Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/12161
DC Field | Value | Language |
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dc.date.accessioned | 2019-01-30T08:12:20Z | en |
dc.date.available | 2019-01-30T08:12:20Z | en |
dc.date.issued | 2018 | en |
dc.identifier.uri | http://hdl.handle.net/2122/12161 | en |
dc.description.abstract | A new method to extract neutral composition (O, O2, N2), exospheric temperature Tex, vertical plasma drift ,W, and the total solar Extreme Ultraviolet (EUV) flux with 1050Å from routine ionosonde bottom-side electron density, Ne(h), observations has been proposed. The method can be used around noontime hours for all months of the year at middle latitudes where the ionospheric F-layer is formed by solar EUV radiation. The uncertainty of the retrieved neutral gas density coincides with the announced absolute uncertainty (10-15%) of Challenging Minisatellite Payload/ Space Three-axis Accelerometer for Research mission (CHAMP/STAR ) neutral gas density observations. The method provides statistically significant better results with Mean Relative Deviation (MRD) < 15% ; Root Mean Square (RMS) < 0.5 in a comparison with modern empirical models Mass-Spectrometer-Incoherent-Scatter ( MSISE00), Jacchia-Bowman 2008 (JB2008), and Drag Temperature Model 2013 ( DTM2013) (MRD>15% and RMS> 0.5). The thermospheric parameters retrieved for the St. Patrick Day magnetic storm and two so called Q-disturbance periods are given as an example of the method application. The retrieved neutral gas densities for the St. Patrick Day storm are compared to Swarm-B accelerometer observations. The proposed method may be considered as an useful tool for analyses of the state of the upper atmosphere under various geophysical conditions. | en |
dc.language.iso | English | en |
dc.relation.ispartof | Journal of Geophysical Research: Space Physics | en |
dc.relation.ispartofseries | /123 (2018) | en |
dc.title | A New Method to Retrieve Thermospheric Parameters From Daytime Bottom-Side Ne(h) Observations | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.description.pagenumber | 10200-10212 | en |
dc.identifier.doi | 10.1029/2018JA025762 | en |
dc.description.obiettivoSpecifico | 2A. Fisica dell'alta atmosfera | en |
dc.description.journalType | JCR Journal | en |
dc.contributor.author | Perrone, Loredana | en |
dc.contributor.author | Mikhailov, A. V. | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | en |
dc.contributor.department | IZMIRAN | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | restricted | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (IZMIRAN), Troitsk, Moscow Region 142190, Russia | - |
crisitem.author.orcid | 0000-0003-4335-0345 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
Appears in Collections: | Article published / in press |
Files in This Item:
File | Description | Size | Format | |
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16131918.pdf | 1.15 MB | Adobe PDF | View/Open |
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