edu.ucar.opensky::articles:23339 UCAR/NCAR - Library OpenSky Support PO Box 3000 Boulder CO 80307-3000 opensky@ucar.edu http://opensky.ucar.edu/ homepage pointOfContact 2025-12-25T15:10:45.730015 ISO 19115-2 Geographic Information - Metadata - Part 2: Extensions for Imagery and Gridded Data ISO 19115-2:2009(E) https://n2t.org/ark:/85065/d7js9sv5 https://doi.org/10.5065/D6RX99HX https Related Service #1 Cheyenne: SGI ICE XA Cluster Dynamics and electrodynamics of an ultra-fast kelvin wave (UFKW) packet in the ionosphere-thermosphere (IT) 2020-05-01T00:00:00Z publication https://n2t.org/ark:/85065/d7js9sv5 https://doi.org/10.1029/2020JA027856 Forbes, J. M. author Maute, Astrid author ZHANG, X. author UCAR/NCAR - Library publisher Numerical experiments are performed using a suite of general circulation models that enable the interaction between a Kelvin wave packet and the ionosphere-thermosphere (IT) to be elucidated. Focus is on an eastward-propagating ultra-fast Kelvin wave (UFKW) packet with periods between 2 and 4 days and zonal wavenumber s =−1 during day of year (DOY) 266–281, 2009. Dissipative processes modify the classic UFKW dynamics (equatorially trapped, small meridional wind component) in three ways: (1) molecular diffusion acts to spread the UFKW zonal (u ) and meridional (v ) wind fields meridionally, pole to pole, as u and v , respectively, decay and grow with increasing height; (2) due to molecular diffusion, the UFKW spectrum at longer periods and with shorter vertical wavelengths preferentially dissipates with height; and (3) interaction with the diurnally varying IT introduces a westward-propagating s =+2 component to the wind field that significantly modifies its longitude-UT structure to include a diurnal modulation. The F-region ionosphere also responds with s =+2, which originates from the influence of diurnally varying E-region conductivity on E ×B drifts. Additional spectral peaks in v and ionospheric parameters arise due to longitude variations in the magnetic field. Maximum excursions in NmF2 (as compared with those from a simulation without UFKW forcing) achieve values as large as ±50% but more commonly occur in the range of ±20-30%. The combination of positive and negative responses, and their relative magnitudes, depends on the phasing of the UFKW as it moves zonally relative to the Sun-synchronous diurnal variation of the ionosphere, in addition to its changing amplitude between DOY 266 and 282. Modifications of order 10 ms−1 and −7% to zonal-mean zonal winds and NmF2, respectively, also result from dissipation of the UFKW packet. UCAR/NCAR - Library OpenSky Support PO Box 3000 Boulder CO 80307-3000 opensky@ucar.edu http://opensky.ucar.edu/ homepage pointOfContact PDF Text theme Resource Type 2016-01-01T00:00:00Z publication Copyright 2020 American Geophysical Union. None eng geoscientificInformation