CDF_spec.md 9.02 KB

Formating CDF files for AMDADB

This specification follows the ISTP guidelines, see the ISTP guide.


Global CDF attributes

See the ISTP guidelines for global attributes.

Acknowledgement

Value of node NumericalData/ResourceHeader/Acknowledgement from SPASE file NumericalData corresponding to the granule.

Ex:

NASA, Prof. Henri Reme, European Space Agency

Data_type

Dataset name

Ex:

PRP

Data_version

1

Descriptor

Instrument name

Ex:

CIS

Discipline

  • If target name is sun or earth : Space Physics
  • otherwise, look for node value of NumericalData/ObservedRegion from the NumericalData SPASE file corresponding to the granule:
    • if it's Magnetosphere: Space Physics>Magnetospheric Science;
    • if it's NearSurface: Space Physics>Ionospheric Science;
    • if it's Heliosphere: Space Physics>Interplanetary Studies.

Generated_by

CDPP>Centre de Donnees de la Physique des Plasmas

Generation_date

Value of node NumericalData/ResourceHeader/ReleaseDate from the NumericalData SPASE file corresponding to the granule, formated as yyyymmdd.

Ex:

20151019
http://amda.cdpp.eu

Instrument_type

Value of node Instrument/InstrumentType from the Instrument SPASE file corresponding to the granule.

Ex:

ElectrostaticAnalyser

Value of node NumericalData/ResourceHeader/AlternateName from the NumericalData SPASE file corresponding to the granule + data are available at.

Ex:

Cluster 1 Prime Parameter CIS data data are available at
CDPP AMDA DATABASE

Logical_file_id

Dataset name + _ + start_time epn-core value, formated as YYYYMMDDHHMMSS.

Note: This is actually the file name without extension.

Ex

CLUST1_CIS_PRP_19900302040000

Logical_source

Dataset name

Ex:

CLUST1_CIS_PRP

Logical_source_description

Value of node NumericalData/ResourceHeader/Description from the NumericalData SPASE file corresponding to the granule.

Ex:

This instrument (CIS: Cluster Ion Spectrometry) is capable of obtaining full 3D ion distributions with high time resolution (in one spacecraft spin) and mass-per-charge resolution. The experiment consists of [...]

Mission_group

  • Last element of the value of node Observatory/ObservatoryGroupID from the Observatory SPASE file corresponding to the granule.
  • if the node doesn't exist: value of node Observatory/ResourceName.

Ex:

Cluster

MODS

Extracted from NetCDF AMDA internal data.

Parents

The NetCDF file name.

Ex

CLUST1_CIS_PRP_19900302040000.nc

PI_affiliation

Value of node Person/OrganisationName from the Person SPASE file corresponding to the granule.

Ex

ESTEC, ESA

PI_name

Value of node NumericalData/Contact/PersonID where Role node value is PrincipalInvestigator, from the NumericalData SPASE file corresponding to the granule.

Ex:

Henri.Reme

Project

A list with:

  • CDPP>Centre de Donnees de la Physique des Plasmas
  • the value of node NumericalData/ProviderName, from the NumericalData SPASE file corresponding to the granule.

Ex:

- CDPP>Centre de Donnees de la Physique des Plasmas
- CSDS-CNES

Rules_of_use

System Use Policy

Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse."

Data use policy from originating <NAME> data center: <URL>

where :

Ex:

System Use Policy

Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse."

Data use policy from originating CDPP data center: http://amda.irap.omp.eu/help/licenceAction.do.html

Software_version

Version of the NetCDF to CDF converter.

Source_name

The mission name

Ex:

clust1

TEXT

The value of node NumericalData/ResourceHeader/InformationURL/Name + , + the value of node NumericalData/ResourceHeader/InformationURL/URL, from the SPASE file NumericalData corresponding to the granule.

Ex:

NSSDC Master Catalog listing for Cluster II Rumba Cluster Ion Spectrometry (CIS), http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02

Time_resolution

time_sampling_step value of epn-core, in seconds + seconds.

Ex:

3 seconds

TITLE

The value of node NumericalData/ResourceHeader/AlternateName, from the SPASE file NumericalData corresponding to the granule.

Ex:

Cluster 1 Prime Parameter CIS data

PDS_Start_time

time_min value of epn-core, in ISO time.

Ex:

2007-02-13T09:08:43Z

PDS_Stop_time

time_max value of epn-core, in ISO time.

Ex:

2007-02-14T09:08:43Z

PDS_Observation_target

target_name value of epn-core. Use a list of values if necessary (split the # character).

Ex:

Saturn

Observation_type

Look for the child node in NumericalData/Parameter node, from the SPASE file NumericalData corresponding to the granule.

It is one of: Field, Particules, Wave, Mixed, Support.

Ex:

Particle

Other epn-core parameters

Add other epn-core parameters, with VESPA_ prefix, only if:

  • the value is not empty;
  • this is not the same value as the other element of a tuple (ie min/max).

Ex:

- VESPA_spase_measurement_type: EnergeticParticles
- VESPA_spatial_frame_type: cartesian

Variable attributes (TBC)

See the ISTP guidelines for variables.

To create new variables with [spacepy.pycdf)(http://pythonhosted.org/SpacePy/pycdf.html), use cdf.new() and not attr[].

To name variables, use the NumericalData/Parameter/ParameterKey parameter from the SPASE file.

CATDESC

type: CDF_CHAR

The value of node NumericalData/Parameter/Description.

Ex

Flux density spectrogram measured on the RH polarized array.

DEPEND_0

type : CDF_CHAR

Epoch

LABL_PTR_1

Note: Only if the node value of NumericalData/Parameter/RenderingHints is time series and the node NumericalData/Parameter/Structure exist.

Note 2: LABL_PTR_1 and DEPEND_1 can not are both presents.

Step 1: Get the labels, which are the nodes value of NumericalData/Parameter/Structure/Element/Name.

Ex (for skr151150000.nc.gz):

- RH 100-400kHz
- LH 100-400kHz
- RH 10-1000kHz
- RH 10-1000kHz

Step 2: Create a new variable stored with these labels. Then LABL_PTR_1 is the ID of this variable.

DEPEND_1

Note: Only if the node value of NumericalData/Parameter/RenderingHints is spectrogram.

Note 2: LABL_PTR_1 and DEPEND_1 can not are both presents.

type : CDF_CHAR

From the file <dataset_name>_info from the dataset directory, look for energy or frequency variables value.

DICT_KEY

type: CDF_CHAR

Ex:

electric_field>power

DISPLAY_TYPE

type: CDF_CHAR

Ex:

time_series

FIELDNAM

type: CDF_CHAR

Ex:

RR

FILLVAL

type: CDF_UINT1

Ex:

255

LABLAXIS

type: CDF_CHAR

Ex:

RH flux density

UNITS

type: CDF_CHAR

Ex:

dB

VALIDMIN

type: CDF_UINT1

Ex:

0

VALIDMAX

type: CDF_UINT1

Ex:

255

VAR_TYPE

type: CDF_CHAR

Ex:

data

SCALETYP

type: CDF_CHAR

Ex:

lin

SCALEMIN

type: CDF_UINT1

Ex:

0

SCALEMAX

Ex:

255

UCD