cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.24400/802406/0skd-dp15
title: CLU3 WHISPER passive electric power spectral density when in sounding mode

description: This dataset contains the electric power spectral density determined on Cluster-3 during passive sweeps of the WHISPER sounder which occur when the sounder is nominally active. These passive sweeps are interspersed with active sweeps to assist the identification of plasma resonances by comparison of active and passive sweeps adjéacent in time. These sweeps are certainly not active sweeps, but neither are they all 100% free of echoes from nearby active sweeps. The following support parameters are provided : Receiving antenna used, Ey or Ez Spectral Frequencies between 1.953 and 79.915 kHz, that is, the frequencies corresponding point-to-point to the 512 elements of the fixed size spectrum Frequency Table Number between 0 and 127 Time interval between two successive emission pulses in units of 40/3 (= 13.3) ms : 0: 1 unit (13.3 ms) 1: 2 units (26.6 ms) 2: 3 units (40 ms) 3: 5 units (66.6 ms) 4: 8 units (106.6 ms) 5: 40 units + 2106.66 ms waiting + 256 units + 2446.66 ms waiting (8.5 s) 6: 6 units + 45 ms waiting (125 ms) 7: 14 units + 63.34 ms waiting (250 ms). Delay between the acquisition intervals used to form the passive spectrum information and the acquisition intervals used to form the correponding active spectrum information Number of gain changes during the acquisition First part of the compressed value which is a fixed point integer defined in the compression algorithm Second part of the compressed value
DOI: 10.24400/802406/6pv3-2p9v
title: CLU3 WHISPER Event information under natural mode

description: This Event Table shows the telecomand status of the WHISPER sounder on the Cluster-3 spacecraft when passive (i.e., when measuring natural plasma waves). For each time interval, the following information is provided : time_tags__C1_CT_WHI_NATURAL_EVENT : The time interval fft_size__C1_CT_WHI_NATURAL_EVENT : The number of frequency bins of the Fast Fourier Transform Receiving_Antenna__C1_CT_WHI_NATURAL_EVENT : The receiving antenna used, Ey or Ez Average_Number__C1_CT_WHI_NATURAL_EVENT : The number of averaged individual spectra. Individual spectra are produced at the rate of one every 13.33 ms Gain_Command__C1_CT_WHI_NATURAL_EVENT : The gain command number : 0: fixed gain +12dB 1: fixed gain +24dB 2: fixed gain +36dB 3: fixed gain +36dB 4: automatic gain+24/+12 dB 5: automatic gain +24/+12 dB 6: automatic gain +36/+24 dB 7: automatic gain +36/+24 dB) Averaged_Spectrum_Select_Rate__C1_CT_WHI_NATURAL_EVENT: Output rate of the averaged spectra Energy_Overflow_Averaging_Flag__C1_CT_WHI_NATURAL_EVENT : Averaging status: 0: OFF 1: ON Compression_Methode_Required__C1_CT_WHI_NATURAL_EVENT: 0 if the exponent size is adjusted 1 if the exponent size is fixed to 5 Compressed_Data_Size__C1_CT_WHI_NATURAL_EVENT : Compressed data size: 0 means 8 bits, 1 means 6 bits
DOI: 10.24400/802406/8svy-d5qz
title: CLU3 WHISPER Information about pulse emission under sounding mode

description: The WHISPER housekeeping datasets contain information about pulse emission used for the WHISPER sounding on Cluster-3. Sounding Pulse time tag Frequency value (kHz) of the emitted sinusoidal wave train Peak-to-peak amplitude of the emitted pulse (V) Duration of the emission (ms) Confidence flag which shows the instantaneous status of the WHISPER sounder : 0 : Sounder OFF 1 : Sounder ON
DOI: 10.24400/802406/bd0a-pybk
title: CLU3 WHISPER electric field power spectral density of natural waves

description: This dataset contains the electric field power spectral density observed by WHISPER on Cluster-3. Compared to the WHI_NATURAL and WHI_ACTIVE datasets, the particularity of this dataset is that bandwidth of the measurements is large, so as to optimise the time resolution. The dataset includes data obtained both when the sounder is active and passive (natural waves). The support data includes : a flag to indicate sounder activity the number of elementary spectra which have been summed. Individual spectral are acquired every 13.33 ms, and these spectra are averaged to improve the statistics. an indicator of how many, if any, of the individual spectra were saturated.
DOI: 10.24400/802406/k4yn-yk03
title: CLU3 WHISPER electric power spectral density in sounding mode

description: This dataset contains electric field power spectral density measured on Cluster-3 by WHISPER when the sounder is active. Each data record contains the following support parameters : Interval centred time tag Receiving antenna used, Ey or Ez Spectral Frequencies between 1.953 and 79.915 kHz, that is, the frequencies corresponding point to point to the 512 elements of the fixed size spectrum Frequency Swept Table Number between 0 and 127 Time interval between two successive emission pulses in units of 40/3 (= 13.3) ms : 0: 1 unit (13.3 ms), 1: 2 units (26.6 ms) , 2: 3 units (40 ms), 3: 5 units (66.6 ms), 4: 8 units (106.6 ms), 5: 40 units + 2106.66 ms waiting + 256 units + 2446.66 ms waiting (8.5 s), 6: 6 units + 45 ms waiting (125 ms), 7: 14 units + 63.34 ms waiting (250 ms). Delay between the leading edge of the emission pulse and the starting edge of the associated reception (acquisition time interval) Number of gain changes during the acquisition First part of the compressed value which is a fixed point integer defined in the compression algorithm
DOI: 10.24400/802406/2150-f6bd
title: CLU3 WHISPER Active to Passive Spectral Power Density Coded Ratio

description: This dataset contains e active to passive power spectral density ratio when WHISPER is in sounding mode on Cluster 3. 512 values, one for each frequency, indicating the ratio (Active received power) / (Passive received power), coded as follows : 0: indicate Active/Passive &lt;= 2 1: 2 &lt; Active/Passive &lt;= 4 2: 4 &lt; Active/Passive &lt;= 16 3: 16 &lt; Active/Passive
DOI: 10.24400/802406/6bha-6b8h
title: CLU3 WHISPER Timings of soundings

description: This dataset contains central time tags of WHISPER soundings on Cluster 3 followed by half the number of seconds corresponding to the sampling time interval
DOI: 10.24400/802406/z1wk-axf9
title: CLU3 WHISPER Electron Density

description: This dataset contains plasma frequencies from Whisper on spacecraft Cluster-3.
DOI: 10.24400/802406/h15b-a67h
title: Cluster 3 STAFF Prime Parameters

description: This data set contains the Cluster 3 STAFF Prime Parameters (spin time resolution) : the parallel and perpendicular (to the FGM measured magnetic field) power of the magnetic field and the power of the spin-plane components of the electric field for several frequency ranges. Caveats The STAFF prime parameters do not have the standard CSDS timing which is synchronous with the spacecraft spin clock. The operation of the STAFF digital spectrum analyser is synchronised with the DWP clock. The summary parameters are the average of all those instrument measurements made during STAFF 4 s periods whose middle times lie within the minute boundaries. The difference from the standard CSDS definition is negligible for all practical purposes. The summary parameter and prime parameter E_pow_f2 is supplied by STAFF only when the satellites are in normal mode. In burst mode both STAFF and EFW measure the waveform to 180 Hz, and the onboard spectrum analyser is not used to determine the spectrum in the band 10--180 Hz. The parameters B_pow_f2, E_pow_f2, B_par_f2, and B_perp_f2 are determined from the waveform measurements which, in the case of the electric field, come from EFW. Thus in normal mode the parameter E_pow_f2 is supplied by STAFF, while in burst mode it is replaced by the parameter of the same name from the EFW experiment.
DOI: 10.24400/802406/nczt-eh3a
title: CLU3 STAFF-SA Caveats - Power Spectral Density negative values

description: This dataset contains caveats for the SM datasets from the STAFF-SA instrument on Cluster 3 spacecraft. For a given time and frequency are given the PSD negative values that have been replaced in the PSD data product by a fillvalue.
DOI: 10.24400/802406/bxbp-qyh4
title: CLU3 STAFF-SA Caveats - Probe failure consequences

description: This dataset contains caveats for PSD, SM and PPP STAFF_SA datasets from the STAFF-SA instrument on Cluster 3 spacecraft. This caveats dataset provides the users time interval when probes have problems and what to do with such data.
DOI: 10.24400/802406/yhn7-9ec4
title: CLU3 STAFF-SA Caveats - Polarization and Propagation Parameters

description: This dataset contains caveats for the PPP (L3) datasets from the STAFF-SA instrument on Cluster 3 spacecraft. Here are given times where there are either low coverage FGM data or too low attitudes magnetic field to transform SM data in MFA coordinate system.
DOI: 10.24400/802406/cxzf-s74p
title: CLU3 STAFF Caveats - Information concerning onboard calibration

description: This data set contains Cluster 3 STAFF Caveats - Information concerning onboard calibration.
DOI: 10.24400/802406/mntx-gn3y
title: CLU3 STAFF Caveats - Time Interval with no Sun Reference Pulse

description: This dataset contains caveats for the SM and PSD datasets from the STAFF-SA instrument on Cluster 3. This caveats dataset provides the users time interval when no Sun pulse (TSRP) was recorded in the S/C housekeeping data. Note that it can be in eclipse period but not especially.
DOI: 10.24400/802406/gad9-a9tb
title: CLU3 STAFF-SC Magnetic Field Waveform - Uncalibrated (25Hz sampling)

description: This dataset contains 0.400000E-01 s resolution measurements of the magnetic field Decommutated WaveForm (DWF) from the STAFF-SC instrument in NBR (Normal Bit Rate) mode on the Cluster C3 spacecraft.
DOI: 10.24400/802406/pbxq-qxg0
title: CLU1 STAFF-SC Magnetic Field Waveform - Uncalibrated (burst - 450Hz sampling)

description: This dataset contains 0.002222 s resolution measurements of the magnetic field Decommutated WaveForm (DWF) from the STAFF-SC instrument in HBR (High Bit Rate) mode on the Cluster C3 spacecraft.
DOI: 10.24400/802406/n3cy-r5w0
title: CLU3 STAFF-SA Automatic Gain Control

description: This data set contains the Cluster 3 STAFF-SA average power spectral density in the passband of the analogue receivers derived from the Automatic Gain Control signal. This is measured in three large passbands with 1 s time resolution, for the axial component of the magnetic field, and the sums of the spin plane components of the magnetic and of the electric field.
DOI: 10.24400/802406/wq53-pb7j
title: Cluster 3 PEACE Prime Parameters

description: This data set contains the Cluster 3 PEACE Prime Parameters (spin averaged). The parameters are the electron density, velocity, temperature and heat flux (derived from a subset of the moment sums calculated onboard) and instrument status. Caveats At the time of writing (March 2002) the moments data provided to CSDS are being derived only from HEEA. Thus the minimum measured electron energy is typically about 34 eV opposed to 10 eV when LEEA is included. This approach is an initial response to the frequently occurring situation that the spacecraft potential does rise above 10 volts. The spacecraft potential is at times above 34 volts, in which case the moments calculations will be include measurements of both plasma and spacecraft electrons and will not accurately describe the plasma population. These cases can usually be recognised as they have particularly high density. The spacecraft potential, when uncontrolled by ASPOC, can often reach such values, particularly in thinner plasmas (e.g., magnetotail lobes, polar cap, etc.) The CSDS Quicklook plots show spacecraft potential from EFW which will further inform the interested reader about which regions characteristically have high spacecraft potential. ASPOC operations do not occur on Spacecraft 1 at all. On about 50% of the orbits there are no ASPOC operations on the other spacecraft, and operations are typically for less than 10 hours at a time when ASPOC is in use. The PEACE Team are reconsidering their approach to provision of and validation of electron moments data to the CSDS, in the light of the problems with spacecraft potential. The PEACE team will report on the outcome in a future update of this document. Please for further relevant information consult the PEACE home page (https://www.mssl.ucl.ac.uk/www_plasma/missions/cluster/).
DOI: 10.24400/802406/v18j-jgg8
title: Cluster 3 JSOC Catalogues Identified Scientific Events

description: Cluster 3 JSOC Catalogues Identified Scientific Events
DOI: 10.24400/802406/vexy-j7wh
title: Cluster 3 FGM Prime Parameters

description: This data set contains the Cluster 3 FGM Prime Parameters (spin averaged). The parameters are a status word, the three averaged components of the magnetic field vector in the GSE coordinate system and 2 variances.
DOI: 10.24400/802406/can7-afpf
title: Cluster 3 orbit data (GSE frame, 1 min resolution)

description: This data set contais Cluster 3 ephemeris data (position and velocity). Each ASCII file represents one day. The coordinate system used is GSE (Geocentric Solar Ecliptic). Data record are arranged chronologically.
DOI: 10.24400/802406/dceg-z3r4
title: Cluster 3 EFW Prime Parameters

description: This data set contains the Cluster 3 EFW Prime Parameters (spin averaged). Caveats The CSDS data are intended for event identification and are not for publication. Some obviously incorrect data have been removed in the validation process, but there may still be occasional data with poor quality in the PPDB and SPDB. Please always contact the EFW PI or the CSDS file validator (information given in the global attributes of each CDF file) for questions on data validity. The electric field E_dusk has not been corrected for offsets present due to, e.g., photoelectron asymmetries. The parameter U_probe_sc can be used as an approximate indicator of the electron density, except during periods when ASPOC is operating. Such periods have not been removed from the data. A more (less) negative value of U_probe_sc indicates lower (higher) density. The operation of WHISPER in the active mode sometimes disturbs the EFW measurements. Such disturbed data have most likely been removed in all quantities except U_probe_sc, where the disturbance is least severe.
DOI: 10.24400/802406/xzhb-6e81
title: Cluster 3 EDI Prime Parameters

description: This data set contains the Cluster 3 EDI Prime Parameters. Those parameters are the 3 components of the electron drift velocity and the 3 components of the electric field (cartesian components, GSE coordinates, corrected for spacecraft motion), the instrument status and a Reduced chi-squared variable which is a floating point scalar. Caveats The measured electron drift velocity cannot always be separated into the electric-field and magnetic-gradient induced parts. In such cases the computed electric fields are subject to contamination by magnetic gradient effects. The data quality is variable, and it is therefore mandatory that the status bytes be consulted before interpreting the data. The number of samples in the averages is variable.
DOI: 10.24400/802406/c6pa-092h
title: Cluster 3 DWP Prime Parameters

description: This data set contains Cluster 3 Digital Wave Processor (DWP) prime parameters (various instrument status and data status flags as well as particle correlator information).
DOI: 10.24400/802406/qn4d-0y9f
title: Cluster 3 CIS Selected Modes

description: This dataset contains CIS status indicators for spacecraft Cluster 3 : Telemetry rate, CIS operational mode, CODIF and HIA operating flags, CIS Solar-wind mode flag - CODIF sensitivity (HS/LS), CODIF RPA and Magnetosheath modes flags
DOI: 10.24400/802406/b0h2-4ra6
title: Cluster 3 CIS-HIA Onboard Moments

description: This dataset contains CIS-HIA (Hot Ion Analyser) onboard computed moments for spacecraft Cluster3
DOI: 10.24400/802406/12kq-tmg0
title: Cluster 3 CIS-HIA 3D Ion Distrib. LS, Solar Wind Mode, Raw Counts

description: This dataset contains 3D Ion distributions (raw particle counts) from the CIS-HIA instrument on the Cluster C3 spacecraft in Low-Sensitivity
DOI: 10.24400/802406/ak0m-7hxr
title: Cluster 3 CIS-HIA 3D Ion Distrib. LS, Solar Wind Mode, Phase Space Density

description: This dataset contains 3D Ion distributions (particle phase space density) from the CIS-HIA instrument on the Cluster C3 spacecraft in Low-Sensitivity Solar Wind mode
DOI: 10.24400/802406/e7wt-s7h5
title: Cluster 3 CIS-HIA 3D Ion Distrib. LS, Solar Wind Mode, Particle Flux

description: This dataset contains 3D Ion distributions (differential particle flux) from the CIS-HIA instrument on the Cluster C3 spacecraft in Low-Sensitivity Solar Wind mode
DOI: 10.24400/802406/r6wr-pyqk
title: Cluster 3 CIS-HIA 3D Ion Distrib. LS, Solar Wind Mode, Particle Energy Flux

description: This dataset contains 3D Ion distributions (particle energy flux) from the CIS-HIA instrument on the Cluster C3 spacecraft in Low-Sensitivity Solar Wind mode
DOI: 10.24400/802406/zkm7-w37w
title: Cluster 3 CIS-HIA 3D Ion Distrib. LS, Solar Wind Mode, Count Rate

description: This dataset contains 3D Ion distributions (corrected particle count rate) from the CIS-HIA instrument on the Cluster C3 spacecraft in Low-Sensitivity, Solar Wind Mode
DOI: 10.24400/802406/evgz-8se7
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Solar Wind Mode, Raw Counts

description: This dataset contains 3D Ion distributions (raw particle counts) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity
DOI: 10.24400/802406/9qwe-v00t
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Solar Wind Mode, Phase Space Density

description: This dataset contains 3D Ion distributions (particle phase space density) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity Solar Wind mode
DOI: 10.24400/802406/1vz1-67vb
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Solar Wind Mode, Particle Flux

description: This dataset contains 3D Ion distributions (differential particle flux) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity Solar Wind mode
DOI: 10.24400/802406/4g88-4qq4
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Solar Wind Mode, Particle Energy Flux

description: This dataset contains 3D Ion distributions (particle energy flux) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity Solar Wind mode
DOI: 10.24400/802406/peq0-x34k
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Solar Wind Mode, Count Rate

description: This dataset contains 3D Ion distributions (corrected particle count rate) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity, Solar Wind mode
DOI: 10.24400/802406/2pe8-330z
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Magnetospheric Mode, Raw Counts

description: This dataset contains 3D Ion distributions(raw particle counts) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity
DOI: 10.24400/802406/3q31-5ka1
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Magnetospheric Mode, Phase Space Density

description: This dataset contains 3D Ion distributions (particle phase space density) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity Magnetospheric mode
DOI: 10.24400/802406/51s5-fkjz
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Magnetospheric Mode, Particle Flux

description: This dataset contains 3D Ion distributions (differential particle flux) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity Magnetospheric Mode
DOI: 10.24400/802406/20x0-fb9j
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Magnetospheric Mode, Particle Energy Flux

description: This dataset contains 3D Ion distributions (particle energy flux) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity Magnetospheric Mode
DOI: 10.24400/802406/mtxx-x22p
title: Cluster 3 CIS-HIA 3D Ion Distrib. HS, Magnetospheric Mode, Count Rate

description: This dataset contains 3D Ion distributions (corrected particle count rate) from the CIS-HIA instrument on the Cluster C3 spacecraft in High-Sensitivity
DOI: 10.24400/802406/2vj1-tah2
title: Cluster 3 CIS-CODIF 3D Oxygen+ Distrib. RPA Mode, Raw Counts

description: This dataset contains 3D Oxygen+ distributions (raw particle counts) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/z22q-wh44
title: Cluster 3 CIS-CODIF 3D Oxygen+ Distrib. RPA Mode, Phase Space Density

description: This dataset contains 3D Oxygen+ distributions (particle phase space density) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/zwps-hag8
title: Cluster 3 CIS-CODIF 3D Oxygen+ Distrib. RPA Mode, Particle Flux

description: This dataset contains 3D Oxygen+ distributions (differential particle flux) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/dpkx-d38w
title: Cluster 3 CIS-CODIF 3D Oxygen+ Distrib. RPA Mode, Particle Energy Flux

description: This dataset contains 3D Oxygen+ distributions (particle energy flux) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/wq0x-t2wz
title: Cluster 3 CIS-CODIF 3D Oxygen+ Distrib. RPA Mode, Count Rate

description: This dataset contains 3D Oxygen+ distributions in (corrected particle count rate) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/y9eb-sr49
title: Cluster 3 CIS-CODIF 3D Alpha Distrib. RPA Mode, Raw Counts

description: This dataset contains 3D Alpha distributions (raw particle counts) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/fpqm-z2gc
title: Cluster 3 CIS-CODIF 3D Alpha Distrib. RPA Mode, Phase Space Density

description: This dataset contains 3D Alpha distributions (particle phase space density) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/cxkt-xy2n
title: Cluster 3 CIS-CODIF 3D Alpha Distrib. RPA Mode, Particle Flux

description: This dataset contains 3D Alpha distributions (differential particle flux) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/bpbm-emx0
title: Cluster 3 CIS-CODIF 3D Alpha Distrib. RPA Mode, Particle Energy Flux

description: This dataset contains 3D Alpha distributions (particle energy flux) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/mep0-gf9v
title: Cluster 3 CIS-CODIF 3D Alpha Distrib. RPA Mode, Count Rate

description: This dataset contains 3D Alpha distributions (corrected particle count rate) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/ejfh-bz52
title: Cluster 3 CIS-CODIF 3D Helium+ Distrib. RPA Mode, Raw Counts

description: This dataset contains 3D Helium++ distributions (raw particle counts) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.5281/zenodo.6327496
title: Test Dataset for OMERO upload

description: Test Dataset for OMERO upload One set with .tif files One set with .flex files Each with corresponding .xml descriptor files
DOI: 10.24400/802406/z5gw-rkn0
title: Cluster 3 CIS-CODIF 3D Helium+ Distrib. RPA Mode, Phase Space Density

description: This dataset contains 3D Helium+ distributions (particle phase space density) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.24400/802406/w0qv-v1ay
title: Cluster 3 CIS-CODIF 3D Helium+ Distrib. RPA Mode, Particle Flux

description: his dataset contains 3D Helium+ distributions (differential particle flux) from the CIS-CODIF instrument on the Cluster C3 spacecraft in RPA mode (Retarding Potential Analyser)
DOI: 10.5281/zenodo.6327495
title: Test Dataset for OMERO upload

description: Test Dataset for OMERO upload One set with .tif files One set with .flex files Each with corresponding .xml descriptor files