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1,445 results for “Irradiance”
Total-Body Irradiation With or Without Fludarabine Phosphate Followed By Donor Stem Cell Transplant in Treating Patients With Hematologic Cancer
ClinicalTrials.gov study NCT00075478. IPD Sharing: Not stated. Countries: 3. Publications: 2.
Photocatalytic degradation of rhodamine B using zinc oxide/silver nanowire nanocomposite films under UV irradiation
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Analysis of the proteomic profile in serum of irradiated nonhuman primates treated with Ex-Rad, a radiation medical countermeasure
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Effects of X-ray irradiation and housing conditions on mitochondria in Peromyscus maniculatus
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RNAseq analysis of heart samples collected from wild-type and ZNF768 null mice 8 hours post-irradiation
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Impact of irradiated Drosophila melanogaster pupae on the quality and population parameters of Trichopria drosophilae
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The role of irradiance in controlling coralline algal calcification
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The temporal response of a glioma cell population to irradiation: modeling the effect of dose and cell density
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Critical PO2 as a diagnostic biomarker for the effects of low-oxygen modified and controlled atmospheres on phytosanitary irradiation treatments in the Cabbage Looper Trichoplusia ni (Hübner)
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PAK3 downregulation induces cognitive impairment following cranial irradiation
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Data from: Predicting photosynthesis-irradiance relationships from satellite remote-sensing observations
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Host suitability and fitness-related parameters in Coptera haywardi ([Hymenoptera]: [Diapriidae]) reared on irradiated Ceratitis capitata ([Diptera]: [Tehritidae]) pupae stemming from the genetic sexing Vienna-8 strain with a temperature-sensitive lethal mutation
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Girasol, a sky imaging and global solar irradiance dataset
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Exploring the roles of iron and irradiance in dynamics of diatoms and Phaeocystis in the Amundsen Sea continental shelf water
<p>The Amundsen Sea continental shelf (ACS) water ecosystem is expected to undergo changes since the increasing melt rate of glaciers and decreasing sea ice extent by global warming would lead to the mitigation of iron and light limitation. We investigated how diatoms and Phaeocystis, two dominant taxa, and primary production in the ACS water would respond to variations in iron and light availabilities by using a 1-D pelagic ecosystem model. In the model, we added sea ice effects that reduce light penetration and optimized model parameters for diatoms and Phaeocystis. The results from our model showed good agreement with 20-year observations of Chl-a as well as the biomass proportion of diatoms and Phaeocystis and nutrient distributions during the growing season. Our model experimental results suggest that the current moderate iron and high light conditions favor the growth of Phaeocystis over diatoms. Moreover, as iron increases, the organic carbon exudation by phytoplankton increases more rapidly than net primary production (NPP), leading to a decline in phytoplankton biomass. On the other hand, irradiance plays a role in controlling NPP in terms of photoinhibition which is reduced by increasing iron. Increases in both iron and irradiance lead to an advance in the timing of the bloom peak (surface Chl-a maximum) due to increases in phytoplankton carbon loss and photoinhibition. Our results imply that the dominance of Phaeocystis can continue and that the carbon uptake capacity of the ACS in the summer seasons might increase given that iron availability will increase with future climate change.</p>
Level 2 spectra of the global solar irradiance in the wavelength range 290 - 500 nm measured at Aosta - Saint Christophe, Italy by the Bentham DTMc300 with serial number 5541 in 2006 - 2019
<p>The provided dataset includes the Level 2 <strong>spectral measurements</strong> (in Watt/m<sup>2</sup>/nm) of the solar irradiance in the range 290 - 500 nm, performed by the Bentham DTMc300 spectroradiometer with serial number 5541. The particular instrument performs automated continuous, high quality measurements at Aosta - Saint Christophe, Italy (45.7° N, 7.4° E, 570 m a.s.l.) since 2006. The Level 2 spectra are re-evaluated and homogenized and are currently available for the period 24 July 2006 - 8 July 2019. Each file contains the spectra for one day. The time (in UTC) for the measurements at 290, 400, and 500 nm is also provided for each spectral scan so that the user has also information for the duration of each scan.</p> <p>The daily <strong>noon UV index</strong> is also provided for the same period in the file "<strong>aao_noon_uvi_l2.dat</strong>". Erythemal doses have been calculated by weighting each spectrum with the CIE (1999) effective spectrum, and then integrating in the range 290 - 400 nm. Then the UV index has been calculated by dividing erythemal dose (in mWatt/m<sup>2</sup>) by 25. The noon UV index for each day has been calculated as the average of available measurements for ±15 minutes around the exact local noon.</p> <p>For further information for file format and contents please see the <strong>readme.txt</strong> file.</p> <p>Reference</p> <p>CIE: CIE S007/E-1998 Erythema reference action spectrum and standard erythema dose, Color Research & Application, 24, 158-158, 10.1002/(sici)1520-6378(199904)24:2<158::aid-col11>3.0.co;2-4, 1999.</p>
Datapack for 'Nanocluster evolution and mechanical properties of ion irradiated T91 ferritic-martensitic steel' paper
<p>Data pack for the paper 'Nanocluster evolution and mechanical properties of ion irradiated T91 ferritic-martensitic steel', Journal of Nuclear Materials, 2021</p>
Cloud motion vectors for irradiance forecasts
<p>This file contains the x and y components of the estimated cloud velocity for the period of 2014-04-05 to 2014-06-30 over Tucson, AZ. The data was extracted from a numerical weather model run at the University of Arizona using the vertical layer with the highest relative humidity. The data was used to make irradiance forecasts via cloud advection and an irradiance monitoring network.</p>
Irradiance monitoring network data
<p>The data.tar.gz archive contains data from an irradiance monitoring network in Tucson, Arizona for the period 2014-04-05 to 2014-06-30. It includes a sensor metadata csv, csv files for the measurements on each day, and csv files for the clearsky-profiles for each sensor on each day. This data was used to make short-term forecasts of solar irradiance.</p>
Irradiance monitoring network data and wind motion vectors
<p>The data.tar.gz archive contains data from an irradiance monitoring network in Tucson, Arizona for the period 2014-04-05 to 2014-06-30. It includes a sensor metadata csv, csv files for the measurements on each day, csv files for the clearsky-profiles for each sensor on each day, and a time-series of the expected wind motion vectors obtained from a numerical weather model. This data was used to make short-term forecasts of solar irradiance.</p>
Data from "Short-Lived Gravitational Instability in Isolated Irradiated Discs"
<p>The paper by Rowther et al. (2024) simulates the evolution of irradiated gravitationally unstable protoplanetary discs with live radiative transfer using Phantom (Price et al. 2018) coupled with MCFOST (Pinte et al. 2006, 2009). The codes used to perform the simulations are available at </p> <ul> <li>Phantom -- <a href="https://github.com/danieljprice/phantom" target="_blank" rel="noopener">https://github.com/danieljprice/phantom</a></li> <li>MCFOST -- <a href="https://github.com/cpinte/mcfost" target="_blank" rel="noopener">https://github.com/cpinte/mcfost</a></li> </ul> <p>The dataset contains the following data to recreate any of the figures:</p> <ol> <li>Selected snapshots of the 5 simulations shown in the paper. </li> <li>Post-processed data to recreate the line-plots shown in the paper.</li> <li>.fits files of the synthetic continuum images created by post-processing the simulation snapshot with MCFOST at 1.3mm.</li> </ol> <p>To recreate any of the simulations in the paper, all relevant files required are in <strong>Simulations.zip</strong>.</p> <ul> <li><strong>.setup: </strong>The file used by phantomsetup to create the initial conditions of the disc.</li> <li><strong>.in: </strong>The file used by phantom to perform the simulation.</li> <li><strong>.para:</strong> A file containing the parameters used by MCFOST to perform the Radiative Transfer calculations.</li> <li>The files for the 0.1 Solar mass disc can be identified by the prefix <strong>Md0p1</strong>. Similarly, the prefix <strong>Md0p25 </strong>identifies the files for 0.25 Solar mass disc.</li> </ul> <p>The data to recreate any of the figures in the paper are found in <strong>Figure_*.zip</strong>.</p> <p>The binary code snapshots (<strong>Md0p1_01400, Md0p25_00300</strong> etc.) containing the raw data (particle positions, velocities, thermal energy etc.) can be visualised by <a href="https://github.com/danieljprice/splash" target="_blank" rel="noopener">Splash</a> (Price 2007) or <a href="https://github.com/ttricco/sarracen/" target="_blank" rel="noopener">Sarracen</a> (Harris & Tricco 2023). The latter was used to create the figures in the paper.</p> <p> </p>
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These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.
Allen Brain Atlas
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International Brain Laboratory public data
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OpenNeuro
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