. model | Derived data
Visualization codes
Documentation and Metadata | III., VII. (WP1330,WP1710) | Internal: int2130.1 III.,VII. int2320.1 III.,VII. int2320.2 III.,VII. External: ext2220.1 III.,VII. ext2220.2 III.,VII. ext2220.3 III.,VII. ext2220.5 III.,VII. ext2230.1 III.,VII. ext2230.2 III.,VII. ext2230.3 III.,VII. ext2330.1 III.,VII. |
42 | Rome neutron monitor (called SVIRCO) data | Pressure corrected nucleonic intensity and barometric pressure data with time resolution of:
-1min from 2007 and in real time; -1hr from1966; -2hr from 1957 to 1965. SVIRCO is managed by INAF. | Calibrated data – Lev2
Visualization codes
Documentation and Metadata | II., VI. (WP1210,WP1610, WP1620)
| Internal: int2130.1 II., VI. int2130.2 II., VI. int2320.1 II., VI. int2320.2 II., VI. External: ext2220.1 II., VI. ext2220.2 II., VI. ext2220.3 II., VI. ext2220.4 II., VI. ext2230.1 II., VI. ext2230.2 II., VI. ext2230.3 II., VI. ext2330.1 II., VI. |
43 | Testa Grigia neutron monitor data | Pressure corrected nucleonic intensity and barometric pressure data with time resolution of:
5 min and hourly from 2015
daily and monthly averaged data from 2015. The Testa grigia neutron monitor is managed by INAF
| Calibrated data – Lev2
Visualization codes
Documentation and Metadata | II., VI. (WP1210, WP1610) | Internal: int2130.1 II., VI. int2130.2 II., VI. int2320.1 II., VI. int2320.2 II., VI. External: ext2220.1 II, VI. ext2220.2 II., VI. ext2220.3 II., VI. ext2220.4 II., VI. ext2230.1 II., VI. ext2230.2 II., VI. ext2230.3 II., VI. ext2330.1 II., VI. |
44 | CSES satellite particle flux data | Evaluation of the quasi-linear diffusion coefficients related to non-adiabatic regime particle accelerations in the inner magnetosphere | Derived data
Visualization codes
Documentation and Metadata | III., IV. (WP1320, WP1420) | Internal: int2130.1 III., IV. int2320.1 III., IV. int2320.2 III., IV. External: ext2220.1 III., IV. ext2220.2 III., IV. ext2220.3 III., IV. ext2230.1 III., IV. ext2230.2 III., IV. ext2230.3 III., IV. ext2330.1 III., IV. |
45 | CSES satellite plasma data | On-track time series and maps of electron density and temperature | Derived data
Visualization codes
Documentation and Metadata | IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
46 | CSES satellite electric field and magnetic field data | On-track time series and maps of vector magnetic and electric fields | Derived data
Visualization codes
Documentation and Metadata | IV. (WP1420) | Internal: int2130.1 IV. int2320.1 IV. int2320.2 IV. External: ext2220.1 IV. ext2220.2 IV. ext2220.3 IV. ext2230.1 IV. ext2230.2 IV. ext2230.3 IV. ext2330.1 IV. |
47 | Computation of the global GIC index | Evaluation of the GIC index for the horizontal components of the geomagnetic field data as obtained from geomagnetic observatories in Italy (managed by INGV) and all over the world (INTERMAGNET and WDC networks) | Derived data
Visualization codes
Documentation and Metadata | II., III., VII. (WP1220,WP1330, WP1710) | Internal: int2130.1 II., III., VII. int2320.1 II., III., VII. int2320.2 II., III., VII. External: ext2220.1 II., III., VII. ext2220.2 II., III., VII. ext2220.3 II., III., VII. ext2230.1 II., III., VII. ext2230.2 II., III., VII. ext2230.3 II., III., VII. ext2330.1 II., III., VII. |
48 | Computation of the GIC index and level alert for Italy | Evaluation of the GIC index for the horizontal components of the geomagnetic field data as obtained from geomagnetic observatories in Italy and evaluation of the GIC level alert | derived data
model codes
Visualization codes
Documentation and Metadata | II., III., VII. (WP1220, WP1330, WP1710) | Internal: int2130.1 II., III., VII. int2130.4 II., III., VII. int2320.1 II., III., VII. int2320.2 II., III., VII. External: ext2220.1 II., III., VII. ext2220.2 II., III., VII. ext2220.3 II., III., VII. ext2220.4 II., III., VII. ext2230.1 II., III., VII. ext2230.2 II., III., VII. ext2230.3 II., III., VII. ext2230.4 II., III., VII. ext2330.1 II., III., VII. |
49 | Maps of Loss of Lock (LoL) events due to solar and geomagnetic activity | Computation and mapping of LoL events as identified through Total Electron Content (TEC) data from the Swarm constellation | Derived data
Visualization codes
Documentation and Metadata | II., IV., VII. (WP1220,WP1420, WP1710) | Internal: int2130.1 II., IV., VII. int2320.1 II., IV., VII. int2320.2 II., IV., VII. External: ext2220.1 II., IV., VII. ext2220.2 II., IV., VII. ext2220.3 II., IV., VII. ext2230.1 II., IV., VII. ext2230.2 II., IV., VII. ext2230.3 II., IV., VII. ext2330.1 II., IV., VII. |
50 | FD profiles at several rigidities for selected events | FD profiles are obtained analysing spacecraft data (PAMELA, AMS) and NMs | Derived Data
Visualization codes
Documentation and Metadata | VI. (WP1610) | Internal: int2130.1 VI. int2130.3 VI. int2320.1 VI. int2320.2 VI. External: ext2220.1 VI. ext2220.2 VI. ext2220.3 VI. ext2230.1 VI. ext2230.2 VI. ext2230.3 VI. ext2330.1 VI.
|
51 | Test-particle simulations | Full-orbit test-particle simulations over a magnetic configuration to provide particle intensity variation profiles as a function of time | Model Output
Visualization codes
Documentation and Metadata
| II., VI. (WP1220, WP1610) | Internal: int2130.1 II., VI. int2320.1 II., VI. int2320.2 II., VI. External: ext2220.1 II., VI. ext2220.2 II.,VI. ext2220.3 II., VI. ext2230.1 II., VI. ext2230.2 II., VI. ext2230.3 II., VI. ext2330.1 II.,VI. |
52 | Modelled GCR spectra | Result of the computation of GCRs differential energy spectra for various charged particles, in a given epoch and at a given position inside the heliosphere | Model Output
Visualization codes
Documentation and Metadata | VI. (WP1620) | Internal: int2130.1 VI. int2320.1 VI. int2320.2 VI. External: ext2220.1 VI. ext2220.2 VI. ext2220.3 VI. ext2230.1 VI. ext2230.2 VI. ext2230.3 VI. ext2220.5 VI. ext2330.1 VI. |
53 | Heliospheric parameters for the GCR propagation | Temporal dependence of heliospheric propagation parameters, i.e. the parameters evaluated at different epochs. | Model Output
Visualization codes
Documentation and Metadata | VI. (WP1620) | Internal: int2130.1 VI. int2320.1 VI. int2320.2 VI. External: ext2220.1 VI. ext2220.2 VI. ext2220.3 VI. ext2230.1 VI. ext2230.2 VI. ext2230.3 VI. ext2220.5 VI. ext2330.1 VI. |
54 | Magnetospheric Simulated data | MHD magnetospheric simulation of MHD instabilities of different non-dimensionless sets of magnetospheric conditions( Mach number, Reynolds number, magnetic Reynold number) | Model output
Visualization codes
Documentation and Metadata | V. (WP1510) | Internal: int2130.1 V. int2320.1 V. int2320.2 V. External: ext2220.1 V. ext2220.2 V. ext2220.3 V. ext2230.1 V. ext2230.2 V. ext2230.3 V. ext2330.1 V. |
55 | Magnetospheric Instability model (MIM) | Local MHD Magnetospheric Model utilized for real-time calculation of Kelvin-Helmholtz and tearing mode instabilities. The simulations will provide local magnetospheric characteristics and determine the plausible conditions of magnetic reconnection at Earth and Mercury magnetospheres | Model output
Visualization codes
Documentation and Metadata | V. (WP1510) | Internal: int2130.1 V. int2130.4 V. int2320.1 V. int2320.2 V. External: ext2220.1 V. ext2220.2 V. ext2220.3 V. ext2230.1 V ext2230.2 V. ext2230.3 V. ext2230.4 V. ext2330.1 V. |
56 | Atmospheric simulated data | Atmospheric mixing ratio vs pressure of Mars and Venus-like atmospheres for different Sun age | Derived data
Visualization codes
Documentation and Metadata | V. (WP1510) | Internal: int2130.1 V. int2320.1 V. int2320.2 V. External: ext2220.1 V. ext2220.2 V. ext2220.3 V. ext2230.1 V. ext2230.2 V. ext2230.3 V. ext2330.1 V. |
57 | Sodium exospheric data of Mercury
| Observed exospheric sodium bidimensional maps from the observations at THEMIS solar telescope (years 2009-2013).
| Calibrated data
Visualization codes
Documentation and Metadata | V. (WP1520) | Internal: int2130.1 V. int2320.1 V. int2320.2 V. External: ext2220.1 V. ext2220.2 V. ext2220.3 V. ext2230.1 V. ext2230.2 V. ext2230.3 V. ext2330.1 V. |
58 | Magnetospheric precipitation model
| 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) | Model output
Visualization codes
Documentation and Metadata | V. (WP1520) | Internal: int2130.1 V. int2320.1 V. int2320.2 V. External: ext2220.1 V. ext2220.2 V. ext2220.3 V. ext2230.1 V. ext2230.2 V. ext2230.3 V. ext2330.1 V. |
59 | Exospheric model
| Montecarlo, single particle exospheric model of Mercury. | Model codes
Visualization codes
Documentation and Metadata | V. (WP1520) | Internal: int2130.1 V. int2130.4 V. int2320.1 V. int2320.2 V. External: ext2220.1 V. ext2220.2 V. ext2220.3 V. ext2220.5 V. ext2230.1 V. ext2230.2 V. ext2230.3 V. ext2230.4 V. ext2330.1 V. |
60 | ALTEA data | Radiation fluxes inside the ISS: time series with variable time resolution ( > 1min) | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
61 | ALTEA data | Released energy spectra | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
62 | ALTEA data | Angular distribution | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
63 | ALTEA data | Dose rate | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
64 | LIDAL data | Radiation fluxes inside the International Space Station | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2130.2 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2220.4 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
65 | LIDAL data | Released energy spectra | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2130.2 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2220.4 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
66 | LIDAL data | Angular distribution | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2130.2 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2220.4 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
67 | LIDAL data | Dose rate | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2130.2 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2220.4 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
68 | LIDAL data | TOF distribution | Derived data
Visualization codes
Documentation and Metadata | VII. (WP1720) | Internal: int2130.1 VII. int2130.2 VII. int2320.1 VII. int2320.2 VII. External: ext2220.1 VII. ext2220.2 VII. ext2220.3 VII. ext2220.4 VII. ext2230.1 VII. ext2230.2 VII. ext2230.3 VII. ext2330.1 VII. |
69 | Method for desaturation of EUV images | inpainting and inverse problems methods for the desaturation of EUV images | Model codes
Visualization codes
Documentation and Metadata | I. (WP1130) | Internal: int2130.1 I. int2320.2 I. External: ext2230.1 I. ext2230.4 I. |
70 | Image reconstruction from Fourier X-ray data | computational methods based on inverse problems for the image reconstruction of X-ray images of solar flares | Model Codes
Visualization codes
Documentation and Metadata | I. (WP1130) | Internal: int2130.1 I. int2320.2 I. External: ext2230.1 I. ext2230.4 I. |
71 | AI methods for flare prediction | Machine learning methods for the prediction of flares events | model codes
Visualization codes
Documentation and Metadata | I. (WP1130) | Internal: int2130.1 I. int2320.2 I. External: ext2230.1 I. ext2230.4 I. |
72 | EUV waves-CME catalogue | catalog of CMEs events (speed, acceleration, direction of propagation) in association with global waves and their characteristics | Derived data
Visualization codes
Documentation and Metadata | I., II. (WP1130, WP1220) | Internal: int2130.1 I., II. int2320.2 I., II. External: ext2220.1 I., II. ext2220.2 I., II. ext2220.3 I., II. ext2230.1 I., II. ext2230.2 I., II. ext2230.3 I., II. ext2330.1 I., II. |
73 | Technical note on the study for the ML-based ESPERTA implementation in real-time | The technical note will contain results of the feasibility study about the use in the ESPERTA model of STEREO and LOFAR radio data. In particular, it will describe data, methodology, expected performances and prospects for real-time implementation
| Document | II. (WP1210)
| ext2330.1 II.
|
74 | Technical note on SEP monitoring/nowcasting algorithm: design study | The technical note will contain results of the feasibility study about design and implementation of a real-time warning suite for high energy SEP events based on in-situ data streams. In particular, it will describe dataset, methodology of the feasibility study, algorithm design, expected performances and prospects for applications and implementation of an algorithm for high energy SEP monitoring/nowcasting
| Document | II., VI. (WP1210, WP1610)
| ext2330.1 II., IV. |