Nonmigrating diurnal tides in the thermosphere

By Jeff Forbes, Xiaoli Zhang, E. Talaat, W. Ward. 2009

170 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/79b9960d7ea684bce95b571b52d1bf851024bdff

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Jeff Forbes
2. J. Oberheide
3. Xiaoli Zhang
4. Sean Bruinsma
5. M. E. Hagan
6. K. Häusler
7. Dong L. Wu
8. M. Mlynczak

In Atmospheric Science

1. Jeff Forbes
2. J. Oberheide
3. Dong L. Wu
4. M. Mlynczak
5. J. Russell
6. M. E. Hagan
7. K. Häusler
8. Xiaoli Zhang

Citations in the corpus

• TIMED Doppler Interferometer: Overview and recent results (2006, unknown): “…altitudes [Morton et al., 1993; Shepherd et al., 1993; Hays et al., 1994;Wu et al., 1995; Burrage et al., 1995a, 1995b McLandress et al., 1996; Wang et al., 1997; Khattatov et al., 1997a, 1997b; Yudin et al., 1998; Huang and Reber, 2003, 2004; Cierpik et al., 2003; Forbes et al., 2003, 2004].”
• Troposphere-Thermosphere Tidal Coupling as Measured by the SABER Instrument on TIMED during July-September, 2002 (2006, methodology): “DE3 was found to be the largest of all the nonmigrating diurnal tidal components in the tidal analysis of UARS winds at 95 km by Talaat and Lieberman [1999], Forbes et al. [2003a, 2003b] , Huang and Reber [2004], and Manson et al. [2004].”
• Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere (2015, background): “These variations are likely generated by a combination of planetary and tidal waves launched in the lower atmosphere that propagate to thermospheric heights [e.g., Forbes et al., 2003; Wilson, 2002; Moudden and Forbes, 2008, 2010].”
• Tropospheric tides from 80 to 400 km: Propagation, interannual variability, and solar cycle effects (2009, methodology): “The uncertainties of the SABER and TIDI tidal diagnostics are unaffected by these updates: DE3 temperature error is 2 K [Forbes et al., 2008] and the DE3 wind accuracy (precision) is about 10% (1 m/s) as detailed by Oberheide et al. [2006]. [12] Figure 1 shows monthly mean time series of DE3 (T, u, ”
• Wavenumber‐4 patterns of the total electron content over the low latitude ionosphere (2008, methodology): “With the HRDI and WINDII instruments on UARS, Forbes et al. [2003a, 2003b] found that the zonal wind of DE3 is stronger and occurs primarily during boreal summer and autumn, while the meridional component is relatively weaker and occurs during the boreal winter.”
• Tidal propagation of deep tropical cloud signatures into the thermosphere from TIMED observations (2008, background): “All DE3 observations in the MLT show a very different seasonal variation in v and (T, u) with the former maximizing in boreal winter and the latter maximizing in boreal summer [Forbes et al., 2003, 2006; Oberheide et al., 2006].”
• Solar tides as revealed by measurements of mesosphere temperature by the MLS experiment on UARS (2006, methodology): “Similar analyses have been performed on wind measurements from UARS (Forbes et al. 2003; Huang and Reber 2004; Manson et al. 2004); however, these studies are restricted to 95 km and between 42° latitude where both day and night data were available to perform unambiguous separation between tidal…”