Nonmigrating tides in the Martian atmosphere as observed by MAVEN IUVS

被引：51

作者：

Lo, Daniel Y. ^{[1
]}

Yelle, Roger V. ^{[1
]}

Schneider, Nicholas M. ^{[2
]}

Jain, Sonal K. ^{[2
]}

Stewart, A. Ian F. ^{[2
]}

England, Scott L. ^{[3
]}

Deighan, Justin I. ^{[2
]}

Stiepen, Arnaud ^{[2
]}

Evans, J. Scott ^{[4
]}

Stevens, Michael H. ^{[5
]}

Chaffin, Michael S. ^{[2
]}

Crismani, Matteo M. J. ^{[2
]}

McClintock, William E. ^{[2
]}

Clarke, John T. ^{[6
]}

Holsclaw, Gregory M. ^{[2
]}

Lefevre, Franck ^{[7
]}

Jakosky, Bruce M. ^{[2
]}

机构：

[1] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA

[2] Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80309 USA

[3] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[4] Computat Phys Inc, Springfield, VA USA

[5] Naval Res Lab, Washington, DC 20375 USA

[6] Boston Univ, Ctr Space Phys, Boston, MA 02215 USA

[7] CNRS, Lab ATmospheres Milieux Observat Spatiales, Paris, France

来源：

GEOPHYSICAL RESEARCH LETTERS | 2015年 / 42卷 / 21期

关键词：

ELECTRON-DENSITY PROFILES; THERMAL TIDES; NEUTRAL ATMOSPHERE; CO CAMERON; MARS; ACCELEROMETER; DAYGLOW; WAVES;

D O I：

10.1002/2015GL066268

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Using the Mars Atmospheric and Volatile EvolutioN mission (MAVEN) Imaging Ultraviolet Spectrograph (IUVS), we found periodic longitudinal variations in CO2 density in the Martian atmosphere. These density variations are derived from observations of the CO2+ (B-2 Sigma(+)-> X-2 Pi) emission from limb scans in the 100-190 km altitude range. The variations exhibit significant structure with longitudinal wave numbers 1, 2, and 3 in an effectively constant local solar time frame, and we attribute this structure to nonmigrating tides. The wave-2 component is dominated by the diurnal eastward moving DE1 tide at the equator and the semidiurnal stationary S0 tide at the midlatitudes. Wave-3 is dominated by the diurnal eastward moving DE2 tide, with possibly the semidiurnal eastward moving SE1 tide causing an amplitude increase at the midlatitudes. Structure in the wave-1 component can be explained by the semidiurnal westward moving SW1 tide.

引用

下载

页码：9057 / 9063

页数：7

共 50 条

[1] Atmospheric Tides at Low Latitudes in the Martian Upper Atmosphere Observed by MAVEN IUVS
Fu, Menghao
Ren, Zhipeng
Cui, Jun
Zhou, Xu
Wu, Zhaopeng
Fan, Kai
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2023, 128 (10)
[2] Martian mesospheric cloud observations by IUVS on MAVEN: Thermal tides coupled to the upper atmosphere
Stevens, M. H.
Siskind, D. E.
Evans, J. S.
Jain, S. K.
Schneider, N. M.
Deighan, J.
Stewart, A. I. F.
Crismani, M.
Stiepen, A.
Chaffin, M. S.
McClintock, W. E.
Holsclaw, G. M.
Lefevre, F.
Lo, D. Y.
Clarke, J. T.
Montmessin, F.
Jakosky, B. M.
GEOPHYSICAL RESEARCH LETTERS, 2017, 44 (10) : 4709 - 4715
[3] Variability of D and H in the Martian upper atmosphere observed with the MAVEN IUVS echelle channel
Clarke, J. T.
Mayyasi, M.
Bhattacharyya, D.
Schneider, N. M.
McClintock, W. E.
Deighan, J. I.
Stewart, A. I. F.
Chaufray, J. -Y.
Chaffin, M. S.
Jain, S. K.
Stiepen, A.
Crismani, M.
Holsclaw, G. M.
Montmessin, F.
Jakosky, B. M.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2017, 122 (02) : 2336 - 2344
[4] Probing the Martian atmosphere with MAVEN/IUVS stellar occultations
Groeller, H.
Yelle, R. V.
Koskinen, T. T.
Montmessin, F.
Lacombe, G.
Schneider, N. M.
Deighan, J.
Stewart, A. I. F.
Jain, S. K.
Chaffin, M. S.
Crismani, M. M. J.
Stiepen, A.
Lefevre, F.
McClintock, W. E.
Clarke, J. T.
Holsclaw, G. M.
Mahaffy, P. R.
Bougher, S. W.
Jakosky, B. M.
GEOPHYSICAL RESEARCH LETTERS, 2015, 42 (21) : 9064 - 9070
[5] Atmospheric Tides at High Latitudes in the Martian Upper Atmosphere Observed by MAVEN and MRO
England, Scott L.
Liu, Guiping
Kumar, Aishwarya
Mahaffy, Paul R.
Elrod, Meredith
Benna, Mehdi
Jain, Sonal
Deighan, Justin
Schneider, Nicholas M.
McClintock, William E.
Evans, J. Scott
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2019, 124 (04) : 2943 - 2953
[6] Martian Atmospheric Tides Revealed From MAVEN/IUVS and MRO/MCS Observations
Yang, Chengyun
Li, Tao
Yuan, Mengzhen
Wu, Zhaopeng
Fang, Xin
GEOPHYSICAL RESEARCH LETTERS, 2024, 51 (12)
[7] New observations of molecular nitrogen in the Martian upper atmosphere by IUVS on MAVEN
Stevens, M. H.
Evans, J. S.
Schneider, N. M.
Stewart, A. I. F.
Deighan, J.
Jain, S. K.
Crismani, M.
Stiepen, A.
Chaffin, M. S.
McClintock, W. E.
Holsclaw, G. M.
Lefevre, F.
Lo, D. Y.
Clarke, J. T.
Montmessin, F.
Bougher, S. W.
Jakosky, B. M.
GEOPHYSICAL RESEARCH LETTERS, 2015, 42 (21) : 9050 - 9056
[8] Imaging of Martian Circulation Patterns and Atmospheric Tides Through MAVEN/IUVS Nightglow Observations
Schneider, N. M.
Milby, Z.
Jain, S. K.
Gonzalez-Galindo, F.
Royer, E.
Gerard, J-C.
Stiepen, A.
Deighan, J.
Stewart, A. I. F.
Forget, F.
Lefevre, F.
Bougher, S. W.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2020, 125 (08)
[9] Isobar Altitude Variations in the Upper Mesosphere Observed With IUVS-MAVEN in Response to Martian Dust Storms
Gkouvelis, L.
Gerard, J-C.
Gonzalez-Galindo, F.
Hubert, B.
Schneider, N. M.
GEOPHYSICAL RESEARCH LETTERS, 2020, 47 (12)
[10] Modeling of nonmigrating tides in the middle atmosphere
Suvorova, E. V.
Pogoreltsev, A. I.
GEOMAGNETISM AND AERONOMY, 2011, 51 (01) : 105 - 115

← 1 2 3 4 5 →