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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004124naa a2200649 4500
001oai:DiVA.org:su-108984
003SwePub
008141110s2014 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1089842 URI
024a https://doi.org/10.1016/j.jastp.2014.07.0022 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Reisin, E. R.4 aut
2451 0a Traveling planetary wave activity from mesopause region airglow temperatures determined by the Network for the Detection of Mesospheric Change (NDMC)
264 1b Elsevier BV,c 2014
338 a print2 rdacarrier
500 a AuthorCount:27;
520 a The global distribution of traveling planetary wave (PW) activity in the mesopause region is estimated for the first time from ground-based airglow measurements. Monthly and total mean climatologies of PW power are determined from rotational temperatures measured at 19 sites from 78 degrees N to 76 degrees S which contribute to the Network for the Detection of Mesospheric Change (NDMC). Wave power is expressed as the standard deviation of nocturnal mean temperature around the seasonal temperature variation. The results from 20 degrees N confirm the SABER traveling PW proxy by Offermann et al. (2009, J. Geophys. Res. 114, D06110) at two altitudes. Most sites between 69 degrees S and 69 degrees N show total mean traveling PW activity of about 6 K, and only some high latitude sites have considerably higher activity levels. At the two tropical sites, there is practically no seasonal variation of PW activity. At 70% of the midlatitude sites, the seasonal variation is moderate for most of the year, but it is quite appreciable at all high latitude sites. Results about traveling PW activity at 87 km and 95 km available from several sites signal similar behavior at both altitudes. The total mean climatological results here obtained have further been used to separate the traveling PW contribution from the superposition of wave types contained in OH rotational temperature fluctuations measured by the SCIAMACHY instrument on Envisat. A narrow equatorial wave activity maximum is probably caused by gravity waves, while a tendency towards greater activity at higher northern latitudes may be due to stationary planetary waves.
650 7a NATURVETENSKAPx Geovetenskap och miljövetenskap0 (SwePub)1052 hsv//swe
650 7a NATURAL SCIENCESx Earth and Related Environmental Sciences0 (SwePub)1052 hsv//eng
653 a Traveling planetary wave activity
653 a Ground-based airglow observations
653 a Rotational temperature
653 a Network for the Detection of Mesospheric Change (NDMC)
700a Scheer, J.4 aut
700a Dyrland, M. E.4 aut
700a Sigernes, F.4 aut
700a Deehr, C. S.4 aut
700a Schmidt, C.4 aut
700a Hoeppner, K.4 aut
700a Bittner, M.4 aut
700a Ammosov, P. P.4 aut
700a Gavrilyeva, G. A.4 aut
700a Stegman, Jaceku Stockholms universitet,Meteorologiska institutionen (MISU)4 aut0 (Swepub:su)stegm
700a Perminov, V. I.4 aut
700a Semenov, A. I.4 aut
700a Knieling, P.4 aut
700a Koppmann, R.4 aut
700a Shiokawa, K.4 aut
700a Lowe, R. P.4 aut
700a Lopez-Gonzalez, M. J.4 aut
700a Rodriguez, E.4 aut
700a Zhao, Y.4 aut
700a Taylor, M. J.4 aut
700a Buriti, R. A.4 aut
700a Espy, P. J.4 aut
700a French, W. J. R.4 aut
700a Eichmann, K. -U4 aut
700a Burrows, J. P.4 aut
700a von Savigny, C.4 aut
710a Stockholms universitetb Meteorologiska institutionen (MISU)4 org
773t Journal of Atmospheric and Solar-Terrestrial Physicsd : Elsevier BVg 119, s. 71-82q 119<71-82x 1364-6826x 1879-1824
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-108984
8564 8u https://doi.org/10.1016/j.jastp.2014.07.002

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