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6 results for “Kelvin wave”
Maintenance of Convectively Coupled Kelvin waves: Relative Importance of Internal Thermodynamic Feedback and External Momentum Forcing (Code and Data)
<p>This is the dataset and code for generating all figures for the journal article named "Maintenance of Convectively Coupled Kelvin Waves: Relative Importance of Internal Thermodynamic Feedback and External Momentum Forcing," The article was written by Mu-Ting Chien and Daehyun Kim and submitted to Geophysical Research Letters in 2024.</p>
Response of convectively coupled Kelvin waves to surface temperature forcing in aquaplanet simulations: data and code
<p>This is the data and code used for a journal paper entitled "Response of convectively coupled Kelvin waves to surface temperature forcing in aquaplanet simulations", written by Mu-Ting Chien and Daehyun Kim in 2024. This paper is in minor revision in the Journal of Advances in Modeling Earth System. The submitted paper is here: (https://essopenarchive.org/doi/full/10.22541/essoar.171322728.86206700/v1).</p>
Thermosphere Hough Mode Extensions (HMEs) for Ultra-Fast Kelvin Waves (UFKWs)
<p>The scientific basis for the UFKW HME files contained here is described in Forbes et al. (2023). The directory "Hough-UV functions" contains solutions to Laplace's Tidal Equation for the s = -1 eastward-propagating first symmetric (Kelvin) modes with periods 2.0-5.0d (48hr-120hr), and a README file containing further information on the data files. The directory "UFKW output files" provides UFKW amplitudes and phases (UT hour of maximum at 0 longitude) of eastward, southward, and vertical winds (m/s), temperatures (K), density perturbations relative to mean, and geopotential height (m) as a function of height (z, every ~4 km) and latitude (deg, every 3 deg), corresponding to wave periods between 2.0d and 5.0d, and a README file containing further information on the data files. The data for each HME extend from pole to pole and from 0 to 400 km altitude.</p> <p>Forbes, J.M., Zhang, X., & Palo, S.E. (2023). UFKW propagation in the dissipative thermosphere. Journal of Geophysical Research: Space Physics, 128, e2022JA030921. https://doi.org/10.1029/2022JA030921</p>
Ground magnetic perturbations associated with "Ultra-Fast Kelvin Wave (UFKW) Variations in the Surface Magnetic Field"
<p>The data set is based on the thermosphere-ionosphere-electrodynamics general circulation model (TIEGCM) simulation results and a post-processing 3D ionospheric current and magnetic perturbation calculation, which is used in the publication "Ultra-Fast Kelvin Wave (UFKW) Variations in the Surface Magnetic Field" by Forbes et al. Focus is on an eastward-propagating ultra-fast Kelvin wave (UFKW) packet with periods between 2-4 days and zonal wavenumber s = -1 during DOY 266-281, 2009. Two sets of simulations are provided with different lower boundary (97km) conditions: 1. forced by daily and zonal mean (S0) 2. forced by S0 and 2-7days with s=-1 perturbations with the planetary wave amplitudes increased by a factor of 1.5. For these simulations the solar flux and geomagnetic forcing is held constant. Hourly output is provided of the neutral wind, neutral temperature, and ground magnetic perturbations.</p>
Supporting information for Spatial scales of the velocity shear layer and Kelvin-Helmholtz waves on the magnetopause: First statistical results
<p>Kelvin-Helmholtz (KH) waves observed by ARTEMIS P1 from 2015 to 2020. From the first column to the last column is: probe, date, time interval of KH waves, the location of KH waves in GSM coordinate, and the dominate period, phase speed, and wavelength of KH waves.</p>
The Roles of Shallow Convection and Cloud Radiative Feedback in Convectively-Coupled Kelvin Wave: MPAS-aquaplanet Model configuration
<p>We provide the model configuration for the MPAS-A aquaplanet used in our journal article titled <em>“The Roles of Shallow Convection and Cloud Radiative Feedback in Convectively-Coupled Kelvin Waves”</em> by Hsu et al., submitted to the <em>Journal of Climate</em> in 2024.</p>
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