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.