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Thermospheric parameters contribution to the formation of Yakutsk F 2-layer diurnal summer time anomaly. Sci Rep 2022; 12:13510. [PMID: 35931714 PMCID: PMC9355984 DOI: 10.1038/s41598-022-17691-1] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/02/2022] [Accepted: 07/29/2022] [Indexed: 11/08/2022] Open
Abstract
The role of thermospheric neutral composition in the formation of the Yakutsk diurnal summer time foF2 anomaly is analyzed. Ionospheric stations inside and outside the anomaly area are considered. The effect of neutral composition in foF2 is the most noticeable around noontime hours. The difference between observed noontime foF2 in two areas is significant at the 99.9% confidence level both for monthly median and individual days. The inferred from ionosonde observations and Swarm neutral gas density thermospheric parameters indicate a significant difference between two areas. The inferred exospheric temperature, Tex at Magadan (inside the anomaly area) is significantly larger than Tex at Tunguska (outside the anomaly area). On the contrary, the inferred atomic oxygen [O] at Tunguska is significantly larger than at Magadan. Different [O] abundance in the two areas is the main reason of the observed difference in noontime foF2 values. Vertical plasma drift depending on magnetic declination, D is the only process responsible for the difference between nighttime foF2 at Tunguska and Magadan. A possible mechanism of the revealed difference in thermospheric parameters inside and outside the anomaly area is discussed.
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Ionospheric Science: An Example of the Importance of Diversity in Approaches to Scientific Research. ATMOSPHERE 2022. [DOI: 10.3390/atmos13030394] [Citation(s) in RCA: 2] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 02/04/2023]
Abstract
This paper discusses the strategic importance of contemporary ionospheric science. It outlines some key features of the evolution of the science from the first practical experiments in the 1920s through to the diverse inter-disciplinary science of today. This science includes fundamental studies of partially ionised plasmas and of the complex systems that arise when those plasmas are coupled to neutral atmospheres and magnetospheres. However, the science also has great potential to deliver societal benefits if the science can be refined to obtain a deep physical understanding of ionospheric phenomena and that understanding is then transitioned into use by operational services such as forecasts of ionospheric conditions. Thus, ionospheric science is now very similar in form to other environment sciences and, the same as them, needs to be positioned in a diverse scientific culture that supports the full range of science research, including not only curiosity-driven studies, but also targeted research to deepen our physical understanding to a level that is sufficient to enable a transition to operational services. That diversity also includes support for that transition and also facilitates feedback from operations teams to researchers. Such feedback can be a powerful stimulus for future research.
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Drob DP, Emmert JT, Crowley G, Picone JM, Shepherd GG, Skinner W, Hays P, Niciejewski RJ, Larsen M, She CY, Meriwether JW, Hernandez G, Jarvis MJ, Sipler DP, Tepley CA, O'Brien MS, Bowman JR, Wu Q, Murayama Y, Kawamura S, Reid IM, Vincent RA. An empirical model of the Earth's horizontal wind fields: HWM07. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2008ja013668] [Citation(s) in RCA: 392] [Impact Index Per Article: 24.5] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- D. P. Drob
- Space Science Division; Naval Research Laboratory; Washington District of Columbia USA
| | - J. T. Emmert
- Space Science Division; Naval Research Laboratory; Washington District of Columbia USA
| | - G. Crowley
- Atmospheric and Space Technology Research Associates; San Antonio Texas USA
| | - J. M. Picone
- Space Science Division; Naval Research Laboratory; Washington District of Columbia USA
| | - G. G. Shepherd
- Centre for Research in Earth and Space Science; York University; Toronto Ontario Canada
| | - W. Skinner
- Space Physics Research Laboratory, Department of Atmospheric, Oceanic, and Space Sciences, College of Engineering; University of Michigan; Ann Arbor Michigan USA
| | - P. Hays
- Space Physics Research Laboratory, Department of Atmospheric, Oceanic, and Space Sciences, College of Engineering; University of Michigan; Ann Arbor Michigan USA
| | - R. J. Niciejewski
- Space Physics Research Laboratory, Department of Atmospheric, Oceanic, and Space Sciences, College of Engineering; University of Michigan; Ann Arbor Michigan USA
| | - M. Larsen
- Department of Physics and Astronomy; Clemson University; Clemson South Carolina USA
| | - C. Y. She
- Physics Department; Colorado State University; Fort Collins Colorado USA
| | - J. W. Meriwether
- Department of Physics and Astronomy; Clemson University; Clemson South Carolina USA
| | - G. Hernandez
- Department of Earth and Space Sciences; University of Washington; Seattle Washington USA
| | | | - D. P. Sipler
- Haystack Observatory; Massachusetts Institute of Technology; Westford Massachusetts USA
| | - C. A. Tepley
- Arecibo Observatory; Cornell University; Arecibo Puerto Rico
| | - M. S. O'Brien
- Science Applications International Corporation; San Diego California USA
| | - J. R. Bowman
- Science Applications International Corporation; San Diego California USA
| | - Q. Wu
- High Altitude Observatory; National Center for Atmospheric Research; Boulder Colorado USA
| | - Y. Murayama
- National Institute of Information and Communications Technology; Tokyo Japan
| | - S. Kawamura
- National Institute of Information and Communications Technology; Tokyo Japan
| | - I. M. Reid
- School of Chemistry and Physics; University of Adelaide; Adelaide, South Australia Australia
| | - R. A. Vincent
- School of Chemistry and Physics; University of Adelaide; Adelaide, South Australia Australia
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