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34 results for “Sunset”
sunset: A database of synthetic atmospheric-escape transmission spectra for nearly every transiting exoplanet
<div> <div> <p><strong>This sunset version belongs to the A&A paper. The sunset database belonging to the arXiv pre-print can be found as version 1 of this Zenodo repository.</strong></p> <p>This repository contains the sunset database of atmospheric-escape transmission spectra for most currently known transiting exoplanets. This database is described in Linssen et al. (2025). The complete zipped (unzipped) database is ~5GB (~28GB). To prevent a huge download just to access a specific single planet model, we have uploaded sunset in a few different batches. The "zip_dictionary.txt" file lists each planet and which zip batch it is in. </p> <p>For each planet, there are three files:<br>- The "info" file contains warnings that pertain to that planet specifically (for general warnings that apply to each planet, see Linssen et al. 2025). It also lists the used planetary parameters, and the transit depth, equivalent width, S/N prefactors and transmission spectroscopy metrics for a few spectral lines. Finally, it gives simple step-by-step instructions on how to reproduce the model results using sunbather.<br>- The "spectrum_sparse" file contains the transmission spectrum. In principle, the spectrum runs from 911 to 11,000 angstroms in 1,000,000 bins (translating to R~400,000). However, in large portions of this wavelength grid, there are no spectral lines and the transit spectrum is simply equal to the continuum. To keep the file size to a minimum, we have removed those continuum regions from the spectrum, resulting in a "sparse" spectrum.<br>- The "structure" file contains the radial atmospheric structure profiles of the density, velocity, temperature and mean molecular weight.</p> <p>Additionally, this repository includes "included_lines_by_species.txt" and "included_lines_by_wavelength.txt", which list all the spectral lines that are present in the transmission spectra. Lines are labeled by the specific ion that they originate from, as well as the energy level. The energy level is expressed as a number, where 1 is the ground state, 2 is the first excited state, etc. Translating this energy level into the atomic configuration can be done by looking in the sunbather source code: in the /sunbather/src/sunbather/RT_tables/ folder, each ion has a file such as "Fe+_levels_processed.txt", which lists the energy levels and their atomic configurations.</p> <p>Finally, there is a large tabular file called "sunset_overview.csv". This file includes the NASA Exoplanet Archive parameters of each exoplanet. Additionally, there are some columns that we added, with calculated variables such as the atmospheric mass-loss rate, the Parker wind temperature, and line depths, equivalent widths, S/N prefactors and TSM metrics for various spectral lines. See the file header for explanation of each column. The file can easily be read in Python using pandas.read_csv("sunset_overview.csv", comments="#")</p> </div> </div>
EVEX rocket experiment: sounding rocket and C/NOFS satellite observations in equatorial regions of the ionosphere at sunset
<p>These data files support the JGR: Space Physics article by Pfaff, R. et al. (2022) entitled "Dual sounding rocket and C/NOFS satellite observations of DC electric fields and plasma density in the equatorial E and F region ionosphere at sunset".</p>
Arecibo measurements of D-region electron densities during sunset and sunrise in August 2016
<p>This dataset is connected to the manuscript 'Arecibo measurements of D-region electron densities during sunset and sunrise: implications for atmospheric composition' submitted to Annales Geophysicae.</p> <p>It contains Arecibo radar data between 28. August 2016 and 01.September 2016, specifically power profiles and plasma line measurements. The data files and associated Matlab reading routines can be found in the appropriate .zip files.</p> <p>The data repository contains also processed data for Fig.3 (afternoon/morning_final_data75.mat/plot_sunset_sunrise_comparison75.m) and Fig. 4(rate_data.mat/plotrate.m) and associated Matlab plotting routines.</p>
Investigation of the Post-Sunset Extra electron density Peak Poleward of the Equatorial Ionization Anomaly Southern Crest
<p>These files are waccmx data to draw the plot in the paper.</p> <p>dwind stands for neutral wind transport</p> <p>dfield stands for E cross B transport</p> <p>ambi stands for transport due to ambipolar diffusion</p> <p>OP40W stands for O+ at 40W</p> <p>VN40W stands for meridional wind at 40W</p> <p>WI40W stands for vertical component of E cross B at 40W</p> <p> </p> <p>OPCHEMP and OPCHEML stand for the production and loss of the O+</p> <p>All these fils are at 40W, and their dimensions are 192*60*288 , 192 stands for number of latitude, 60 stands for number of altitudes and 288 stands for number of times</p> <p> </p> <p>HMF2 and NMF2 stand for the hmf2 and nmf2 global</p>
NERC MSTRF Sky-Camera Time-Lapse Video for 2010-09-07 16:50 UTC (showing Cumulonimbus cloud development at sunset).
<p>A time-lapse video showing Cumulonimbus cloud development at sunset. Most of the first Cumulonimbus cloud is obscured by the smaller Cumulus clouds in the foreground. Its anvil is clearly visible. Three further Cumulonimbus clouds cast crepuscular rays from the light of the setting sun. Their anvils merge together. This video has been created from images taken by the NERC MST Radar Facility's Sky-Camera, which is located near Aberystwyth in West Wales. The images are freely available, under an Open (UK) Government License, from http://tinyurl.com/nerc-mstrf-sky-camera/ . For an explanation of the atmospheric phenomena that can be seen, download the resource available at http://cedadocs.ceda.ac.uk/1259/ .</p>
Sunset at Agri
Textured version of Agri SRTM data. Landsat RGB image was used for texturing. Source: Objaverse 1.0 / Sketchfab
Calculation of times relative to sunset and sunrise for mountain hare Lepus timidus camera trap records Scotland (S1b)
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Data from: A comparison of the life history and distribution of vermilion rockfish (<em>Sebastes miniatus</em>) and its cryptic pair, sunset rockfish (<em>S. crocotulus</em>) along the Pacific Coast
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FIGURE 5. A. Pterostylis jeanesii habitat. B. Inflorescence, side view. C in Two new species of Pterostylis (Orchidaceae; Orchidoideae) from the Sunset Country, Victoria, Australia
FIGURE 5. A. Pterostylis jeanesii habitat. B. Inflorescence, side view. C. Inflorescence, front view. Photographer: June Niejalke.
FIGURE 2 in Two new species of Pterostylis (Orchidaceae; Orchidoideae) from the Sunset Country, Victoria, Australia
FIGURE 2. Dendrogram of group 1 (P. biseta)= purple circle, group 2 (P. jeanesii)= brown square and group 3 (P. peakallana)= green triangle. Dendrogram based on cluster analysis of morphometric measurements of the top 5 Kruskal Wallis characters with a value greater than 18. Distance matrices were calculated using the Gower metric (GM) and cluster analysis was performed using unweighted pair-group method using arithmetic averages (UPGMA) to produce dendrograms.
FIGURE 3 in Two new species of Pterostylis (Orchidaceae; Orchidoideae) from the Sunset Country, Victoria, Australia
FIGURE 3. Comparison between labellums side on of group 2 (P. jeanesii) (A), group 1 (P. biseta) (B) and group 3 (P. peakallana) (C). Scale = 1.1mm.
FIGURE 1 in Two new species of Pterostylis (Orchidaceae; Orchidoideae) from the Sunset Country, Victoria, Australia
FIGURE 1. Distribution of study sites surveyed: black circles= group 1 (P. biseta); black squares = group 2 (P. jeanesii); white squares = P. jeanesii sites from which there are collected specimens but no plants were found in recent surveys; black triangles = (group 3) P. peakallana.
FIGURE 4 in Two new species of Pterostylis (Orchidaceae; Orchidoideae) from the Sunset Country, Victoria, Australia
FIGURE 4. Comparison of labella from above of group 2 (P. jeanesii) (A), group 1 (P. biseta) (B) and group 3 (P. peakallana) (C). Scale = 1 mm.
SUNSET: SBRT for Ultra-central NSCLC- a Safety and Efficacy Trial
ClinicalTrials.gov study NCT03306680. IPD Sharing: NO. Countries: 1. Publications: 1.
Processed carbon mass loading data from DRI and Sunset analyzers
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Latitude variation of the post-sunset plasma density enhancement during the minor geomagnetic storm on 27 May 2021
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Latitude characteristic of the post-sunset plasma density enhancement during the geomagnetic quiet period in May 2021
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SUNSET METACLIP example
<p>Example <a href="http://metaclip.org/">METACLIP</a> provenance graph serialized in JSON. This example was created using <a href="https://doi.org/10.5194/ems2024-361">SUNSET</a> (SUbseasoNal to decadal climate forecast post-processing and asSEssmenT suite), a modular tool for subseasonal to seasonal to decadal forecast verification workflows.</p> <p>This JSON file can be used to plot the provenance graph using <a href="https://metaclip.org/">METACLIP's Web Interpreter</a> online or running it locally with Java or Docker.</p>
Leaf gene expression profile of rice during sunset
GEO Series GSE36044. Oryza sativa; Oryza sativa Japonica Group. 19 samples. Type: Expression profiling by array.
ROSE in Sunset Park
ClinicalTrials.gov study NCT04940585. IPD Sharing: YES. Countries: 1. Publications: 0.
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