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Gravity wave characteristics observed over a tropical station using high‐resolution GPS radiosonde soundings
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Several investigations of the dominant period gravity waves (GWs) were conducted earlier using Indian mesosphere‐stratosphere‐troposphere (MST) radar located at Gadanki (13.5°N, 79.2°E). However, these works had their own limitations of unavailability of continuous data, low SNR, and lack of reliable data at the stratospheric heights (in the case of MST radar) and low spatial resolution (for routine balloon data). For the present study, high‐resolution GPS radiosonde data for more than 2 years (2006–2008) has been used for the first time to characterize the dominant GWs and their associated source mechanisms. Particular attention is paid (1) to check the consistency in GW characteristics observed with MST radar, (2) to estimate potential energy, kinetic energy, and hence total energy, (3) to extend the analysis up to 25 km and check whether vertical wavelength is the same as that observed by MST radar in the lower stratosphere, and finally (4) to estimate the exact direction of propagation in horizontal, which was not possible from MST radar alone. Clear semiannual variation in GW energy, with maximum during monsoon and winter and minimum during premonsoon and postmonsoon in the troposphere, is noticed during 2006 but not clear in 2007. Annual variation is observed in the lower stratosphere with maximum during monsoon (winter enhancement is not significant) season. Strong eastward shear due to tropical easterly jet and orography is found to be responsible for generating the GWs during the monsoon and winter, respectively. Although several features are consistent with that observed earlier, a few new features have been observed by GPS radiosonde and are reported in the present study.
American Geophysical Union (AGU)
Title: Gravity wave characteristics observed over a tropical station using high‐resolution GPS radiosonde soundings
Description:
Several investigations of the dominant period gravity waves (GWs) were conducted earlier using Indian mesosphere‐stratosphere‐troposphere (MST) radar located at Gadanki (13.
5°N, 79.
2°E).
However, these works had their own limitations of unavailability of continuous data, low SNR, and lack of reliable data at the stratospheric heights (in the case of MST radar) and low spatial resolution (for routine balloon data).
For the present study, high‐resolution GPS radiosonde data for more than 2 years (2006–2008) has been used for the first time to characterize the dominant GWs and their associated source mechanisms.
Particular attention is paid (1) to check the consistency in GW characteristics observed with MST radar, (2) to estimate potential energy, kinetic energy, and hence total energy, (3) to extend the analysis up to 25 km and check whether vertical wavelength is the same as that observed by MST radar in the lower stratosphere, and finally (4) to estimate the exact direction of propagation in horizontal, which was not possible from MST radar alone.
Clear semiannual variation in GW energy, with maximum during monsoon and winter and minimum during premonsoon and postmonsoon in the troposphere, is noticed during 2006 but not clear in 2007.
Annual variation is observed in the lower stratosphere with maximum during monsoon (winter enhancement is not significant) season.
Strong eastward shear due to tropical easterly jet and orography is found to be responsible for generating the GWs during the monsoon and winter, respectively.
Although several features are consistent with that observed earlier, a few new features have been observed by GPS radiosonde and are reported in the present study.
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