Kelvin Waves as Observed by the SABER Instrument on the TIMED Spacecraft Jeffrey M. Forbes, Xiaoli Zhang, Saburo Miyahara, Scott E. Palo, James Russell, Christopher J. Mertens and Martin Mlynczak This Paper: Main Focus on Equatorial Temperatures, km Wavenumber vs. Period Spectra as a Function of Height Ultra-Fast Kelvin Waves (UFKW), Periods days Intraseasonal Oscillation (ISO) of UFKW and Zonal Mean Temperatures

Data processing Sliding 60-day window, 1 day at a time, covering all local times and longitudes Extract zonal mean, diurnal & semidiurnal solar & lunar tides, & stationary planetary waves Analyze residuals from above fit Raw Temperature Residuals at Equator ascending descending 30 km October-November, km: ~10-day eastward-propagating structures (Kelvin waves) clearly visible ascending descending 90 km October-November, km: Larger amplitudes, but no clear patterns. Kelvin waves probably masked by day-to- day variability of tides, gravity waves, etc.

Data processing: sliding fits performed zonal wavenumbers s = -6 (eastward) to s = +6 (westward) periods 2 to 20 days in increments of 0.5 days window length = 3 x wave period all data during “Background spectrum” due to various sources of variability, e.g., tides, gravity waves day Ultra-fast Kelvin Wave 6-7 day oscillation~16-day normal mode ISO, possibly driven by UFKW & diurnal tide EPFD (e.g.,Miyoshi & Fujiwara, GRL, 2006) Multi-Year Mean Spectrum

z = vertical wavelength x = zonal wavelength T = wave period N = buoyancy frequency u bar = zonal mean u (= 0) e.g. Holton et al. (2001) Dominant Kelvin waves (s = -1, s = -2) transition from long-periods (5-10 days) and short-wavelengths (9-13 km) in the stratosphere, to shorter periods (2-3 days) and longer wavelengths (35-45 km) in the MLT Zonal phase speed ms

Slow Kelvin waves Ultra fast Kelvin waves In Addition to Kelvin Waves, Other Parts of the Spectrum also Vary with Height, e.g., s = 0

Results similar to the previous were obtained by examining the symmetric component of the temperature residuals No notable results were obtained when the anti-symmetric component of the temperature residuals was examined. We now concentrate on MLT Kelvin waves, periods days, i.e., UFKW Characterizing IS variability of MLT UFKW, and possible connections with IS variability of the zonal mean state

In the context of a full-atmosphere GCM, Miyoshi and Fujiwara (2006) established connections between EPFD due to DT and UFKW, and day ISO in zonal mean winds. Variations in DT and UFKW are connected with established troposphere ISO’s at days (Hartmann et al., 1992) and days (Madden and Julian, 1994) manifested in tropical convection, e.g., latent heating rates. Existence of UFKW are well-established in the tropical MLT: Lieberman and Riggin (1997), Riggin et al. (1997), Yoshida et al. (1999) Previous similar suggestions and supportive observations relating waves and ISO in the MLT provided by Eckerman et al. (1997), Isoda et al. (2004), Lieberman et al. (1998). Ultra-Fast Kelvin Waves (UFKW), Diurnal Tides (DT) and Intraseasonal Oscillations (ISO) in the MLT The SABER data provide the first look at the above that extends continuously from km, -50 o to +50 o latitude, 2002 to 2006

ISO of day Wave Amplitudes, 90 km, Eastward s = -1

3.3 km day-1 Filtered zonal mean days ~± 2-4K UFKW and Zonal Mean Variability at the Equator, 2003

UFKW Zonal Mean Spectra show some similarities, but not close correspondence. However, the “UFKW” omits the effects of longer-period and s  -1 KW & DT

SABER temperature data provide the first opportunity to “see” vertical coupling from the lower stratosphere to lower thermosphere in the equatorial region vis-à-vis vertically-propagating waves with periods > 2 days. The dominant waves responsible for this coupling are symmetric eastward- propagating waves, i.e., Kelvin waves. Dominant Kelvin waves transition from long-periods (5-10 days) and short- wavelengths (9-13 km) in the stratosphere, to shorter periods (2-3 days) and longer wavelengths (35-45 km) in the MLT. UFKW (periods days) intermittently exist at similar amplitudes (3-10 K, km) during all months of the year, with variability in the day range. An ISO of zonal mean temperatures also exists with periods days that may be driven by EPFD due, at least in part, to UFKW. The zonal mean ISO preferentially exists above 70 km, consistent with in- situ generation at these altitudes. Possible F-region effects of UFKW vis-à-vis dynamo, similar to DE3? (see Takahashi et al. Paper ) SUMMARY & CONCLUSIONS