FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3097674047> ?p ?o ?g. }

• W3097674047 endingPage "149" @default.
• W3097674047 startingPage "133" @default.
• W3097674047 abstract "We present an analysis of the ionosphere and thermosphere response to Solar Proton Events (SPE) and magnetospheric proton precipitation in January 2005, which was carried out using the model of the entire atmosphere EAGLE. The ionization rates for the considered period were acquired from the AIMOS (Atmospheric Ionization Module Osnabrück) dataset. For numerical experiments, we applied only the proton-induced ionization rates of that period, while all the other model input parameters, including the electron precipitations, corresponded to the quiet conditions. In January 2005, two major solar proton events with different energy spectra and proton fluxes occurred on January 17 and January 20. Since two geomagnetic storms and several sub-storms took place during the considered period, not only solar protons but also less energetic magnetospheric protons contributed to the calculated ionization rates. Despite the relative transparency of the thermosphere for high-energy protons, an ionospheric response to the SPE and proton precipitation from the magnetotail was obtained in numerical experiments. In the ionospheric E layer, the maximum increase in the electron concentration is localized at high latitudes, and at heights of the ionospheric F2 layer, the positive perturbations were formed in the near-equatorial region. An analysis of the model-derived results showed that changes in the ionospheric F2 layer were caused by a change in the neutral composition of the thermosphere. We found that in the recovery phase after both solar proton events and the enhancement of magnetospheric proton precipitations associated with geomagnetic disturbances, the TEC and electron density in the F region and in topside ionosphere/plasmasphere increase at low- and mid-latitudes due to an enhancement of atomic oxygen concentration. Our results demonstrate an important role of magnetospheric protons in the formation of negative F-region ionospheric storms. According to our results, the topside ionosphere/plasmasphere and bottom-side ionosphere can react to solar and magnetospheric protons both with the same sign of disturbances or in different way. The same statement is true for TEC and foF2 disturbances. Different disturbances of foF2 and TEC at high and low latitudes can be explained by topside electron temperature disturbances." @default.
• W3097674047 created "2020-11-09" @default.
• W3097674047 creator A5012934125 @default.
• W3097674047 creator A5027594355 @default.
• W3097674047 creator A5032548201 @default.
• W3097674047 creator A5038754822 @default.
• W3097674047 creator A5039260556 @default.
• W3097674047 creator A5048037725 @default.
• W3097674047 creator A5053914363 @default.
• W3097674047 creator A5056107742 @default.
• W3097674047 creator A5066814798 @default.
• W3097674047 date "2021-01-01" @default.
• W3097674047 modified "2023-09-27" @default.
• W3097674047 title "Ionospheric response to solar and magnetospheric protons during January 15–22, 2005: EAGLE whole atmosphere model results" @default.
• W3097674047 cites W1490807372 @default.
• W3097674047 cites W1830138900 @default.
• W3097674047 cites W1842825350 @default.
• W3097674047 cites W1875923372 @default.
• W3097674047 cites W1956162636 @default.
• W3097674047 cites W1964565573 @default.
• W3097674047 cites W1965893780 @default.
• W3097674047 cites W1970971613 @default.
• W3097674047 cites W1981840914 @default.
• W3097674047 cites W1983557014 @default.
• W3097674047 cites W1984627585 @default.
• W3097674047 cites W1990614090 @default.
• W3097674047 cites W1992215890 @default.
• W3097674047 cites W1992914118 @default.
• W3097674047 cites W1993458619 @default.
• W3097674047 cites W1998730290 @default.
• W3097674047 cites W2000766667 @default.
• W3097674047 cites W2001385006 @default.
• W3097674047 cites W2008381097 @default.
• W3097674047 cites W2015052435 @default.
• W3097674047 cites W2018665955 @default.
• W3097674047 cites W2028928817 @default.
• W3097674047 cites W2032395098 @default.
• W3097674047 cites W2043355057 @default.
• W3097674047 cites W2043553680 @default.
• W3097674047 cites W2045604722 @default.
• W3097674047 cites W2045957544 @default.
• W3097674047 cites W2047699542 @default.
• W3097674047 cites W2048276280 @default.
• W3097674047 cites W2052017234 @default.
• W3097674047 cites W2064333355 @default.
• W3097674047 cites W2072449921 @default.
• W3097674047 cites W2073121551 @default.
• W3097674047 cites W2079985720 @default.
• W3097674047 cites W2083548637 @default.
• W3097674047 cites W2090718018 @default.
• W3097674047 cites W2090855432 @default.
• W3097674047 cites W2098543448 @default.
• W3097674047 cites W2102870084 @default.
• W3097674047 cites W2107258400 @default.
• W3097674047 cites W2112615418 @default.
• W3097674047 cites W2120227873 @default.
• W3097674047 cites W2124715982 @default.
• W3097674047 cites W2126627645 @default.
• W3097674047 cites W2128158076 @default.
• W3097674047 cites W2138824764 @default.
• W3097674047 cites W2143663420 @default.
• W3097674047 cites W2151841146 @default.
• W3097674047 cites W2165223925 @default.
• W3097674047 cites W2169441385 @default.
• W3097674047 cites W2211878899 @default.
• W3097674047 cites W2212609344 @default.
• W3097674047 cites W2343069412 @default.
• W3097674047 cites W2601229246 @default.
• W3097674047 cites W2742658677 @default.
• W3097674047 cites W2758743206 @default.
• W3097674047 cites W2792164424 @default.
• W3097674047 cites W2794752868 @default.
• W3097674047 cites W2810588822 @default.
• W3097674047 cites W2946805808 @default.
• W3097674047 cites W2955900571 @default.
• W3097674047 cites W2989617868 @default.
• W3097674047 cites W3121721952 @default.
• W3097674047 cites W4233845421 @default.
• W3097674047 cites W4248775868 @default.
• W3097674047 cites W4252102052 @default.
• W3097674047 cites W2793295700 @default.
• W3097674047 doi "https://doi.org/10.1016/j.asr.2020.10.026" @default.
• W3097674047 hasPublicationYear "2021" @default.
• W3097674047 type Work @default.
• W3097674047 sameAs 3097674047 @default.
• W3097674047 citedByCount "6" @default.
• W3097674047 countsByYear W30976740472021 @default.
• W3097674047 countsByYear W30976740472022 @default.
• W3097674047 countsByYear W30976740472023 @default.
• W3097674047 crossrefType "journal-article" @default.
• W3097674047 hasAuthorship W3097674047A5012934125 @default.
• W3097674047 hasAuthorship W3097674047A5027594355 @default.
• W3097674047 hasAuthorship W3097674047A5032548201 @default.
• W3097674047 hasAuthorship W3097674047A5038754822 @default.
• W3097674047 hasAuthorship W3097674047A5039260556 @default.
• W3097674047 hasAuthorship W3097674047A5048037725 @default.
• W3097674047 hasAuthorship W3097674047A5053914363 @default.
• W3097674047 hasAuthorship W3097674047A5056107742 @default.

• next