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Figure 3c. from: Defining the Scholarly Commons - Reimagining Research Communication. Report of Force11 SCWG Workshop, Madrid, Spain, February 25-27, 2016 - Research Ideas and Outcomes 2: e9340 (26 May 2016) https://doi.org/10.3897/rio.2.e9340
Figure 3c. - Islands of possibilities (part of YKON facilitation) at Madrid workshopFigure 3a.Islands of possibilities located in workshop roomFigure 3b.Personality modification islandFigure 3c.Observation island <br> Observation island
Figure 3a. from: Defining the Scholarly Commons - Reimagining Research Communication. Report of Force11 SCWG Workshop, Madrid, Spain, February 25-27, 2016 - Research Ideas and Outcomes 2: e9340 (26 May 2016) https://doi.org/10.3897/rio.2.e9340
Figure 3a. - Islands of possibilities (part of YKON facilitation) at Madrid workshopFigure 3a.Islands of possibilities located in workshop roomFigure 3b.Personality modification islandFigure 3c.Observation island <br> Islands of possibilities located in workshop room
Figure 8a. from: Defining the Scholarly Commons - Reimagining Research Communication. Report of Force11 SCWG Workshop, Madrid, Spain, February 25-27, 2016 - Research Ideas and Outcomes 2: e9340 (26 May 2016) https://doi.org/10.3897/rio.2.e9340
Figure 8a. - Workshop visualization - collection of ideas and group visionsFigure 8a.Visualization showing all ideas generated collectively in the first round (session 3, dark grey) or second round (session 4, light grey), and those generated by the respective groups (solid colors) as part of their vision of scholarly communication. Figure 8b.Visualizaton showing all groups' visions as interconnected elements (triples), with common elements overlapping. <br>
Fig. 25. First leg pair. A in Revision of the genus Ommatoiulus Latzel, 1884 (Julida, Diplopoda) in Portugal, with description of six new species
Fig. 25. First leg pair. A. Ommatoiulus alacygni sp. nov. B. O. andalusius (Attems, 1927). C. O. camurus sp. nov. D. O. denticulatus sp. nov. E. O. litoralis sp. nov. F. O. porathi (Verhoeff, 1893). G. O. staglae sp. nov.. H. O. stellaris sp. nov. Scale bars 0.1 mm.
The Kühtai dataset: 25 years of lysimetric, snow pillow and meteorological measurements
<p>This dataset presents long-term observations from an experimental snow lysimeter plot in Kühtai (Austrian Alps). The data set includes 15 minutes data of snow water equivalent from a 10 m² snow pillow, snow melt outflow from a 10 m² snow lysimeter placed at the same location as the pillow, meteorological data (precipitation, incoming global radiation, reflected short wave radiation, air temperature, relative air humidity and wind speed), and other data (snow depths, snow temperatures at seven heights) from the period October, 1990 – May, 2015. All data have been quality checked, and gaps in the meteorological data have been filled in.</p>
Figs. 25-28 — Apostenus maroccanus n in The genera Agroeca, Agraecina, Apostenus and Scotina in the Maghreb countries (Araneae: Liocranidae)
Figs. 25-28 — Apostenus maroccanus n. sp. - 25. Male palp, lateral view; - 26 Idem, ventral view; - 27. Epigyne, ventral view. - 2S. Vulva, ventral view. Figs. 29-30 — Apostenus algericus n. sp. - 29. Male palp, lateral view; - 30. Idem, ventral view.
WWV 15 MHz reception test -- 60 minutes starting at 1937 UTC, July 25, 2017.
<p>Steven Reyer, WA9VNJ. Approx.Lat/Long: 43.218, -87.951. This 60-minute 15 MHz WWV recording was started at 1937 UTC on July 25, 2017, in preparation for the Solar Eclipse experiment in late August.</p> <p>The radio is a Yaesu FT-857D locked to a Trimble Thunderbolt GPSDO using an XRef-FT oscillator interface. Antenna is an RF-PRO-1B shielded magnetic loop, aimed N-S. Calibration of the radio and sample rate correction is determined using a second Trimble Thunderbolt GPS and Rigol DG1022Z GPS-locked signal generator.</p> <p>Spectrum Lab software is used to record the WAV file and to analyze incoming audio with sample rate of 11025 Hz. FFTs are 512k-point, 75% overlapping, yielding a new measurement every 12 seconds. Radio is tuned to 14999.00 kHz USB yielding audio around 1kHz (labeled "PeakFreq" in the txt file). Thus, the measured radio frequencies are near 15000 kHz. Calibration tests show that the audio frequency measurements are approximately 0.0384 Hz high, due the approximations in both the radio's DDS and the sample rate. This 0.0384 Hz number can be subtracted from the PeakFreq values to get corrected audio frequencies, which can then be added to the 14999 kHz number.</p>
Supporting Information for "Electron and proton peak intensities as observed by a five-spacecraft fleet in solar cycle 25"
<p>Table of parameters employed in the study "Electron and proton peak intensities as observed by a five-spacecraft fleet in solar cycle 25". The table contains the original peak intensities directly taken from the <em>SERPENTINE SEP event catalog</em>, without any scaling or inter-calibration factors that are applied in the study. All information provided in the table is based on the <em>SERPENTINE SEP event catalog</em> and <em>SERPENTINE CME and coronal shocks catalog</em><strong>,</strong> only limiting the variables to those used in this study. The dataset is in CSV format.</p> <p>For more information, and if you use this table, please refer to the corresponding publication:</p> <blockquote> <div> <p>Electron and proton peak intensities as observed by a five-spacecraft fleet in solar cycle 25<br>G. U. Farwa, N. Dresing, J. Gieseler, L. Vuorinen, I. G. Richardson, C. Palmroos, S. Valkila, B. Heber, S. Jensen, P. Kühl, L. Rodríguez-García and R. Vainio<br>A&A, 693 (2025) A198<br>DOI: <a href="https://doi.org/10.1051/0004-6361/202450945">10.1051/0004-6361/202450945</a></p> </div> </blockquote> <div> <div> </div> </div> <p><strong>Field descriptions</strong></p> <ul> <li>id: ID</li> <li>date: Event date [UTC]</li> <li>flare_time: Flare time [UTC]</li> <li>flare_lat: Flare Carrington latitude [deg]</li> <li>flare_lon: Flare Carrington longitude [deg]</li> <li>flare_class: Flare class (GOES)</li> <li>flare_comments: Flare Comments</li> <li>radio_type2: Radio type II bursts</li> <li>decametric_type2_start: Decametric type II burst start time [UT]</li> <li>decametric_type2_stop: Decametric type II burst end time [UT]</li> <li>radio_type2_start: Metric radio type II burst start time [UT]</li> <li>radio_type2_stop: Metric radio type II burst end time [UT]</li> <li>solar_mach_link: Solar-Mach link</li> <li>S/C codes <ul> <li>BepiC: BepiColombo</li> <li>L1: L1 (SOHO/Wind)</li> <li>PSP: Parker Solar Probe</li> <li>STA: STEREO A</li> <li>SolO: Solar Orbiter</li> </ul> </li> <li>S/C related field descriptions <ul> <li>{sc}_sc_lat: S/C Carrington latitude [deg]</li> <li>{sc}_sc_lon: S/C Carrington longitude [deg]</li> <li>{sc}_dist: S/C radial distance [au]</li> <li>{sc}_p25MeV_onset_date: S/C protons 25 MeV onset date [UTC]</li> <li>{sc}_p25MeV_onset_time: S/C protons 25 MeV onset time [UTC]</li> <li>{sc}_p25MeV_onset_time_formatted: S/C protons 25 MeV onset time [UTC] (Formatted)</li> <li>{sc}_p25MeV_onset_averaging: S/C protons 25 MeV averaging used for onset [min]</li> <li>{sc}_p25MeV_onset_sector: S/C protons 25 MeV sector used for onset</li> <li>{sc}_p25MeV_peak_date: S/C protons 25 MeV peak date [UTC]</li> <li>{sc}_p25MeV_peak_time: S/C protons 25 MeV peak time [UTC]</li> <li>{sc}_p25MeV_peak_time_formatted: S/C protons 25 MeV peak time [UTC] (Formatted)</li> <li>{sc}_p25MeV_peak_flux: S/C protons 25 MeV original peak flux [cm^-2 s^-1 sr^-1 MeV^-1]</li> <li>{sc}_p25MeV_peak_flux_formatted: S/C protons 25 MeV original peak flux [cm^-2 s^-1 sr^-1 MeV^-1] (Formatted)</li> <li>{sc}_p25MeV_peak_averaging: S/C protons 25 MeV averaging used for peak [min]</li> <li>{sc}_p25MeV_peak_sector: S/C protons 25 MeV sector used for peak</li> <li>{sc}_p25MeV_injection_date: S/C protons 25 MeV inferred injection date [UTC]</li> <li>{sc}_p25MeV_injection_time: S/C protons 25 MeV inferred injection time [UTC]</li> <li>{sc}_p25MeV_sw_speed: S/C protons 25 MeV onset solar wind speed [km/s]</li> <li>{sc}_p25MeV_comments: S/C protons 25 MeV comments</li> <li>{sc}_e100keV_onset_date: S/C electrons 100 keV onset date [UTC]</li> <li>{sc}_e100keV_onset_time: S/C electrons 100 keV onset time [UTC]</li> <li>{sc}_e100keV_onset_time_formatted: S/C electrons 100 keV onset time [UTC] (Formatted)</li> <li>{sc}_e100keV_onset_averaging: S/C electrons 100 keV averaging used for onset [min]</li> <li>{sc}_e100keV_onset_sector: S/C electrons 100 keV sector used for onset</li> <li>{sc}_e100keV_peak_date: S/C electrons 100 keV peak date [UTC]</li> <li>{sc}_e100keV_peak_time: S/C electrons 100 keV peak time [UTC]</li> <li>{sc}_e100keV_peak_time_formatted: S/C electrons 100 keV peak time [UTC] (Formatted)</li> <li>{sc}_e100keV_peak_flux: S/C electrons 100 keV original peak flux [cm^-2 s^-1 sr^-1 MeV^-1]</li> <li>{sc}_e100keV_peak_flux_formatted: S/C electrons 100 keV original peak flux [cm^-2 s^-1 sr^-1 MeV^-1] (Formatted)</li> <li>{sc}_e100keV_peak_averaging: S/C electrons 100 keV averaging used for peak [min]</li> <li>{sc}_e100keV_peak_sector: S/C electrons 100 keV sector used for peak</li> <li>{sc}_e100keV_injection_date: S/C electrons 100 keV inferred injection date [UTC]</li> <li>{sc}_e100keV_injection_time: S/C electrons 100 keV inferred injection time [UTC]</li> <li>{sc}_e100keV_sw_speed: S/C electrons 100 keV onset solar wind speed [km/s]</li> <li>{sc}_e100keV_comments: S/C electrons 100 keV comments</li> <li>{sc}_e1MeV_onset_date: S/C electrons 1 MeV onset date [UTC]</li> <li>{sc}_e1MeV_onset_time: S/C electrons 1 MeV onset time [UTC]</li> <li>{sc}_e1MeV_onset_time_formatted: S/C electrons 1 MeV onset time [UTC] (Formatted)</li> <li>{sc}_e1MeV_onset_averaging: S/C electrons 1 MeV averaging used for onset [min]</li> <li>{sc}_e1MeV_onset_sector: S/C electrons 1 MeV sector used for onset</li> <li>{sc}_e1MeV_peak_date: S/C electrons 1 MeV peak date [UTC]</li> <li>{sc}_e1MeV_peak_time: S/C electrons 1 MeV peak time [UTC]</li> <li>{sc}_e1MeV_peak_time_formatted: S/C electrons 1 MeV peak time [UTC] (Formatted)</li> <li>{sc}_e1MeV_peak_flux: S/C electrons 1 MeV original peak flux [cm^-2 s^-1 sr^-1 MeV^-1]</li> <li>{sc}_e1MeV_peak_flux_formatted: S/C electrons 1 MeV original peak flux [cm^-2 s^-1 sr^-1 MeV^-1] (Formatted)</li> <li>{sc}_e1MeV_peak_averaging: S/C electrons 1 MeV averaging used for peak [min]</li> <li>{sc}_e1MeV_peak_sector: S/C electrons 1 MeV sector used for peak</li> <li>{sc}_e1MeV_injection_date: S/C electrons 1 MeV inferred injection date [UTC]</li> <li>{sc}_e1MeV_injection_time: S/C electrons 1 MeV inferred injection time [UTC]</li> <li>{sc}_e1MeV_sw_speed: S/C electrons 1 MeV onset solar wind speed [km/s]</li> <li>{sc}_e1MeV_comments: S/C electrons 1 MeV comments</li> <li>{sc}_ep_ratio: Ratio of Electrons (~1MeV) / Protons (25-40 MeV)</li> </ul> </li> <li>CME related descriptions <ul> <li>cme_id: CME ID</li> <li>L1_date: Date of CME identification at L1</li> <li>L1_time: Time of CME identification at L1</li> <li>L1_pos_speed: Plane of sky speed of CME measured at L1</li> </ul> </li> </ul> <div><strong>CHANGELOG:</strong></div> <div> <ul> <li>2025-06-12 <ul> <li>Updated peak fluxes and peak times of PSP 1 MeV electrons, as well as PSP's e/p ratios (the previous flux values are erroneous!)</li> </ul> </li> </ul> </div>
Fig. 25. Guaranita goloboffi Huber, 2000 in Revision of the South American Ninetinae genus Guaranita (Araneae, Pholcidae)
Fig. 25. Guaranita goloboffi Huber, 2000; males from Cabra Corral (A–C, G–I; ZFMK Ar 24129) and from NW of Chumbicha (D–F; ZFMK Ar 24130). A–C. Chelicerae, frontal, lateral, and ventral views. D–F. Left procursus, prolateral, dorsal, and retrolateral views. G–I. Left genital bulb, prolateral, dorsal, and retrolateral views. Scale bars = 0.1 mm.
Fig. 25 in Epimeria of the Southern Ocean with notes on their relatives (Crustacea, Amphipoda, Eusiroidea)
Fig. 25. Epimeria (Drakepimeria) colemani subgen. et sp. nov., adult ♀, Adélie Coast, CEAMARC 2724, MNHN-IU-2014-4337. A. Lateral habitus. B. Dorsal habitus.
Figs. 25-29 in A Review Of The Genus Stilpon Loew, 1859 (Empidoidea: Hybotidae) From The Oriental Region
Figs. 25-29. Stilpon nhamyaaw, new species, male. 25, mid leg, anterior view, 26, hypopygium, ventral view, 27, upper lobe of left surstylus, dorsal view, 28, left cercus and subepandrial sclerite, right lateral view, 29, right surstylus, dorsal view. Scale bar: 0.1 mm.
Dataset of the publication Phys. Chem. Chem. Phys., 2023,25, 23614-23625
<p>The experimental work was partially done within the project PROMETH2O (EMPIR 20IND06), which received funding from the EMPIR programme co-financed by the Participating States and from the European Unions Horizon 2020 research and innovation programme.</p>
Fig. 25 in Two new species of the genus Camponotus Mayr, 1861 (Hymenoptera: Formicidae) with five new records from India
Fig. 25. Body in profile view. A. Camponotus binghamii Forel, 1894. B. Camponotus parius Forel, 1889. Scale bars = 0.5 mm.
FIGURE 25 in Head and otolith morphology of the genera Hymenocephalus, Hymenogadus and Spicomacrurus (Macrouridae), with the description of three new species
FIGURE 25. Hymenocephalus punt: A—Paratype, ZMMGU-P 23600, TL 140 mm (photo M. Krag). B—Holotype ZMMGU- P 23599, TL 106+ mm (photo M. Krag).
Fig. 25 in Early Ordovician Conodonts from Far Western New South Wales, Australia
Fig. 25. Scalpellodus latus (van Wamel, 1974): A,B, Sa element, AMF120452, Y4–2, A, inner lateral view of the basal part showing the fine striae, B, lateral view; C, Sb element, AMF120453, Y4–2, inner lateral view; D, Sb element, AMF120454, M/A11-1, inner lateral view; E,H, Sd element, AMF120455, M/A7, E, inner lateral view, H, close up showing fine striae; F, Sd element, AMF120456, M/A7, posterior view; G, P element, AMF120457, TAB1/39.5, inner lateral view; I, Sd element, AMF120458, M/A7, inner lateral view; J, Sc element, AMF120459, Y4–2, lateral view. Scale bars 100 µm, unless otherwise indicated.
Figure 25. Lepidepecreum tourville n in The Lysianassoid Amphipod Genera Lepidepecreoides and Lepidepecreum in Southern Waters (Crustacea: Lysianassidae: Tryphosinae)
Figure 25. Lepidepecreum tourville n.sp. Holotype female, 5.8 mm, NMV J47730; paratype male, 5.6 mm, NMV J17159; Cape Tourville, Australia. Scales for U1–3 represent 0.1 mm, remainder represent 0.5 mm.
Figure 25. Eogammarus psammophilus Bousfield, 1979 in A revision of Eogammarus Birstein, 1933 (Crustacea, Amphipoda, Anisogammaridae), with a description of a new species
Figure 25. Eogammarus psammophilus Bousfield, 1979, Amchitka Island, Aleutian Islands, paratype, female, 16.0 mm, CMNC 1982-0321. (A) Antenna 1; (B) antenna 2; (C) gnathopod 1; (D) dactylus and palm of gnathopod 1 (slender setae on palm are omitted); (E) gnathopod 2; (F) dactylus and palm of gnathopod 2 (slender setae on palm are omitted); (G–I) coxa–ischium of pereopods 5–7; (J) brood plate of gnathopod 2; (K) uropod 3. Scale bars: 0.1 mm.
Abb. 25-30 in Zur Kenntnis paläarktischer Bienen der Gattung Nomada SCOPOLI, 1770 (Hymenoptera, Apidae)
Abb. 25-30: (25) N. dilleri ♂ Dörnchen Hinterschiene; (26) N. flavoorbitalis ♀ Habitus dorsal; (27) N. flavoorbitalis ♀ Höcker des Scutellums von vorne gesehen; (28) N. flavoorbitalis ♀ Dorn der Vordercoxen; (29) N. flavoorbitalis ♀ Metatarsus der Hinterbeine; (30) N. gusenleitneriella ♀ Habitus dorsal.
Fig. 25 in Cephalopods From The Cretaceous/Tertiary Boundary Interval On The Atlantic Coastal Plain, With A Description Of The Highest Ammonite Zones In North America. Part 2. Northeastern Monmouth County, New Jersey
Fig. 25. Sphenodiscus lobatus (Tuomey, 1856), Tinton Formation, AMNH loc. 3348, Tinton Falls, Monmouth County, New Jersey. A. MAPS 2002a9, suture at the adapical end of the specimen at a whorl height of approximately 139 mm. B. MAPS A2002a8, suture at a whorl height of approximately 91 mm.
Figure 25 in A preliminary report on the World species of Bemisia Quaintance and Baker and its congeners (Hemiptera: Aleyrodidae) with a comparative analysis of morphological variation and its role in the recognition of species Raymond Gill
Figure 25. Type material, Bemisia caudasculptura Quaintance and Baker, Cholula, Mexico, Dec. 1910, ex. Fraxinus sp., USNM# 6517.
ScienceDex guides
Understand access before you commit
These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.
Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.
DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.