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5 results for “broadband emissivity”

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zenodo36/100

Products and Models for "A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b"

<p>Close-in giant exoplanets with temperatures greater than 2,000 K (&ldquo;ultra-hot Jupiters&rdquo;) have been the subject of extensive efforts to determine their atmospheric properties using thermal emission measurements from the Hubble and Spitzer Space Telescopes1&ndash;3. However, previous studies have yielded inconsistent results because the small sizes of the spectral features and the limited information content of the data resulted in high sensitivity to the varying assumptions made in the treatment of instrument systematics and the atmospheric retrieval analysis3&ndash;12. Here we present a dayside thermal emission spectrum of the ultra-hot Jupiter WASP-18b obtained with the NIRISS13 instrument on JWST. The data span 0.85 to 2.85 &mu;m in wavelength at an average resolving power of 400 and exhibit minimal systematics. The spectrum shows three water emission features (at &lt;6&sigma; confidence) and evidence for optical opacity, possibly due to H-, TiO, and VO (combined significance of 3.8&sigma;). Models that fit the data require a thermal inversion, molecular dissociation as predicted by chemical equilibrium, a solar heavy-element abundance (&ldquo;metallicity&rdquo;, M/H = 1.03-0.51+1.11 x solar), and a carbon-to-oxygen (C/O) ratio less than unity. The data also yield a dayside brightness temperature map, which shows a peak in temperature near the sub-stellar point that decreases steeply and symmetrically with longitude toward the terminators.</p>

opencc-by-4.0May 2023View details →
zenodo32/100

Annotated data of simultaneous broadband radio and optical emission of meteor trains imaged by LOFAR / AARTFAAC and CAMS

<p>This data set contains simultaneous 30 - 60 MHz LOFAR / AARTFAAC12 radio observations and CAMS low-light video observations of +4 to -10 magnitude meteors at the peak of the Perseid meteor shower on August 12/13, 2020. 204 meteor trains were imaged in both the radio and optical domain.</p>

opencc-by-4.0Nov 2021View details →
zenodo32/100

Global high-resolution sea surface hemispherical broadband emissivity dataset (1980-2020)

<p>This is the global sea surface hemispherical broadband emissivity (BBE, 8-13.5 micrometer) dataset (0.1&deg;) derived by a lookup table-based method developed by Cheng et al., (2017). The accuracy of the estimated hemispherical BBE was 0.003 given a wind speed of zero. The foam effect was also incorporated&nbsp;into the BBE dataset.</p> <p>This dataset spans from 1980 to 2020.</p> <p><strong>Dataset Characteristics:</strong></p> <ul> <li>Spatial Coverage: Global</li> <li>Temporal Coverage: 1980.01-2020.12</li> <li>Spectral Range: 8~13.5&mu;m</li> <li>Spatial Resolution: 0.1&deg;</li> <li>Temporal Resolution: Daily (instantaneous at 12:30)</li> <li>Projection: GCS_WGS_1984</li> <li>Data Format: HDF</li> </ul> <p><strong>Citation&nbsp;</strong>(Please cite these papers when using the data)<strong>:</strong></p> <ol> <li> <p>Cheng, J., et al. (2017). A Lookup Table-Based Method for Estimating Sea Surface Hemispherical Broadband Emissivity Values (8&ndash;13.5 &mu;m). <em>Remote Sensing, 9</em></p> </li> <li> <p>Cheng, J., et al. (2013). Estimating the Optimal Broadband Emissivity Spectral Range for Calculating Surface Longwave Net Radiation. IEEE Geoscience and Remote Sensing Letters, 10, 401-405</p> <p>If you have any questions, please contact Prof. Jie Cheng (Jie_Cheng@bnu.edu.cn).</p> </li> </ol>

opencc-by-4.0Feb 2023View details →
zenodo32/100

ELITE broadband emissivity: global sea 0.1° CMG daily BBE (2010)

<p>The <strong>E</strong>ssential therma<strong>L</strong> <strong>I</strong>nfrared remo<strong>T</strong>e s<strong>E</strong>nsing (<strong>ELITE</strong>) product suite currently has four types of products, including land surface temperature (LST: clear-sky and all-sky), emissivity (NBE: narrowband emissivity; BBE: broadband emissivity; and spectral emissivity), the component of surface radiation and energy budget (SLUR: surface longwave upwelling radiation; SLDR: surface longwave downward radiation SLDR; SLNR: surface longwave net radiation), and the component of Earth&rsquo;s radiation budget (OLR; outgoing longwave radiation; RSR: reflected solar radiation). The spatial-temporal resolutions of the ELITE products are mainly determined by the employed satellite data sources. For more information about ELITE products, please refer to the website (<a href="https://elite.bnu.edu.cn">https://elite.bnu.edu.cn</a>).</p> <p>This dataset is the ELITE global sea BBE product at 0.1&deg; spatial resolution and daily (at 13:00 UTC) temporal resolution. It is provided on a climate modeling grid (CMG) and ranges from 1981 to 2022 (continuously updated). This dataset was generated from the MERRA2 reanalysis wind speed data using the look-up-table method developed by Cheng et al. (2017).</p> <p>This dataset is the ELITE BBE product in 2010. Please <strong><em>click here</em></strong> to download the ELITE BBE product in 2009 and <strong><em>click here</em></strong> to download the ELITE BBE product in 2011.</p> <p><strong>Dataset Characteristics:</strong></p> <ul> <li>Spatial Coverage: Global</li> <li>Temporal Coverage: 2010</li> <li>Spatial Resolution: 0.1&deg;</li> <li>Temporal Resolution: daily</li> <li>Data Format: HDF</li> <li>Scale: 0.0001</li> </ul> <p><strong>Citation&nbsp;</strong>(Please cite these papers when using the data)<strong>:</strong></p> <ol> <li>Cheng, J., Cheng, X., Liang, S., Nicl&ograve;s, R., Nie, A., &amp; Liu, Q. (2017). A Lookup Table-Based Method for Estimating Sea Surface Hemispherical Broadband Emissivity Values (8&ndash;13.5 &mu;m). <em>Remote Sensing, 9</em>, 245</li> </ol> <p>If you have any questions, please contact Prof. Jie Cheng (eliteqrs@126.com).</p>

opencc-by-4.0Aug 2023View details →
nasa12/100

TIMED Sounding of the Atmosphere using Broadband Emission Radiometry (SABER)IR Radiances in 10 channels (1.27 to 17ym) from 0 to 150 km, Version 1.07, Level 1B (L1B), 42 s Data

Contains the SABER Level 1B calibrated radiance profiles converted to radiance units with instrument effects removed, geolocated and gridded to uniform angle spacing.

restrictednotspecifiedAug 2025View details →

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