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Commit 3068206d authored by Stefano Scardigli's avatar Stefano Scardigli
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yes yes yes...

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docs/source/products/data/external_ace_swepam_timeseries.rst
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ACE Solar Wind 1 min
====================
.. contents:: The tiny table of contents
.. contents:: Table of contents
qui dovra' esserci la descrizione del prodotto
**References**
References
~~~~~~~~~~
qui invece la bibliografia
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** external_ace_swepam_timeseries
**publisher:** not available in DBF
**alphanumeric_code:** 101A
**id_tmp:** 101
**short_name:** ace_1minute
**identifier:** aspis:///external/ace_swepam_timeseries
**dynamic:** Approx 2MB every week
**size:** 100kB
**format:** csv
**type:** timeseries
**records_number:** 21599
**time_start:** 2016-12-14
**time_stop:** 2020-12-31
**spatial:** L1
**messenger:** protons,electrons
**spectral_min:** 0.26
**spectral_max:** 36
**spectral_units:** keV
**observable:** CME,SW,SEP
.. list-table::
**latest update:** 2024-03-29 12:01:32
* - **internal_name:**
- external_ace_swepam_timeseries
* - **publisher:**
- not available in DBF
* - **alph_code:**
- 101A
* - **id_tmp:**
- 101
* - **short_name:**
- ace_1minute
* - **identifier:**
- aspis:///external/ace_swepam_timeseries
* - **dynamic:**
- Approx 2MB every week
* - **size:**
- 100kB
* - **format:**
- csv
* - **type:**
- timeseries
* - **records_number:**
- 21599
* - **time_start:**
- 2016-12-14
* - **time_stop:**
- 2020-12-31
* - **spatial:**
- L1
* - **messenger:**
- protons,electrons
* - **spectral_min:**
- 0.26
* - **spectral_max:**
- 36
* - **spectral_units:**
- keV
* - **observable:**
- CME,SW,SEP
* - **latest update:**
- 2024-03-29 12:01:32
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/external_flux_goes_timeseries.rst
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GOES X-ray Flux
===============
.. contents:: The tiny table of contents
.. contents:: Table of contents
not available in DBF
**References**
References
~~~~~~~~~~
not available in DBF
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** external_flux_goes_timeseries
**publisher:** not available in DBF
**alphanumeric_code:** 102A
**id_tmp:** 102
**short_name:** goesx1min
**identifier:** aspis:///external/flux_goes_timeseries
**dynamic:** Approx 1MB every week
**size:** 5MB
**format:** csv
**type:** timeseries
**records_number:** 21599
**time_start:** 2016-12-14
**time_stop:** 2020-12-31
**spatial:** L1
**messenger:** photons
**spectral_min:** 1
**spectral_max:** 8
**spectral_units:** Angstrom
**observable:** flare
.. list-table::
**latest update:** 2024-03-28 05:08:04
* - **internal_name:**
- external_flux_goes_timeseries
* - **publisher:**
- not available in DBF
* - **alph_code:**
- 102A
* - **id_tmp:**
- 102
* - **short_name:**
- goesx1min
* - **identifier:**
- aspis:///external/flux_goes_timeseries
* - **dynamic:**
- Approx 1MB every week
* - **size:**
- 5MB
* - **format:**
- csv
* - **type:**
- timeseries
* - **records_number:**
- 21599
* - **time_start:**
- 2016-12-14
* - **time_stop:**
- 2020-12-31
* - **spatial:**
- L1
* - **messenger:**
- photons
* - **spectral_min:**
- 1
* - **spectral_max:**
- 8
* - **spectral_units:**
- Angstrom
* - **observable:**
- flare
* - **latest update:**
- 2024-03-28 05:08:04
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/external_part_goes_timeseries.rst
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GOES proton Flux
================
.. contents:: The tiny table of contents
.. contents:: Table of contents
not available in DBF
**References**
References
~~~~~~~~~~
not available in DBF
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** external_part_goes_timeseries
**publisher:** not available in DBF
**alphanumeric_code:** 103A
**id_tmp:** 103
**short_name:** GOES_particle1min
**identifier:** aspis:///external/part_goes_timeseries
**dynamic:** Approx 2MB every week
**size:** 2MB
**format:** csv
**type:** timeseries
**records_number:** 4319
**time_start:** 2016-12-14
**time_stop:** 2020-12-31
**spatial:** L1
**messenger:** protons,electrons
**spectral_min:** 1
**spectral_max:** 100
**spectral_units:** MeV
**observable:** flare,SEP,CME,ESP,SW
.. list-table::
**latest update:** 2024-03-28 05:08:04
* - **internal_name:**
- external_part_goes_timeseries
* - **publisher:**
- not available in DBF
* - **alph_code:**
- 103A
* - **id_tmp:**
- 103
* - **short_name:**
- GOES_particle1min
* - **identifier:**
- aspis:///external/part_goes_timeseries
* - **dynamic:**
- Approx 2MB every week
* - **size:**
- 2MB
* - **format:**
- csv
* - **type:**
- timeseries
* - **records_number:**
- 4319
* - **time_start:**
- 2016-12-14
* - **time_stop:**
- 2020-12-31
* - **spatial:**
- L1
* - **messenger:**
- protons,electrons
* - **spectral_min:**
- 1
* - **spectral_max:**
- 100
* - **spectral_units:**
- MeV
* - **observable:**
- flare,SEP,CME,ESP,SW
* - **latest update:**
- 2024-03-28 05:08:04
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_cpcp_superdarn_datacube.rst
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SuperDARN Polar Cap Potential
=============================
.. contents:: The tiny table of contents
.. contents:: Table of contents
The Super Dual Auroral Radar Network (SuperDARN) is an international network of
High Frequency coherent scatter radars. A map of the fields of view of the radars
......@@ -22,7 +22,8 @@ As ionospheric irregularities are dragged in the large scale convection at high
allows to infer the velocity of the ambient plasma with respect to the sounded direction
and gate.
**References**
References
~~~~~~~~~~
https://www.sciencedirect.com/science/article/abs/pii/S136468260600263X
......@@ -48,48 +49,51 @@ https://doi.org/10.1002/2018JA025280
and Functional Approximations, J. Geophys. Res., Space Physics, 119(9), 7501-7521
(2014). https://doi.org/10.1002/2014JA020264
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_cpcp_superdarn_datacube
**publisher:** INAF
**alphanumeric_code:** 31
**id_tmp:** 71
**short_name:** SuperDARN CPCP
**identifier:** aspis://inaf/cpcp_superdarn_datacube
**dynamic:** static
**size:** 200MB
**format:** csv
**type:** timeseries
**records_number:** 1515672
**time_start:** 2015-06-21
**time_stop:** 2017-09-11
**spatial:** IONO
**messenger:** electrons,
**spectral_min:** 0
**spectral_max:** 1
**spectral_units:** dimensionless
**observable:** IMF,GEOINDEX
.. list-table::
**latest update:** 2024-04-04 01:53:25
* - **internal_name:**
- inaf_cpcp_superdarn_datacube
* - **publisher:**
- INAF
* - **alph_code:**
- 31
* - **id_tmp:**
- 71
* - **short_name:**
- SuperDARN CPCP
* - **identifier:**
- aspis://inaf/cpcp_superdarn_datacube
* - **dynamic:**
- static
* - **size:**
- 200MB
* - **format:**
- csv
* - **type:**
- timeseries
* - **records_number:**
- 1515672
* - **time_start:**
- 2015-06-21
* - **time_stop:**
- 2017-09-11
* - **spatial:**
- IONO
* - **messenger:**
- electrons,
* - **spectral_min:**
- 0
* - **spectral_max:**
- 1
* - **spectral_units:**
- dimensionless
* - **observable:**
- IMF,GEOINDEX
* - **latest update:**
- 2024-04-04 01:53:25
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_data_solopas_timeseries.rst
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INAF-IAPS Solar Orbiter-PAS data
================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
The product contains density N, speed vector V, pressure tensor P, temperature components (Tx, Ty, Tz), and the velocity of the satellite V_solo, computed using the data collected by the Proton-Alpha Sensor (PAS) onboard Solar Orbiter.
PAS measures the 3D distribution functions of the dominant ions of the solar wind, from 200 eV to 20 KeV, without mass and charge selection. In practice, this concerns mostly the proton and alfa populations (unseparated). At full resolution, PAS collects the 3D ion distribution function in about 1 second, even though the moments have a cadence of 4 seconds, while in “snapshot” mode the phase space sampling is reduced, allowing a greater cadence for the moments.
Data is hosted on http://soar.esac.esa.int/soar/
**References**
References
~~~~~~~~~~
R. D’Amicis et al, Astronomy &Astrophysics 656, A21 (2021)
......@@ -19,48 +20,51 @@ D. Perrone et al, Astronomy &Astrophysics 668, A189 (2022)
R. De Marco et al, Astronomy &Astrophysics, 669, A108 (2023)
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_data_solopas_timeseries
**publisher:** INAF-IAPS, Plasma & Space Weather Group
**alphanumeric_code:** 14
**id_tmp:** 72
**short_name:** SolO-PAS_data
**identifier:** aspis://inaf/data_solopas_timeseries
**dynamic:** a file each day (file size between 3 and 4 Mb). As a general rule, one month of data is uploaded each month, generally relating to 3 months before the upload date
**size:** 2GB
**format:** dsv
**type:** timeseries
**records_number:** 38653
**time_start:** 2020-07-06
**time_stop:** 2022-01-31
**spatial:** IP
**messenger:** Protons
**spectral_min:**
**spectral_max:**
**spectral_units:**
**observable:** SW,SEP
.. list-table::
**latest update:** 2024-04-04 01:54:59
* - **internal_name:**
- inaf_data_solopas_timeseries
* - **publisher:**
- INAF-IAPS, Plasma & Space Weather Group
* - **alph_code:**
- 14
* - **id_tmp:**
- 72
* - **short_name:**
- SolO-PAS_data
* - **identifier:**
- aspis://inaf/data_solopas_timeseries
* - **dynamic:**
- a file each day (file size between 3 and 4 Mb). As a general rule, one month of data is uploaded each month, generally relating to 3 months before the upload date
* - **size:**
- 2GB
* - **format:**
- dsv
* - **type:**
- timeseries
* - **records_number:**
- 38653
* - **time_start:**
- 2020-07-06
* - **time_stop:**
- 2022-01-31
* - **spatial:**
- IP
* - **messenger:**
- Protons
* - **spectral_min:**
-
* - **spectral_max:**
-
* - **spectral_units:**
-
* - **observable:**
- SW,SEP
* - **latest update:**
- 2024-04-04 01:54:59
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_flux1h_svirco_timeseries.rst
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SVIRCO Observatory - the Rome neutron monitor
=============================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 1h. Average intensity of January-February 1997 = 100%
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_flux1h_svirco_timeseries
**publisher:** INAF
**alphanumeric_code:** 42C
**id_tmp:** 73
**short_name:** flux1h_SVIRCO
**identifier:** inaf_flux1h_svirco_timeseries
**dynamic:** Data collection grows in time.
**size:** 13MB
**format:** CSV
**type:** timeseries
**records_number:** 479976
**time_start:** 1966-04-01
**time_stop:** 2020-12-31
**spatial:** GROUND
**messenger:** Nucleons
**spectral_min:** 6.3
**spectral_max:** 9999
**spectral_units:** GeV
**observable:** GLE,GCR
.. list-table::
**latest update:** 2024-03-28 05:08:05
* - **internal_name:**
- inaf_flux1h_svirco_timeseries
* - **publisher:**
- INAF
* - **alph_code:**
- 42C
* - **id_tmp:**
- 73
* - **short_name:**
- flux1h_SVIRCO
* - **identifier:**
- inaf_flux1h_svirco_timeseries
* - **dynamic:**
- Data collection grows in time.
* - **size:**
- 13MB
* - **format:**
- CSV
* - **type:**
- timeseries
* - **records_number:**
- 479976
* - **time_start:**
- 1966-04-01
* - **time_stop:**
- 2020-12-31
* - **spatial:**
- GROUND
* - **messenger:**
- Nucleons
* - **spectral_min:**
- 6.3
* - **spectral_max:**
- 9999
* - **spectral_units:**
- GeV
* - **observable:**
- GLE,GCR
* - **latest update:**
- 2024-03-28 05:08:05
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_flux5m_svirco_timeseries.rst
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SVIRCO Obser vatory - the Rome neutron monitor
==============================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 5min Average intensity of January-February 1997 = 100%
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_flux5m_svirco_timeseries
**publisher:** INAF
**alphanumeric_code:** 42B
**id_tmp:** 74
**short_name:** flux5m_SVIRCO
**identifier:** inaf_flux5m_svirco_timeseries
**dynamic:** Data collection grows in time.
**size:** 80MB
**format:** CSV
**type:** timeseries
**records_number:** 2007072
**time_start:** 1997-05-21
**time_stop:** 2017-01-01
**spatial:** GROUND
**messenger:** Neutrons
**spectral_min:** 6.3
**spectral_max:** 9999
**spectral_units:** GeV
**observable:** GLE,GCR
.. list-table::
**latest update:** 2024-03-28 05:08:05
* - **internal_name:**
- inaf_flux5m_svirco_timeseries
* - **publisher:**
- INAF
* - **alph_code:**
- 42B
* - **id_tmp:**
- 74
* - **short_name:**
- flux5m_SVIRCO
* - **identifier:**
- inaf_flux5m_svirco_timeseries
* - **dynamic:**
- Data collection grows in time.
* - **size:**
- 80MB
* - **format:**
- CSV
* - **type:**
- timeseries
* - **records_number:**
- 2007072
* - **time_start:**
- 1997-05-21
* - **time_stop:**
- 2017-01-01
* - **spatial:**
- GROUND
* - **messenger:**
- Neutrons
* - **spectral_min:**
- 6.3
* - **spectral_max:**
- 9999
* - **spectral_units:**
- GeV
* - **observable:**
- GLE,GCR
* - **latest update:**
- 2024-03-28 05:08:05
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_gsmaps_datacube.rst
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......@@ -2,56 +2,60 @@
IAPS Grad-Shafranov Reconstruction of Magnetic Clouds
=====================================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
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.
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_gsmaps_datacube
**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali
**alphanumeric_code:** 25
**id_tmp:** 96
**short_name:** gsmaps-cubes
**identifier:** aspis://inaf/gsmaps_datacube
**dynamic:** static
**size:** 300kB
**format:** nc
**type:** spectrum
**records_number:** 3
**time_start:** 1997-01-01
**time_stop:** 2022-01-01
**spatial:** IP
**messenger:** Magnetic field,Magnetic vector potential,Flux rope coordinates
**spectral_min:**
**spectral_max:**
**spectral_units:**
**observable:** phys.magField,phys.potential,phys.size
.. list-table::
**latest update:** 2024-03-28 05:08:05
* - **internal_name:**
- inaf_gsmaps_datacube
* - **publisher:**
- INAF - Istituto di Astrofisica e Planetologia Spaziali
* - **alph_code:**
- 25
* - **id_tmp:**
- 96
* - **short_name:**
- gsmaps-cubes
* - **identifier:**
- aspis://inaf/gsmaps_datacube
* - **dynamic:**
- static
* - **size:**
- 300kB
* - **format:**
- nc
* - **type:**
- spectrum
* - **records_number:**
- 3
* - **time_start:**
- 1997-01-01
* - **time_stop:**
- 2022-01-01
* - **spatial:**
- IP
* - **messenger:**
- Magnetic field,Magnetic vector potential,Flux rope coordinates
* - **spectral_min:**
-
* - **spectral_max:**
-
* - **spectral_units:**
-
* - **observable:**
- phys.magField,phys.potential,phys.size
* - **latest update:**
- 2024-03-28 05:08:05
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_m2flare_tableset.rst
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IAPS ≥M2 SXR Flare Catalogue
==============================
.. contents:: The tiny table of contents
.. contents:: Table of contents
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.
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_m2flare_tableset
**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali
**alphanumeric_code:** 7
**id_tmp:** 75
**short_name:** IAPS-M2SXR
**identifier:** aspis://inaf/m2flare_tableset
**dynamic:** static
**size:** 100kB
**format:** xlsx
**type:** tableset
**records_number:** 1040
**time_start:** 1995-01-01
**time_stop:** 2017-05-03
**spatial:** SUN
**messenger:** Photons
**spectral_min:**
**spectral_max:**
**spectral_units:**
**observable:** phys.flux
.. list-table::
**latest update:** 2024-03-28 05:08:05
* - **internal_name:**
- inaf_m2flare_tableset
* - **publisher:**
- INAF - Istituto di Astrofisica e Planetologia Spaziali
* - **alph_code:**
- 7
* - **id_tmp:**
- 75
* - **short_name:**
- IAPS-M2SXR
* - **identifier:**
- aspis://inaf/m2flare_tableset
* - **dynamic:**
- static
* - **size:**
- 100kB
* - **format:**
- xlsx
* - **type:**
- tableset
* - **records_number:**
- 1040
* - **time_start:**
- 1995-01-01
* - **time_stop:**
- 2017-05-03
* - **spatial:**
- SUN
* - **messenger:**
- Photons
* - **spectral_min:**
-
* - **spectral_max:**
-
* - **spectral_units:**
-
* - **observable:**
- phys.flux
* - **latest update:**
- 2024-03-28 05:08:05
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_na_mercexo_image.rst
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......@@ -2,11 +2,12 @@
INAF-bidimensional maps of Mercury Na exosphere
===============================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
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 data base (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).
**References**
References
~~~~~~~~~~
Leblanc, F., Doressoundiram, A., Schneider, N., Mangano, V., López Ariste, A., Lemen, C., Gelly, B., Barbieri, C. and Cremonese, G., 2008. High latitude peaks in Mercury's sodium exosphere: Spectral signature using THEMIS solar telescope. Geophysical Research Letters, 35(18).
......@@ -20,48 +21,51 @@ Massetti, S., Mangano, V., Milillo, A., Mura, A., Orsini, S. and Plainaki, C., 2
Orsini, S., Mangano, V., Milillo, A., Plainaki, C., Mura, A., Raines, J.M., De Angelis, E., Rispoli, R., Lazzarotto, F. and Aronica, A., 2018. Mercury sodium exospheric emission as a proxy for solar perturbations transit. Scientific reports, 8(1), p.928.
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_na_mercexo_image
**publisher:** Valeria Mangano, INAF-IAPS
**alphanumeric_code:** 57
**id_tmp:** 76
**short_name:** Merc_exos_Na_fts
**identifier:** aspis://inaf/na_mercexo_image
**dynamic:** period 2009-2013 is static, but if we decide to include also most recent data, it will grow in time.
**size:** 1GB
**format:** fits
**type:** image
**records_number:** 7
**time_start:** 2009-04-17
**time_stop:** 2013-05-25
**spatial:** Mercury
**messenger:** photons
**spectral_min:** 5890
**spectral_max:** 5896
**spectral_units:** Angstrom
**observable:** IMF,SW,CME
.. list-table::
**latest update:** 2024-04-04 01:59:34
* - **internal_name:**
- inaf_na_mercexo_image
* - **publisher:**
- Valeria Mangano, INAF-IAPS
* - **alph_code:**
- 57
* - **id_tmp:**
- 76
* - **short_name:**
- Merc_exos_Na_fts
* - **identifier:**
- aspis://inaf/na_mercexo_image
* - **dynamic:**
- period 2009-2013 is static, but if we decide to include also most recent data, it will grow in time.
* - **size:**
- 1GB
* - **format:**
- fits
* - **type:**
- image
* - **records_number:**
- 7
* - **time_start:**
- 2009-04-17
* - **time_stop:**
- 2013-05-25
* - **spatial:**
- Mercury
* - **messenger:**
- photons
* - **spectral_min:**
- 5890
* - **spectral_max:**
- 5896
* - **spectral_units:**
- Angstrom
* - **observable:**
- IMF,SW,CME
* - **latest update:**
- 2024-04-04 01:59:34
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_s1sep_tableset.rst
+ 51
− 47
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IAPS S1 SEP events Catalogue
============================
.. contents:: The tiny table of contents
.. contents:: Table of contents
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.
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_s1sep_tableset
**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali
**alphanumeric_code:** 16A
**id_tmp:** 77
**short_name:** IAPS-S1 SEP events
**identifier:** aspis://inaf/s1sep_tableset
**dynamic:** static
**size:** 100kB
**format:** csv
**type:** tableset
**records_number:** 68
**time_start:** 1995-01-01
**time_stop:** 2014-09-10
**spatial:** Earth
**messenger:** Protons,Photons
**spectral_min:**
**spectral_max:**
**spectral_units:**
**observable:** flare,CME,SEP
.. list-table::
**latest update:** 2024-03-28 05:08:05
* - **internal_name:**
- inaf_s1sep_tableset
* - **publisher:**
- INAF - Istituto di Astrofisica e Planetologia Spaziali
* - **alph_code:**
- 16A
* - **id_tmp:**
- 77
* - **short_name:**
- IAPS-S1 SEP events
* - **identifier:**
- aspis://inaf/s1sep_tableset
* - **dynamic:**
- static
* - **size:**
- 100kB
* - **format:**
- csv
* - **type:**
- tableset
* - **records_number:**
- 68
* - **time_start:**
- 1995-01-01
* - **time_stop:**
- 2014-09-10
* - **spatial:**
- Earth
* - **messenger:**
- Protons,Photons
* - **spectral_min:**
-
* - **spectral_max:**
-
* - **spectral_units:**
-
* - **observable:**
- flare,CME,SEP
* - **latest update:**
- 2024-03-28 05:08:05
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_s2sep_tableset.rst
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− 47
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......@@ -2,56 +2,60 @@
IAPS S2 SEP events Catalogue
============================
.. contents:: The tiny table of contents
.. contents:: Table of contents
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.
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_s2sep_tableset
**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali
**alphanumeric_code:** 16B
**id_tmp:** 78
**short_name:** IAPS-S2 SEP events
**identifier:** aspis://inaf/s1sep_tableset
**dynamic:** static
**size:** 100kB
**format:** csv
**type:** tableset
**records_number:** 60
**time_start:** 1995-01-01
**time_stop:** 2014-09-10
**spatial:** Earth
**messenger:** Protons,Photons
**spectral_min:**
**spectral_max:**
**spectral_units:**
**observable:** flare,CME,SEP
.. list-table::
**latest update:** 2024-03-28 05:08:06
* - **internal_name:**
- inaf_s2sep_tableset
* - **publisher:**
- INAF - Istituto di Astrofisica e Planetologia Spaziali
* - **alph_code:**
- 16B
* - **id_tmp:**
- 78
* - **short_name:**
- IAPS-S2 SEP events
* - **identifier:**
- aspis://inaf/s1sep_tableset
* - **dynamic:**
- static
* - **size:**
- 100kB
* - **format:**
- csv
* - **type:**
- tableset
* - **records_number:**
- 60
* - **time_start:**
- 1995-01-01
* - **time_stop:**
- 2014-09-10
* - **spatial:**
- Earth
* - **messenger:**
- Protons,Photons
* - **spectral_min:**
-
* - **spectral_max:**
-
* - **spectral_units:**
-
* - **observable:**
- flare,CME,SEP
* - **latest update:**
- 2024-03-28 05:08:06
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_tps_datacube.rst
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− 47
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IAPS Test Particle Simulation on Magnetic Clouds
================================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
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.
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_tps_datacube
**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali
**alphanumeric_code:** 51
**id_tmp:** 97
**short_name:** IAPS-TPS
**identifier:** aspis://inaf/tps_datacube
**dynamic:** static
**size:** 300kB
**format:** nc
**type:** spectrum
**records_number:** 3
**time_start:** 1997-01-01
**time_stop:** 2022-01-01
**spatial:** Interplanetary Space (not L1 and Planets),Sun-Earth L1
**messenger:** Particle intensity variation
**spectral_min:**
**spectral_max:**
**spectral_units:**
**observable:** phys.flux,phys.particle.proton
.. list-table::
**latest update:** 2024-03-28 05:08:06
* - **internal_name:**
- inaf_tps_datacube
* - **publisher:**
- INAF - Istituto di Astrofisica e Planetologia Spaziali
* - **alph_code:**
- 51
* - **id_tmp:**
- 97
* - **short_name:**
- IAPS-TPS
* - **identifier:**
- aspis://inaf/tps_datacube
* - **dynamic:**
- static
* - **size:**
- 300kB
* - **format:**
- nc
* - **type:**
- spectrum
* - **records_number:**
- 3
* - **time_start:**
- 1997-01-01
* - **time_stop:**
- 2022-01-01
* - **spatial:**
- Interplanetary Space (not L1 and Planets),Sun-Earth L1
* - **messenger:**
- Particle intensity variation
* - **spectral_min:**
-
* - **spectral_max:**
-
* - **spectral_units:**
-
* - **observable:**
- phys.flux,phys.particle.proton
* - **latest update:**
- 2024-03-28 05:08:06
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/inaf_vbcorr_wind_tableset.rst
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IAPS - Wind velocity-magnetic field correlation coefficient data of solar wind streams
======================================================================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two.
**References**
References
~~~~~~~~~~
D’Amicis et al, GRL, 34, L05108, 2007; Frontiers in Physics, 8, 541, 2020
......@@ -16,48 +17,51 @@ D’Amicis et al, A&A, 656, A21, 2021
Tu et al., JGR, 94, 11739, 1989
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** inaf_vbcorr_wind_tableset
**publisher:** INAF-IAPS, Fisica dei Plasmi Spaziali e Space Weather
**alphanumeric_code:** 24C
**id_tmp:** 98
**short_name:** wind_v-b_corr
**identifier:** aspis://inaf/vbcorr_wind_tableset
**dynamic:** static
**size:** 35MB
**format:** csv
**type:** tableset
**records_number:** 538
**time_start:** 1998-10-01
**time_stop:** 2022-05-06
**spatial:** L1
**messenger:** protons
**spectral_min:** 0
**spectral_max:** 0
**spectral_units:** -
**observable:** SW
.. list-table::
**latest update:** 2024-04-04 02:05:02
* - **internal_name:**
- inaf_vbcorr_wind_tableset
* - **publisher:**
- INAF-IAPS, Fisica dei Plasmi Spaziali e Space Weather
* - **alph_code:**
- 24C
* - **id_tmp:**
- 98
* - **short_name:**
- wind_v-b_corr
* - **identifier:**
- aspis://inaf/vbcorr_wind_tableset
* - **dynamic:**
- static
* - **size:**
- 35MB
* - **format:**
- csv
* - **type:**
- tableset
* - **records_number:**
- 538
* - **time_start:**
- 1998-10-01
* - **time_stop:**
- 2022-05-06
* - **spatial:**
- L1
* - **messenger:**
- protons
* - **spectral_min:**
- 0
* - **spectral_max:**
- 0
* - **spectral_units:**
- -
* - **observable:**
- SW
* - **latest update:**
- 2024-04-04 02:05:02
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/infn_cses_hepd_spectrum.rst
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− 44
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HEPD-01 time-integrated proton spectrum during the Ground-Level Enhancement of October 28, 2021
===============================================================================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
Time-integrated spectrum of solar protons measured by the HEPD-01 detector from space during the Ground-Level Enhancement of October 28, 2021
**References**
References
~~~~~~~~~~
https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022SW003191
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** infn_cses_hepd_spectrum
**publisher:** not available in DBF
**alphanumeric_code:** 44C
**id_tmp:** 106
**short_name:** HEPD-proton
**identifier:** aspis://infn/infn_cses_hepd_spectrum
**dynamic:**
**size:** 10kB
**format:** csv
**type:** spectrum
**records_number:** 1
**time_start:** 2021-10-28
**time_stop:** 2021-11-03
**spatial:** GEOMAG
**messenger:** protons
**spectral_min:** 55
**spectral_max:** 250
**spectral_units:** MeV
**observable:** GLE,flare,SEP,GCR,CME
.. list-table::
**latest update:** 2024-04-04 02:08:35
* - **internal_name:**
- infn_cses_hepd_spectrum
* - **publisher:**
- not available in DBF
* - **alph_code:**
- 44C
* - **id_tmp:**
- 106
* - **short_name:**
- HEPD-proton
* - **identifier:**
- aspis://infn/infn_cses_hepd_spectrum
* - **dynamic:**
-
* - **size:**
- 10kB
* - **format:**
- csv
* - **type:**
- spectrum
* - **records_number:**
- 1
* - **time_start:**
- 2021-10-28
* - **time_stop:**
- 2021-11-03
* - **spatial:**
- GEOMAG
* - **messenger:**
- protons
* - **spectral_min:**
- 55
* - **spectral_max:**
- 250
* - **spectral_units:**
- MeV
* - **observable:**
- GLE,flare,SEP,GCR,CME
* - **latest update:**
- 2024-04-04 02:08:35
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/infn_iss_ams_flux_timeseries.rst
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− 44
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INFN AMS daily proton time dependent fluxes
===========================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
Daily proton fluxes in cosmic rays were measured with the Alpha Magnetic Spectrometer aboard the International Space Station, from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV, based on 5.5×10^9 protons collected. Several Forbush decreases were also observed during the whole period, in connection with transient magnetic perturbations. The product provides these data as time-profiles from May 20, 2011 to October 29 2019 as a function of rigidity. In particular the daily proton fluxes are measured in 30 bins from 1.00 to 100 GV. The errors include statistics, time-dependent systematic errors and the total systematic error.
**References**
References
~~~~~~~~~~
https://doi.org/10.1103/PhysRevLett.127.271102
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** infn_iss_ams_flux_timeseries
**publisher:** not available in DBF
**alphanumeric_code:** 50A
**id_tmp:** 89
**short_name:** AMS_daily_H
**identifier:** aspis:///infn/ams_protons
**dynamic:** static
**size:** 4.1MB
**format:** csv
**type:** timeseries
**records_number:** 83757
**time_start:** 2011-05-20
**time_stop:** 2019-10-29
**spatial:** GEOMAG
**messenger:** Protons
**spectral_min:** 1
**spectral_max:** 100
**spectral_units:** GV
**observable:** GCR
.. list-table::
**latest update:** 2024-04-04 02:10:23
* - **internal_name:**
- infn_iss_ams_flux_timeseries
* - **publisher:**
- not available in DBF
* - **alph_code:**
- 50A
* - **id_tmp:**
- 89
* - **short_name:**
- AMS_daily_H
* - **identifier:**
- aspis:///infn/ams_protons
* - **dynamic:**
- static
* - **size:**
- 4.1MB
* - **format:**
- csv
* - **type:**
- timeseries
* - **records_number:**
- 83757
* - **time_start:**
- 2011-05-20
* - **time_stop:**
- 2019-10-29
* - **spatial:**
- GEOMAG
* - **messenger:**
- Protons
* - **spectral_min:**
- 1
* - **spectral_max:**
- 100
* - **spectral_units:**
- GV
* - **observable:**
- GCR
* - **latest update:**
- 2024-04-04 02:10:23
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/infn_pamela_flux_timeseries.rst
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......@@ -2,56 +2,60 @@
PAMELA time-profiles of protons during 4 Forbush Decreases
==========================================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
Time-profiles of galactic cosmic-ray protons measured by the PAMELA detector in space during 4 Forbush Decreases from March 2012 to June 2015 in various rigidity intervals. Each profile is scaled for a suitable period of quiet Sun, estimated about 10 days before each Forbush Decrease
**References**
References
~~~~~~~~~~
https://iopscience.iop.org/article/10.3847/1538-4357/aaa0c8
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** infn_pamela_flux_timeseries
**publisher:** not available in DBF
**alphanumeric_code:** 50B
**id_tmp:** 90
**short_name:** PAMELA-proton
**identifier:** aspis://INFN-PAMELA/proton
**dynamic:** Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015
**size:** 200kB
**format:** csv
**type:** timeseries
**records_number:** 2394
**time_start:** 2012-03-01
**time_stop:** 2015-07-17
**spatial:** GEOMAG
**messenger:** protons
**spectral_min:** 0.85
**spectral_max:** 8.68
**spectral_units:** GV
**observable:** GCR
.. list-table::
**latest update:** 2024-04-04 02:12:29
* - **internal_name:**
- infn_pamela_flux_timeseries
* - **publisher:**
- not available in DBF
* - **alph_code:**
- 50B
* - **id_tmp:**
- 90
* - **short_name:**
- PAMELA-proton
* - **identifier:**
- aspis://INFN-PAMELA/proton
* - **dynamic:**
- Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015
* - **size:**
- 200kB
* - **format:**
- csv
* - **type:**
- timeseries
* - **records_number:**
- 2394
* - **time_start:**
- 2012-03-01
* - **time_stop:**
- 2015-07-17
* - **spatial:**
- GEOMAG
* - **messenger:**
- protons
* - **spectral_min:**
- 0.85
* - **spectral_max:**
- 8.68
* - **spectral_units:**
- GV
* - **observable:**
- GCR
* - **latest update:**
- 2024-04-04 02:12:29
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/infn_saandose_samadha_timeseries.rst
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SAMADHA neutron dose rate at Mount Chacaltaya
=============================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) is an INFN project aimed to monitor the neutron dose rate due to cosmic rays at the Chacaltaya Station (Bolivia, 5200 m) inside the South Atlantic Anomaly region, to study possible correlation between space weather events and dose rate at the ground, considering the proximity of the Van Allen Belts to the Earth's surface in the SAA region.
**References**
References
~~~~~~~~~~
http://samadha.to.infn.it
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** infn_saandose_samadha_timeseries
**publisher:** SAMADHA
**alphanumeric_code:** 75A
**id_tmp:** 99
**short_name:** SAA_Ndose
**identifier:** aspis://infn/saandose_samadha_timeseries
**dynamic:** one dataset per day (50 kB/day)
**size:** 50kB
**format:** text
**type:** tableset
**records_number:** 2358
**time_start:** 2022-10-01
**time_stop:** 2023-12-31
**spatial:** Earth's Ground
**messenger:** neutrons
**spectral_min:** 0
**spectral_max:** 0
**spectral_units:** 0
**observable:**
.. list-table::
**latest update:** 2024-04-04 02:14:12
* - **internal_name:**
- infn_saandose_samadha_timeseries
* - **publisher:**
- SAMADHA
* - **alph_code:**
- 75A
* - **id_tmp:**
- 99
* - **short_name:**
- SAA_Ndose
* - **identifier:**
- aspis://infn/saandose_samadha_timeseries
* - **dynamic:**
- one dataset per day (50 kB/day)
* - **size:**
- 50kB
* - **format:**
- text
* - **type:**
- tableset
* - **records_number:**
- 2358
* - **time_start:**
- 2022-10-01
* - **time_stop:**
- 2023-12-31
* - **spatial:**
- Earth's Ground
* - **messenger:**
- neutrons
* - **spectral_min:**
- 0
* - **spectral_max:**
- 0
* - **spectral_units:**
- 0
* - **observable:**
-
* - **latest update:**
- 2024-04-04 02:14:12
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/infn_tgndose_samadha_timeseries.rst
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SAMADHA neutron dose rate at Testa Grigia
=========================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
Monitoring of the neutron dose rate due to cosmic rays at the Testa Grigia Station (3480 m, Cervinia, Italy), to study possible correlation between space weather events and dose rate at the ground. This measurement is part of the INFN project SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) aimed to monitor the neutron dose inside the South Atlantic Anomaly (SAA) region in Bolivia. The data taken at Testa Grigia are a term of comparison for those collected in the SAA region.
**References**
References
~~~~~~~~~~
http://samadha.to.infn.it
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** infn_tgndose_samadha_timeseries
**publisher:** samadha
**alphanumeric_code:** 75B
**id_tmp:** 79
**short_name:** TG_Ndose
**identifier:** aspis://infn/tgndose_samadha_timeseries
**dynamic:** one dataset per day (50 kB/day)
**size:** 50kB
**format:** text
**type:** timeseries
**records_number:** 2835
**time_start:** 2021-09-01
**time_stop:** 2023-12-31
**spatial:** Earth's Ground
**messenger:** neutrons
**spectral_min:** 0
**spectral_max:** 0
**spectral_units:** 0
**observable:**
.. list-table::
**latest update:** 2024-04-04 02:15:39
* - **internal_name:**
- infn_tgndose_samadha_timeseries
* - **publisher:**
- samadha
* - **alph_code:**
- 75B
* - **id_tmp:**
- 79
* - **short_name:**
- TG_Ndose
* - **identifier:**
- aspis://infn/tgndose_samadha_timeseries
* - **dynamic:**
- one dataset per day (50 kB/day)
* - **size:**
- 50kB
* - **format:**
- text
* - **type:**
- timeseries
* - **records_number:**
- 2835
* - **time_start:**
- 2021-09-01
* - **time_stop:**
- 2023-12-31
* - **spatial:**
- Earth's Ground
* - **messenger:**
- neutrons
* - **spectral_min:**
- 0
* - **spectral_max:**
- 0
* - **spectral_units:**
- 0
* - **observable:**
-
* - **latest update:**
- 2024-04-04 02:15:39
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
docs/source/products/data/ingv_alert_aqu_timeseries.rst
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......@@ -2,59 +2,63 @@
INGV geomagnetic data, GIC indices and alert: L'Aquila
======================================================
.. contents:: The tiny table of contents
.. contents:: Table of contents
From both components of GIC index for L'Aquila observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data)
This tableset contains a set of data corresponding to products with ids 8, 47 and 48. In detail it contains the definitive values of the X,Y and Z components (in NEC coordinates) and of total intensity F of the geomagnetic field recorded at ground magnetic observatories managed by INGV. Besides, it contains the values of the GicX and GicY indices calculated from the Y and X components, respectively. To finish it contains values of the risk (i.e. alertX and alertY) , corresponding to the estimated values of the GicX and GicY indices.
Data sampling is of 1-minute.
**References**
References
~~~~~~~~~~
Data description
~~~~~~~~~~~~~~~~
Dataset summary
~~~~~~~~~~~~~~~
**internal_name:** ingv_alert_aqu_timeseries
**publisher:** INGV
**alphanumeric_code:** 48A
**id_tmp:** 80
**short_name:** INGV_AQU_alert
**identifier:** aspis:///ingv/INGV_AQU_alert
**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow.
**size:** 10MB
**format:** csv
**type:** timeseries
**records_number:** 84960
**time_start:** 2012-03-07
**time_stop:** 2017-09-15
**spatial:** GROUND
**messenger:**
**spectral_min:** 1
**spectral_max:** 1
**spectral_units:** 1/minute
**observable:** GIC,GEOINDEX
.. list-table::
**latest update:** 2024-04-04 02:27:54
* - **internal_name:**
- ingv_alert_aqu_timeseries
* - **publisher:**
- INGV
* - **alph_code:**
- 48A
* - **id_tmp:**
- 80
* - **short_name:**
- INGV_AQU_alert
* - **identifier:**
- aspis:///ingv/INGV_AQU_alert
* - **dynamic:**
- This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow.
* - **size:**
- 10MB
* - **format:**
- csv
* - **type:**
- timeseries
* - **records_number:**
- 84960
* - **time_start:**
- 2012-03-07
* - **time_stop:**
- 2017-09-15
* - **spatial:**
- GROUND
* - **messenger:**
-
* - **spectral_min:**
- 1
* - **spectral_max:**
- 1
* - **spectral_units:**
- 1/minute
* - **observable:**
- GIC,GEOINDEX
* - **latest update:**
- 2024-04-04 02:27:54
Columns specification
~~~~~~~~~~~~~~~~~~~~~
......
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