Matches in SemOpenAlex for { <https://semopenalex.org/work/W3124938325> ?p ?o ?g. }
- W3124938325 endingPage "169" @default.
- W3124938325 startingPage "169" @default.
- W3124938325 abstract "Connecting in-situ measured solar-wind plasma properties with typical regions on the Sun can provide an effective constraint and test to various solar wind models. We examine the statistical characteristics of the solar wind with an origin in different types of source regions. We find that the speed distribution of coronal hole (CH) wind is bimodal with the slow wind peaking at ~400 km/s and a fast at ~600 km/s. An anti-correlation between the solar wind speeds and the O7+/O6+ ion ratio remains valid in all three types of solar wind as well during the three studied solar cycle activity phases, i.e. solar maximum, decline and minimum. The N_Fe/N_O range and its average values all decrease with the increasing solar wind speed in different types of solar wind. The N_Fe/N_O range (0.06-0.40, FIP bias range 1-7) for AR wind is wider than for CH wind (0.06-0.20, FIP bias range 1-3) while the minimum value of N_Fe/N_O (0.06) does not change with the variation of speed, and it is similar for all sourceregions. The two-peak distribution of CH wind and the anti-correlation between the speed and O7+/O6+ in all three types of solar wind can be explained qualitatively by both the wave-turbulence-driven (WTD) and reconnection-loop-opening (RLO) models, whereas the distribution features of N_Fe/N_O in different source regions of solar wind can be explained more reasonably by the RLO models." @default.
- W3124938325 created "2021-02-01" @default.
- W3124938325 creator A5040036303 @default.
- W3124938325 creator A5047803811 @default.
- W3124938325 creator A5051839986 @default.
- W3124938325 creator A5062562320 @default.
- W3124938325 creator A5066133781 @default.
- W3124938325 creator A5090292495 @default.
- W3124938325 date "2017-02-17" @default.
- W3124938325 modified "2023-09-27" @default.
- W3124938325 title "Charge States and FIP Bias of the Solar Wind from Coronal Holes, Active Regions, and Quiet Sun" @default.
- W3124938325 cites W1484030292 @default.
- W3124938325 cites W1487280089 @default.
- W3124938325 cites W1628830896 @default.
- W3124938325 cites W1968072462 @default.
- W3124938325 cites W1969080773 @default.
- W3124938325 cites W1971603863 @default.
- W3124938325 cites W1976352369 @default.
- W3124938325 cites W1976456772 @default.
- W3124938325 cites W1977620253 @default.
- W3124938325 cites W1979831896 @default.
- W3124938325 cites W1985238204 @default.
- W3124938325 cites W1993163546 @default.
- W3124938325 cites W1995430462 @default.
- W3124938325 cites W1998577440 @default.
- W3124938325 cites W2002642641 @default.
- W3124938325 cites W2005652611 @default.
- W3124938325 cites W2012858076 @default.
- W3124938325 cites W2013135325 @default.
- W3124938325 cites W2029326078 @default.
- W3124938325 cites W2031079080 @default.
- W3124938325 cites W2031714062 @default.
- W3124938325 cites W2032795093 @default.
- W3124938325 cites W2032977025 @default.
- W3124938325 cites W2037981626 @default.
- W3124938325 cites W2038674983 @default.
- W3124938325 cites W2043968417 @default.
- W3124938325 cites W2044489048 @default.
- W3124938325 cites W2053274638 @default.
- W3124938325 cites W2056135380 @default.
- W3124938325 cites W2057180224 @default.
- W3124938325 cites W2058768995 @default.
- W3124938325 cites W2060142157 @default.
- W3124938325 cites W2060283668 @default.
- W3124938325 cites W2060756091 @default.
- W3124938325 cites W2063154175 @default.
- W3124938325 cites W2063259496 @default.
- W3124938325 cites W2070423545 @default.
- W3124938325 cites W2071154966 @default.
- W3124938325 cites W2073937826 @default.
- W3124938325 cites W2075147663 @default.
- W3124938325 cites W2077529393 @default.
- W3124938325 cites W2080885950 @default.
- W3124938325 cites W2091317050 @default.
- W3124938325 cites W2094245529 @default.
- W3124938325 cites W2109145288 @default.
- W3124938325 cites W2110370705 @default.
- W3124938325 cites W2114510274 @default.
- W3124938325 cites W2130623925 @default.
- W3124938325 cites W2139980067 @default.
- W3124938325 cites W2157461267 @default.
- W3124938325 cites W2158692711 @default.
- W3124938325 cites W2465941559 @default.
- W3124938325 cites W2899497983 @default.
- W3124938325 cites W3038099711 @default.
- W3124938325 cites W3098141724 @default.
- W3124938325 cites W3099420272 @default.
- W3124938325 cites W3099700090 @default.
- W3124938325 cites W3099782431 @default.
- W3124938325 cites W3102745897 @default.
- W3124938325 cites W3104164378 @default.
- W3124938325 cites W3104913842 @default.
- W3124938325 cites W3105381298 @default.
- W3124938325 cites W3105794360 @default.
- W3124938325 cites W3177773949 @default.
- W3124938325 cites W4245192593 @default.
- W3124938325 cites W4250828756 @default.
- W3124938325 cites W4298270558 @default.
- W3124938325 doi "https://doi.org/10.3847/1538-4357/aa5cba" @default.
- W3124938325 hasPublicationYear "2017" @default.
- W3124938325 type Work @default.
- W3124938325 sameAs 3124938325 @default.
- W3124938325 citedByCount "26" @default.
- W3124938325 countsByYear W31249383252017 @default.
- W3124938325 countsByYear W31249383252018 @default.
- W3124938325 countsByYear W31249383252019 @default.
- W3124938325 countsByYear W31249383252020 @default.
- W3124938325 countsByYear W31249383252021 @default.
- W3124938325 countsByYear W31249383252022 @default.
- W3124938325 countsByYear W31249383252023 @default.
- W3124938325 crossrefType "journal-article" @default.
- W3124938325 hasAuthorship W3124938325A5040036303 @default.
- W3124938325 hasAuthorship W3124938325A5047803811 @default.
- W3124938325 hasAuthorship W3124938325A5051839986 @default.
- W3124938325 hasAuthorship W3124938325A5062562320 @default.
- W3124938325 hasAuthorship W3124938325A5066133781 @default.
- W3124938325 hasAuthorship W3124938325A5090292495 @default.
- W3124938325 hasBestOaLocation W31249383251 @default.