Articles | Volume 36, issue 6
https://doi.org/10.5194/angeo-36-1597-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-36-1597-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Comparison of gravity wave propagation directions observed by mesospheric airglow imaging at three different latitudes using the M-transform
Septi Perwitasari
CORRESPONDING AUTHOR
National Institute of Polar Research, Tokyo, 190-8518, Japan
National Institute of Aeronautics and Space (LAPAN) of Indonesia,
Bandung, 40173, Indonesia
Takuji Nakamura
National Institute of Polar Research, Tokyo, 190-8518, Japan
Department of Polar Science, SOKENDAI (The Graduate University for
Advanced Studies), Tokyo, 190-8518, Japan
Masaru Kogure
Department of Polar Science, SOKENDAI (The Graduate University for
Advanced Studies), Tokyo, 190-8518, Japan
National Institute of Polar Research, Tokyo, 190-8518, Japan
Yoshihiro Tomikawa
National Institute of Polar Research, Tokyo, 190-8518, Japan
Department of Polar Science, SOKENDAI (The Graduate University for
Advanced Studies), Tokyo, 190-8518, Japan
Mitsumu K. Ejiri
National Institute of Polar Research, Tokyo, 190-8518, Japan
Department of Polar Science, SOKENDAI (The Graduate University for
Advanced Studies), Tokyo, 190-8518, Japan
Kazuo Shiokawa
Institute for Space-Earth Environmental Research, Nagoya University,
Nagoya, 464-8601, Japan
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Ann. Geophys., 39, 1013–1035, https://doi.org/10.5194/angeo-39-1013-2021, https://doi.org/10.5194/angeo-39-1013-2021, 2021
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We present a detailed account of the science programme PRESTO (PREdictability of the variable Solar–Terrestrial cOupling), covering the period 2020 to 2024. PRESTO was defined by a dedicated committee established by SCOSTEP (Scientific Committee on Solar-Terrestrial Physics). We review the current state of the art and discuss future studies required for the most effective development of solar–terrestrial physics.
Viswanathan Lakshmi Narayanan, Satonori Nozawa, Shin-Ichiro Oyama, Ingrid Mann, Kazuo Shiokawa, Yuichi Otsuka, Norihito Saito, Satoshi Wada, Takuya D. Kawahara, and Toru Takahashi
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In the past, additional sodium peaks occurring above the main sodium layer of the upper mesosphere were discussed. Here, formation of an additional sodium peak below the main sodium layer peak is discussed in detail. The event coincided with passage of multiple mesospheric bores, which are step-like disturbances occurring in the upper mesosphere. Hence, this work highlights the importance of such mesospheric bores in causing significant changes to the minor species concentration in a short time.
Hideaki Nakajima, Isao Murata, Yoshihiro Nagahama, Hideharu Akiyoshi, Kosuke Saeki, Takeshi Kinase, Masanori Takeda, Yoshihiro Tomikawa, Eric Dupuy, and Nicholas B. Jones
Atmos. Chem. Phys., 20, 1043–1074, https://doi.org/10.5194/acp-20-1043-2020, https://doi.org/10.5194/acp-20-1043-2020, 2020
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This paper presents temporal evolution of stratospheric chlorine and minor species related to Antarctic ozone depletion, based on FTIR measurements at Syowa Station, and satellite measurements by MLS and MIPAS in 2007 and 2011. After chlorine reservoir species were processed on PSCs and active ClO was formed, different chlorine deactivation pathways into reservoir species were identified, depending on the relative location of Syowa Station to the polar vortex boundary.
Takuo T. Tsuda, Yuta Hozumi, Kento Kawaura, Keisuke Hosokawa, Hidehiko Suzuki, and Takuji Nakamura
Atmos. Meas. Tech., 11, 6163–6168, https://doi.org/10.5194/amt-11-6163-2018, https://doi.org/10.5194/amt-11-6163-2018, 2018
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Polar mesospheric clouds (PMCs) or noctilucent clouds (NLCs) are the highest clouds in the Earth's atmosphere. In this paper, we introduce new PMC observations by the Japanese Geostationary Earth Orbit (GEO) meteorological satellite Himawari-8, which was launched in October 2014.
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Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2018-505, https://doi.org/10.5194/acp-2018-505, 2018
Revised manuscript not accepted
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This paper presents characteristics of temporal evolution of stratospheric chlorine and minor species related to Antarctic ozone depletion, based on both ground-based FTIR and satellite measurements by MLS and MIPAS in 2007 and 2011. After chlorine reservoir species (HCl or ClONO2) were processed on PSCs and active ClO was formed, different chlorine deactivation pathways into reservoir species were identified, depending on availability of ambient available O3 and NOx amounts.
Heqiucen Xu, Kazuo Shiokawa, and Dennis Frühauff
Ann. Geophys., 35, 1131–1142, https://doi.org/10.5194/angeo-35-1131-2017, https://doi.org/10.5194/angeo-35-1131-2017, 2017
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In this study, we statistically analyzed severe magnetic fluctuations in the nightside near-Earth plasma sheet. For the first time, we showed the occurrence rates of these fluctuations. The superposed epoch analysis also indicated that the flow speed increases before the severe magnetic fluctuations. We also discussed how both the inside-out and outside-in substorm models can be used to explain these observed results.
Ryosuke Shibuya, Kaoru Sato, Masaki Tsutsumi, Toru Sato, Yoshihiro Tomikawa, Koji Nishimura, and Masashi Kohma
Atmos. Chem. Phys., 17, 6455–6476, https://doi.org/10.5194/acp-17-6455-2017, https://doi.org/10.5194/acp-17-6455-2017, 2017
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The first observations made by a complete PANSY radar system (Program of the Antarctic Syowa MST/IS radar) installed at Syowa Station were successfully performed from 16 to 24 March 2015. Over this period, quasi-12 h period disturbances in the mesosphere at heights of 70 to 80 km were observed. Combining the observational data and numerical simulation outputs, we found that quasi-12 h disturbances are due to large-scale inertia–gravity waves, not to semi-diurnal migrating tides.
Y. Tomikawa
Ann. Geophys., 33, 1479–1484, https://doi.org/10.5194/angeo-33-1479-2015, https://doi.org/10.5194/angeo-33-1479-2015, 2015
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A possibility of gravity wave propagation from a source region to the airglow layer around the mesopause has been discussed based on the gravity wave blocking diagram taking into account the critical level filtering alone. This paper proposes a new gravity wave transmission diagram in which both the critical level filtering and turning level reflection of gravity waves are considered. It shows a significantly different distribution of gravity wave transmissivity from the blocking diagram.
J. A. Wanliss, K. Shiokawa, and K. Yumoto
Nonlin. Processes Geophys., 21, 347–356, https://doi.org/10.5194/npg-21-347-2014, https://doi.org/10.5194/npg-21-347-2014, 2014
H. Suzuki, T. Nakamura, M. K. Ejiri, T. Ogawa, M. Tsutsumi, M. Abo, T. D. Kawahara, Y. Tomikawa, A. S. Yukimatu, and N. Sato
Ann. Geophys., 31, 1793–1803, https://doi.org/10.5194/angeo-31-1793-2013, https://doi.org/10.5194/angeo-31-1793-2013, 2013
R. Kataoka, Y. Miyoshi, K. Shigematsu, D. Hampton, Y. Mori, T. Kubo, A. Yamashita, M. Tanaka, T. Takahei, T. Nakai, H. Miyahara, and K. Shiokawa
Ann. Geophys., 31, 1543–1548, https://doi.org/10.5194/angeo-31-1543-2013, https://doi.org/10.5194/angeo-31-1543-2013, 2013
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Ann. Geophys., 31, 163–172, https://doi.org/10.5194/angeo-31-163-2013, https://doi.org/10.5194/angeo-31-163-2013, 2013
Related subject area
Subject: Earth's ionosphere & aeronomy | Keywords: Waves and tides
High-time-resolution analysis of meridional tides in the upper mesosphere and lower thermosphere at mid-latitudes measured by the Falkland Islands SuperDARN radar
Identifying gravity waves launched by the Hunga Tonga–Hunga Ha′apai volcanic eruption in mesosphere/lower-thermosphere winds derived from CONDOR and the Nordic Meteor Radar Cluster
A case study of a ducted gravity wave event over northern Germany using simultaneous airglow imaging and wind-field observations
Seasonal evolution of winds, atmospheric tides, and Reynolds stress components in the Southern Hemisphere mesosphere–lower thermosphere in 2019
Migrating tide climatologies measured by a high-latitude array of SuperDARN HF radars
Diurnal mesospheric tidal winds observed simultaneously by meteor radars in Costa Rica (10° N, 86° W) and Brazil (7° S, 37° W)
Forcing mechanisms of the migrating quarterdiurnal tide
Investigation of sources of gravity waves observed in the Brazilian equatorial region on 8 April 2005
Characterization of gravity waves in the lower ionosphere using very low frequency observations at Comandante Ferraz Brazilian Antarctic Station
Impact of gravity wave drag on the thermospheric circulation: implementation of a nonlinear gravity wave parameterization in a whole-atmosphere model
Nonlinear forcing mechanisms of the migrating terdiurnal solar tide and their impact on the zonal mean circulation
Climatologies and long-term changes in mesospheric wind and wave measurements based on radar observations at high and mid latitudes
Seasonal variability of atmospheric tides in the mesosphere and lower thermosphere: meteor radar data and simulations
Gareth Chisham, Andrew J. Kavanagh, Neil Cobbett, Paul Breen, and Tim Barnes
Ann. Geophys., 42, 1–15, https://doi.org/10.5194/angeo-42-1-2024, https://doi.org/10.5194/angeo-42-1-2024, 2024
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Solar tides in the atmosphere are driven by solar heating on the dayside of the Earth. They result in large-scale periodic motion of the upper atmosphere. This motion can be measured by ground-based radars. This paper shows that making measurements at a higher time resolution than the standard operation provides a better description of higher-frequency tidal variations. This will improve the inputs to empirical atmospheric models and the benefits of data assimilation.
Gunter Stober, Alan Liu, Alexander Kozlovsky, Zishun Qiao, Witali Krochin, Guochun Shi, Johan Kero, Masaki Tsutsumi, Njål Gulbrandsen, Satonori Nozawa, Mark Lester, Kathrin Baumgarten, Evgenia Belova, and Nicholas Mitchell
Ann. Geophys., 41, 197–208, https://doi.org/10.5194/angeo-41-197-2023, https://doi.org/10.5194/angeo-41-197-2023, 2023
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The Hunga Tonga–Hunga Ha‘apai volcanic eruption was one of the most vigorous volcanic explosions in the last centuries. The eruption launched many atmospheric waves traveling around the Earth. In this study, we identify these volcanic waves at the edge of space in the mesosphere/lower-thermosphere, leveraging wind observations conducted with multi-static meteor radars in northern Europe and with the Chilean Observation Network De Meteor Radars (CONDOR).
Sumanta Sarkhel, Gunter Stober, Jorge L. Chau, Steven M. Smith, Christoph Jacobi, Subarna Mondal, Martin G. Mlynczak, and James M. Russell III
Ann. Geophys., 40, 179–190, https://doi.org/10.5194/angeo-40-179-2022, https://doi.org/10.5194/angeo-40-179-2022, 2022
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A rare gravity wave event was observed on the night of 25 April 2017 over northern Germany. An all-sky airglow imager recorded an upward-propagating wave at different altitudes in mesosphere with a prominent wave front above 91 km and faintly observed below. Based on wind and satellite-borne temperature profiles close to the event location, we have found the presence of a leaky thermal duct layer in 85–91 km. The appearance of this duct layer caused the wave amplitudes to diminish below 91 km.
Gunter Stober, Diego Janches, Vivien Matthias, Dave Fritts, John Marino, Tracy Moffat-Griffin, Kathrin Baumgarten, Wonseok Lee, Damian Murphy, Yong Ha Kim, Nicholas Mitchell, and Scott Palo
Ann. Geophys., 39, 1–29, https://doi.org/10.5194/angeo-39-1-2021, https://doi.org/10.5194/angeo-39-1-2021, 2021
Willem E. van Caspel, Patrick J. Espy, Robert E. Hibbins, and John P. McCormack
Ann. Geophys., 38, 1257–1265, https://doi.org/10.5194/angeo-38-1257-2020, https://doi.org/10.5194/angeo-38-1257-2020, 2020
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Global-scale wind measurements from the upper regions of the atmosphere are used to isolate those atmospheric waves that follow the apparent motion of the sun over the course of a day. We present 16 years of near-continuous measurements, demonstrating the unique capabilities of the array of high-latitude SuperDARN radars. The validation steps outlined in our work also provide a methodology for future studies using wind measurements from the (expanding) network of SuperDARN radars.
Ricardo A. Buriti, Wayne Hocking, Paulo P. Batista, Igo Paulino, Ana R. Paulino, Marcial Garbanzo-Salas, Barclay Clemesha, and Amauri F. Medeiros
Ann. Geophys., 38, 1247–1256, https://doi.org/10.5194/angeo-38-1247-2020, https://doi.org/10.5194/angeo-38-1247-2020, 2020
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Solar atmospheric tides are natural oscillations of 24, 12, 8... hours that contribute to the circulation of the atmosphere from low to high altitudes. The Sun heats the atmosphere periodically because, mainly, water vapor and ozone absorb solar radiation between the ground and 50 km height during the day. Tides propagate upward and they can be observed in, for example, the wind field. This work presents diurnal tides observed by meteor radars which measure wind between 80 and 100 km height.
Christoph Geißler, Christoph Jacobi, and Friederike Lilienthal
Ann. Geophys., 38, 527–544, https://doi.org/10.5194/angeo-38-527-2020, https://doi.org/10.5194/angeo-38-527-2020, 2020
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This is an extensive model study to analyze the migrating quarterdiurnal solar tide (QDT) and its forcing mechanisms in the middle atmosphere. We first show a climatology of the QDT amplitudes and examine the contribution of the different forcing mechanisms, including direct solar, nonlinear and gravity wave forcing, on the QDT amplitude. We then investigate the destructive interference between the individual forcing mechanisms.
Oluwakemi Dare-Idowu, Igo Paulino, Cosme A. O. B. Figueiredo, Amauri F. Medeiros, Ricardo A. Buriti, Ana Roberta Paulino, and Cristiano M. Wrasse
Ann. Geophys., 38, 507–516, https://doi.org/10.5194/angeo-38-507-2020, https://doi.org/10.5194/angeo-38-507-2020, 2020
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Some strong gravity wave activity occurred and was observed on 8 April 2005. This work reports the spectral characteristics of these waves using OH airglow images captured by the all-sky imager installed at São João do Cariri (7.4° S, 36.5° W). A preferential propagation direction was observed due to the positioning of the source and also due to the wind filtering effect. Furthermore, the source of these waves was identified by performing reverse-ray tracing analysis.
Emilia Correia, Luis Tiago Medeiros Raunheitte, José Valentin Bageston, and Dino Enrico D'Amico
Ann. Geophys., 38, 385–394, https://doi.org/10.5194/angeo-38-385-2020, https://doi.org/10.5194/angeo-38-385-2020, 2020
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Here the investigation of gravity wave (GW) properties in the low ionosphere using very low frequency (VLF) radio signals is presented. The VLF technique is a powerful tool to obtain the wave period and duration of GW events in the low ionosphere. It can be used independent of sky conditions, during daytime and year-round, which is an advantage in comparison with airglow all-sky imagers.
Yasunobu Miyoshi and Erdal Yiğit
Ann. Geophys., 37, 955–969, https://doi.org/10.5194/angeo-37-955-2019, https://doi.org/10.5194/angeo-37-955-2019, 2019
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Our numerical simulation shows that the drag due to the dissipation and/or breaking of the gravity wave plays an important role in the general circulation in the thermosphere. This means that the parameterization for the gravity wave drag is necessary for numerical simulation in the thermosphere.
Friederike Lilienthal and Christoph Jacobi
Ann. Geophys., 37, 943–953, https://doi.org/10.5194/angeo-37-943-2019, https://doi.org/10.5194/angeo-37-943-2019, 2019
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We analyzed the forcing mechanisms of the migrating terdiurnal solar tide in the middle atmosphere, focusing the impact on the zonal mean circulation. We show that the primary solar forcing is the most dominant one but secondary wave–wave interactions also contribute in the lower thermosphere region. We further demonstrate that small-scale gravity waves can strongly and irregularly influence the amplitude of the terdiurnal tide as well as the background circulation in the thermosphere.
Sven Wilhelm, Gunter Stober, and Peter Brown
Ann. Geophys., 37, 851–875, https://doi.org/10.5194/angeo-37-851-2019, https://doi.org/10.5194/angeo-37-851-2019, 2019
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We report on long-term observations of atmospheric parameters in the mesosphere and lower thermosphere made over the last 2 decades for the northern-latitude locations of Andenes, Juliusruh, and Tavistock. The observations are based on meteor wind measurements and further include the long-term variability of winds, tides, and the kinetic energy of gravity waves and planetary waves. Furthermore, the influence on an 11-year oscillation on the winds and tides is presented.
Dimitry Pokhotelov, Erich Becker, Gunter Stober, and Jorge L. Chau
Ann. Geophys., 36, 825–830, https://doi.org/10.5194/angeo-36-825-2018, https://doi.org/10.5194/angeo-36-825-2018, 2018
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Atmospheric tides are produced by solar heating of the lower atmosphere. The tides propagate to the upper atmosphere and ionosphere playing an important role in the vertical coupling. Ground radar measurements of the seasonal variability of tides are compared with global numerical simulations. The agreement with radar data and limitations of the numerical model are discussed. The work represents a first step in modelling the impact of tidal dynamics on the upper atmosphere and ionosphere.
Cited articles
Alexander, M. J.: Interpretations of observed climatological patterns in
stratospheric gravity wave variance, J. Geophys. Res., 103, 8627–8640,
https://doi.org/10.1029/97JD03325, 1998.
Coble, M., Papen, G. C., and Gardner, C. S.: Computing two-dimensional
unambiguous horizontal wavenumber spectra from OH airglow images, IEEE T.
Geosci. Remote Sens., 36, 368–382, https://doi.org/10.1109/36.662723, 1998.
Dwyer, R. A.: A faster divide-and-conquer algorithm for constructing Delaunay
triangulations, Algorithmica, 2, 137–151, 1987.
Ejiri, M. K., Shiokawa, K., Ogawa, T., Igarashi, K., Nakamura, T., and Tsuda,
T.: Statistical study of short-period gravity waves in OH and OI nightglow
images at two separated sites, J. Geophys. Res., 108, 4679,
https://doi.org/10.1029/2002JD002795, 2003.
Fritts, D. C.: Gravity wave saturation in the middle atmosphere: A review of
theory and observations, Rev. Geophys., 22, 275–308,
https://doi.org/10.1029/RG022i003p00275, 1984.
Fritts, D. C. and Alexander, M. J.: Gravity wave dynamics and effects in the
middle atmosphere, Rev. Geophys., 41, 1003, https://doi.org/10.1029/2001RG000106, 2003.
Gelaro, R., McCarty, W., Suarez, M. J., Todling, R., Molod, A., Takacs, L.,
Randles, C. A., Darmenov, A., Bosilovich, M. G., Reichle, R., Wargan, K.,
Coy, L., Cullather, R., Draper, C., Akella, S., Buchard, V., Conaty, A., Gu,
W., Kim, G. K., Koster, R., Lucchesi, R., Merkova, D., Nielsen, J. E.,
Partyka, G., Pawson, S., Putman, W., Rienecker, M., Schubert, S. D.,
Sienkiewicz, M., and Zhao, B.: The Modern-Era Retrospective Analysis for
Research and Applications, Version-2 (MERRA-2), J. Climate, 30, 5419–5454,
https://doi.org/10.1175/JCLI-D-16-0758.1, 2017.
Haffke, C., Magnusdottir, G., Henke, D., Smyth, P., and Peings, Y.: Daily
states of the March-April east Pacific ITCZ in three decades of
high-resolution satellite data, J. Climate, 29, 2981–2995,
https://doi.org/10.1175/JCLI-D-15-0224.1, 2016.
Kubota, M., Fukunishi, H., and Okano, S.: Characteristics of medium and
large-scale TIDs over Japan derived from OI 630-nm nightglow observation,
Earth Planets Space, 53, 741–751, 2001.
Lindzen, R.: Turbulence and stress owing to gravity wave and tidal breakdown,
J. Geophys. Res., 86, 9707–9714, https://doi.org/10.1029/JC086iC10p09707, 1981.
Matsuda, T. S., Nakamura, T., Ejiri, M. K., Tsutsumi, M., and Shiokawa, K.:
New statistical analysis of the horizontal phase velocity distribution of
gravity waves observed by airglow imaging, J. Geophys. Res.-Atmos., 119,
9707–9718, https://doi.org/10.1002/2014JD021543, 2014.
Matsuda, T. S., Nakamura, T., Ejiri, M. K., Tsutsumi, M., Tomikawa, Y.,
Taylor, M. J., Zhao, Y., Pautet, P.D., Murphy, D. J., and Moffat-Griffin, T.:
Characteristics of mesospheric gravity waves over Antarctica observed by
Antarctic Gravity Wave Instrument Network imagers using 3-D spectral
analyses, J. Geophys. Res.-Atmos., 122, 8969–8981, https://doi.org/10.1002/2016JD026217,
2017.
Matsuno, T.: A quasi-one-dimensional model of the middle atmospheric
circulation interacting with internal gravity waves, J. Meteorol. Soc. Jpn.,
60, 215–226, 1982.
Nakamura, T., Higashikawa, A., Tsuda, T., and Matsushita, Y.: Seasonal
variations of gravity wave structures in OH airglow with a CCD imager at
Shigaraki, Earth Planets Space, 51, 897–906, 1999.
Nakamura, T., Aono, T., and Tsuda, T.: Mesospheric gravity waves over a
tropical convective region observed by OH airglow imaging in Indonesia,
Geophys. Res. Lett., 30, 1882, https://doi.org/10.1029/2003GL017619, 2003.
Shiokawa, K., Otsuka, Y., and Ogawa, T.: Propagation characteristics of
nighttime mesospheris and thermospheric waves observed by optical mesosphere
thermosphere imagers at middle and low latitudes, Earth Planets Sci., 61,
479–491, 2009.
Su, P. and Scot Drysdale, R. L.: A comparison of sequential Delaunay
triangulation algorithms, Comput. Geom.-Theor. Appl., 7, 361–385, 1997.
Suzuki, S., Shiokawa, K., Otsuka, Y., Ogawa, T., Nakamura, K., and Nakamura,
T.: A concentric gravity wave structure in the mesospheric airglow images, J.
Geophys. Res., 112, D02102, https://doi.org/10.1029/2005JD006558, 2007.
Takeo, D., Shiokawa, K., Fujinami, H., Otsuka, Y., Matsuda, T. S., Ejiri, M.
K., Nakamura, T., and Yamamoto, M.: Sixteen-year variation of horizontal
phase velocity and propagation direction of mesospheric and thermospheric
waves in airglow images at Shigaraki, Japan, J. Geophys. Res.-Space, 122,
8770–8780, https://doi.org/10.1002/2017JA023919, 2017.
Taylor, M. J., Ryan, E. H., Tuan, T. F., and Edwards, R.: Evidence of
preferential directions for gravity wave propagation due to wind filtering in
the middle atmosphere, J. Geophys. Res., 98, 6047–6057,
https://doi.org/10.1029/92JA02604, 1993.
Tomikawa, Y.: Gravity wave transmission diagram, Ann. Geophys., 33,
1479–1484, https://doi.org/10.5194/angeo-33-1479-2015, 2015.
Tsuchiya, S., Shiokawa, K., Fujinami, H., Otsuka, Y., Nakamura, T., and
Yamamoto, M.: Statistical analysis of the phase velocity distribution of
mesospheric and ionospheric waves observed in airglow images over a 16-year
period: Comparison between Rikubetsu and Shigaraki, Japan, J. Geophys. Res.,
123, 6930–6947, https://doi.org/10.1029/2018JA025585, 2018.
Wright, C. J., Hindley, N. P., Moss, A. C., and Mitchell, N. J.:
Multi-instrument gravity-wave measurements over Tierra del Fuego and the
Drake Passage – Part 1: Potential energies and vertical wavelengths from
AIRS, COSMIC, HIRDLS, MLS-Aura, SAAMER, SABER and radiosondes, Atmos. Meas.
Tech., 9, 877–908, https://doi.org/10.5194/amt-9-877-2016, 2016.
Short summary
We have developed a user-friendly program that can efficiently deal with extensive amounts of airglow data. We have applied this new program to airglow data obtained at different latitudes in polar, midlatitude, and equatorial regions and demonstrated distinct differences in atmospheric gravity wave (AGW) propagation characteristics and energy distribution. We aim to encourage other AGW research groups to use the program and do comparisons to reveal AGW characteristics on a more global scale.
We have developed a user-friendly program that can efficiently deal with extensive amounts of...