Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100545818> ?p ?o ?g. }
- W3100545818 endingPage "1688" @default.
- W3100545818 startingPage "1679" @default.
- W3100545818 abstract "Many studies of the Loop I magnetic superbubble place the Sun at the edges of the bubble. One recent study models the polarized radio continuum of Loop I as two magnetic shells with the Sun embedded in the rim of the S1 shell. If the Sun is in such a shell, it should be apparent in both the local interstellar magnetic field and the distribution of nearby interstellar material. The properties of these subshells are compared to the interstellar magnetic field and the distribution of interstellar Fe+ and Ca+ within ∼55 pc of the Sun. Although the results are not conclusive, the interstellar magnetic field direction obtained from polarized stars within ∼30 pc is consistent with the interstellar magnetic field direction of the S1 shell. The distribution of nearby interstellar Fe+ with log N(Fe+) < 12.5 cm−2 is described equally well by a uniform distribution or an origin in spherical shell-like features. Higher column densities of Fe+ (log N(Fe+)>12.5 cm−2) tend to be better described by the path length of the sightline through the S1 and S2 subshells. Column densities of the recombinant ion Ca+ are found to increase with the strength of the interstellar radiation field, rather than with star distance or total pathlength through the two magnetic subshells. The ion Ca+ cannot be used to trace the distribution of local interstellar gas unless the spatial variations in the radiation field are included in the calculation of the ionization balance, in addition to possible abundance variations. The result is that a model of Loop I as composed of two spherical magnetic subshells remains a viable description of the distribution of nearby low density interstellar medium, but is not yet proven." @default.
- W3100545818 created "2020-11-23" @default.
- W3100545818 creator A5064620659 @default.
- W3100545818 date "2010-04-22" @default.
- W3100545818 modified "2023-09-25" @default.
- W3100545818 title "THE S1 SHELL AND INTERSTELLAR MAGNETIC FIELD AND GAS NEAR THE HELIOSPHERE" @default.
- W3100545818 cites W1571949045 @default.
- W3100545818 cites W1966786356 @default.
- W3100545818 cites W1970860842 @default.
- W3100545818 cites W1972766402 @default.
- W3100545818 cites W1975572109 @default.
- W3100545818 cites W1980891956 @default.
- W3100545818 cites W1987603205 @default.
- W3100545818 cites W1988213367 @default.
- W3100545818 cites W1997558661 @default.
- W3100545818 cites W1999417414 @default.
- W3100545818 cites W2008837559 @default.
- W3100545818 cites W2011543926 @default.
- W3100545818 cites W2012220297 @default.
- W3100545818 cites W2014144733 @default.
- W3100545818 cites W2020719413 @default.
- W3100545818 cites W2030302906 @default.
- W3100545818 cites W2032806516 @default.
- W3100545818 cites W2036200883 @default.
- W3100545818 cites W2037170534 @default.
- W3100545818 cites W2046876515 @default.
- W3100545818 cites W2047798490 @default.
- W3100545818 cites W2049975802 @default.
- W3100545818 cites W2050012434 @default.
- W3100545818 cites W2051029254 @default.
- W3100545818 cites W2066257068 @default.
- W3100545818 cites W2071125642 @default.
- W3100545818 cites W2079400690 @default.
- W3100545818 cites W2079799652 @default.
- W3100545818 cites W2082272630 @default.
- W3100545818 cites W2082740167 @default.
- W3100545818 cites W2086826787 @default.
- W3100545818 cites W2088450475 @default.
- W3100545818 cites W2095534601 @default.
- W3100545818 cites W2099236038 @default.
- W3100545818 cites W2111617466 @default.
- W3100545818 cites W2143847916 @default.
- W3100545818 cites W2951458773 @default.
- W3100545818 cites W3098003749 @default.
- W3100545818 cites W3098685927 @default.
- W3100545818 cites W3098861760 @default.
- W3100545818 cites W3098992670 @default.
- W3100545818 cites W3100780402 @default.
- W3100545818 cites W3102207702 @default.
- W3100545818 cites W3103216464 @default.
- W3100545818 cites W3103355245 @default.
- W3100545818 cites W3103512617 @default.
- W3100545818 cites W3106006618 @default.
- W3100545818 cites W3122499570 @default.
- W3100545818 cites W3203341223 @default.
- W3100545818 cites W4238358225 @default.
- W3100545818 doi "https://doi.org/10.1088/0004-637x/714/2/1679" @default.
- W3100545818 hasPublicationYear "2010" @default.
- W3100545818 type Work @default.
- W3100545818 sameAs 3100545818 @default.
- W3100545818 citedByCount "19" @default.
- W3100545818 countsByYear W31005458182012 @default.
- W3100545818 countsByYear W31005458182013 @default.
- W3100545818 countsByYear W31005458182014 @default.
- W3100545818 countsByYear W31005458182015 @default.
- W3100545818 countsByYear W31005458182016 @default.
- W3100545818 countsByYear W31005458182017 @default.
- W3100545818 countsByYear W31005458182022 @default.
- W3100545818 crossrefType "journal-article" @default.
- W3100545818 hasAuthorship W3100545818A5064620659 @default.
- W3100545818 hasBestOaLocation W31005458181 @default.
- W3100545818 hasConcept C108411613 @default.
- W3100545818 hasConcept C115260700 @default.
- W3100545818 hasConcept C121332964 @default.
- W3100545818 hasConcept C145148216 @default.
- W3100545818 hasConcept C150846664 @default.
- W3100545818 hasConcept C151465644 @default.
- W3100545818 hasConcept C172809573 @default.
- W3100545818 hasConcept C190895841 @default.
- W3100545818 hasConcept C196939603 @default.
- W3100545818 hasConcept C198291218 @default.
- W3100545818 hasConcept C199635899 @default.
- W3100545818 hasConcept C2776073818 @default.
- W3100545818 hasConcept C44870925 @default.
- W3100545818 hasConcept C54834619 @default.
- W3100545818 hasConcept C62520636 @default.
- W3100545818 hasConcept C98444146 @default.
- W3100545818 hasConceptScore W3100545818C108411613 @default.
- W3100545818 hasConceptScore W3100545818C115260700 @default.
- W3100545818 hasConceptScore W3100545818C121332964 @default.
- W3100545818 hasConceptScore W3100545818C145148216 @default.
- W3100545818 hasConceptScore W3100545818C150846664 @default.
- W3100545818 hasConceptScore W3100545818C151465644 @default.
- W3100545818 hasConceptScore W3100545818C172809573 @default.
- W3100545818 hasConceptScore W3100545818C190895841 @default.
- W3100545818 hasConceptScore W3100545818C196939603 @default.
- W3100545818 hasConceptScore W3100545818C198291218 @default.
- W3100545818 hasConceptScore W3100545818C199635899 @default.