FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1985166977> ?p ?o ?g. }

• W1985166977 abstract "[1] This study is concerned with the identification and description of a special subset of four Wind interplanetary rotational discontinuities (from an earlier study of 134 directional discontinuities by Lepping et al. (2003)) with some “extreme” characteristics, in the sense that every case has (1) an almost planar current sheet surface, (2) a very large discontinuity angle (ω), (3) at least moderately strong normal field components (>0.8 nT), and (4) the overall set has a very broad range of transition layer thicknesses, with one being as thick as 50 RE and another at the other extreme being 1.6 RE, most being much thicker than are usually studied. Each example has a well-determined surface normal (n) according to minimum variance analysis and corroborated via time delay checking of the discontinuity with observations at IMP 8 by employing the local surface planarity. From the variance analyses, most of these cases had unusually large ratios of intermediate-to-minimum eigenvalues (λI/λmin), being on average 32 for three cases (with a fourth being much larger), indicating compact current sheet transition zones, another (the fifth) extreme property. For many years there has been a controversy as to the relative distribution of rotational (RDs) to tangential discontinuities (TDs) in the solar wind at 1 AU (and elsewhere, such as between the Sun and Earth), even to the point where some authors have suggested that RDs with large ∣Bn∣s are probably not generated or, if generated, are unstable and therefore very rare. Some of this disagreement apparently has been due to the different selection criteria used, e.g., some allowed eigenvalue ratios (λI/λmin) to be almost an order of magnitude lower than 32 in estimating n, usually introducing unacceptable error in n and therefore also in ∣Bn∣. However, we suggest that RDs may not be so rare at 1 AU, but good quality cases (where ∣Bn∣ confidently exceeds the error in ∣Bn∣) appear to be uncommon, and further, cases of large ∣Bn∣ may indeed be rare. Finally, the issue of estimating the number of RDs-to-TDs was revisited using the full 134 events of the original Lepping et al. (2003) study (which utilized the RDs' propagation speeds for this estimation, an unconventional approach) but now by considering only normal field components, the more conventional approach. This resulted in slightly different conclusions, depending on specific assumptions used, making the unconventional approach suspect." @default.
• W1985166977 created "2016-06-24" @default.
• W1985166977 creator A5003625506 @default.
• W1985166977 creator A5018300832 @default.
• W1985166977 date "2005-01-01" @default.
• W1985166977 modified "2023-09-24" @default.
• W1985166977 title "Extreme interplanetary rotational discontinuities at 1 AU" @default.
• W1985166977 cites W1626012255 @default.
• W1985166977 cites W1634991999 @default.
• W1985166977 cites W1975764847 @default.
• W1985166977 cites W1978160524 @default.
• W1985166977 cites W1992286704 @default.
• W1985166977 cites W1998706063 @default.
• W1985166977 cites W1999788028 @default.
• W1985166977 cites W2017806331 @default.
• W1985166977 cites W2021314575 @default.
• W1985166977 cites W2024893532 @default.
• W1985166977 cites W2028977994 @default.
• W1985166977 cites W2031155710 @default.
• W1985166977 cites W2036453218 @default.
• W1985166977 cites W2037205331 @default.
• W1985166977 cites W2038527638 @default.
• W1985166977 cites W2056151613 @default.
• W1985166977 cites W2062264389 @default.
• W1985166977 cites W2070919551 @default.
• W1985166977 cites W2080060728 @default.
• W1985166977 cites W2087498478 @default.
• W1985166977 cites W2089354378 @default.
• W1985166977 cites W2097208940 @default.
• W1985166977 cites W2105889112 @default.
• W1985166977 cites W2131283943 @default.
• W1985166977 cites W2136602702 @default.
• W1985166977 cites W2162328719 @default.
• W1985166977 cites W2990635787 @default.
• W1985166977 cites W4255851711 @default.
• W1985166977 doi "https://doi.org/10.1029/2004ja010518" @default.
• W1985166977 hasPublicationYear "2005" @default.
• W1985166977 type Work @default.
• W1985166977 sameAs 1985166977 @default.
• W1985166977 citedByCount "1" @default.
• W1985166977 crossrefType "journal-article" @default.
• W1985166977 hasAuthorship W1985166977A5003625506 @default.
• W1985166977 hasAuthorship W1985166977A5018300832 @default.
• W1985166977 hasBestOaLocation W19851669771 @default.
• W1985166977 hasConcept C108411613 @default.
• W1985166977 hasConcept C114614502 @default.
• W1985166977 hasConcept C121332964 @default.
• W1985166977 hasConcept C127313418 @default.
• W1985166977 hasConcept C134306372 @default.
• W1985166977 hasConcept C15627037 @default.
• W1985166977 hasConcept C2777042112 @default.
• W1985166977 hasConcept C30475298 @default.
• W1985166977 hasConcept C33923547 @default.
• W1985166977 hasConcept C62520636 @default.
• W1985166977 hasConcept C68260962 @default.
• W1985166977 hasConcept C82706917 @default.
• W1985166977 hasConceptScore W1985166977C108411613 @default.
• W1985166977 hasConceptScore W1985166977C114614502 @default.
• W1985166977 hasConceptScore W1985166977C121332964 @default.
• W1985166977 hasConceptScore W1985166977C127313418 @default.
• W1985166977 hasConceptScore W1985166977C134306372 @default.
• W1985166977 hasConceptScore W1985166977C15627037 @default.
• W1985166977 hasConceptScore W1985166977C2777042112 @default.
• W1985166977 hasConceptScore W1985166977C30475298 @default.
• W1985166977 hasConceptScore W1985166977C33923547 @default.
• W1985166977 hasConceptScore W1985166977C62520636 @default.
• W1985166977 hasConceptScore W1985166977C68260962 @default.
• W1985166977 hasConceptScore W1985166977C82706917 @default.
• W1985166977 hasIssue "A11" @default.
• W1985166977 hasLocation W19851669771 @default.
• W1985166977 hasOpenAccess W1985166977 @default.
• W1985166977 hasPrimaryLocation W19851669771 @default.
• W1985166977 hasRelatedWork W2037205331 @default.
• W1985166977 hasRelatedWork W2135609211 @default.
• W1985166977 hasRelatedWork W2154970467 @default.
• W1985166977 hasRelatedWork W2163911608 @default.
• W1985166977 hasRelatedWork W2912044456 @default.
• W1985166977 hasRelatedWork W3001187027 @default.
• W1985166977 hasRelatedWork W3011567282 @default.
• W1985166977 hasRelatedWork W3039499377 @default.
• W1985166977 hasRelatedWork W3126645578 @default.
• W1985166977 hasRelatedWork W3178253643 @default.
• W1985166977 hasVolume "110" @default.
• W1985166977 isParatext "false" @default.
• W1985166977 isRetracted "false" @default.
• W1985166977 magId "1985166977" @default.
• W1985166977 workType "article" @default.