FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2025401966> ?p ?o ?g. }

• W2025401966 abstract "[1] The intense modifications in the ionosphere-thermosphere system in the equatorial and low-latitude regions associated with the dynamic and electrodynamic coupling from high to low latitudes and chemical changes during geomagnetic storms are important space weather issues. In the second half of October 2003, the intense solar activity resulted in one intense and two major geomagnetic storms on 29 and 30 October. In this paper we present and discuss the ionospheric sounding observations carried out from Palmas and São José dos Campos, Brazil (the Brazilian sector), and Ho Chi Minh City, Vietnam, and Okinawa, Japan (the East Asian sector), during these storms. The two sectors are separated by about 12 hours in local time (so while one sector is in daytime, the other one is in nighttime) and provide valuable information related to the storm-time longitudinal differences. Copious storm-time changes were observed in both sectors. It should be pointed out that the two longitudinal sectors investigated in the present study clearly show the global nature of the storm-time effects. However, the responses to the storm-time effects are also associated with the local time in the two sectors. The present investigations show that there are both similarities and differences in the storm-time response in the two sectors. During the storm main phases, with sharp decreases of the Dst index, both sectors showed (dusk or dawn periods) fast uplifting of the F layer associated with magnetospheric electric field penetration. Although in the East Asian sector, Ho Chi Minh City and Okinawa are located fairly close in longitude, with only 2 hour difference in local lime, on occasions the storm-time responses have been very different. Some differences in the latitudinal response of the F region were also observed in the two sectors. Both positive and negative storm phases have been observed at all the four stations. A comparison of the ionospheric parameters obtained from the TIMEGCM model runs and the observed ionospheric parameters at the four stations shows a reasonable agreement during the quiet periods. During the geomagnetic disturbance period, when there were sharp decreases in Dst, some of the observed rapid uplifts of the F region peak heights are not reproduced by the model results. Also, sometimes the model foF2 results differ considerably from the observed foF2 variations. The period investigated represents an extreme storm situation for validation of the model and points to ways in which the model might be improved in the future." @default.
• W2025401966 created "2016-06-24" @default.
• W2025401966 creator A5003153404 @default.
• W2025401966 creator A5006411837 @default.
• W2025401966 creator A5014652856 @default.
• W2025401966 creator A5019531961 @default.
• W2025401966 creator A5042447263 @default.
• W2025401966 creator A5044469788 @default.
• W2025401966 creator A5048136106 @default.
• W2025401966 creator A5054100706 @default.
• W2025401966 creator A5055118286 @default.
• W2025401966 creator A5067169255 @default.
• W2025401966 creator A5070561481 @default.
• W2025401966 creator A5075805756 @default.
• W2025401966 creator A5083339670 @default.
• W2025401966 creator A5084429024 @default.
• W2025401966 date "2005-01-01" @default.
• W2025401966 modified "2023-10-08" @default.
• W2025401966 title "Effects of the major geomagnetic storms of October 2003 on the equatorial and low-latitude<i>F</i>region in two longitudinal sectors" @default.
• W2025401966 cites W1585936640 @default.
• W2025401966 cites W1673977746 @default.
• W2025401966 cites W1965638893 @default.
• W2025401966 cites W1970036327 @default.
• W2025401966 cites W1982903954 @default.
• W2025401966 cites W1985967985 @default.
• W2025401966 cites W1986429732 @default.
• W2025401966 cites W2001326760 @default.
• W2025401966 cites W2005906898 @default.
• W2025401966 cites W2006145128 @default.
• W2025401966 cites W2010949540 @default.
• W2025401966 cites W2010949667 @default.
• W2025401966 cites W2017360177 @default.
• W2025401966 cites W2018554399 @default.
• W2025401966 cites W2019388546 @default.
• W2025401966 cites W2022822277 @default.
• W2025401966 cites W2026253822 @default.
• W2025401966 cites W2029308148 @default.
• W2025401966 cites W2029445959 @default.
• W2025401966 cites W2031764511 @default.
• W2025401966 cites W2037149905 @default.
• W2025401966 cites W2039177136 @default.
• W2025401966 cites W2041097427 @default.
• W2025401966 cites W2042651878 @default.
• W2025401966 cites W2043327550 @default.
• W2025401966 cites W2043534404 @default.
• W2025401966 cites W2050119970 @default.
• W2025401966 cites W2051071569 @default.
• W2025401966 cites W2058535605 @default.
• W2025401966 cites W2059606560 @default.
• W2025401966 cites W2059825387 @default.
• W2025401966 cites W2060085273 @default.
• W2025401966 cites W2070007833 @default.
• W2025401966 cites W2072185069 @default.
• W2025401966 cites W2072455171 @default.
• W2025401966 cites W2077658274 @default.
• W2025401966 cites W2079794170 @default.
• W2025401966 cites W2088813412 @default.
• W2025401966 cites W2095057999 @default.
• W2025401966 cites W2101968821 @default.
• W2025401966 cites W2108697558 @default.
• W2025401966 cites W2137775923 @default.
• W2025401966 cites W2143841763 @default.
• W2025401966 cites W4245039911 @default.
• W2025401966 doi "https://doi.org/10.1029/2004ja010999" @default.
• W2025401966 hasPublicationYear "2005" @default.
• W2025401966 type Work @default.
• W2025401966 sameAs 2025401966 @default.
• W2025401966 citedByCount "62" @default.
• W2025401966 countsByYear W20254019662012 @default.
• W2025401966 countsByYear W20254019662013 @default.
• W2025401966 countsByYear W20254019662014 @default.
• W2025401966 countsByYear W20254019662015 @default.
• W2025401966 countsByYear W20254019662016 @default.
• W2025401966 countsByYear W20254019662017 @default.
• W2025401966 countsByYear W20254019662018 @default.
• W2025401966 countsByYear W20254019662019 @default.
• W2025401966 countsByYear W20254019662020 @default.
• W2025401966 countsByYear W20254019662021 @default.
• W2025401966 countsByYear W20254019662022 @default.
• W2025401966 crossrefType "journal-article" @default.
• W2025401966 hasAuthorship W2025401966A5003153404 @default.
• W2025401966 hasAuthorship W2025401966A5006411837 @default.
• W2025401966 hasAuthorship W2025401966A5014652856 @default.
• W2025401966 hasAuthorship W2025401966A5019531961 @default.
• W2025401966 hasAuthorship W2025401966A5042447263 @default.
• W2025401966 hasAuthorship W2025401966A5044469788 @default.
• W2025401966 hasAuthorship W2025401966A5048136106 @default.
• W2025401966 hasAuthorship W2025401966A5054100706 @default.
• W2025401966 hasAuthorship W2025401966A5055118286 @default.
• W2025401966 hasAuthorship W2025401966A5067169255 @default.
• W2025401966 hasAuthorship W2025401966A5070561481 @default.
• W2025401966 hasAuthorship W2025401966A5075805756 @default.
• W2025401966 hasAuthorship W2025401966A5083339670 @default.
• W2025401966 hasAuthorship W2025401966A5084429024 @default.
• W2025401966 hasBestOaLocation W20254019661 @default.
• W2025401966 hasConcept C105306849 @default.
• W2025401966 hasConcept C105795698 @default.
• W2025401966 hasConcept C111368507 @default.
• W2025401966 hasConcept C115260700 @default.
• W2025401966 hasConcept C116403925 @default.

• next