<_Note>Nodes prefixed with a _ are not valid SPASE, but are included for debugging. Values prefixed with a x_ are not valid SPASE but may considered for addition for completeness. 2.6.1 <_MasterURL>https://cdaweb.gsfc.nasa.gov/pub/software/cdawlib/0JSONS/ia_k0_epi_00000000_v01.json (from all.xml) spase://NASA/NumericalData/Interball-2/DOK2A/KP/PT120S <_ResourceID>Source: https://github.com/rweigel/cdawmeta-spase/blob/main/ResourceID.json Interball Auroral Energetic Particle Instruments, KeyParameters <_ResourceName>Source: Master/CDFglobalAttributes/Logical_source_description IA_K0_EPI <_AlternateName>Source: Master/CDFglobalAttributes/Logical_source <_Rights> SPDX Creative Commons Zero v1.0 Universal https://spdx.org/licenses/CC0-1.0.html https://spdx.org/licenses/ Auroral Probe Energetic Particle Fluxes <_DOI>Source: https://github.com/rweigel/cdawmeta-spase/blob/main/DOI.json <_AccessInformation>Source: https://github.com/rweigel/cdawmeta-spase/blob/main/AccessInformation.json 1996-09-03T09:39:00Z 1997-10-30T12:51:00Z <_TemporalDescription>Generated from all.xml/@timerange_start and all.xml/@timerange_stop PT2M <_Cadence>Counts based on variable 'Epoch' in https://cdaweb.gsfc.nasa.gov/sp_phys/data/interball/aurora/epi/1996/ia_k0_epi_19960903_v01.cdf. The most common cadence, 120000 [ms] = PT2M, occurred for 99.4764% of the 380 timesteps. <_ObservedRegion>Source: https://github.com/rweigel/cdawmeta-spase/blob/main/ObservedRegion.json <_ProcessingLevel>Processing level is not available in the master file; it should be there instead of, say, https://github.com/rweigel/cdawmeta-spase/blob/main/ProcessingLevel.json spase://SMWG/Instrument/Interball-2/DOK2A EnergeticParticles spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia HTTPS from SPDF https://cdaweb.gsfc.nasa.gov/pub/data/interball/aurora/epi In CDF via HTTP from CDAWeb ia_k0_epi_%Y%m%d_%Q.cdf %Y IA_K0_EPI CDF spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia FTPS from SPDF ftps://cdaweb.gsfc.nasa.gov/pub/data/interball/aurora/epi In CDF via HTTP from CDAWeb ia_k0_epi_%Y%m%d_%Q.cdf %Y IA_K0_EPI CDF spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia CDAWeb Web Service https://cdaweb.gsfc.nasa.gov/WebServices/ Instructions for using web services to access this dataset an other other metadata and options for CDAWeb datasets. The ProductKey here corresponds to the query parameter 'dataset' in the tables at the AccessURL in a dataset-related request can be made. IA_K0_EPI CDF CSV GIF NetCDF PNG PS PDF XML x_Script.IDL x_Script.Python Text.ASCII x_WAV spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia CDAWeb Web Service user interface https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?index=sp_phys&dataset=IA_K0_EPI IA_K0_EPI Web service user interface for this product. CDF GIF PDF Text.ASCII x_WAV spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia CDAWeb Python Script https://cdaweb.gsfc.nasa.gov/WS/cdasr/1/dataviews/sp_phys/datasets/IA_K0_EPI/clientLibraryExample/ IA_K0_EPI Web service that generates a Python script to access this product. x_Script.IDL x_Script.Python spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/SSCWeb. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia 4D Orbit Viewer https://sscweb.gsfc.nasa.gov/4dorbit/?sc=IA_K0_EPI IA_K0_EPI Web Service to this product. HTML spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb and the HAPI project. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia CDAWeb HAPI Server https://hapi-server.org/servers/#server=CDAWeb&dataset=IA_K0_EPI IA_K0_EPI Web Service to this product using the HAPI interface. CSV JSON Binary spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb and the HAPI project. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia CDAWeb HAPI Script in Multiple Languages https://hapi-server.org/servers/#server=CDAWeb&dataset=IA_K0_EPI&return=script IA_K0_EPI Web Service user interface that generates scripts in IDL, Javascript, MATLAB, Python, Autoplot, curl, wget to access this product. See https://hapi-server.org/servers/api for the API. x_Script.IDL x_Script.Javascript x_Script.MATLAB x_Script.Python x_Script.Autoplot x_Script.curl x_Script.wget spase://SMWG/Repository/NASA/GSFC/SPDF Online Open SPDF/CDAWeb and the HAPI project. Please also acknowledge the data producer: DOK-2: K.Kudela at DOK-2: Institute of experimental physics Slovak Acad. Sci., Kosize, Slovakia HAPI visualizations https://hapi-server.org/plot/?server=https://cdaweb.gsfc.nasa.gov/hapi&dataset=IA_K0_EPI&format=gallery IA_K0_EPI Web Service that generates plots. See https://hapi-server.org/plot/ for the API. PNG PDF SVG Interball Auroral Probe (from all.xml/observatory/description/@short) Auroral Probe Energetic Particle Instrument (from all.xml/instrument/description/@short) Space Physics (from Master/CDFglobalAttributes/Discipline) Magnetospheric Science (from Master/CDFglobalAttributes/Discipline) INTERBALL-AURORAL (from Master/CDFglobalAttributes/Source_name) Interball Auroral Probe (from Master/CDFglobalAttributes/Source_name) K0 (from Master/CDFglobalAttributes/Data_type) Key Parameter (from Master/CDFglobalAttributes/Data_type) EPI (from all.xml/instrument/@ID) Earth.Magnetosphere Heliosphere.NearEarth Time Epoch CATDESC: 'Time, centered'. Notes not in Master CDF: 'The units are the units in CDF files. For other web services, this variable is may be represented as a time string.' ms Scalar Temporal Electron Flux, 26-29 keV Fe1 Master CDF CATDESC: 'Electron Flux, 26-29 keV (DOK-2 firstelectron sensor, fixed)'. Master CDF VAR_NOTES: 'sensor offset at an angle 180 deg withrespect to the sunward directed spacecraft spin axis'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' no/cm^2/s/keV/st -1e+31 Electron Flux, 25-28 keV Fe2 Master CDF CATDESC: 'Electron Flux, 25-28 keV (DOK-2 firstelectron sensor, fixed)'. Master CDF VAR_NOTES: 'sensor offset at an angle 180 deg withrespect to the sunward directed spacecraft spin axis'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' no/cm^2/s/keV/st -1e+31 Proton Flux, 18-24 keV Fp1 Master CDF CATDESC: 'Proton Flux, 18-24 keV (DOK-2 first proton sensor, fixed)'. Master CDF VAR_NOTES: 'sensor offset at an angle 180 deg withrespect to the sunward directed spacecraft spin axis'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' no/cm^2/s/keV/st -1e+31 Proton Flux, 20-26 keV Fp2 Master CDF CATDESC: 'Proton Flux, 20-26 keV (DOK-2 second proton sensor, scan)'. Master CDF VAR_NOTES: 'The value is taken from the sensorthat can scan the angle's interval 45-180deg or can be fixed at angles 45, 90,135, 180 deg. with respect to the sunward directed spacecraft spin axis'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' no/cm^2/s/keV/st -1e+31 SF, DOK-2 1st electron range SF_Fe1 Master CDF CATDESC: 'Status Flag: energy and positioncoded, see description'. Master CDF VAR_NOTES: 'Standard flags are used in the case ofdata absence. SFs are set to 11-15 and21-25 for all valid data values ofeach parameter. Most significant digit (1- low or 2 - high) indicates level of the energy threshold. Higher energy threshold will be used only in case ofdegradation of a sensor. Less significant digit indicates sensor orientation ( 1, 2, 3, 4, 5 correspondrespectively to 45, 90, 135, 180 deg.and scan)'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' 128 SF, DOK-2 2nd electron range SF_Fe2 Master CDF CATDESC: 'Status Flag: energy and positioncoded, see description'. Master CDF VAR_NOTES: 'Standard flags are used in the case ofdata absence. SFs are set to 11-15 and21-25 for all valid data values ofeach parameter. Most significant digit (1- low or 2 - high) indicates level of the energy threshold. Higher energy threshold will be used only in case ofdegradation of a sensor. Less significant digit indicates sensor orientation ( 1, 2, 3, 4, 5 correspondrespectively to 45, 90, 135, 180 deg.and scan)'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' 128 SF, DOK-2 1st proton sensor SF_Fp1 Master CDF CATDESC: 'Status Flag: energy and position coded, see description'. Master CDF VAR_NOTES: 'Standard flags are used in the case ofdata absence. SFs are set to 11-15 and21-25 for all valid data values of each parameter. Most significant digit (1- low or 2 - high) indicates level of the energy threshold. Higher energy threshold will be used only in case ofdegradation of a sensor. Less significant digit indicates sensor orientation ( 1, 2, 3, 4, 5 correspondrespectively to 45, 90, 135, 180 deg.and scan)'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' 128 SF, DOK-2 2nd proton sensor SF_Fp2 Master CDF CATDESC: 'Status Flag: energy and position coded, see description'. Master CDF VAR_NOTES: 'Standard flags are used in the case ofdata absence. SFs are set to 11-15 and21-25 for all valid data values of each parameter. Most significant digit (1- low or 2 - high) indicates level of the energy threshold. Higher energy threshold will be used only in case ofdegradation of a sensor. Less significant digit indicates sensor orientation ( 1, 2, 3, 4, 5 correspondrespectively to 45, 90, 135, 180 deg.and scan)'. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' 128 Post Gap Flag Gap_Flag Master CDF CATDESC: 'Post Gap Flag (0 no gap before this point, 1-5 gap reason)'. Master CDF VAR_NOTES: ' '. Notes not in Master CDF: 'The time index (the ISTP DEPEND_0 variable) for this parameter is Epoch.' -2147483648