FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1985280677> ?p ?o ?g. }

• W1985280677 endingPage "29567" @default.
• W1985280677 startingPage "29551" @default.
• W1985280677 abstract "The first ever fully three-dimensional magnetohydrodynamic (MHD) simulations of the detailed effects of MHD discontinuities on the magnetosheath have been performed. The simulation results predict that the interaction between a rotational discontinuity (RD) and the bow shock produces an MHD wave pulse that propagates downstream from the bow shock to the magnetopause. The main components of this pulse are two slow shocks sandwiched between two time-dependent intermediate shocks; in perfectly ideal MHD, these shocks would presumably resolve into slow shocks sandwiched between two RDs. Inside the pulse, the plasma density, thermal pressure, dynamic pressure (ρυ2), and total pressure all increase, while the magnetic field magnitude decreases. The pulse convects with the downstream flow through the magnetosheath at a speed that is markedly slower than that of the original RD. It comes to rest on the magnetopause, where it raises the total pressure by as much as 75% in some locations. The pulse eventually disappears, as it is convected away by the solar wind flow around the magnetopause. The pulse remains in the magnetosheath for a few Alfvén times (i.e., solar wind Alfvén velocity divided by the Earth's radius, perhaps 1–3 min depending on the actual solar wind parameters) after the initial RD has propagated downstream past the magnetopause. Comparisons are made with previous one-dimensional and two-dimensional studies of this problem. We conclude that the pulses seen in these simulations are possible causes of magnetic impulse events observed in the ionosphere and slow mode structures observed in the inner subsolar magnetosheath." @default.
• W1985280677 created "2016-06-24" @default.
• W1985280677 creator A5022737945 @default.
• W1985280677 creator A5059768204 @default.
• W1985280677 date "1998-12-01" @default.
• W1985280677 modified "2023-09-24" @default.
• W1985280677 title "Three-dimensional MHD simulations of interplanetary rotational discontinuities impacting the Earth's bow shock and magnetosheath" @default.
• W1985280677 cites W1609920523 @default.
• W1985280677 cites W1966921113 @default.
• W1985280677 cites W1972126583 @default.
• W1985280677 cites W1973618634 @default.
• W1985280677 cites W1982219419 @default.
• W1985280677 cites W1982765652 @default.
• W1985280677 cites W1996691170 @default.
• W1985280677 cites W2001768624 @default.
• W1985280677 cites W2005466934 @default.
• W1985280677 cites W2008236329 @default.
• W1985280677 cites W2014123079 @default.
• W1985280677 cites W2016958337 @default.
• W1985280677 cites W2017912972 @default.
• W1985280677 cites W2025325976 @default.
• W1985280677 cites W2026229679 @default.
• W1985280677 cites W2026699650 @default.
• W1985280677 cites W2044605417 @default.
• W1985280677 cites W2051250938 @default.
• W1985280677 cites W2068235963 @default.
• W1985280677 cites W2070099050 @default.
• W1985280677 cites W2087584307 @default.
• W1985280677 cites W2089354378 @default.
• W1985280677 cites W2101422669 @default.
• W1985280677 cites W2115814208 @default.
• W1985280677 cites W2116702074 @default.
• W1985280677 cites W2120102917 @default.
• W1985280677 cites W2145258266 @default.
• W1985280677 cites W4246315662 @default.
• W1985280677 doi "https://doi.org/10.1029/1998ja900025" @default.
• W1985280677 hasPublicationYear "1998" @default.
• W1985280677 type Work @default.
• W1985280677 sameAs 1985280677 @default.
• W1985280677 citedByCount "26" @default.
• W1985280677 countsByYear W19852806772012 @default.
• W1985280677 countsByYear W19852806772021 @default.
• W1985280677 countsByYear W19852806772022 @default.
• W1985280677 crossrefType "journal-article" @default.
• W1985280677 hasAuthorship W1985280677A5022737945 @default.
• W1985280677 hasAuthorship W1985280677A5059768204 @default.
• W1985280677 hasBestOaLocation W19852806771 @default.
• W1985280677 hasConcept C108411613 @default.
• W1985280677 hasConcept C115260700 @default.
• W1985280677 hasConcept C121332964 @default.
• W1985280677 hasConcept C130443932 @default.
• W1985280677 hasConcept C140161248 @default.
• W1985280677 hasConcept C155991500 @default.
• W1985280677 hasConcept C172860338 @default.
• W1985280677 hasConcept C30475298 @default.
• W1985280677 hasConcept C31532427 @default.
• W1985280677 hasConcept C32546565 @default.
• W1985280677 hasConcept C33643480 @default.
• W1985280677 hasConcept C44870925 @default.
• W1985280677 hasConcept C57879066 @default.
• W1985280677 hasConcept C61922881 @default.
• W1985280677 hasConcept C62520636 @default.
• W1985280677 hasConcept C70477161 @default.
• W1985280677 hasConcept C8058405 @default.
• W1985280677 hasConceptScore W1985280677C108411613 @default.
• W1985280677 hasConceptScore W1985280677C115260700 @default.
• W1985280677 hasConceptScore W1985280677C121332964 @default.
• W1985280677 hasConceptScore W1985280677C130443932 @default.
• W1985280677 hasConceptScore W1985280677C140161248 @default.
• W1985280677 hasConceptScore W1985280677C155991500 @default.
• W1985280677 hasConceptScore W1985280677C172860338 @default.
• W1985280677 hasConceptScore W1985280677C30475298 @default.
• W1985280677 hasConceptScore W1985280677C31532427 @default.
• W1985280677 hasConceptScore W1985280677C32546565 @default.
• W1985280677 hasConceptScore W1985280677C33643480 @default.
• W1985280677 hasConceptScore W1985280677C44870925 @default.
• W1985280677 hasConceptScore W1985280677C57879066 @default.
• W1985280677 hasConceptScore W1985280677C61922881 @default.
• W1985280677 hasConceptScore W1985280677C62520636 @default.
• W1985280677 hasConceptScore W1985280677C70477161 @default.
• W1985280677 hasConceptScore W1985280677C8058405 @default.
• W1985280677 hasIssue "A12" @default.
• W1985280677 hasLocation W19852806771 @default.
• W1985280677 hasOpenAccess W1985280677 @default.
• W1985280677 hasPrimaryLocation W19852806771 @default.
• W1985280677 hasRelatedWork W1632707852 @default.
• W1985280677 hasRelatedWork W2007128499 @default.
• W1985280677 hasRelatedWork W2023460744 @default.
• W1985280677 hasRelatedWork W2028153831 @default.
• W1985280677 hasRelatedWork W2054990668 @default.
• W1985280677 hasRelatedWork W2079210884 @default.
• W1985280677 hasRelatedWork W2093508016 @default.
• W1985280677 hasRelatedWork W210355118 @default.
• W1985280677 hasRelatedWork W3157085511 @default.
• W1985280677 hasRelatedWork W994179962 @default.
• W1985280677 hasVolume "103" @default.
• W1985280677 isParatext "false" @default.
• W1985280677 isRetracted "false" @default.

• next