Secular variability of the geocoronal Balmer-alpha brightness: magnetic activity and possible human influences
| Autor: | R. S. Lancaster, John Noto, X. He, Sixto A. González, R. A. Doe, B. McCormack, Robert B. Kerr, Craig A. Tepley, Jonathan S. Friedman, M. Lappen, R. Garcia |
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| Rok vydání: | 2001 |
| Předmět: |
Absolute magnitude
Atmospheric Science Brightness Soil Science Astrophysics Aquatic Science Oceanography Atmospheric sciences Atmosphere symbols.namesake Geochemistry and Petrology Earth and Planetary Sciences (miscellaneous) Earth-Surface Processes Water Science and Technology Physics Ecology Airglow Paleontology Balmer series Forestry Solar cycle Geophysics Earth's magnetic field Space and Planetary Science symbols Exosphere |
| Zdroj: | Scopus-Elsevier |
| ISSN: | 0148-0227 |
| DOI: | 10.1029/1999ja900187 |
| Popis: | Measurements of the geocoronal Balmer-alpha (Hα) brightness taken between 1983 and 1994 at the Arecibo Observatory (18.35° N, 66.75° W) occasionally display aperiodic brightness variations that we attribute to a local response of exospheric hydrogen abundance to geomagnetic activity. Approximately twofold Hα brightness enhancements in the days following moderate storm onset conditions are demonstrated, and the absolute brightness during these events is significantly greater than modeled brightness based on quiet geomagnetic conditions. Although there are no direct measurements of the line center solar Lyman beta (Ly β) flux that pumps Hα during these events, the magnitude of the brightness enhancements and the temporal reproducibility of the phenomena (following onset of all storms in our data) make it likely that the enhanced Hα brightness is due to enhanced column abundances of hydrogen in the exosphere above Arecibo and not to sporadic increases in the solar Ly β flux. Increased hydrogen abundance due to thermal expansion of the midlatitude atmosphere following propagation of the auroral heating event cannot account for the entire enhancement. The data also suggest that Hα. brightness has become systematically stronger from 1984 to 1994, independent of solar cycle variability or variations due to geomagnetic activity. An increase of ∼ 3% per year, may be attributable to real change in the geocoronal hydrogen column abundance during the period, and is possibly a consequence of increasing hydrogenous species concentrations in the lower atmosphere. The enhancement of geocoronal Hα brightness between 1984 and 1994 may be the consequence of increasing methane in the troposphere and may signal that the effects of methane deposition in the lower atmosphere have propagated throughout the atmosphere. |
| Databáze: | OpenAIRE |
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