Climatology of medium-scale traveling ionospheric disturbances observed by a GPS network in central China
The 15‐month climatology of medium‐scale traveling ionospheric disturbances (MSTIDs) during a solar minimum period has been constructed from observations of a dense GPS receiver array in Central China. In total, 793 MSTID events are identified, with peaks in occurrence at 1500 LT and 0100 LT. The oc...
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| Published in | Journal of Geophysical Research: Space Physics Vol. 116; no. A9 |
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| Main Authors | , , , , , |
| Format | Journal Article |
| Language | English |
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Blackwell Publishing Ltd
01.09.2011
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| Abstract | The 15‐month climatology of medium‐scale traveling ionospheric disturbances (MSTIDs) during a solar minimum period has been constructed from observations of a dense GPS receiver array in Central China. In total, 793 MSTID events are identified, with peaks in occurrence at 1500 LT and 0100 LT. The occurrence of MSTIDs decreases following an increase in geomagnetic activity, with 46% of the MSTIDS occurring in the daytime. Daytime MSTIDs are characterized by a major occurrence maximum around the winter solstice and by an equatorward propagation direction. The period, phase velocity, azimuth, and amplitude of daytime MSTIDs are 20–60 min, 100–400 m/s, 130°–270°, and 0.8–1.5%, respectively. The remaining 54% of the MSTIDs occurred at night, and were characterized by a peak in occurrence at the summer solstice and by a southwestward propagation direction. The period, phase velocity, azimuth, and amplitude of nighttime MSTIDs are 20–70 min, 50–230 m/s, 170°–300°, and 2–7%, respectively. The propagation directions and the seasonal behaviors support the view that daytime MSTIDs are an ionospheric manifestation of atmospheric gravity waves from the lower atmosphere, while a possible excitation mechanism of nighttime MSTIDs is the electrodynamics process caused by plasma instability in the F layer.
Key Points
Daytime MSTIDs have a peak at winter solstice and propagated southward
Nighttime MSTIDs have a peak at summer solstice and a southwestward direction
Comparing with HF Doppler observation, we find a height dependence of MSTIDs |
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| AbstractList | Daytime MSTIDs have a peak at winter solstice and propagated southward Nighttime MSTIDs have a peak at summer solstice and a southwestward direction Comparing with HF Doppler observation, we find a height dependence of MSTIDs The 15-month climatology of medium-scale traveling ionospheric disturbances (MSTIDs) during a solar minimum period has been constructed from observations of a dense GPS receiver array in Central China. In total, 793 MSTID events are identified, with peaks in occurrence at 1500 LT and 0100 LT. The occurrence of MSTIDs decreases following an increase in geomagnetic activity, with 46% of the MSTIDS occurring in the daytime. Daytime MSTIDs are characterized by a major occurrence maximum around the winter solstice and by an equatorward propagation direction. The period, phase velocity, azimuth, and amplitude of daytime MSTIDs are 2060 min, 100400 m/s, 130°270°, and 0.81.5%, respectively. The remaining 54% of the MSTIDs occurred at night, and were characterized by a peak in occurrence at the summer solstice and by a southwestward propagation direction. The period, phase velocity, azimuth, and amplitude of nighttime MSTIDs are 2070 min, 50230 m/s, 170°300°, and 27%, respectively. The propagation directions and the seasonal behaviors support the view that daytime MSTIDs are an ionospheric manifestation of atmospheric gravity waves from the lower atmosphere, while a possible excitation mechanism of nighttime MSTIDs is the electrodynamics process caused by plasma instability in the F layer. Daytime MSTIDs have a peak at winter solstice and propagated southward Nighttime MSTIDs have a peak at summer solstice and a southwestward direction Comparing with HF Doppler observation, we find a height dependence of MSTIDs The 15-month climatology of medium-scale traveling ionospheric disturbances (MSTIDs) during a solar minimum period has been constructed from observations of a dense GPS receiver array in Central China. In total, 793 MSTID events are identified, with peaks in occurrence at 1500 LT and 0100 LT. The occurrence of MSTIDs decreases following an increase in geomagnetic activity, with 46% of the MSTIDS occurring in the daytime. Daytime MSTIDs are characterized by a major occurrence maximum around the winter solstice and by an equatorward propagation direction. The period, phase velocity, azimuth, and amplitude of daytime MSTIDs are 20-60 min, 100-400 m/s, 130 degree -270 degree , and 0.8-1.5%, respectively. The remaining 54% of the MSTIDs occurred at night, and were characterized by a peak in occurrence at the summer solstice and by a southwestward propagation direction. The period, phase velocity, azimuth, and amplitude of nighttime MSTIDs are 20-70 min, 50-230 m/s, 170 degree -300 degree , and 2-7%, respectively. The propagation directions and the seasonal behaviors support the view that daytime MSTIDs are an ionospheric manifestation of atmospheric gravity waves from the lower atmosphere, while a possible excitation mechanism of nighttime MSTIDs is the electrodynamics process caused by plasma instability in the F layer. The 15‐month climatology of medium‐scale traveling ionospheric disturbances (MSTIDs) during a solar minimum period has been constructed from observations of a dense GPS receiver array in Central China. In total, 793 MSTID events are identified, with peaks in occurrence at 1500 LT and 0100 LT. The occurrence of MSTIDs decreases following an increase in geomagnetic activity, with 46% of the MSTIDS occurring in the daytime. Daytime MSTIDs are characterized by a major occurrence maximum around the winter solstice and by an equatorward propagation direction. The period, phase velocity, azimuth, and amplitude of daytime MSTIDs are 20–60 min, 100–400 m/s, 130°–270°, and 0.8–1.5%, respectively. The remaining 54% of the MSTIDs occurred at night, and were characterized by a peak in occurrence at the summer solstice and by a southwestward propagation direction. The period, phase velocity, azimuth, and amplitude of nighttime MSTIDs are 20–70 min, 50–230 m/s, 170°–300°, and 2–7%, respectively. The propagation directions and the seasonal behaviors support the view that daytime MSTIDs are an ionospheric manifestation of atmospheric gravity waves from the lower atmosphere, while a possible excitation mechanism of nighttime MSTIDs is the electrodynamics process caused by plasma instability in the F layer. Key Points Daytime MSTIDs have a peak at winter solstice and propagated southward Nighttime MSTIDs have a peak at summer solstice and a southwestward direction Comparing with HF Doppler observation, we find a height dependence of MSTIDs |
| Author | Wan, Weixing Yang, Guanglin Wang, Jing-song Ding, Feng Xu, Guirong Yu, Tao |
| Author_xml | – sequence: 1 givenname: Feng surname: Ding fullname: Ding, Feng email: dingf@mail.iggcas.ac.cn organization: Beijing National Observatory of Space Environment, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China – sequence: 2 givenname: Weixing surname: Wan fullname: Wan, Weixing organization: Beijing National Observatory of Space Environment, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China – sequence: 3 givenname: Guirong surname: Xu fullname: Xu, Guirong organization: Institute of Heavy Rain, China Meteorological Administration, Wuhan, China – sequence: 4 givenname: Tao surname: Yu fullname: Yu, Tao organization: National Center for Space Weather, China Meteorological Administration, Beijing, China – sequence: 5 givenname: Guanglin surname: Yang fullname: Yang, Guanglin organization: National Center for Space Weather, China Meteorological Administration, Beijing, China – sequence: 6 givenname: Jing-song surname: Wang fullname: Wang, Jing-song organization: National Center for Space Weather, China Meteorological Administration, Beijing, China |
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| Snippet | The 15‐month climatology of medium‐scale traveling ionospheric disturbances (MSTIDs) during a solar minimum period has been constructed from observations of a... Daytime MSTIDs have a peak at winter solstice and propagated southward Nighttime MSTIDs have a peak at summer solstice and a southwestward direction Comparing... |
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| SubjectTerms | Atmospheric sciences Climatology GPS Gravity waves medium-scale traveling ionospheric disturbance Solstices Summer Winter |
| Title | Climatology of medium-scale traveling ionospheric disturbances observed by a GPS network in central China |
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