Abstract. The present study describes Rossby wave packet (RWP) properties in the upper troposphere and
lower stratosphere (UTLS) with the use of Global Navigation Satellite System radio occultation
(GNSS-RO) measurements. This global study covering both hemispheres' extratropics is the first to
tackle medium- and synoptic-scale waves with GNSS-RO. We use 1 decade of GNSS-RO temperature and
pressure data from the CHAMP, COSMIC, GRACE, Metop-A, Metop-B, SAC-C and TerraSAR-X missions,
combining them into one gridded dataset for the years 2007–2016. Our approach to extract RWP
anomalies and their envelope uses Fourier and Hilbert transforms over longitude without pre- or
post-processing the data. Our study is purely based on observations, only using ERA-Interim winds
to provide information about the background wind regimes. The RWP structures that we obtain in the UTLS agree well with theory and earlier studies, in terms
of coherent phase or group propagation, zonal scale and distribution over latitudes. Furthermore, we
show that RWP pressure anomalies maximize around the tropopause, while RWP temperature anomalies
maximize right above the tropopause height with a contrasting minimum right below. RWP activity
follows the zonal-mean tropopause during all seasons. RWP anomalies in the lower stratosphere are dynamically coupled to the upper troposphere. They are
part of the same system with a quasi-barotropic structure across the UTLS. RWP activity often
reaches up to 20 km height and occasionally higher, defying the Charney–Drazin criterion. We note
enhanced amplitude and upward propagation of RWP activity during sudden stratospheric warmings. We provide observational support for improvements in RWP diagnostics and wave trend analysis in
models and reanalyses. Wave quantities follow the tropopause, and diagnosing them on fixed
pressure levels (which the tropopause does not follow) can lead to aliasing. Our novel approach
analyzing GNSS-RO pressure anomalies provides wave signals with better continuity and coherence
across the UTLS and the stratosphere, compared to temperature anomalies. Thus, RWP vertical
propagation is much easier to analyze with pressure data.