TY - JOUR
T1 - Planetary waves observed by TIMED/SABER in coupling the stratosphere-mesosphere-lower thermosphere during the winter of 2003/2004: Part 2-Altitude and latitude planetary wave structure
AU - Pancheva, D
AU - Mukhtarov, R
AU - Andonov, B
AU - Mitchell, Nicholas J
AU - Forbes, J M
PY - 2009
Y1 - 2009
N2 - Part 2 of the present paper is focused on the planetary wave coupling from the stratosphere to the lower thermosphere (30-120 km) during the Arctic winter of 2003/2004. The planetary waves seen in the TIMED/SABER temperature data in the latitudinal range 50°N–50°S are studied in detail. The altitude and latitude structures of the planetary wave (stationary and travelling) clearly indicate that the stratosphere and mesosphere (30-90 km) are coupled by direct vertical propagation of the planetary waves, while the lower thermosphere (above 90-95km altitude) is only partly connected with the lower levels probably indirectly through in-situ generation of disturbances by the dissipation and breaking of gravity waves filtered by lower atmospheric planetary waves. A peculiar feature of the thermal regime in the lower thermosphere is that it is dominated by zonally symmetric planetary waves.
AB - Part 2 of the present paper is focused on the planetary wave coupling from the stratosphere to the lower thermosphere (30-120 km) during the Arctic winter of 2003/2004. The planetary waves seen in the TIMED/SABER temperature data in the latitudinal range 50°N–50°S are studied in detail. The altitude and latitude structures of the planetary wave (stationary and travelling) clearly indicate that the stratosphere and mesosphere (30-90 km) are coupled by direct vertical propagation of the planetary waves, while the lower thermosphere (above 90-95km altitude) is only partly connected with the lower levels probably indirectly through in-situ generation of disturbances by the dissipation and breaking of gravity waves filtered by lower atmospheric planetary waves. A peculiar feature of the thermal regime in the lower thermosphere is that it is dominated by zonally symmetric planetary waves.
UR - http://www.scopus.com/inward/record.url?scp=58149234101&partnerID=8YFLogxK
UR - http://dx.doi.org/10.1016/j.jastp.2008.09.027
U2 - 10.1016/j.jastp.2008.09.027
DO - 10.1016/j.jastp.2008.09.027
M3 - Article
SN - 1364-6826
VL - 71
SP - 75
EP - 87
JO - Journal of Atmospheric and Solar-Terrestrial Physics
JF - Journal of Atmospheric and Solar-Terrestrial Physics
IS - 1
ER -