FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2025476977> ?p ?o ?g. }

• W2025476977 endingPage "n/a" @default.
• W2025476977 startingPage "n/a" @default.
• W2025476977 abstract "[1] One of the main sources of uncertainty in quantifying the kinematic properties of coronal mass ejections (CMEs) using coronagraphs is the fact that coronagraph images are projected into the sky plane, resulting in measurements which can differ significantly from their actual values. By identifying solar surface source regions of CMEs using X-ray and Hα flare and disappearing filament data, and through considerations of CME trajectories in three-dimensional (3-D) geometry, we have devised a methodology to correct for the projection effect. We outline this method here. The methodology was automated and applied to over 10,000 CMEs in the Coordinated Data Analysis Workshop (CDAW) (SOHO Large Angle Spectroscopic Coronagraph) catalog spanning 1996–2005, in which we could associate 1961 CMEs with an appropriate surface event. In the latter subset, deprojected speeds, accelerations, and launch angles were determined to study CME kinematics. Our analysis of this subset of events reconfirms some important trends, notably that previously uncovered solar cycle variation of CME properties are preserved, CMEs with greater width have higher speeds, and slower CMEs tend to accelerate while faster CMEs tend to decelerate. This points out that statistical trends in CME properties, recovered from plane-of-sky measurements, may be preserved even in the face of more sophisticated 3-D measurements from spacecrafts such as STEREO, if CME trajectories are predominantly radial. However, our results also show that the magnitude of corrected measurements can differ significantly from the projected plane-of-sky measurements on a case-by-case basis and that acceleration is more sensitive to the deprojection process than speed. Average corrected speed and acceleration tend to be a factor of 1.7 and 4.4 higher than their projected values, with mean corrected speed and acceleration magnitudes being on the order of 1000 km/s and 50 m/s2, respectively. We conclude that while using the plane-of-sky measurements may be suitable for studies of general trends in a large sample of events, correcting for projection effects is mandatory for those investigations which rely on a numerically precise determination of the properties of individual CMEs." @default.
• W2025476977 created "2016-06-24" @default.
• W2025476977 creator A5016418435 @default.
• W2025476977 creator A5055188681 @default.
• W2025476977 creator A5082269238 @default.
• W2025476977 date "2008-01-01" @default.
• W2025476977 modified "2023-10-09" @default.
• W2025476977 title "Kinematic properties of solar coronal mass ejections: Correction for projection effects in spacecraft coronagraph measurements" @default.
• W2025476977 cites W1970673104 @default.
• W2025476977 cites W1978301203 @default.
• W2025476977 cites W1985214372 @default.
• W2025476977 cites W1986214388 @default.
• W2025476977 cites W1994308416 @default.
• W2025476977 cites W2006958834 @default.
• W2025476977 cites W2013735155 @default.
• W2025476977 cites W2013909909 @default.
• W2025476977 cites W2018405851 @default.
• W2025476977 cites W2035843295 @default.
• W2025476977 cites W2043419218 @default.
• W2025476977 cites W2048452676 @default.
• W2025476977 cites W2050344634 @default.
• W2025476977 cites W2056311425 @default.
• W2025476977 cites W2056890589 @default.
• W2025476977 cites W2058113402 @default.
• W2025476977 cites W2076889914 @default.
• W2025476977 cites W2086893799 @default.
• W2025476977 cites W2102994651 @default.
• W2025476977 cites W2109481954 @default.
• W2025476977 cites W3167896805 @default.
• W2025476977 cites W4211063551 @default.
• W2025476977 doi "https://doi.org/10.1029/2007ja012500" @default.
• W2025476977 hasPublicationYear "2008" @default.
• W2025476977 type Work @default.
• W2025476977 sameAs 2025476977 @default.
• W2025476977 citedByCount "42" @default.
• W2025476977 countsByYear W20254769772012 @default.
• W2025476977 countsByYear W20254769772013 @default.
• W2025476977 countsByYear W20254769772014 @default.
• W2025476977 countsByYear W20254769772015 @default.
• W2025476977 countsByYear W20254769772016 @default.
• W2025476977 countsByYear W20254769772017 @default.
• W2025476977 countsByYear W20254769772018 @default.
• W2025476977 countsByYear W20254769772019 @default.
• W2025476977 countsByYear W20254769772020 @default.
• W2025476977 countsByYear W20254769772021 @default.
• W2025476977 countsByYear W20254769772022 @default.
• W2025476977 crossrefType "journal-article" @default.
• W2025476977 hasAuthorship W2025476977A5016418435 @default.
• W2025476977 hasAuthorship W2025476977A5055188681 @default.
• W2025476977 hasAuthorship W2025476977A5082269238 @default.
• W2025476977 hasBestOaLocation W20254769771 @default.
• W2025476977 hasConcept C108411613 @default.
• W2025476977 hasConcept C11413529 @default.
• W2025476977 hasConcept C115260700 @default.
• W2025476977 hasConcept C117896860 @default.
• W2025476977 hasConcept C121332964 @default.
• W2025476977 hasConcept C126691448 @default.
• W2025476977 hasConcept C1276947 @default.
• W2025476977 hasConcept C133286888 @default.
• W2025476977 hasConcept C163479331 @default.
• W2025476977 hasConcept C193145208 @default.
• W2025476977 hasConcept C29829512 @default.
• W2025476977 hasConcept C39920418 @default.
• W2025476977 hasConcept C41008148 @default.
• W2025476977 hasConcept C44870925 @default.
• W2025476977 hasConcept C51244244 @default.
• W2025476977 hasConcept C57493831 @default.
• W2025476977 hasConcept C62520636 @default.
• W2025476977 hasConcept C72886185 @default.
• W2025476977 hasConcept C73329638 @default.
• W2025476977 hasConcept C74650414 @default.
• W2025476977 hasConcept C82706917 @default.
• W2025476977 hasConceptScore W2025476977C108411613 @default.
• W2025476977 hasConceptScore W2025476977C11413529 @default.
• W2025476977 hasConceptScore W2025476977C115260700 @default.
• W2025476977 hasConceptScore W2025476977C117896860 @default.
• W2025476977 hasConceptScore W2025476977C121332964 @default.
• W2025476977 hasConceptScore W2025476977C126691448 @default.
• W2025476977 hasConceptScore W2025476977C1276947 @default.
• W2025476977 hasConceptScore W2025476977C133286888 @default.
• W2025476977 hasConceptScore W2025476977C163479331 @default.
• W2025476977 hasConceptScore W2025476977C193145208 @default.
• W2025476977 hasConceptScore W2025476977C29829512 @default.
• W2025476977 hasConceptScore W2025476977C39920418 @default.
• W2025476977 hasConceptScore W2025476977C41008148 @default.
• W2025476977 hasConceptScore W2025476977C44870925 @default.
• W2025476977 hasConceptScore W2025476977C51244244 @default.
• W2025476977 hasConceptScore W2025476977C57493831 @default.
• W2025476977 hasConceptScore W2025476977C62520636 @default.
• W2025476977 hasConceptScore W2025476977C72886185 @default.
• W2025476977 hasConceptScore W2025476977C73329638 @default.
• W2025476977 hasConceptScore W2025476977C74650414 @default.
• W2025476977 hasConceptScore W2025476977C82706917 @default.
• W2025476977 hasIssue "A1" @default.
• W2025476977 hasLocation W20254769771 @default.
• W2025476977 hasOpenAccess W2025476977 @default.
• W2025476977 hasPrimaryLocation W20254769771 @default.
• W2025476977 hasRelatedWork W1968056726 @default.

• next