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
orearth
: 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.
- if it's
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_LINK
http://amda.cdpp.eu
Instrument_type
Value of node Instrument/InstrumentType
from the Instrument SPASE file corresponding to the granule.
Ex:
ElectrostaticAnalyser
LINK_TEXT
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
LINK_TITLE
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 :
- is the value of node
NumericalData/ProviderName
from the SPASE file NumericalData corresponding to the granule, or CDPP if the value doesn't exist. and is kept from this dictionary (according to ).
MAPSKP: http://mapskp.cesr.fr/use_policy
MAVEN: http://lasp.colorado.edu/home/maven/files/2014/09/MAVEN_public-rules-of-the-road-v3.pdf
CASSINI/RPWS/SKR: http://amda.irap.omp.eu/help/SKR.html
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