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.
The catalogue contains SEP events observed at the Earth of class S1, i.e. with flux in the range [10, 100) pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux >= 100 pfu at > 10 MeV are listed in the companion table S2 SEP Catalogue.
The catalogue contains SEP events observed at the Earth of class S2, i.e. with flux >100 pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux in the interval [10, 100) pfu at > 10 MeV are listed in the companion table S1 SEP Catalogue.
The differential energy spectral index is listed for all the SEP/ESP events analyzed.
Data Description
----------------
| **Data type**: tableset
| **Data formats**: - txt
| **Version**: v1.0
Data Provider
---------------
Data are collected by the following instruments:
- **STEREO-A** - sources:
- IMPACT/SEPT
- IMPACT/LET
- IMPACT/HET
- **ACE** - source:
- EPAM
- **PSP** - sources:
- EPIHI-LET
- EPIHI-HET
Data Relationships
-----------------
- type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- description: 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.
- relatedproduct: ESP spectra
- relatedproductid: 21
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events.
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
.
Data are ND with - type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- description: 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.
- relatedproduct: ESP spectra
- relatedproductid: 21
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events.
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
marked as id: - type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- description: 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.
- relatedproduct: ESP spectra
- relatedproductid: 21
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events.
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
- :ref:`- type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- description: 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.
- relatedproduct: ESP spectra
- relatedproductid: 21
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events.
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Interplanetary Space (not L1 and Planets)
For each SEP/ESP event, in case of anomalous (superdiffusive) transport, as deduced from energetic particle fluxes, the exponent of the mean square displacement as a function of time is derived. Then, diffusion coefficients are computed either in case of normal or in case of superdiffusive transport (derived from the analysis of the particle fluxes upstream in different energy channels). From the diffusion coefficients the acceleration times are calculated in each energy channel.
Data Description
----------------
| **Data type**: tableset
| **Data formats**: - txt
| **Version**: v1.0
Data Provider
---------------
Data are collected by the following instruments:
- **STEREO-A** - sources:
- IMPACT/SEPT
- IMPACT/LET
- IMPACT/HET
- **ACE** - sources:
- EPAM
- SWEPAM
- **PSP** - sources:
- EPIHI-LET
- EPIHI-HET
- SWEAP SPAN-I
Data Relationships
-----------------
- type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- relatedproduct: ESP spectra
- description: 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
- relatedproductid: 21
- type: related-to
- description: 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
- relatedproduct: Parameters of shocks associated with SEP and ESP events
- relatedproductid: 22
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
.
Data are ND with - type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- relatedproduct: ESP spectra
- description: 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
- relatedproductid: 21
- type: related-to
- description: 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
- relatedproduct: Parameters of shocks associated with SEP and ESP events
- relatedproductid: 22
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
marked as id: - type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- relatedproduct: ESP spectra
- description: 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
- relatedproductid: 21
- type: related-to
- description: 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
- relatedproduct: Parameters of shocks associated with SEP and ESP events
- relatedproductid: 22
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
- :ref:`- type: related-to
- description: Proton spectra for: 1) geoeffective target SWE events (at L1); 2) widespread target SWE events (at different heliographic locations from multiple spacecraft)
- relatedproduct: SEP spectra
- relatedproductid: 20
- type: related-to
- relatedproduct: ESP spectra
- description: 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
- relatedproductid: 21
- type: related-to
- description: 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
- relatedproduct: Parameters of shocks associated with SEP and ESP events
- relatedproductid: 22
- type: related-to
- description: 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 spa cecraft measurements for widespread target SWE events
- relatedproduct: Turbulence and intermittency data nearby IP shocks
- relatedproductid: 23
`
Data Coverage
-----------------
The product cover measurements for the ND messangers.
Data coverage is listed below:
| **Spatial** - Interplanetary Space (not L1 and Planets)
