cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.14548706
title: Supplementary data to "Diverse dust populations in the near-Sun environment characterized by PSP/ISʘIS"

description: Supplementary data to "Diverse dust populations in the near-Sun environment characterized by PSP/ISʘIS." 

The ISʘIS data and visualization tools are available to the community at https://spacephysics.princeton.edu/missions-instruments/PSP; data are also available via the NASA Space Physics Data Facility (https://spdf.gsfc.nasa.gov/) and ISʘIS science operation center (SOC, https://spp-isois.sr.unh.edu/home.html). The FIELDS data are available at https://fields.ssl.berkeley.edu/data/.
DOI: 10.15468/dl.2epyfg
title: Occurrence Download

description: A dataset containing 20614789 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is Finland",
 "OccurrenceStatus is Present",
 "Year 2009-2023"
 ]
}

 The dataset includes 20614789 records from 411 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0046887-241126133413365/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.5ukjd3
title: Occurrence Download

description: A dataset containing 2651255 species occurrences available in GBIF matching the query:
{
 "and" : [
 "BasisOfRecord is Human Observation",
 "Continent is South America",
 "Issue is one of (Coordinate rounded, Geodetic datum assumed WGS84, Country derived from coordinates, Continent derived from coordinates, Occurrence status inferred from individual count, Taxon match higher rank, Taxon match fuzzy, The taxon ID was not used in backbone matching, The scientific name ID was not used in backbone matching, Continent derived from country)",
 "TaxonKey is Plantae",
 "Year 1990-2024"
 ]
}

 The dataset includes 2651255 records from 755 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0046886-241126133413365/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.qe7bzw
title: Occurrence Download

description: A dataset containing 2156 species occurrences available in GBIF matching the query:
{
 "and" : [
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "TaxonKey is Sula nebouxii excisa Todd, 1948"
 ]
}

 The dataset includes 2156 records from 7 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0046906-241126133413365/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5281/zenodo.13755560
title: The Punctuated Evolution of the Venusian Atmosphere from a Transition in Mantle Convective Style and Volcanic Outgassing

description: Outgassed species for model runs. see header for information
DOI: 10.15468/dl.5mznqf
title: Occurrence Download

description: A dataset containing 78 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON Z((-68.83228 -32.8667 0,-68.8331 -32.86666 0,-68.83325 -32.86723 0,-68.83352 -32.86827 0,-68.83376 -32.8692 0,-68.83384 -32.86949 0,-68.83397 -32.86998 0,-68.83409 -32.87046 0,-68.83441 -32.87166 0,-68.83468 -32.87266 0,-68.83496 -32.87371 0,-68.83536 -32.87511 0,-68.83567 -32.8763 0,-68.83597 -32.87746 0,-68.83627 -32.87859 0,-68.83656 -32.8797 0,-68.83627 -32.87973 0,-68.83614 -32.87974 0,-68.83509 -32.87982 0,-68.83376 -32.87992 0,-68.83236 -32.88002 0,-68.83097 -32.88013 0,-68.82956 -32.88023 0,-68.82816 -32.88034 0,-68.82728 -32.8804 0,-68.82644 -32.87706 0,-68.82639 -32.87686 0,-68.82632 -32.87676 0,-68.82621 -32.87662 0,-68.82611 -32.87652 0,-68.826 -32.87647 0,-68.82351 -32.87532 0,-68.82065 -32.87402 0,-68.82024 -32.87282 0,-68.82009 -32.87226 0,-68.82007 -32.87217 0,-68.81959 -32.87135 0,-68.81925 -32.87081 0,-68.81923 -32.8708 0,-68.81908 -32.87063 0,-68.81871 -32.8703 0,-68.81829 -32.8699 0,-68.81814 -32.86968 0,-68.8181 -32.86961 0,-68.81767 -32.8688 0,-68.81749 -32.86838 0,-68.81744 -32.8682 0,-68.81743 -32.86814 0,-68.8173 -32.8673 0,-68.81848 -32.86716 0,-68.81881 -32.86712 0,-68.81976 -32.86706 0,-68.82004 -32.86704 0,-68.82133 -32.86701 0,-68.82137 -32.86701 0,-68.82206 -32.8667 0,-68.82253 -32.86649 0,-68.82269 -32.86647 0,-68.82404 -32.86646 0,-68.82539 -32.86645 0,-68.82721 -32.86644 0,-68.82836 -32.86643 0,-68.82873 -32.86648 0,-68.82901 -32.8666 0,-68.82934 -32.86675 0,-68.82954 -32.86679 0,-68.82974 -32.8668 0,-68.83025 -32.86678 0,-68.83176 -32.86672 0,-68.83228 -32.8667 0))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false"
 ]
}

 The dataset includes 78 records from 7 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0046907-241126133413365/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.cntd3k
title: Occurrence Download

description: A dataset containing 662427 species occurrences available in GBIF matching the query:
{
 "and" : [
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Danaus plexippus (Linnaeus, 1758)"
 ]
}

 The dataset includes 662427 records from 299 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0046905-241126133413365/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48577/jpl.4bhlyi
title: The ALMA-ATOMS survey: Vibrationally excited HC3N lines in hot cores

description: Interstellar molecules are excellent tools for studying the physical and chemical environments of massive star-forming regions. In particular, vibrationally excited HC3N (HC3N*) lines are the key tracers for probing hot cores environments. We present the Atacama Large Millimeter/submillimeter Array (ALMA) 3 mm observations of HC3N* lines in 60 hot cores, aiming to investigate how physical conditions affect the excitation of HC3N* transitions. We have used the XCLASS for line identification. Under the assumption of local thermodynamic equilibrium (LTE), we derived the rotation temperature, column density, and line width of HC3N* transitions in hot cores. Additionally, we calculated the H2 column density and number density, along with the abundance of HC3N* relative to H2, to enable a comparison of the physical properties of hot cores with different numbers of HC3N* states. We have detected HC3N* lines in 52 hot cores, in which 29 cores showing more than one vibrationally excited state. Hot cores with higher gas temperatures have more detections of these vibrationally excited lines. The line width of each HC3N* line tends to decrease with increasing vibrational energy level. The excitation of HC3N* requires dense environments, with its spatial distribution and abundance influenced by the presence of UC Hii regions. The observed rotation temperature and column density of HC3N* both contribute to the number of HC3N* states in hot core environments. After analyzing the various factors influencing HC3N* excitation in hot cores, we conclude that the excitation of HC3N* is mainly driven by mid-IR pumping, while collisional excitation is ineffective.
DOI: 10.48577/jpl.sfiv5b
title: Observations of Loki Patera by Juno during close flybys

description: We used data from the Juno spacecraft to investigate both the spatial and temporal properties of Loki Patera on Io, acquired in two infrared bands between December 2022 and April 2024, at spatial resolutions ranging from 400 m to 15 km. Loki shows a thermal structure unlike other active lava lakes previously reported, with some brightening near the lake’s perimeter but lacking the continuous “hot ring” seen at other paterae. Modeling the slow rate of cooling suggests there is a significant volume of magma beneath the crust to provide the latent heat necessary to decelerate the cooling rate. A thermal propagation that may represent the signature of a resurfacing wave, going from the southwest of the lake to the north, was observed with a velocity of ~2 3 km/day. Data collected in 2024 may indicate the onset of a new resurfacing wave originating from a point source, rather than the foundering of a linear section of the crust. We also observed many small (~3 km wide), closely spaced (~ 10 km apart) islands that have persisted in the same locations for at least 45 years, since first being imaged by Voyager 1. The persistence of these islands challenges resurfacing models of Loki, as they have remained fixed likely anchored to the lava lake floor and have not noticeably changed in size, arguing against large scale thermal erosion. The central island of Loki shows a few thermal structures associated with the fractures that cross the island, indicating that the 19 fractures most likely contain molten lava.
DOI: 10.48577/jpl.p1oe7b
title: Europa Clipper Payload Accommodation Overview and Lessons Learned

description: NASA’s Europa Clipper spacecraft is equipped with a suite of ten science instruments, or payloads, to investigate Jupiter’s icy moon Europa. These ten science instruments collectively enable the spacecraft to meet the mission’s science objectives: (1) determine the thickness of Europa’s icy shell and how the ocean interacts with the surface, (2) investigate Europa’s composition, and (3) characterize the geology of Europa. All ten instruments were delivered from different institutions across the country to the Jet Propulsion Laboratory (JPL) for system-level integration from March 2022 to June 2023.
DOI: 10.48577/jpl.hw2jxt
title: Estimating the impact of a 2017 smoke plume on surface climate over northern Canada with a climate model, satellite retrievals, and weather forecasts

description: In August 2017, a smoke plume from wildfires in British Columbia and the Northwest Territories recirculated and persisted over northern Canada for over two weeks. We compared a full-factorial set of NASA Goddard Institute for Space Studies ModelE simulations of the plume to satellite retrievals of aerosol optical depth and carbon monoxide, finding that ModelE performance was dependent on the model configuration, and more so on the choice of injection height approach, aerosol scheme and biomass burning emissions estimates than to the choice of horizontal winds for nudging. In particular, ModelE simulations with free-tropospheric smoke injection, a mass-based aerosol scheme and comparatively high fire NOx emissions led to unrealistically high aerosol optical depth. Using paired simulations with and without fire emissions, we estimated that for 16 days over an 850 000 km2 region, the smoke decreased planetary boundary layer heights by between 253 m and 547 m, decreased downward shortwave radiation by between 52 Wm-2 and 172 Wm-2, and decreased surface temperature by between 1.5 oC and 4.9 oC, the latter spanning an independent estimate from operational weather forecasts of a 3.7 oC cooling. The strongest surface climate effects were for ModelE configurations with more detailed aerosol microphysics that led to a stronger first indirect effect.
DOI: 10.48577/jpl.favkb8
title: Identifying and Quantifying Greenhouse Gas Emissions with the AVIRIS-3 Airborne Imaging Spectrometer

description: Remotely sensed data from imaging spectrometers can identify both methane (CH4) and carbon dioxide (CO2) enhancements, subsequently enabling the quantification and direct sectoral attribution necessary to better constrain greenhouse gas emissions and inform mitigation strategies at local, regional, and national scales. We validate the ability of the Airborne Visible/Infrared Imaging Spectrometer 3 (AVIRIS-3), a NASA imaging spectrometer, to detect greenhouse gas enhancements from an airborne platform for the first time. Multiple CH4 controlled release experiments demonstrate that AVIRIS-3 can detect emissions at variable emission rates (&lt; 4 − 10 kg CH4/hour) and multiple flight altitudes (e.g., both 2,500 ft and 27,000 ft above ground level). The AVIRIS-3 instrument design provides several key improvements over earlier generations of airborne imaging spectrometers that enable detailed and precise greenhouse gas mapping from a range of emission sectors.
DOI: 10.48577/jpl.2ptegf
title: Making Hydrology Data More Accessible—2024 WaterSciCon Workshop Reflections

description: Earth observing data come in many different formats, resolutions, accuracies, and archival systems, making it challenging to navigate how to gather and harmonize all relevant data for a specific need. At WaterSciCon 2024, in a workshop dedicated to approaching how to overcome these challenges, participants from federal agencies, academic institutions, and the private sector came together to discuss and reflect on existing data access and visualization gaps in the hydrology community, identifying opportunities for connection, improvement, and collaboration. During the workshop, participants discussed what data accessibility means to them and noted existing pain points that create barriers to data access. Suggestions for improvement like the need for peer reviewed metadata, clear documentation, and user-centered design were championed across the board. As we move toward open science and open data, it is vital that we continue to have conversations about improving data accessibility for a wide range of audiences.
DOI: 10.48577/jpl.elogs2
title: Mineral Alteration in Water-Saturated Liquid CO2 on Early Mars

description: Liquid CO2 was likely present at various places and times in martian history, at least in the subsurface, and liquid CO2 floods have been suggested in the literature to explain morphological features ranging from small gullies to massive valley networks. This paper adds two important aspects to that discussion. First, extensive research into liquid CO2 sequestration on Earth has revealed remarkable chemical activity if the liquid is water-saturated, as it would likely have been on Mars. Second, it is plausible that surface liquid CO2 was stable in some regions on early Mars if atmospheric pressure exceeded 5.18 bar. In some cases, single-episode liquid CO2 reactions can result in rapid and copious production of altered minerals that would require multiple episodes in different aqueous pH environments to explain in a liquid water paradigm.
DOI: 10.48577/jpl.7yq1dv
title: Comment on “Zambon, F. et al. Io Hot Spot Distribution Detected by Juno/JIRAM. Geophysical Research Letters, 50, e2022GL100597 (2023)”

description: The quantification and distribution of thermal emission from Io’s active volcanoes reflects volcanic advection within Io and provides some insight as to patterns of internal heating (Davies et al., 2015; Hay et al., 2020; Matsuyama et al., 2022; Ross et al., 1990; Veeder et al., 2012; Veeder et al., 2015). Davies et al. (2024) analysed all image data of Io obtained by the Jovian Infrared Auroral Mapper (JIRAM) (Adriani et al., 2017) on the Juno spacecraft from Juno orbits PJ5 (March 2017) to PJ43 (July 2022). Davies et al. processed images collected at 3.5 and 4.8 μm and identified 266 hot spots. They compared their hot spot detections with those of Zambon et al. (2023), who published a list of 242 hot spots detected in the same JIRAM data from orbits PJ10 (December 2017) through PJ33 (April 2021). However, Davies et al. found only 156 of the Zambon et al. (2023) hot spots, as well as others that Zambon et al. did not report. Both Davies et al. (2023) and Zambon et al. (2003) stacked JIRAM images obtained during a given flyby in order to increase signal to noise, enhancing thermal emission from faint hot spots. These methodologies used NAIF SPICE kernels to identify Io in the image frame, and allowed the position and viewing geometry for every on-planet pixel to be determined. Where sufficient observations existed, and to allow for the spacecraft geometry changing over a number of acquisitions, Zambon et al. grouped images into a series of superposition products (“super images”), and identified and determined the position of hot spots in each product. Davies et al. (2024) used the same approach, co-registering and stacking images. However, Davies et al. (2024) found that use of SPICE kernels alone was insufficient to accurately determine the position of hot spots on Io’s surface. Without further adjustment, uncertainty in position could be up to four pixels. At resolutions of 40 to &gt;100 km/pixel, this is a significant distance, especially when processing data in Io’s polar regions where such uncertainty would translate into substantial movement in estimated hot spot longitude. To minimise positional error, for each orbit Davies et al. (2023) reprojected a selection of JIRAM frames to point perspective and adjusted and aligned each individual frame using the position of Io’s limb and any surface features that were visible. This accurate superpositioning and stacking improved contrast and revealed many faint hot spots.
DOI: 10.48577/jpl.b5kqw0
title: On The Lunar Origin of Near-Earth Asteroid 2024 PT5

description: The Near-Earth Asteroid (NEA) 2024 PT5 is on an Earth-like orbit which remained in Earth’s immediate vicinity for several months at the end of 2024. PT5’s orbit is challenging to populate with asteroids originating from the Main Belt and is more commonly associated with rocket bodies mistakenly identified as natural objects or with debris ejected from impacts on the Moon. We obtained visible and near-infrared reflectance spectra of PT5 with the Lowell Discovery Telescope and NASA Infrared Telescope Facility on 2024 August 16. The combined reflectance spectrum matches lunar samples but does not match any known asteroid types – it is pyroxene-rich while asteroids of comparable spectral redness are olivine-rich. Moreover, the amount of solar radiation pressure observed on the PT5 trajectory is orders of magnitude lower than what would expected for an artificial object. We therefore conclude that 2024 PT5 is ejecta from an impact on the Moon, thus making PT5 the second NEA suggested to be sourced from the surface of the Moon. While one object might be an outlier, two suggest that there is an underlying population to be characterized. Long-term predictions of the position of 2024 PT5 are challenging due to the slow Earth encounters characteristic of objects in these orbits. A population of near-Earth objects which are sourced by the Moon would be important to characterize for understanding how impacts work on our nearest neighbor and for identifying the source regions of asteroids and meteorites from this under-studied population of objects on very Earth-like orbits.
DOI: 10.48577/jpl.kwddsz
title: Searching for Planets Orbiting Vega with the James Webb Space Telescope

description: The most prominent of the IRAS debris disk systems, $\alpha$ Lyrae (Vega), at a distance of 7.7 pc, has been observed by both the NIRCam and MIRI instruments on the James Webb Space Telescope (JWST). This paper describes NIRCam coronagraphic observations which have achieved F444W contrast levels of 3$\times10^{-7}$ at 1\arcsec, 1$\times10^{-7}$ at 2\arcsec\ and few $\times 10^{-8}$ beyond 5\arcsec\, corresponding to masses of $&lt;$ 3, 2 and 0.5 \mj\ for a system age of 700 Myr. Three F444W objects are identified close to or interior to the MIRI debris disk. One is also detected by MIRI, appears to be extended and has a spectral energy distribution similar to those of distant extragalactic sources. The second one also appears extended in the NIRCam data suggestive of an extragalactic nature. The third object, detected at low SNR=3.5, is located 1.4\arcsec\ south of Vega and has no counterpart in either F210M or MIRI. With an inferred mass of 2$\sim$3 \mj\, the object, if an exoplanet, would likely be disruptive of the smooth disk seen in the MIRI observations. Observations at another epoch will be required to provide definitive confirmation or rejection of this object as associated with Vega. Eight additional objects are found within 60\arcsec\ of Vega, but none has astrometric properties or colors consistent with planet candidates. These observations reach a level consistent with expected Jeans Mass limits. Deeper observations achieving contrast levels $&lt;10^{-8}$ outside of $\sim$4\arcsec\ and reaching masses below that of Saturn are possible, but may not reveal a large population of new objects.
DOI: 10.48577/jpl.stemi6
title: The NASA-ISRO Synthetic Aperture Radar Mission – A Story of Partnership and Possibilities

description: No abstract available.
DOI: 10.25907/00130
title: Genomes of vertebrate populations

description: Deleterious mutation load in human populations; Conservation genetics of Dingoes; Genomics of fish and marine invetebrate populations.
DOI: 10.15468/dl.npb35d
title: Occurrence Download

description: A dataset containing 3471 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Leopardus guigna (Molina, 1782)"
 ]
}

 The dataset includes 3471 records from 22 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0046908-241126133413365/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.34740/kaggle/dsv/10280832
title: Top 10,000 Anime Dataset (2024)
DOI: 10.15468/dl.w4tczp
title: Occurrence Download

description: A dataset containing 107424170 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is United Kingdom of Great Britain and Northern Ireland",
 "OccurrenceStatus is Present",
 "Year 2002-2023"
 ]
}

 The dataset includes 107424170 records from 1568 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0046890-241126133413365/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.3535/4d5-4sc-jcs
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wsr-zpt-mfx
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/00t-vep-eqn
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/57s-2bv-ng5
title: Lepidoptera Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/gpf-4fl-ph6
title: Lepidoptera Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/pe1-5jl-eps
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/7xy-n04-w9h
title: Lepidoptera Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/dqr-bfb-1ts
title: Lepidoptera Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/mcb-nya-pfl
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/cad-vn3-x5w
title: Lepidoptera Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/q8j-5tq-7d2
title: Lepidoptera Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/r46-101-bc6
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/42x-jq7-9v9
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/05c-x03-ksn
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/zde-c3z-kh6
title: Animalia

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/2tq-m42-4xp
title: Lepidoptera Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.