Electrodynamic influence on the diurnal behaviour of neutral daytime airglow emissions
-
Published:2016-11-16
Issue:11
Volume:34
Page:1019-1030
-
ISSN:1432-0576
-
Container-title:Annales Geophysicae
-
language:en
-
Short-container-title:Ann. Geophys.
Author:
Karan Deepak K., Pallamraju Duggirala, Phadke Kedar A.ORCID, Vijayalakshmi Tatiparti, Pant Tarun K., Mukherjee Shyamoli
Abstract
Abstract. The diurnal variations in daytime airglow emission intensity measurements at three wavelengths OI 777.4 nm, OI 630.0 nm, and OI 557.7 nm made from a low-latitude location, Hyderabad (17.5° N, 78.4° E; 8.9° N MLAT) in India have been investigated. The intensity patterns showed both symmetric and asymmetric behaviour in their respective diurnal emission variability with respect to local noon. The asymmetric diurnal behaviour is not expected considering the photochemical nature of the production mechanisms. The reason for this observed asymmetric diurnal behaviour has been found to be predominantly the temporal variation in the equatorial electrodynamics. The plasma that is transported across latitudes due to the action of varying electric field strengths over the magnetic equator in the daytime contributes to the asymmetric diurnal behaviour in the neutral daytime airglow emissions. Independent magnetic and radio measurements support this finding. It is also noted that this asymmetric diurnal behaviour in the neutral emission intensities has a solar cycle dependence with a greater number of days during high solar activity period showing asymmetric diurnal behaviour compared to those during a low solar activity epoch. These intensity variations over a long timescale demonstrate that the daytime neutral optical emissions are extremely sensitive to the changes in the eastward electric field over low and equatorial latitudes.
Publisher
Copernicus GmbH
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geology,Astronomy and Astrophysics
Reference49 articles.
1. Chakrabarty, D., Sekar, R., Chandra, H., Narayanan, R., Pathan, B. M., and Subbarao, K. S. V.: Characterizations of the diurnal shapes of OI 630.0 nm dayglow intensity variations: inferences, Ann. Geophys., 20, 1851–1855, https://doi.org/10.5194/angeo-20-1851-2002, 2002. 2. Chakrabarti, S., Pallamraju, D., Baumgardner, J., and Vaillancourt, J.: HiTIES: a high throughput imaging echelle spectrograph for ground-based visible airglow and auroral studies, J. Geophys. Res., 106, 30337–30348, 2001. 3. Das, U., Pallamraju, D., and Chakrabarti, S.: Effect of an X-Class solar flare on the OI 630 nm dayglow emissions, J. Geophys. Res., 115, A08302, https://doi.org/10.1029/2010JA015370, 2010. 4. Drob, D. P., Emmert, J. T., Meriwether, J. W., Makela, J. J., Doornbos, E., Conde, M., Hernandez, G., Noto, J., Zawdie, K. A., McDonald, S. E., Huba, J. D., and Klenzing, J. H.: An update to the Horizontal Wind Model (HWM): The quiet time thermosphere, Earth and Space Science, 2, 301–319, https://doi.org/10.1002/2014EA000089, 2015. 5. Emmert, J. T., Richmond, A. D., and Drob D. P.: A computationally compact representation of Magnetic-Apex and Quasi-Dipole coordinates with smooth base vectors, J. Geophys. Res., 115, A08322, https://doi.org/10.1029/2010JA015326, 2010.
Cited by
16 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
|
|