cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.19397138
title: Supplementary Material for: Bioactive Properties and Phytochemical Screening of Mad Honey Bee Pollen

description: <b><i>Introduction:</i></b> Mad honey is widely used in folk medicine in the Black Sea region of Turkey for its medicinal properties, but its pollen is not collected by mad honey producers and its benefits are unknown. <b><i>Methods:</i></b> In this study, water and ethanol extracts of mad honey bee pollen from four different plateaus in the Black Sea region of Turkey were researched for their antioxidant and antimicrobial properties. Phytochemical analyses were carried out and the data were supported with UV-Vis spectrophotometry. Antimicrobial activity was researched against four Gram-positive and four Gram-negative bacteria, one fungus, and one yeast. The results were compared with standard antioxidants and antibiotics. <b><i>Results:</i></b> The ethanol extracts of the samples from Sinop (P5), Giresun (P7), and Trabzon (P8) were the most active samples as antioxidants, and almost all the extracts of <i>R. ponticum</i> bee pollen were effective on the tested microorganisms. However, P5–8 showed better values for <i>B. cereus</i>, <i>E. feacalis</i>, <i>E. coli</i>, and <i>P. aeruginosa.</i> <b><i>Conclusion:</i></b> It has been proven that mad honey bee pollen is a natural product with previously unknown medicinal properties and rich phytochemical content. Future research and clinical trials are important to scientifically support its benefits in complementary medicine.
DOI: 10.6084/m9.figshare.19397138.v1
title: Supplementary Material for: Bioactive Properties and Phytochemical Screening of Mad Honey Bee Pollen

description: <b><i>Introduction:</i></b> Mad honey is widely used in folk medicine in the Black Sea region of Turkey for its medicinal properties, but its pollen is not collected by mad honey producers and its benefits are unknown. <b><i>Methods:</i></b> In this study, water and ethanol extracts of mad honey bee pollen from four different plateaus in the Black Sea region of Turkey were researched for their antioxidant and antimicrobial properties. Phytochemical analyses were carried out and the data were supported with UV-Vis spectrophotometry. Antimicrobial activity was researched against four Gram-positive and four Gram-negative bacteria, one fungus, and one yeast. The results were compared with standard antioxidants and antibiotics. <b><i>Results:</i></b> The ethanol extracts of the samples from Sinop (P5), Giresun (P7), and Trabzon (P8) were the most active samples as antioxidants, and almost all the extracts of <i>R. ponticum</i> bee pollen were effective on the tested microorganisms. However, P5–8 showed better values for <i>B. cereus</i>, <i>E. feacalis</i>, <i>E. coli</i>, and <i>P. aeruginosa.</i> <b><i>Conclusion:</i></b> It has been proven that mad honey bee pollen is a natural product with previously unknown medicinal properties and rich phytochemical content. Future research and clinical trials are important to scientifically support its benefits in complementary medicine.
DOI: 10.5281/zenodo.6374928
title: Monitoring data second-life battery Cloverleaf demonstrator Circusol

description: This dataset includes monitoring data on the second-life battery system that was implemented in the Cloverleaf demonstrator in the context of Circusol. The following data are included:<br> - State of Health evolution<br> - Round trip Efficiency<br> - Typical day V I<br> - Typical day Vcell
DOI: 10.5281/zenodo.6374927
title: Monitoring data second-life battery Cloverleaf demonstrator Circusol

description: This dataset includes monitoring data on the second-life battery system that was implemented in the Cloverleaf demonstrator in the context of Circusol. The following data are included:<br> - State of Health evolution<br> - Round trip Efficiency<br> - Typical day V I<br> - Typical day Vcell
DOI: 10.5445/ir/1000143659
title: Experimental Dataset of the PhD Dissertation on Airblast Atomization
DOI: 10.48370/ofd/jrp1gd/mzqgjv
title: Tragosoma depsarium.JPG

description: :unav
DOI: 10.48370/ofd/jrp1gd
title: Gracz borowy (Tragosoma depsarium (Linnaeus, 1767)), C-614

description: Coleoptera collection
DOI: 10.24400/802406/qm8g-n5w4
title: Magnetic Field

description: The aim of the TRAC data set from the AUREOL-3 magnetometer is to measure the perturbations of the local geomagnetic fiels that result from the flow of Birkeland currents parallel to the field lines. The data period covers the interval from November 1981 to March 1986. Most data were produced during the 1981-1982 time period (the 1983-1986 time period covered only several orbits). The sampling rates of the TRAC outputs for various telemetry regimes are the following : 100 pts/s TMS4 ZAP1 10 ms 12.5 pts/s TMS30 ZAP2 80 ms 3 pts/s TMS120 ZAP3 330 ms 0.4 pts/s TMS960 ZAP4 2.5 s
DOI: 10.24400/802406/se7r-wfe0
title: ARCAD3 TBF Waveforms : E and B fields

description: This data set contains ARCAD3 TBF waveforms, E and B fields. The TBF experiment onboard the AUREOL3 satellite (ARCAD3 project) was designed to measure two electric and three magnetic wave field components in the range from 10 Hz to 16 kHz. Two telemetry systems were available on AUREOL3, high bit-rate real-time telemetry (TMF) and tape-recorded telemetry (TMS). The Waveform data are related to the TMF one. The ground stations mostly used are Tromsö (Norway) and Terre-Adélie (French Antartica). Two electric and three magnetic components were digitized with a sampling frequency of 5000 Hz. The electric field is measured using spherical probes located at the tip of booms and the alternative magnetic field is measured using a search-coil instrument. The set of data contains : general information (date, time, orbit, telemetry, ...), orbit parameters (latitude, longitude, ...), attitude parameters (angles, matrices for coordinate system changes), waveform data (component, unit, gain, amplitude). TBF Waveforms data use TBF data presented in the 'Waveform' archive have to be validated prior to any interpretation. Questionable electric and magnetic field data can be due to : telemetry noise, calibrations performed every 128 seconds, possible saturation of the input electronics (ULF turbulence), wrong gain variations, gain variation inside a 960 ms data frame. The transfer functions used for the conversion in physical values do not allow any utilization of the data below 5 Hz. Concerning the ancillary data, for several sets, the orbit parameters can be equal to zero even the related flag is correctly set (OK_AUXI).
DOI: 10.24400/802406/tpsf-remk
title: ELF/VLF Filter-Banks: E and B fields

description: This data set contains ARCAD-3 TBF magnetometer data and filter-bank data (filter information, frequencies, component, unit, reliability flag, amplitude). The TBF experiment onboard the AUREOL3 satellite (ARCAD3 project) was designed to measure two electric and three magnetic wave field components in the range from 10 Hz to 16 kHz. Two telemetry systems were available on AUREOL3, real-time telemetry (TMF) and tape-recorded telemetry (TMS). The Filter-Bank data, related to the TMS one, cover the Earth in geographical coordinates. Four TMS modes ZAP1, ZAP2, ZAP3, ZAP4 were used with the respective filter sampling intervals of 0.01, 0.08, 0.32 and 2.56 seconds. Three types of filters were used, FB, FBF and FBS. The two electric components EH and EZ are processed in a bank of six filters named FB with center frequencies of 15, 32, 72, 150, 325 and 725 Hz. Two components, among the two electric and the three magnetic components, were selected and fed two identical sets of seven adjacent wide-band (FBF) and five spaced narrow-band (FBS) filters. The center frequencies of the FBF are 250, 700, 1250, 2200, 3900, 7000 and 12500 Hz. The center frequencies of the FBS are 140, 450, 800, 4500 and 15000 Hz. All the output filter amplitudes are given in physical units, mV/m/(Hz)^-2 for the electric field and nT/(Hz)^-2 for the magnetic field. Data use TBF data presented in the 'Filter-Bank' archive have to be validated prior to any interpretation. Questionable electric and magnetic field data can be due to : telemetry noise, calibrations performed every 128 seconds, possible saturation of the input electronics (ULF turbulence), wrong gain variations, amplitude values equal to zero although the reliability and mode flags are correct. Concerning the ancillary data, for several sets, the orbit parameters can be equal to zero even the related flag is correctly set (OK_AUXI). The reliability of the recorded formats is given with the flag OK_VALID or PB_VALID. The reliability of the filter data (filter commutation) is given with the flag OK_MODE or PB_MODE.
DOI: 10.24400/802406/ry0j-v1at
title: Auroral Ion/Electron Energy Spectra

description: This data set contains ARCAD-3 Auroral Ion/Electron Energy Spectra from ROBE experiment. The SPECTRO/ROBE experiment onboard the AUREOL-3 satellite has been designed to measure auroral particle energy spectra, angular distributions in the energy range 10 eV- 21 keV/q. A number of various studies have been carried out, e.g., acceleration of auroral electrons, heating and acceleration of ionospheric ions, structure of large and small scale field aligned currents in the cusp, structure of the cusp region for various interplanetary conditions, auroral signature of acceleration mechanisms acting in the near Earth and distant tail. Archived data were provided by a set of independent and complementary instruments: (1) the low-energy plasma instrument ROBE, (2) the very low energy sensor TBE: 1. The main ROBE high sensitive instrument (double quadrispherical analyzer + an array of channel electron multipliers, CEMs) is designed to obtain the 2D distributions of precipitating and trapped electrons and protons (ions) from ~200 eV to ~21 keV in 8 or 16 logarithmically spaced energy steps, without a mass selection. As AUREOL-3 was a 3-axis stabilized satellite (with ~30° oscillations), an array of 18 detectors (E1-E9 for electrons, P1-P9 for ions) can be potentially used to cover the pitch angle range between ~0° and 90°. Basic characteristics of the instrument were DE/E ~28% (FWHM) and a field-of-view of ~13°x 6°. According to the operating DATA MODE chosen that depends of the telemetry rate, ROBE count rates can be transmitted in different ways through 3 count rate chains named BE1, ROT, and BE2. The BE1 chain transmits count rates from a pair (Ei-Pi) of detectors from the group E1-E4/P1-P4 (low pitch angles), while a pair (Ej-Pj) from the group E5-E9/P5-P9 is transmitted through the BE2 chain (large pitch angles). For the ROT chain, the data may either come from only 1 pair (Ek-Pk) from the group E2-E9/P2-P9, or sequentially from the full set of detectors E2-E9/P2-P9 (pitch angle scanning mode). The SPECTRO particle instruments operated successfully until the end of the mission at different basic bit-rate modes depending of the telemetry rate and/or the chosen sharing between instruments. Among these modes the most useful for the ROBE instrument included record of 2D electron and proton distributions (16 energies x 9 pitch angle pixels) in ~1.6 s. 2. The TBE instrument (double hemispherical analyzer + CEMs) was designed to study field aligned (pitch angle 0-20°) low-energy (~10 eV - ~1000 eV) precipitating electrons and protons (ions) in 16 linear-spaced energy steps. Characteristics of the instrument are: deltaE/E ~7% and field-of-view: ~6 x 21°. Each archived sequence of ROBE and TBE data includes all needed information. Results are organized in time sequences of successive electron and proton spectra, presented in corrected physical units (differential fluxes in (cm2.sec.sr.keV)^-1) and accompanied by corresponding energy and background tables, as well as by the full set of useful geophysical and orbital parameters (MLT, ILAT, ...).
DOI: 10.24400/802406/6rmb-6cvv
title: Auroral Ion Mass/Energy Spectra

description: This data set contains ARCAD-3 Spectro Auroral Ion Mass/Energy Spectra. The ARCAD-3 Spectro suprathermal ion spectrometers, ION1 and ION2 measured the abundance of ionospheric (H+, He+, O+) and solar wind/magnetospheric ion species (H+, He++), from ~10 eV to ~14 keV/charge and from 1 to ~32 AMU, in two different viewing directions, ~60° and ~120° pitch angle. The basic design included a collimator followed by a retarding potential analyzer (RPA), the electrostatic energy analyzer (cylindrical). Subsequent mass analysis was carried out by an ExB Wien filter and detection by an array of CEMs. Performances were the following: internal energy resolution: deltaE/E ~ 5%, mass resolution: M/deltaM ~ 4, energy range divided in two sub-ranges: 10-120 eV/q (ionospheric RPA mode) and suprathermal, 50 eV to 14 keV/q. For each ion spectrometer different operating modes were selected by commands setting: (i) the number of scanned mass channels (64, 32, or 4), (ii) the number of energy steps (16, 8, or 4), (iii) their central energy, (iv) use of either the suprathermal section or the RPA section. ION1 and ION2 data are continuously transmitted with basic modes including complete mass-energy scans (64M x 16E or 32M x 4E) in ~12.8 s. to ~1 min. Each archived sequence of ION1 and ION2 data includes all needed information. All the results, organized in time sequences of successive energy-mass spectra, are given in corrected physical units (differential fluxes in (cm2.sec.sr.keV)^-1 units) and accompanied by corresponding energy and background tables, as well as by the full set of useful geophysical and orbital parameters (MLT, ILAT, ...). For RPA modes, only 4 energy steps (100 eV/q for ION1, 95 eV/q for ION2) were set up. Associated fluxes are integrated fluxes between the set up threshold and ~120 eV/q. High voltages applied to the electrostatic energy analyzer and the Wien mass filter were commanded by the onboard computer so that successive ion peaks may be easily recognized in successive mass per charge spectra at set channels whatever was the energy per charge selected. For example, for 32M and 64M scanning modes, (H+, He++, He+, O+) ions were detected at channels (4, 12, 18, 24) and (8, 24, 36, 48), respectively, independently of the selected energy steps.
DOI: 10.24400/802406/88dd-ej46
title: ARCAD3 SPECTRO : Informal file on processing status

description: This data set contains an informal file with information about the processing status of the ARCAD3 SPECTRO experiment Each data ION file has an associated informal file. Its name is given in the file general header. The informal file is a sequential ASCII file. It contains information about ROBE data too.
DOI: 10.24400/802406/dkqp-a89v
title: High resolution density waveform

description: This data set contains ARCAD-3 Isoprobe waveform data (data set information, tracking frequency of the extremum). The high resolution data correspond to a frequency tracking of the resonance or an anti-resonance of the mutual impedance response. As the resonance frequency is related to the electron density and the anti-resonance frequency to the Debye length, these data (used as waveform data) allow studies of density and/or temperature fluctuations. The extremum trackings, one per probe, are available in the Self-Oscillating mode, Maximum and Minimum search modes. The different combinations are : AUT-AUT, MAX-MAX, MAX-MIN and MIN-MIN. The number of samples and the time resolution depend on the type of telemetry : 256 samples with a resolution of 50 ms in TMS120, 200 samples with a resolution of 20 ms in TMS30, 1680 samples with a resolution of 2.5 ms in TMS4 and 19672 samples with a resolution of 0.2 ms in TMF.
DOI: 10.24400/802406/tc6w-m7mt
title: Electron density and temperature

description: This data set contains electron density and temperature from ARCAD-3 Isoprobe experiment. The plasma frequency (and hence the electron density) is determined from the frequency of one or several resonance peaks. For high plasma density, the frequency response exhibits only one peak located at the upper hybrid frequency. For low density plasma, the determination is more complicated since the frequency response is influenced by the magnetic field, and multiple resonances can be observed. A specific chart has been created to take into account all the main resonances as upper hybrid, plasma and Bernstein mode frequencies. The Debye length (and hence the electron temperature, knowing the density) has been determined from the amplitude of the main resonance peaks. A chart has been created to allow an estimation of the Debye length as a function of the amplitude and of the plasma frequency. For high density plasma, electron temperature can also be determined from the frequency interference pattern above the upper hybrid resonance. The resolution is a few seconds (low time resolution), depending on the type of telemetry.
DOI: 10.24400/802406/3zr5-hfas
title: Probe sweeps

description: This data set contains ARCAD-3 Isoprobe probe sweeps (sweep information, amplitude and phase). The logarithmic amplitude and the phase values of the mutual impedance are given versus the frequency (log(|Z|) and PHI(Z)). Four basic sweeps are stored : B1 active sweep from 100 kHz to 9675 kHz with the DC configuration, B2 active sweep from 100 kHz to 9675 kHz with the DL configuration, B3 passive sweep from 100 kHz to 9675 kHz with the DL configuration and B4 active sweep from 100 kHz to 1587.5 kHz with the DL configuration. The frequency resolution depends on the telemetry type (TMF, TMS4, TMS30 and TMS120) and on the operating mode (BAFA, BAFI, BAFP and BAFC). A fifth sweep (status sweep) is recorded when the experiment is set in a high resolution mode (extremum tracking).
DOI: 10.24400/802406/b6y2-5ybe
title: ARCAD3 orbit data and geomagnetic parameters

description: This data set contains ARCAD-3 ephemeris (position) and geomagnetic characteristics (Invariant Latitude, Magnetic Local Time, Magnetospheric Regions where the satellite may be located)
DOI: 10.24400/802406/58wt-jgjp
title: ARCAD3 orbit data (GSE frame, 1 min resolution)

description: This data set contains 1 min resolution ARCAD-3 ephemeris (position and velocity)
DOI: 10.34740/kaggle/dsv/3339451
title: AutoXGB
DOI: 10.48370/ofd/3lxk0p/cqs7kz
title: Prionus besicanus.JPG

description: :unav
DOI: 10.48370/ofd/3lxk0p
title: Prionus besicanus (Fairmaire, 1855), C-615

description: Coleoptera collection
DOI: 10.48370/ofd/upnxx2/efof2y
title: Prionus lefebvrei.JPG

description: :unav
DOI: 10.48370/ofd/upnxx2
title: Prionus levebvrei (Marsham, 1856), C-616

description: Coleoptera collection
DOI: 10.5281/zenodo.6373929
title: Monitoring data_2021 (1)

description: Monitoring data of the soil suction and volumetric water content measured at the standard vegetation area (A) and deep-rooting vegetation area (P), together with atmospheric data and rainfalls, for 2021.
DOI: 10.5281/zenodo.6373928
title: Monitoring data_2021 (1)

description: Monitoring data of the soil suction and volumetric water content measured at the standard vegetation area (A) and deep-rooting vegetation area (P), together with atmospheric data and rainfalls, for 2021.
DOI: 10.5281/zenodo.6364464
title: dataset of scopus

description: dataset from Scopus related to the publication with topic embryo of broiler chicken published in journals indexed by Scopus. The data extracted at 16 February 2022.
DOI: 10.6084/m9.figshare.18777650
title: [ICPC22] Demystifying Software Release Note Issues on GitHub —— Dataset

description: Release notes (RNs) summarize main changes between two consecutive software versions and serve as a central source of information when users upgrade software. While producing high quality RNs can be hard and poses a variety of challenges to developers, a comprehensive empirical understanding on these challenges is still lacking. In this paper, we bridge this knowledge gap by manually analyzing 1,731 latest GitHub issues to build a comprehensive taxonomy of RN issues with four dimensions: Content, Presentation, Accessibility, and Production. Among these issues, nearly half (48.47%) of them focus on Production; Content, Accessibility, and Presentation take 25.61%, 17.65%, and 8.27%, respectively. We find that: 1) RN producers are more likely to miss information than to include incorrect information, especially for breaking changes; 2) improper layout may bury important information and confuse users; 3) many users find RNs inaccessible due to link deterioration, lack of notification, and obfuscate RN locations; 4) automating and regulating RN production is challenging despite producers’ great needs. Our taxonomy pictures a roadmap to improve RN production in practice and reveals interesting future research directions.
DOI: 10.6084/m9.figshare.18777650.v1
title: [ICPC22] Demystifying Software Release Note Issues on GitHub —— Dataset

description: Release notes (RNs) summarize main changes between two consecutive software versions and serve as a central source of information when users upgrade software. While producing high quality RNs can be hard and poses a variety of challenges to developers, a comprehensive empirical understanding on these challenges is still lacking. In this paper, we bridge this knowledge gap by manually analyzing 1,731 latest GitHub issues to build a comprehensive taxonomy of RN issues with four dimensions: Content, Presentation, Accessibility, and Production. Among these issues, nearly half (48.47%) of them focus on Production; Content, Accessibility, and Presentation take 25.61%, 17.65%, and 8.27%, respectively. We find that: 1) RN producers are more likely to miss information than to include incorrect information, especially for breaking changes; 2) improper layout may bury important information and confuse users; 3) many users find RNs inaccessible due to link deterioration, lack of notification, and obfuscate RN locations; 4) automating and regulating RN production is challenging despite producers’ great needs. Our taxonomy pictures a roadmap to improve RN production in practice and reveals interesting future research directions.
DOI: 10.26255/heal.1y6b-2rho
title: test2test2
DOI: 10.26255/heal.xcv8-re27
title: test3s
DOI: 10.5281/zenodo.6375278
title: dataset of scopus

description: dataset from Scopus related to the publication with topic embryo of broiler chicken published in journals indexed by Scopus. The data extracted at 16 February 2022.
DOI: 10.5281/zenodo.6364463
title: dataset of scopus

description: dataset from Scopus related to the publication with topic embryo of broiler chicken published in journals indexed by Scopus. The data extracted at 16 February 2022.
DOI: 10.48370/ofd/ogs73z/iviskg
title: Prionus brachypterus.JPG

description: :unav
DOI: 10.48370/ofd/ogs73z
title: Prionus brachypterus (Gebler, 1830), C-617

description: Coleoptera collection
DOI: 10.5281/zenodo.6373846
title: CPTu results

description: CPTu performed at the riverside of the embankment site, Panaro river, in October 2020.
DOI: 10.5281/zenodo.6373845
title: CPTu results

description: CPTu performed at the riverside of the embankment site, Panaro river, in October 2020.