FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4200380507> ?p ?o ?g. }

• W4200380507 endingPage "A190" @default.
• W4200380507 startingPage "A190" @default.
• W4200380507 abstract "We derive a simple analytical model for the propagation of HSSs from the Sun to Earth and thereby show how the area of coronal holes and the size of their boundary regions affect the HSS velocity, temperature, and density near Earth. We presume that velocity, temperature, and density profiles form across the HSS cross section close to the Sun and that these spatial profiles translate into corresponding temporal profiles in a given radial direction due to the solar rotation. These temporal distributions drive the stream interface to the preceding slow solar wind plasma and disperse with distance from the Sun. The HSS properties at 1 AU are then given by all HSS plasma parcels launched from the Sun that did not run into the stream interface at Earth distance. We show that the velocity plateau region of HSSs as seen at 1 AU, if apparent, originates from the center region of the HSS close to the Sun, whereas the velocity tail at 1 AU originates from the trailing boundary region. The peak velocity of HSSs at Earth further depends on the longitudinal width of the HSS close to the Sun. The temperature and density of HSS plasma parcels at Earth depend on their radial expansion from the Sun to Earth. The radial expansion is determined by the velocity gradient across the HSS boundary region close to the Sun and gives the velocity-temperature and density-temperature relationships at Earth their specific shape. When considering a large number of HSSs, the presumed correlation between the HSS velocities and temperatures close to the Sun degrades only slightly up to 1 AU, but the correlation between the velocities and densities is strongly disrupted up to 1 AU due to the radial expansion. Finally, we show how the number of particles of the piled-up slow solar wind in the stream interaction region depends on the velocities and densities of the HSS and preceding slow solar wind plasma." @default.
• W4200380507 created "2021-12-31" @default.
• W4200380507 creator A5004382986 @default.
• W4200380507 creator A5014791457 @default.
• W4200380507 creator A5016592655 @default.
• W4200380507 creator A5016815182 @default.
• W4200380507 creator A5027717010 @default.
• W4200380507 creator A5028220931 @default.
• W4200380507 creator A5035170594 @default.
• W4200380507 creator A5035946004 @default.
• W4200380507 creator A5037708150 @default.
• W4200380507 creator A5042366978 @default.
• W4200380507 creator A5064964680 @default.
• W4200380507 creator A5065530713 @default.
• W4200380507 creator A5067147682 @default.
• W4200380507 date "2022-03-01" @default.
• W4200380507 modified "2023-10-13" @default.
• W4200380507 title "How the area of solar coronal holes affects the properties of high-speed solar wind streams near Earth: An analytical model" @default.
• W4200380507 cites W1557706148 @default.
• W4200380507 cites W1658904891 @default.
• W4200380507 cites W1979475923 @default.
• W4200380507 cites W1981927944 @default.
• W4200380507 cites W1997383614 @default.
• W4200380507 cites W2000763115 @default.
• W4200380507 cites W2001885164 @default.
• W4200380507 cites W2021584072 @default.
• W4200380507 cites W2037981626 @default.
• W4200380507 cites W2040746075 @default.
• W4200380507 cites W2045483269 @default.
• W4200380507 cites W2049440614 @default.
• W4200380507 cites W2067638142 @default.
• W4200380507 cites W2076622845 @default.
• W4200380507 cites W2080223350 @default.
• W4200380507 cites W2080568992 @default.
• W4200380507 cites W2095396013 @default.
• W4200380507 cites W2096411542 @default.
• W4200380507 cites W2100723408 @default.
• W4200380507 cites W2124202657 @default.
• W4200380507 cites W2164212757 @default.
• W4200380507 cites W2529561424 @default.
• W4200380507 cites W2810615273 @default.
• W4200380507 cites W2896549139 @default.
• W4200380507 cites W2954138483 @default.
• W4200380507 cites W2965791341 @default.
• W4200380507 cites W3091852361 @default.
• W4200380507 cites W3098866881 @default.
• W4200380507 cites W3099047318 @default.
• W4200380507 cites W3101550875 @default.
• W4200380507 cites W3104009810 @default.
• W4200380507 cites W3104436423 @default.
• W4200380507 cites W3105713965 @default.
• W4200380507 cites W3110813457 @default.
• W4200380507 cites W3125847058 @default.
• W4200380507 cites W4226419217 @default.
• W4200380507 cites W4288079687 @default.
• W4200380507 doi "https://doi.org/10.1051/0004-6361/202141919" @default.
• W4200380507 hasPublicationYear "2022" @default.
• W4200380507 type Work @default.
• W4200380507 citedByCount "7" @default.
• W4200380507 countsByYear W42003805072022 @default.
• W4200380507 countsByYear W42003805072023 @default.
• W4200380507 crossrefType "journal-article" @default.
• W4200380507 hasAuthorship W4200380507A5004382986 @default.
• W4200380507 hasAuthorship W4200380507A5014791457 @default.
• W4200380507 hasAuthorship W4200380507A5016592655 @default.
• W4200380507 hasAuthorship W4200380507A5016815182 @default.
• W4200380507 hasAuthorship W4200380507A5027717010 @default.
• W4200380507 hasAuthorship W4200380507A5028220931 @default.
• W4200380507 hasAuthorship W4200380507A5035170594 @default.
• W4200380507 hasAuthorship W4200380507A5035946004 @default.
• W4200380507 hasAuthorship W4200380507A5037708150 @default.
• W4200380507 hasAuthorship W4200380507A5042366978 @default.
• W4200380507 hasAuthorship W4200380507A5064964680 @default.
• W4200380507 hasAuthorship W4200380507A5065530713 @default.
• W4200380507 hasAuthorship W4200380507A5067147682 @default.
• W4200380507 hasBestOaLocation W42003805071 @default.
• W4200380507 hasConcept C108411613 @default.
• W4200380507 hasConcept C121332964 @default.
• W4200380507 hasConcept C150846664 @default.
• W4200380507 hasConcept C2524010 @default.
• W4200380507 hasConcept C30475298 @default.
• W4200380507 hasConcept C33923547 @default.
• W4200380507 hasConcept C41074950 @default.
• W4200380507 hasConcept C44870925 @default.
• W4200380507 hasConcept C62520636 @default.
• W4200380507 hasConcept C64162976 @default.
• W4200380507 hasConcept C72886185 @default.
• W4200380507 hasConcept C82706917 @default.
• W4200380507 hasConceptScore W4200380507C108411613 @default.
• W4200380507 hasConceptScore W4200380507C121332964 @default.
• W4200380507 hasConceptScore W4200380507C150846664 @default.
• W4200380507 hasConceptScore W4200380507C2524010 @default.
• W4200380507 hasConceptScore W4200380507C30475298 @default.
• W4200380507 hasConceptScore W4200380507C33923547 @default.
• W4200380507 hasConceptScore W4200380507C41074950 @default.
• W4200380507 hasConceptScore W4200380507C44870925 @default.
• W4200380507 hasConceptScore W4200380507C62520636 @default.
• W4200380507 hasConceptScore W4200380507C64162976 @default.

• next