Interhemispheric comparison of mesospheric ice layers from the LIMA model
F. Lubken, и U. Berger. Journal of Atmospheric and Solar-Terrestrial Physics, 69 (17-18):
2292-2308(2007)Cited References:
BAILEY SM, 2005, J GEOPHYS RES, V110
BAILEY SM, 2007, J ATMOS SOL-TERR PHY, V69, P1407, DOI
10.1016/j.jastp.2007.02.008
BALSLEY BB, 1993, GEOPHYS RES LETT, V20, P1983
BECKER E, 2003, J ATMOS SCI, V60, P103
BECKER E, 2004, GEOPHYS RES LETT, V31
BERGER U, 2003, J GEOPHYS RES, V107
BERGER U, 2006, GEOPHYS RES LETT, V33
BERGER U, 2007, J GEOPHYS RES, V112
BERGER U, 2007, UNPUB J ATMOSPHERIC
BREMER J, 2006, J ATMOS SOL-TERR PHY, V68, P1940, DOI
10.1016/j.jastp.2006.02.012
CARBARY JF, 2001, GEOPHYS RES LETT, V28, P725
CHU X, 2004, GEOPHYS RES LETT, V31
CHU X, 2006, J GEOPHYS RESDOI 10.1029/2006JD007086
CZECHOWSKY P, 1979, GEOPHYS RES LETT, V6, P459
DELAND MT, 2006, J ATMOS SOL-TERR PHY, V68, P9, DOI
10.1016/j.jastp.2005.08.003
DONAHUE TM, 1972, J ATMOS SCI, V29, P1205
ECKLUND WL, 1981, J GEOPHYS RES, V86, P7775
FIEDLER J, 2003, J GEOPHYS RES, V108
FIEDLER J, 2005, ANN GEOPHYS-GERMANY, V23, P1175
GERDING M, 2007, J GEOPHYS RES, V112
GOLDBERG RA, 2004, GEOPHYS RES LETT, V31
HANSEN G, 1989, GEOPHYS RES LETT, V16, P1445
HERVIG M, 2006, J ATMOS SOL-TERR PHY, V68, P30, DOI
10.1016/j.jastp.2005.08.010
HOFFNER J, 2003, ATMOS CHEM PHYS, V3, P1101
HUNTEN DM, 1980, J ATMOS SCI, V37, P1342
KARLSSON B, 2007, GEOPHYS RES LETT, V34
KUTEPOV AA, 2006, GEOPHYS RES LETT
LATTECK R, 2007, GEOPHYS RES LETT, V34
LESLIE R, 1885, NATURE, V32, P245
LUBKEN FJ, 1996, J GEOPHYS RES-ATMOS, V101, P9489
LUBKEN FJ, 1997, J GEOPHYS RES-ATMOS, V102, P13441
LUBKEN FJ, 1999, J GEOPHYS RES-ATMOS, V104, P9135
LUBKEN FJ, 2004, J GEOPHYS RES, V109
LUBKEN FJ, 2004, J GEOPHYS RES, V109
LUBKEN FJ, 2007, ADV SPACE RES, V40, P794, DOI 10.1016/J.ASR.2007.01.014
MAUERSBERGER K, 2003, GEOPHYS RES LETT, V30
MORRIS RJ, 2004, GEOPHYS RES LETT, V31
MULLEMANN A, 2005, ADV SPACE RES, V35, P1890, DOI
10.1016/J.ASR.2004.11.014
MURPHY DM, 2005, Q J ROY METEOR SOC B, V131, P1539, DOI 10.1256/qj.04.94
OLIVERO JJ, 1986, J ATMOS SCI, V43, P1263
PETELINA SV, 2006, J ATMOS SOL-TERR PHY, V68, P42, DOI
10.1016/j.jastp.2005.08.004
RAPP M, 2003, J GEOPHYS RES-ATMOS, V108, ARTN 8441
RAPP M, 2004, ATMOS CHEM PHYS, V4, P2601
RAPP M, 2006, J ATMOS SOL-TERR PHY, V68, P715, DOI
10.1016/j.jastp.2005.10.015
SEELE C, 1999, GEOPHYS RES LETT, V26, P1517
SISKIND DE, 2003, J GEOPHYS RES, V108
SISKIND DE, 2005, J ATMOS SOL-TERR PHY, V67, P501, DOI
10.1016/j.jastp.2004.11.007
SONNEMANN GR, 2005, J ATMOS SOL-TERR PHY, V67, P177, DOI
10.1016/j.jastp.2004.07.026
STEVENS MH, 2005, GEOPHYS RES LETT, V32
THAYER JP, 1995, GEOPHYS RES LETT, V22, P2961
THOMAS GE, 1984, J ATMOS TERR PHYS, V46, P819
THOMAS GE, 1989, J GEOPHYS RES-ATMOSP, V94, P14673
THOMAS GE, 1991, REV GEOPHYS, V29, P553
VONSAVIGNY C, 2007, GEOPHYS RES LETT, V34
VONZAHN U, 2003, J GEOPHYS RES, V108
WOODMAN RF, 1999, J GEOPHYS RES-SPACE, V104, P22577
WROTNY JE, 2006, J ATMOS SOL-TERR PHY, V68, P1352, DOI
10.1016/j.jastp.2006.05.014
ZECHA M, 2003, J GEOPHYS RES, V108
Luebken, F. -J. Berger, U..
Аннотация
The new LIMA/ice model is used to study interhemispheric temperature differences at the summer upper mesosphere and their impact on the morphology of ice particle related phenomena such as noctilucent clouds (NLC), polar mesosphere clouds (PMC), and polar mesosphere summer echoes (PMSE). LIMA/ice nicely reproduces the mean characteristics of observed ice layers, for example their variation with season, altitude, and latitude. The southern hemisphere (SH) is slightly warmer compared to the NH but the difference is less than 3 K at NLC/PMC/PMSE altitudes and poleward of 70 degrees N/S. This is consistent with in situ temperature measurements by falling spheres performed at 69 degrees N and 68 degrees S. Earth's eccentricity leads to a SH mesosphere being warmer compared to the NH by similar to 2-3 K up to approximately 85 km and fairly independent of latitude. In general, NH/SH temperature differences in LIMA increase with decreasing latitude and reach similar to 10 K at 50 degrees. The latitudinal variation of NH/SH temperature differences is presumably caused by dynamical forcing and explains why PMSE are basically absent at midlatitudes in the SH whereas they are still rather common at similar colatitudes in the NH. The occurrence frequency and brightness of NLC and PMC are larger in the NH but the differences decrease with increasing latitude. Summer conditions in the SH terminate earlier compared to NH, leading to an earlier weakening and end of the ice layer season. The NLC altitude in the SH is slightly higher by 0.6-1 km, whereas the NLC altitudes itself depend on season in both hemispheres. Compared to other models LIMA/ice shows smaller interhemispheric temperature differences but still generates the observed NH/SH differences in ice layer characteristics. This emphasizes the importance of temperature controlling the existence and morphology of ice particles. Interhemispheric differences in NLC/PMC/PMSE characteristics deduced from LIMA/ice basically agree with observations from lidars, satellites, and radars. (c) 2007 Elsevier Ltd. All rights reserved.
%0 Journal Article
%1 LubkenIce
%A Lubken, F. J.
%A Berger, U.
%D 2007
%J Journal of Atmospheric and Solar-Terrestrial Physics
%K ECHOES EXPLORER HIGH-LATITUDES LEO LIDAR MESOPAUSE POLAR STRUCTURE SUMMER THERMAL WATER-VAPOR clouds differences ice interhemispheric layers mesosphere modeling noctilucent numerical polar summer
%N 17-18
%P 2292-2308
%T Interhemispheric comparison of mesospheric ice layers from the LIMA model
%V 69
%X The new LIMA/ice model is used to study interhemispheric temperature differences at the summer upper mesosphere and their impact on the morphology of ice particle related phenomena such as noctilucent clouds (NLC), polar mesosphere clouds (PMC), and polar mesosphere summer echoes (PMSE). LIMA/ice nicely reproduces the mean characteristics of observed ice layers, for example their variation with season, altitude, and latitude. The southern hemisphere (SH) is slightly warmer compared to the NH but the difference is less than 3 K at NLC/PMC/PMSE altitudes and poleward of 70 degrees N/S. This is consistent with in situ temperature measurements by falling spheres performed at 69 degrees N and 68 degrees S. Earth's eccentricity leads to a SH mesosphere being warmer compared to the NH by similar to 2-3 K up to approximately 85 km and fairly independent of latitude. In general, NH/SH temperature differences in LIMA increase with decreasing latitude and reach similar to 10 K at 50 degrees. The latitudinal variation of NH/SH temperature differences is presumably caused by dynamical forcing and explains why PMSE are basically absent at midlatitudes in the SH whereas they are still rather common at similar colatitudes in the NH. The occurrence frequency and brightness of NLC and PMC are larger in the NH but the differences decrease with increasing latitude. Summer conditions in the SH terminate earlier compared to NH, leading to an earlier weakening and end of the ice layer season. The NLC altitude in the SH is slightly higher by 0.6-1 km, whereas the NLC altitudes itself depend on season in both hemispheres. Compared to other models LIMA/ice shows smaller interhemispheric temperature differences but still generates the observed NH/SH differences in ice layer characteristics. This emphasizes the importance of temperature controlling the existence and morphology of ice particles. Interhemispheric differences in NLC/PMC/PMSE characteristics deduced from LIMA/ice basically agree with observations from lidars, satellites, and radars. (c) 2007 Elsevier Ltd. All rights reserved.
@article{LubkenIce,
abstract = {The new LIMA/ice model is used to study interhemispheric temperature differences at the summer upper mesosphere and their impact on the morphology of ice particle related phenomena such as noctilucent clouds (NLC), polar mesosphere clouds (PMC), and polar mesosphere summer echoes (PMSE). LIMA/ice nicely reproduces the mean characteristics of observed ice layers, for example their variation with season, altitude, and latitude. The southern hemisphere (SH) is slightly warmer compared to the NH but the difference is less than 3 K at NLC/PMC/PMSE altitudes and poleward of 70 degrees N/S. This is consistent with in situ temperature measurements by falling spheres performed at 69 degrees N and 68 degrees S. Earth's eccentricity leads to a SH mesosphere being warmer compared to the NH by similar to 2-3 K up to approximately 85 km and fairly independent of latitude. In general, NH/SH temperature differences in LIMA increase with decreasing latitude and reach similar to 10 K at 50 degrees. The latitudinal variation of NH/SH temperature differences is presumably caused by dynamical forcing and explains why PMSE are basically absent at midlatitudes in the SH whereas they are still rather common at similar colatitudes in the NH. The occurrence frequency and brightness of NLC and PMC are larger in the NH but the differences decrease with increasing latitude. Summer conditions in the SH terminate earlier compared to NH, leading to an earlier weakening and end of the ice layer season. The NLC altitude in the SH is slightly higher by 0.6-1 km, whereas the NLC altitudes itself depend on season in both hemispheres. Compared to other models LIMA/ice shows smaller interhemispheric temperature differences but still generates the observed NH/SH differences in ice layer characteristics. This emphasizes the importance of temperature controlling the existence and morphology of ice particles. Interhemispheric differences in NLC/PMC/PMSE characteristics deduced from LIMA/ice basically agree with observations from lidars, satellites, and radars. (c) 2007 Elsevier Ltd. All rights reserved.},
added-at = {2009-03-30T22:21:12.000+0200},
author = {Lubken, F. J. and Berger, U.},
biburl = {https://www.bibsonomy.org/bibtex/2818ba95f1e1f45f69f1aca0f706b6445/bobsica},
description = {Leo's paper references II},
interhash = {2c240630bc8a92ae520e7d77c67d13d5},
intrahash = {818ba95f1e1f45f69f1aca0f706b6445},
journal = {Journal of Atmospheric and Solar-Terrestrial Physics},
keywords = {ECHOES EXPLORER HIGH-LATITUDES LEO LIDAR MESOPAUSE POLAR STRUCTURE SUMMER THERMAL WATER-VAPOR clouds differences ice interhemispheric layers mesosphere modeling noctilucent numerical polar summer},
note = {Cited References:
BAILEY SM, 2005, J GEOPHYS RES, V110
BAILEY SM, 2007, J ATMOS SOL-TERR PHY, V69, P1407, DOI
10.1016/j.jastp.2007.02.008
BALSLEY BB, 1993, GEOPHYS RES LETT, V20, P1983
BECKER E, 2003, J ATMOS SCI, V60, P103
BECKER E, 2004, GEOPHYS RES LETT, V31
BERGER U, 2003, J GEOPHYS RES, V107
BERGER U, 2006, GEOPHYS RES LETT, V33
BERGER U, 2007, J GEOPHYS RES, V112
BERGER U, 2007, UNPUB J ATMOSPHERIC
BREMER J, 2006, J ATMOS SOL-TERR PHY, V68, P1940, DOI
10.1016/j.jastp.2006.02.012
CARBARY JF, 2001, GEOPHYS RES LETT, V28, P725
CHU X, 2004, GEOPHYS RES LETT, V31
CHU X, 2006, J GEOPHYS RESDOI 10.1029/2006JD007086
CZECHOWSKY P, 1979, GEOPHYS RES LETT, V6, P459
DELAND MT, 2006, J ATMOS SOL-TERR PHY, V68, P9, DOI
10.1016/j.jastp.2005.08.003
DONAHUE TM, 1972, J ATMOS SCI, V29, P1205
ECKLUND WL, 1981, J GEOPHYS RES, V86, P7775
FIEDLER J, 2003, J GEOPHYS RES, V108
FIEDLER J, 2005, ANN GEOPHYS-GERMANY, V23, P1175
GERDING M, 2007, J GEOPHYS RES, V112
GOLDBERG RA, 2004, GEOPHYS RES LETT, V31
HANSEN G, 1989, GEOPHYS RES LETT, V16, P1445
HERVIG M, 2006, J ATMOS SOL-TERR PHY, V68, P30, DOI
10.1016/j.jastp.2005.08.010
HOFFNER J, 2003, ATMOS CHEM PHYS, V3, P1101
HUNTEN DM, 1980, J ATMOS SCI, V37, P1342
KARLSSON B, 2007, GEOPHYS RES LETT, V34
KUTEPOV AA, 2006, GEOPHYS RES LETT
LATTECK R, 2007, GEOPHYS RES LETT, V34
LESLIE R, 1885, NATURE, V32, P245
LUBKEN FJ, 1996, J GEOPHYS RES-ATMOS, V101, P9489
LUBKEN FJ, 1997, J GEOPHYS RES-ATMOS, V102, P13441
LUBKEN FJ, 1999, J GEOPHYS RES-ATMOS, V104, P9135
LUBKEN FJ, 2004, J GEOPHYS RES, V109
LUBKEN FJ, 2004, J GEOPHYS RES, V109
LUBKEN FJ, 2007, ADV SPACE RES, V40, P794, DOI 10.1016/J.ASR.2007.01.014
MAUERSBERGER K, 2003, GEOPHYS RES LETT, V30
MORRIS RJ, 2004, GEOPHYS RES LETT, V31
MULLEMANN A, 2005, ADV SPACE RES, V35, P1890, DOI
10.1016/J.ASR.2004.11.014
MURPHY DM, 2005, Q J ROY METEOR SOC B, V131, P1539, DOI 10.1256/qj.04.94
OLIVERO JJ, 1986, J ATMOS SCI, V43, P1263
PETELINA SV, 2006, J ATMOS SOL-TERR PHY, V68, P42, DOI
10.1016/j.jastp.2005.08.004
RAPP M, 2003, J GEOPHYS RES-ATMOS, V108, ARTN 8441
RAPP M, 2004, ATMOS CHEM PHYS, V4, P2601
RAPP M, 2006, J ATMOS SOL-TERR PHY, V68, P715, DOI
10.1016/j.jastp.2005.10.015
SEELE C, 1999, GEOPHYS RES LETT, V26, P1517
SISKIND DE, 2003, J GEOPHYS RES, V108
SISKIND DE, 2005, J ATMOS SOL-TERR PHY, V67, P501, DOI
10.1016/j.jastp.2004.11.007
SONNEMANN GR, 2005, J ATMOS SOL-TERR PHY, V67, P177, DOI
10.1016/j.jastp.2004.07.026
STEVENS MH, 2005, GEOPHYS RES LETT, V32
THAYER JP, 1995, GEOPHYS RES LETT, V22, P2961
THOMAS GE, 1984, J ATMOS TERR PHYS, V46, P819
THOMAS GE, 1989, J GEOPHYS RES-ATMOSP, V94, P14673
THOMAS GE, 1991, REV GEOPHYS, V29, P553
VONSAVIGNY C, 2007, GEOPHYS RES LETT, V34
VONZAHN U, 2003, J GEOPHYS RES, V108
WOODMAN RF, 1999, J GEOPHYS RES-SPACE, V104, P22577
WROTNY JE, 2006, J ATMOS SOL-TERR PHY, V68, P1352, DOI
10.1016/j.jastp.2006.05.014
ZECHA M, 2003, J GEOPHYS RES, V108
Luebken, F. -J. Berger, U.},
number = {17-18},
pages = {2292-2308},
timestamp = {2009-03-30T22:21:12.000+0200},
title = {Interhemispheric comparison of mesospheric ice layers from the LIMA model},
volume = 69,
year = 2007
}