cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.48322/vkfc-zw89
title: SOHO LASCO C2 Polarized Brightness FITS Data

description: The Polarized Brightness data from the LASCO C2 coronagraph.

LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona from 1.1--30 solar radii (C1: 1.1--3; C2: 1.5--6; and C3: 3--30). The inner coronagraph (C1) is a newly developed mirror version of the classic Lyot coronagraph without an external occulter, while the middle coronagraph (C2) and the outer one (C3) are externally occulted. C1 is equipped with a Fabry-Perot interferometer that can take monochromatic images over the whole field of view with a spectral resolution of 0.07 nm. By stepping the bandpass across a spectral line, line profiles and Doppler shifts can be derived from all 1024 x 1024 pixels simultaneously. With an equivalent pixel size of 5.6 arcsec, the spatial resolution of C1 is ~11 arcsec. The resolution is ~23 arcsec for C2, and 112 arcsec for C3. The calculated expected precision of the emission line measurements, for example, of the 637.4 nm Fe X line is 0.05 Km/s at 1.1 solar radii, 1.0 km/s at 2 solar radii, and 8.0 km/s at 3 solar radii, all for a 60 s exposure. All three devices use a 1024 x 1024 pixel CCD. The CCDs are passively cooled to 193 K, but can be heated above ambient temperatures to drive off condensed material. The readout rate is ~21 s for a full image, but any line on the CCD can be accessed within about 60 ms, the unwanted lines being dumped. The electronics box provides overall control, including observation programs and scheduling. An observation program can be scheduled to be run at an absolute time or just next in sequence. It can run for a certain number of iterations, an interval of time, or stop at an absolute time. The observation program tasks included, e.g., taking single images from one of the telescopes, a series of images through the three linear polarizers, and a sequence of images at a series of Fabry-Perot wavelength steps. The image processing tasks are primarily image compression, with seven different techniques being available. On average, the readout time should be ~6 minutes or about 200 images/day. This information is from the paper ``The Large Angle Spectroscopic Coronagraph (LASCO): Visible Light Coronal Imaging and Spectroscopy,'' by G. E. Brueckner et al. (Proceedings of the First SOHO Workshop, ESA SP-348, pp. 27-34, November 1992).
DOI: 10.48322/78a3-pg24
title: SOHO LASCO C3 Level 1.0 FITS Data

description: The LASCO C3 Calibrated FITS Data. 

LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona from 1.1--30 solar radii (C1: 1.1--3; C2: 1.5--6; and C3: 3--30). The inner coronagraph (C1) is a newly developed mirror version of the classic Lyot coronagraph without an external occulter, while the middle coronagraph (C2) and the outer one (C3) are externally occulted. C1 is equipped with a Fabry-Perot interferometer that can take monochromatic images over the whole field of view with a spectral resolution of 0.07 nm. By stepping the bandpass across a spectral line, line profiles and Doppler shifts can be derived from all 1024 x 1024 pixels simultaneously. With an equivalent pixel size of 5.6 arcsec, the spatial resolution of C1 is ~11 arcsec. The resolution is ~23 arcsec for C2, and 112 arcsec for C3. The calculated expected precision of the emission line measurements, for example, of the 637.4 nm Fe X line is 0.05 Km/s at 1.1 solar radii, 1.0 km/s at 2 solar radii, and 8.0 km/s at 3 solar radii, all for a 60 s exposure. All three devices use a 1024 x 1024 pixel CCD. The CCDs are passively cooled to 193 K, but can be heated above ambient temperatures to drive off condensed material. The readout rate is ~21 s for a full image, but any line on the CCD can be accessed within about 60 ms, the unwanted lines being dumped. The electronics box provides overall control, including observation programs and scheduling. An observation program can be scheduled to be run at an absolute time or just next in sequence. It can run for a certain number of iterations, an interval of time, or stop at an absolute time. The observation program tasks included, e.g., taking single images from one of the telescopes, a series of images through the three linear polarizers, and a sequence of images at a series of Fabry-Perot wavelength steps. The image processing tasks are primarily image compression, with seven different techniques being available. On average, the readout time should be ~6 minutes or about 200 images/day. This information is from the paper ``The Large Angle Spectroscopic Coronagraph (LASCO): Visible Light Coronal Imaging and Spectroscopy,'' by G. E. Brueckner et al. (Proceedings of the First SOHO Workshop, ESA SP-348, pp. 27-34, November 1992).
DOI: 10.48322/897w-pq47
title: SOHO LASCO C3 Polarized Brightness FITS Data

description: The Polarized Brightness data from the LASCO C3 coronagraph.

LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona from 1.1--30 solar radii (C1: 1.1--3; C2: 1.5--6; and C3: 3--30). The inner coronagraph (C1) is a newly developed mirror version of the classic Lyot coronagraph without an external occulter, while the middle coronagraph (C2) and the outer one (C3) are externally occulted. C1 is equipped with a Fabry-Perot interferometer that can take monochromatic images over the whole field of view with a spectral resolution of 0.07 nm. By stepping the bandpass across a spectral line, line profiles and Doppler shifts can be derived from all 1024 x 1024 pixels simultaneously. With an equivalent pixel size of 5.6 arcsec, the spatial resolution of C1 is ~11 arcsec. The resolution is ~23 arcsec for C2, and 112 arcsec for C3. The calculated expected precision of the emission line measurements, for example, of the 637.4 nm Fe X line is 0.05 Km/s at 1.1 solar radii, 1.0 km/s at 2 solar radii, and 8.0 km/s at 3 solar radii, all for a 60 s exposure. All three devices use a 1024 x 1024 pixel CCD. The CCDs are passively cooled to 193 K, but can be heated above ambient temperatures to drive off condensed material. The readout rate is ~21 s for a full image, but any line on the CCD can be accessed within about 60 ms, the unwanted lines being dumped. The electronics box provides overall control, including observation programs and scheduling. An observation program can be scheduled to be run at an absolute time or just next in sequence. It can run for a certain number of iterations, an interval of time, or stop at an absolute time. The observation program tasks included, e.g., taking single images from one of the telescopes, a series of images through the three linear polarizers, and a sequence of images at a series of Fabry-Perot wavelength steps. The image processing tasks are primarily image compression, with seven different techniques being available. On average, the readout time should be ~6 minutes or about 200 images/day. This information is from the paper ``The Large Angle Spectroscopic Coronagraph (LASCO): Visible Light Coronal Imaging and Spectroscopy,'' by G. E. Brueckner et al. (Proceedings of the First SOHO Workshop, ESA SP-348, pp. 27-34, November 1992).
DOI: 10.48322/n7aj-3053
title: SOHO LASCO C3 Percent Polarized FITS Data

description: The Percent Polarized data from the LASCO C3 coronagraph.

LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona from 1.1--30 solar radii (C1: 1.1--3; C2: 1.5--6; and C3: 3--30). The inner coronagraph (C1) is a newly developed mirror version of the classic Lyot coronagraph without an external occulter, while the middle coronagraph (C2) and the outer one (C3) are externally occulted. C1 is equipped with a Fabry-Perot interferometer that can take monochromatic images over the whole field of view with a spectral resolution of 0.07 nm. By stepping the bandpass across a spectral line, line profiles and Doppler shifts can be derived from all 1024 x 1024 pixels simultaneously. With an equivalent pixel size of 5.6 arcsec, the spatial resolution of C1 is ~11 arcsec. The resolution is ~23 arcsec for C2, and 112 arcsec for C3. The calculated expected precision of the emission line measurements, for example, of the 637.4 nm Fe X line is 0.05 Km/s at 1.1 solar radii, 1.0 km/s at 2 solar radii, and 8.0 km/s at 3 solar radii, all for a 60 s exposure. All three devices use a 1024 x 1024 pixel CCD. The CCDs are passively cooled to 193 K, but can be heated above ambient temperatures to drive off condensed material. The readout rate is ~21 s for a full image, but any line on the CCD can be accessed within about 60 ms, the unwanted lines being dumped. The electronics box provides overall control, including observation programs and scheduling. An observation program can be scheduled to be run at an absolute time or just next in sequence. It can run for a certain number of iterations, an interval of time, or stop at an absolute time. The observation program tasks included, e.g., taking single images from one of the telescopes, a series of images through the three linear polarizers, and a sequence of images at a series of Fabry-Perot wavelength steps. The image processing tasks are primarily image compression, with seven different techniques being available. On average, the readout time should be ~6 minutes or about 200 images/day. This information is from the paper ``The Large Angle Spectroscopic Coronagraph (LASCO): Visible Light Coronal Imaging and Spectroscopy,'' by G. E. Brueckner et al. (Proceedings of the First SOHO Workshop, ESA SP-348, pp. 27-34, November 1992).
DOI: 10.48322/22dk-a715
title: SOHO/MDI Line Of Sight (LOS) Magnetic Field Data

description: Line of sight magnetic field inferred from the frequency/wavelength Zeeman splitting between opposite circular polarizations of a magnetically-sensitive line.
DOI: 10.48322/4x4p-sr85
title: SOHO MDI Line Of Sight (LOS) Velocity Data

description: Line of sight magnetic field inferred from the frequency/wavelength Zeeman splitting between opposite circular polarizations of a magnetically-sensitive line.
DOI: 10.20350/digitalcsic/17862
title: Data from: Phenotypic rebuilding after fire: understanding within-individual variability in a Mediterranean shrub

description: The “Full Data” dataset includes separate tables for each organ studied (leaves, flowers, inflorescences…) with the trait data registered either in the field or in the lab. Depending on the trait, this dataset can have one or several data per module (‘Module’ and ‘Within module’ levels respectively in Table 1). The “Aggregated” dataset includes two tables, one with all the mean and variance values of each trait per module (one row per module) and another one with data aggregated at the individual level (one row per individual).
DOI: 10.20350/digitalcsic/17864
title: July ichthyoplankton surveys [Dataset]

description: Data obtained in oceanographic surveys conducted off the Catalan coast (from 40.15˚N to 42˚N and from 0.5˚E to 3.5˚E). The dataset contains: • The stations sampled in each survey, with location data (longitude and latitude) and data for the year sampled. • At each sampling station, the environmental variables analysed are provided: bottom depth (m); surface oceanographic variables from the CTD casts (temperature, in ºC, salinity and chlorophyll-a, in µg L-1), maximum value of chlorophyll-a in the water column (Chla_CM); maximum density gradient (Gmax); pycnocline depth (PD); geostrophic velocity components (VelX_U, VelY_V); and surface (10 m) dynamic height (DH_10). • Abundance of fish larvae collected with the Bongo net, standardized per unit area (No. larvae 10 m 2), at each sampling station
description: In this study, we aim to investigate the contribution of various sources of variability, environmental, spatial and interannual on the larval fish assemblages (LFA) in summer off the Catalan coast, an area with a wide array of environmental conditions.The hydrodynamics of the area is controlled by the Northern Current, flowing southwestwards along the continental slope. This current displays high mesoscale variability presenting a meandering path and a series of anticyclonic eddies over the shelf. The study was based on three ichthyoplankton surveys carried out in July 2003, 2004 and 2012. The number of identified taxa, belonging to shelf and oceanic fish species, was quite similar among cruises, around 80, with the small pelagics Engraulis encrasicolus and Sardinella aurita being the dominant species. A high spatial heterogeneity in LFA was detected throughout the studied area. Most of this heterogeneity was related to the spatial variability of environmental factors, such as the continental shelf structure, latitudinal difference in surface temperature, chlorophyll-a concentration and stratification level. Hydrodynamic structures, mainly instabilities of the Northern Current and anticyclonic eddies, and the thermal front across the shelf, also played an important role in the configuration of the LFA. Although these showed certain interannual variability, mainly related to the 2003 heat wave and the low surface productivity of 2012, the recurrence of hydrodynamic structures, together with the spawning habits of adults, means that the spatial structure of LFA is maintained in different years
description: Survey: CACO 1, July03/C1 2003. Survey: CACO 4, July04/C4 2004. Survey: FISHJELLY 12, July12/F2 2012
DOI: 10.5281/zenodo.18091379
title: Stand development reshapes depth-dependent microbial pathways of mineral-associated carbon formation in monoculture plantations
DOI: 10.5281/zenodo.18091380
title: Stand development reshapes depth-dependent microbial pathways of mineral-associated carbon formation in monoculture plantations
DOI: 10.5281/zenodo.14352787
title: Japanese Vowel Length Acoustic Data

description: This dataset contains detailed acoustic measurements of Japanese long and short vowels, as reported in Yazawa and Kondo (2019).

Speakers

16 native speakers of Tokyo Japanese (8 male, 8 female), aged between 21 and 30 years.

Materials

The materials consisted of disyllabic nonce words of the form /C1V1C2V2/, produced in isolation and within a carrier sentence (see ReadingList.txt).



V1 (target vowel): Long (/ii, ee, aa, oo, uu/) and short (/i, e, a, o, u/)

C1 & C2 (consonantal context): /b_p/, /d_t/, /g_k/, /z_s/, /h_d/

V2 (following vowel): /e/ and /o/


Acoustic parameters

The following acoustic parameters were extracted:



Duration

Formant frequencies (F1, F2, F3) measured using Praat



Fn_Midpoint: the nth formant measured at the temporal midpoint of each vowel interval

Fn_x: the nth formant measured at the xth of 30 equidistant points within the central 60% of the vowel interval
DOI: 10.5281/zenodo.15227304
title: Japanese Vowel Length Acoustic Data

description: This dataset contains detailed acoustic measurements of Japanese long and short vowels, as reported in Yazawa and Kondo (2019).

Speakers

16 native speakers of Tokyo Japanese (8 male, 8 female), aged between 21 and 30 years.

Materials

The materials consisted of disyllabic nonce words of the form /C1V1C2V2/, produced in isolation and within a carrier sentence (see ReadingList.txt).



V1 (target vowel): Long (/ii, ee, aa, oo, uu/) and short (/i, e, a, o, u/)

C1 & C2 (consonantal context): /b_p/, /d_t/, /g_k/, /z_s/, /h_d/

V2 (following vowel): /e/ and /o/


Acoustic parameters

The following acoustic parameters were extracted:



Duration

Formant frequencies (F1, F2, F3) measured using Praat



Fn_Midpoint: the nth formant measured at the temporal midpoint of each vowel interval

Fn_x: the nth formant measured at the xth of 30 equidistant points within the central 60% of the vowel interval
DOI: 10.15468/ddjdgc
title: On some Moroccan Pamphagidae, with the description of a new species of Euryparyphes (Orthoptera: Caelifera)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Chobanov, Dragan, Massa, Bruno (2022): On some Moroccan Pamphagidae, with the description of a new species of Euryparyphes (Orthoptera: Caelifera). Zootaxa 5104 (3): 409-425, DOI: 10.11646/zootaxa.5104.3.3AbstractAn update to the distribution records of the Moroccan Pamphagidae is presented. One new species to science, Euryparyphes minor sp. n., is described, and one new combination is proposed.
DOI: 10.15468/dl.eqmjfb
title: Occurrence Download

description: A dataset containing 316615 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Passer hispaniolensis",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "Geometry POLYGON((-180 -90, 180 -90, 180 90, -180 90, -180 -90))"
 ]
}

 The dataset includes 316615 records from 147 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068895-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5281/zenodo.18091404
title: BIG-Bench Hard (BBH) Data Quality Investigation Report

description: This dataset documents 49 ground truth labeling errors discovered in the BIG-Bench Hard (BBH) benchmark through systematic multi-model cross-verification and mathematical proof.
v1.5.0 Updates

Added comprehensive 8-model verification analysis (GPT-5.2 Pro, Claude Opus 4.5, DeepSeek-Reasoner, Llama 3.3 70B, Gemini Pro 3)
Included mathematical SVG coordinate proofs for all 42 geometric shape errors
Documented Gemini discrepancy resolution through mathematical verification
Error Summary

date_understanding: 7 errors (date calculation)
geometric_shapes: 42 errors (22 circle K→A, 20 rectangle K→H)
Verification
All corrections verified by 6+ language models AND mathematical proof (SVG coordinate analysis).
DOI: 10.15468/dl.557cgy
title: Occurrence Download

description: A dataset containing 4 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((-71.46983 -34.14804,-68.56922 -34.59633,-68.56922 -32.93696,-69.83951 -32.67163,-71.46983 -34.14804))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Leopardus guigna"
 ]
}

 The dataset includes 4 records from 2 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068903-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.u4vpvf
title: Occurrence Download

description: A dataset containing 37034 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Nudibranchia",
 "Country is one of (Indonesia, Philippines)",
 "HasCoordinate is true",
 "HasGeospatialIssue is false"
 ]
}

 The dataset includes 37034 records from 42 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068904-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.6084/m9.figshare.29453330
title: Shrubification effects on litter decomposition are dependent on plant species and organs in grazed meadows

description: The files include the Dataset for litter decomposition and Code for random forest analysis for the statistical analyses presented in Li et al 2025. Shrubification effects on litter decomposition are dependent on plant species and organs in grazed meadows.
DOI: 10.6084/m9.figshare.29453330.v1
title: Shrubification effects on litter decomposition are dependent on plant species and organs in grazed meadows

description: The files include the Dataset for litter decomposition and Code for random forest analysis for the statistical analyses presented in Li et al 2025. Shrubification effects on litter decomposition are dependent on plant species and organs in grazed meadows.
DOI: 10.15468/dl.uzycjy
title: Occurrence Download

description: A dataset containing 3 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((-71.13471 -33.67226,-70.35701 -33.54013,-69.93428 -32.96434,-71.19816 -33.36325,-71.13471 -33.67226))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Leopardus colocola"
 ]
}

 The dataset includes 3 records from 2 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068906-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.8579up
title: Occurrence Download

description: A dataset containing 34451 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is United States of America",
 "Geometry POLYGON((-73.44 41,-71.47 41,-71.47 42.03,-73.44 42.03,-73.44 41))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Dryocopus pileatus",
 "Year 2020-2025"
 ]
}

 The dataset includes 34451 records from 3 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068907-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/nw2vj4
title: Mohonk Preserve Riparian Invasive Vegetation Species Sampling

description: The StreamWatch citizen science program includes surveying riparian zones in the Hudson River Valley of New York State for the presence of invasive species, including garlic mustard, barberry, purple loosestrife, Japanese stiltgrass, oriental bittersweet, phragmites, multiflora rose, Japanese knotweed, Dame's rocket, and wineberry.
DOI: 10.15468/cgbub0
title: USGS ASC - Copper River Delta - Birds - 1997-2005

description: Waterbirds were observed during breeding season in the Copper River Delta Area of Alaska. These data include 14 unique taxa observed over a seven-year period. In 1964, an earthquake changed the wetlands of this area, uplifting them by 1.9 meters and draining large areas. Goose breeding populations have since been in decline. These data provide occurrence information at nests.
DOI: 10.15468/yvek7u
title: USGS NRP - Submerged Aquatic Plants - 1966-2009

description: Molecular methods reveal new information on the range and recent history of four related and similar appearing species: Hydrilla verticillata, Egeria densa, Elodea canadensis, and Elodea nuttallii (family Hydrocharitaceae). We also distinguish monoecious from dioecious hydrilla for each of the hydrilla samples. We examined implications of the confirmed distribution relative to previous records and demonstrated the regional and national need for reverification of these species collected recently or as much as a half century ago. USGS National Research Program (NRP).