Matches in SemOpenAlex for { <https://semopenalex.org/work/W2891076087> ?p ?o ?g. }
- W2891076087 endingPage "49" @default.
- W2891076087 startingPage "49" @default.
- W2891076087 abstract "Following the derivation of a more accurate model of the evolution of the solar Lyman-$alpha$ line with the changing solar activity by Kowalska-leszczynska et al. 2018 (IKL18) than the formerly used model by Tarnopolski et al. 2009 (ST09), we investigate potential consequences that adoption of the resulting refined model of radiation pressure has for the model distribution of interstellar neutral (ISN) H in the inner heliosphere and on the interpretation of selected observations. We simulated the ISN H densities using the two alternative radiation pressure models and identical models of all other factors affecting the ISN H distribution. We found that during most of the solar cycle, the IKL18 model predicts larger densities of ISN H and PUIs than ST09 in the inner heliosphere, especially in the downwind hemisphere. However, the density of ISN H at the termination shock estimated by Bzowski et al. 2008 obtained using ST09 does not need revision, and the detection of ISN D by IBEX is supported. However, we point out the existence of a considerable absorption of a portion of the solar Lyman-$alpha$ spectral flux inside the heliosphere. Therefore, the model of radiation pressure for ISN H is still likely to need revision, and hence the available models of ISN H are not self-consistent." @default.
- W2891076087 created "2018-09-27" @default.
- W2891076087 creator A5001252122 @default.
- W2891076087 creator A5007887074 @default.
- W2891076087 creator A5009584506 @default.
- W2891076087 creator A5070696742 @default.
- W2891076087 date "2018-11-19" @default.
- W2891076087 modified "2023-10-16" @default.
- W2891076087 title "Evolution of the Solar Ly<i>α</i> Line Profile during the Solar Cycle. II. How Accurate Is the Present Radiation Pressure Paradigm for Interstellar Neutral H in the Heliosphere?" @default.
- W2891076087 cites W1594862810 @default.
- W2891076087 cites W1670546161 @default.
- W2891076087 cites W1891250076 @default.
- W2891076087 cites W1898740785 @default.
- W2891076087 cites W1964394311 @default.
- W2891076087 cites W1970731804 @default.
- W2891076087 cites W1971188011 @default.
- W2891076087 cites W1971582378 @default.
- W2891076087 cites W1990266150 @default.
- W2891076087 cites W1990420403 @default.
- W2891076087 cites W1999417414 @default.
- W2891076087 cites W2000264375 @default.
- W2891076087 cites W2003836651 @default.
- W2891076087 cites W2016165875 @default.
- W2891076087 cites W2019303882 @default.
- W2891076087 cites W2027924553 @default.
- W2891076087 cites W2038395475 @default.
- W2891076087 cites W2040122111 @default.
- W2891076087 cites W2051239539 @default.
- W2891076087 cites W2052974749 @default.
- W2891076087 cites W2068654390 @default.
- W2891076087 cites W2100815884 @default.
- W2891076087 cites W2107504732 @default.
- W2891076087 cites W2110875666 @default.
- W2891076087 cites W2111996542 @default.
- W2891076087 cites W2116042083 @default.
- W2891076087 cites W2129690380 @default.
- W2891076087 cites W2134106600 @default.
- W2891076087 cites W2136298014 @default.
- W2891076087 cites W2155793055 @default.
- W2891076087 cites W2164500104 @default.
- W2891076087 cites W2166633024 @default.
- W2891076087 cites W2167397422 @default.
- W2891076087 cites W2227979387 @default.
- W2891076087 cites W2258268298 @default.
- W2891076087 cites W2275834326 @default.
- W2891076087 cites W2325584210 @default.
- W2891076087 cites W2517970846 @default.
- W2891076087 cites W2527134057 @default.
- W2891076087 cites W2531151841 @default.
- W2891076087 cites W2545414232 @default.
- W2891076087 cites W2563639658 @default.
- W2891076087 cites W2765697619 @default.
- W2891076087 cites W3098541241 @default.
- W2891076087 cites W3098755985 @default.
- W2891076087 cites W3099342373 @default.
- W2891076087 cites W3102467280 @default.
- W2891076087 cites W3102644927 @default.
- W2891076087 cites W3103833839 @default.
- W2891076087 cites W3103835246 @default.
- W2891076087 cites W3104111100 @default.
- W2891076087 cites W3104178917 @default.
- W2891076087 cites W3104812597 @default.
- W2891076087 cites W3105081052 @default.
- W2891076087 cites W3105333631 @default.
- W2891076087 doi "https://doi.org/10.3847/1538-4357/aae70b" @default.
- W2891076087 hasPublicationYear "2018" @default.
- W2891076087 type Work @default.
- W2891076087 sameAs 2891076087 @default.
- W2891076087 citedByCount "22" @default.
- W2891076087 countsByYear W28910760872019 @default.
- W2891076087 countsByYear W28910760872020 @default.
- W2891076087 countsByYear W28910760872021 @default.
- W2891076087 countsByYear W28910760872022 @default.
- W2891076087 countsByYear W28910760872023 @default.
- W2891076087 crossrefType "journal-article" @default.
- W2891076087 hasAuthorship W2891076087A5001252122 @default.
- W2891076087 hasAuthorship W2891076087A5007887074 @default.
- W2891076087 hasAuthorship W2891076087A5009584506 @default.
- W2891076087 hasAuthorship W2891076087A5070696742 @default.
- W2891076087 hasBestOaLocation W28910760871 @default.
- W2891076087 hasConcept C108411613 @default.
- W2891076087 hasConcept C120665830 @default.
- W2891076087 hasConcept C121332964 @default.
- W2891076087 hasConcept C1276947 @default.
- W2891076087 hasConcept C138560296 @default.
- W2891076087 hasConcept C153385146 @default.
- W2891076087 hasConcept C196939603 @default.
- W2891076087 hasConcept C43867161 @default.
- W2891076087 hasConcept C44870925 @default.
- W2891076087 hasConcept C54834619 @default.
- W2891076087 hasConcept C62520636 @default.
- W2891076087 hasConcept C68337447 @default.
- W2891076087 hasConcept C82706917 @default.
- W2891076087 hasConcept C98444146 @default.
- W2891076087 hasConceptScore W2891076087C108411613 @default.
- W2891076087 hasConceptScore W2891076087C120665830 @default.
- W2891076087 hasConceptScore W2891076087C121332964 @default.
- W2891076087 hasConceptScore W2891076087C1276947 @default.