Updated products divided by spatial (f77f83d3) · Commits · caesar / WP2330 / wiki

docs/source/products/data/external_ace_swepam_timeseries.rst

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Original line number	Diff line number	Diff line
		====================
		ACE Solar Wind 1 min
		====================

		.. contents:: Table of contents

		qui dovra' esserci la descrizione del prodotto

		References
		~~~~~~~~~~

		qui invece la bibliografia

		Dataset summary
		~~~~~~~~~~~~~~~

		.. list-table::

		* - 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
		~~~~~~~~~~~~~~~~~~~~~

		.. list-table::
		:widths: 7 20 15 10 48
		:align: right
		:header-rows: 1

		* - progr
		- column
		- units
		- type
		- description
		* - 1
		- time
		- UTC
		- datetime
		- UTC
		* - 2
		- ProtonDensity
		- p/cc
		- double
		- p/cm^3
		* - 3
		- BulkSpeed
		- km/s
		- double
		- km/s
		* - 4
		- IonTemperature
		- K
		- double
		- K

docs/source/products/data/external_flux_goes_timeseries.rst

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Original line number	Diff line number	Diff line
		===============
		GOES X-ray Flux
		===============

		.. contents:: Table of contents

		not available in DBF

		References
		~~~~~~~~~~

		not available in DBF

		Dataset summary
		~~~~~~~~~~~~~~~

		.. list-table::

		* - 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
		~~~~~~~~~~~~~~~~~~~~~

		.. list-table::
		:widths: 7 20 15 10 48
		:align: right
		:header-rows: 1

		* - progr
		- column
		- units
		- type
		- description
		* - 1
		- time
		- UTC
		- datetime
		- UTC
		* - 2
		- Short_Wave
		- Watts/m^2
		- double
		- W/m^2
		* - 3
		- Long_Wave
		- Watts/m^2
		- double
		- W/m^2

docs/source/products/data/external_part_goes_timeseries.rst

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Original line number	Diff line number	Diff line
		================
		GOES proton Flux
		================

		.. contents:: Table of contents

		not available in DBF

		References
		~~~~~~~~~~

		not available in DBF

		Dataset summary
		~~~~~~~~~~~~~~~

		.. list-table::

		* - 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
		~~~~~~~~~~~~~~~~~~~~~

		.. list-table::
		:widths: 7 20 15 10 48
		:align: right
		:header-rows: 1

		* - progr
		- column
		- units
		- type
		- description
		* - 1
		- time
		- UTC
		- datetime
		- UTC
		* - 2
		- P1
		- Protons/cm^2 - s^-1 - sr
		- double
		- >=1Mev integral proton flux 5min average
		* - 3
		- P5
		- Protons/cm^2 - s^-1 - sr
		- double
		- >=5Mev integral proton flux 5min average
		* - 4
		- P10
		- Protons/cm^2 - s^-1 - sr
		- double
		- >=10Mev integral proton flux 5min average
		* - 5
		- P30
		- Protons/cm^2 - s^-1 - sr
		- double
		- >=30Mev integral proton flux 5min average
		* - 6
		- P50
		- Protons/cm^2 - s^-1 - sr
		- double
		- >=50Mev integral proton flux 5min average
		* - 7
		- P100
		- Protons/cm^2 - s^-1 - sr
		- double
		- >=100Mev integral proton flux 5min average
		* - 8
		- E_8
		- Electrons/cm^2 - s^-1 - sr
		- double
		- >=0.8Mev integral electron flux 5min average
		* - 9
		- E2_0
		- Electrons/cm^2 - s^-1 - sr
		- double
		- >=2Mev integral electron flux 5min average
		* - 10
		- E4_0
		- Electrons/cm^2 - s^-1 - sr
		- double
		- >=4Mev integral electron flux 5min average

docs/source/products/data/inaf_cpcp_superdarn_datacube.rst

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Original line number	Diff line number	Diff line
		=============================
		SuperDARN Polar Cap Potential
		=============================

		.. 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
		currently in operation can be seen in Figure 1: INAF-IAPS manages the radar pair of
		Dome C East (DCE) and Dome C North (DCN) located at the Concordia station, in
		Antarctica, whose fields of view are shaded in green in the figure.
		The SuperDARN concept is described in detail in [2]. A SuperDARN radar is a bistatic
		apparatus (i.e. the same antennae and the same electronics are used to both transmit
		and receive signals to/from the ionosphere), which works in the 8-20 MHz frequency
		range: coded sequences of radio pulses are steered through a field of view several tens
		degrees wide along a number of “beams” (directions), so that the whole field of view
		is covered in one or two minutes, depending on the operating mode. Along each beam,
		the pulse sequence defines from 75 to 100 range gates, from 180 km up to 3000 km
		from the radar site, where the radio signals encounter plasma density irregularities in
		the ionosphere, which cause such signals to be scattered back along the same direction.
		As ionospheric irregularities are dragged in the large scale convection at high latitudes, the measure of the Doppler phase shift between the emitted and backscattered waves
		allows to infer the velocity of the ambient plasma with respect to the sounded direction
		and gate.

		References
		~~~~~~~~~~

		https://www.sciencedirect.com/science/article/abs/pii/S136468260600263X

		[1] SuperDARN Data Analysis Working Group, Thomas, E. G., Reimer, A. S., Bland,
		E. C., Burrell, A. G., Grocott, A., Ponomarenko, P. V., Schmidt, M. T., Shepherd, S. G.,
		Sterne, K. T., and Walach, M.-T, SuperDARN Radar Software Toolkit (RST) 5.0 (v5.0).
		Zenodo (2022). https://doi.org/10.5281/zenodo.7467337

		[2] Greenwald, R.A., Baker, K.B., Dudeney, J.R. et al., DARN/SuperDARN, A global
		view of the dynamics of high-latitude convection, Space Sci Rev, 71, 761–796 (1995).
		https://doi.org/10.1007/BF00751350

		[3] Ruohoniemi, J.M., and K.B. Baker, Large-scale imaging of high-latitude
		convection with Super Dual Auroral Radar Network HF radar observations, J. Geophys. Res., Space Physics, 103, 20797-20811 (1998).https://doi.org/10.1029/98JA01288

		[4] Thomas, E. G., and S. G. Shepherd, Statistical Patterns of Ionospheric Convection
		Derived From Mid-latitude, High-Latitude, and Polar SuperDARN HF Radar
		Observations, J. Geophys. Res., Space Physics, 123(4), 3196-3216 (2018).
		https://doi.org/10.1002/2018JA025280

		[5] Baker, K. B., and S. Wing, A new coordinate system for conjugate studies at high latitudes, J. Geophys. Res., 94(A7), 9139 (1989).https://doi.org/10.1029/JA094iA07p09139
		[6] Shepherd, S. G., Altitude-Adjusted Corrected Geomagnetic Coordinates: Definition
		and Functional Approximations, J. Geophys. Res., Space Physics, 119(9), 7501-7521
		(2014). https://doi.org/10.1002/2014JA020264

		Dataset summary
		~~~~~~~~~~~~~~~

		.. list-table::

		* - 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
		~~~~~~~~~~~~~~~~~~~~~

		.. list-table::
		:widths: 7 20 15 10 48
		:align: right
		:header-rows: 1

		* - progr
		- column
		- units
		- type
		- description
		* - 1
		- time
		- UTC
		- datetime
		- Time representation ISO8601: YYYY-MO-DYTHR:MN:SC
		* - 2
		- hem
		-
		- string
		- Flag identifying the hemisphere where data are taken for a given record. “N”=North; “S”=South
		* - 3
		- ndata
		- counts
		- int
		- Number of velocity vectors actually measured by the radars in the given time interval
		* - 4
		- minlat
		- deg
		- int
		- Low latitude limit for the convection: it is the 0 described in Section 2.
		* - 5
		- latpole
		- deg
		- float
		- Geographic latitude of the AACGM pole (North or South). It can be useful for coordinate transformations.
		* - 6
		- lonpole
		- deg
		- float
		- Geographic longitude of the AACGM pole (North or South). It can be useful for coordinate transformations.
		* - 7
		- radpole
		- Earth radii (Re=6371.2 km)
		- float
		- Distance from the centre of the Earth of the AACGM pole.
		* - 8
		- imfbx
		- nT
		- float
		- GSM* x component of the interplanetary magnetic field. Data are taken from DSCOVR spacecraft, ballistically propagated to the centre of the Earth, median filtered and averaged in the 2 minutes time intervals of the radar scans. IMF is used to select the model patterns to be added to the measured vectors in order to reconstruct convection in the whole polar cap.
		* - 9
		- imfby
		- nT
		- float
		- GSM* y component of the interplanetary magnetic field.
		* - 10
		- imfbz
		- nT
		- float
		- GSM* z component of the interplanetary magnetic field.
		* - 11
		- imfbt
		- nT
		- float
		- IMF strength. Btot = sqrt(Bx^2 + By^2 + Bz^2)
		* - 12
		- kpr
		-
		- string
		- Range of geomagnetic Kp index during the given time interval. This parameter is used to select the model patterns to be added to the measured vectors in order to reconstruct convection in the whole polar cap. This field represents an information useful to be reported in the convection maps.
		* - 13
		- cpcp
		- V
		- float
		- Cross Polar Cap Potential: Maximum potential difference through the polar cap.
		* - 14
		- maxpot
		- V
		- float
		- Maximum positive value of the electric potential.
		* - 15
		- minpot
		- V
		- float
		- Minimum negative value of the electric potential.
		* - 16
		- l
		- counts
		- int
		- l-order of the harmonic expansion of the potential.
		* - 17
		- m
		- counts
		- int
		- m-order of the harmonic expansion of the potential. -l ≤ m ≤ l
		* - 18
		- coef
		- V
		- float
		- Alm coefficient of the harmonic expansion of the potential. If m<0, then the coefficient is the Blm in Eq. 2.

docs/source/products/data/inaf_data_solopas_timeseries.rst

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Original line number	Diff line number	Diff line
		================================
		INAF-IAPS Solar Orbiter-PAS data
		================================

		.. 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
		~~~~~~~~~~

		R. D’Amicis et al, Astronomy &Astrophysics 656, A21 (2021)

		B. Lavraud et al, Astronomy &Astrophysics 656, A37 (2021)

		D. Perrone et al, Astronomy &Astrophysics 668, A189 (2022)

		R. De Marco et al, Astronomy &Astrophysics, 669, A108 (2023)

		Dataset summary
		~~~~~~~~~~~~~~~

		.. list-table::

		* - 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
		~~~~~~~~~~~~~~~~~~~~~

		.. list-table::
		:widths: 7 20 15 10 48
		:align: right
		:header-rows: 1

		* - progr
		- column
		- units
		- type
		- description
		* - 1
		- time
		- UTC
		- datetime
		- Datetime [UTC ]
		* - 2
		- N
		- cm^-3
		- float
		- Protono Density [cm^-3]
		* - 3
		- VR
		- Km/s
		- float
		- Proton Velocity along the R direction [Km/s]
		* - 4
		- VT
		- Km/s
		- float
		- Proton Velocity along the T direction [Km/s]
		* - 5
		- VN
		- Km/s
		- float
		- Proton Velocity along the N direction [Km/s]
		* - 6
		- T
		- eV
		- float
		- Proton Temperature [eV]
		* - 7
		- VR_SolO
		- Km/s
		- float
		- Spacecraft Velocity along the R direction [Km/s]
		* - 8
		- VT_SolO
		- Km/s
		- float
		- Spacecraft Velocity along the T direction [Km/s]
		* - 9
		- VN_SolO
		- Km/s
		- float
		- Spacecraft Velocity along the N direction [Km/s]