FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1712846871> ?p ?o ?g. }

• W1712846871 endingPage "n/a" @default.
• W1712846871 startingPage "n/a" @default.
• W1712846871 abstract "[1] The ionization and excitation of atoms and molecules in the upper atmospheres of the Earth and planets are computed by a number of physical models. From these calculations, quantities measurable by dedicated satellite experiments such as airglow and electron fluxes can be derived. It is then possible to compare model and observation to derive more fundamental physical properties of the upper atmospheres, for example, the density as a function of altitude. To ensure the accuracy of these retrieval techniques, it is important to have an estimation of the uncertainty of these models and to have ways to account for these uncertainties. The complexity of kinetic models for computing the secondary production of excited state species (including ions) makes it a difficult evaluation, and studies usually neglect or underestimate it. We present here a Monte-Carlo approach to the computation of model uncertainties. As an example, we studied several aspects of the model uncertainties in the upper atmosphere of Mars, including the computed secondary electron flux and the production of the main ion species. Our simulations show the importance of improving solar flux models, especially on the energy binning and on the photon impact cross sections, which are the main sources of uncertainties on the dayside. The risk of modifying cross sections on the basis of aeronomical observations is highlighted for the case of Mars, while accurate uncertainties are shown to be crucial for the interpretation of data from the particle detectors onboard Mars Global Surveyor. Finally, it shows the importance of AtMoCiad, a public database dedicated to the evaluation of aeronomy cross section uncertainties. A detailed study of the resulting emissions cross sections uncertainties is the focus of a forthcoming paper (Gronoff et al., 2012) in which the outputs discussed in the present paper are used to compute airglow uncertainty, and the overall result is compared with the data from the SPICAM UV spectrometer onboard Mars Express." @default.
• W1712846871 created "2016-06-24" @default.
• W1712846871 creator A5031385192 @default.
• W1712846871 creator A5035062621 @default.
• W1712846871 creator A5036404345 @default.
• W1712846871 creator A5078848129 @default.
• W1712846871 date "2012-04-01" @default.
• W1712846871 modified "2023-10-08" @default.
• W1712846871 title "Computing uncertainties in ionosphere-airglow models: I. Electron flux and species production uncertainties for Mars" @default.
• W1712846871 cites W1526914239 @default.
• W1712846871 cites W1631211053 @default.
• W1712846871 cites W1963806811 @default.
• W1712846871 cites W1964399604 @default.
• W1712846871 cites W1975919625 @default.
• W1712846871 cites W1977435008 @default.
• W1712846871 cites W1978629252 @default.
• W1712846871 cites W1982965867 @default.
• W1712846871 cites W1987747075 @default.
• W1712846871 cites W1992276888 @default.
• W1712846871 cites W1992410455 @default.
• W1712846871 cites W1996330646 @default.
• W1712846871 cites W1996401378 @default.
• W1712846871 cites W2003399742 @default.
• W1712846871 cites W2006406420 @default.
• W1712846871 cites W2006844701 @default.
• W1712846871 cites W2007755532 @default.
• W1712846871 cites W2015333173 @default.
• W1712846871 cites W2016033843 @default.
• W1712846871 cites W2018805210 @default.
• W1712846871 cites W2022690643 @default.
• W1712846871 cites W2023546176 @default.
• W1712846871 cites W2025866983 @default.
• W1712846871 cites W2027671426 @default.
• W1712846871 cites W2029048346 @default.
• W1712846871 cites W2030261000 @default.
• W1712846871 cites W2036314405 @default.
• W1712846871 cites W2047039407 @default.
• W1712846871 cites W2054823429 @default.
• W1712846871 cites W2056787479 @default.
• W1712846871 cites W2057064827 @default.
• W1712846871 cites W2064181215 @default.
• W1712846871 cites W2067833884 @default.
• W1712846871 cites W2070259289 @default.
• W1712846871 cites W2075348910 @default.
• W1712846871 cites W2082742684 @default.
• W1712846871 cites W2089518253 @default.
• W1712846871 cites W2100153697 @default.
• W1712846871 cites W2113031116 @default.
• W1712846871 cites W2117474626 @default.
• W1712846871 cites W2132393892 @default.
• W1712846871 cites W2141161260 @default.
• W1712846871 cites W2154402469 @default.
• W1712846871 cites W2157506307 @default.
• W1712846871 cites W2165027382 @default.
• W1712846871 cites W3207975128 @default.
• W1712846871 doi "https://doi.org/10.1029/2011ja016930" @default.
• W1712846871 hasPublicationYear "2012" @default.
• W1712846871 type Work @default.
• W1712846871 sameAs 1712846871 @default.
• W1712846871 citedByCount "10" @default.
• W1712846871 countsByYear W17128468712012 @default.
• W1712846871 countsByYear W17128468712013 @default.
• W1712846871 countsByYear W17128468712014 @default.
• W1712846871 countsByYear W17128468712015 @default.
• W1712846871 countsByYear W17128468712016 @default.
• W1712846871 countsByYear W17128468712022 @default.
• W1712846871 crossrefType "journal-article" @default.
• W1712846871 hasAuthorship W1712846871A5031385192 @default.
• W1712846871 hasAuthorship W1712846871A5035062621 @default.
• W1712846871 hasAuthorship W1712846871A5036404345 @default.
• W1712846871 hasAuthorship W1712846871A5078848129 @default.
• W1712846871 hasBestOaLocation W17128468711 @default.
• W1712846871 hasConcept C105795698 @default.
• W1712846871 hasConcept C116403925 @default.
• W1712846871 hasConcept C121332964 @default.
• W1712846871 hasConcept C121864883 @default.
• W1712846871 hasConcept C145148216 @default.
• W1712846871 hasConcept C156034889 @default.
• W1712846871 hasConcept C19499675 @default.
• W1712846871 hasConcept C198291218 @default.
• W1712846871 hasConcept C30475298 @default.
• W1712846871 hasConcept C33923547 @default.
• W1712846871 hasConcept C39432304 @default.
• W1712846871 hasConcept C62520636 @default.
• W1712846871 hasConcept C8058405 @default.
• W1712846871 hasConcept C83260615 @default.
• W1712846871 hasConcept C87355193 @default.
• W1712846871 hasConcept C91586092 @default.
• W1712846871 hasConceptScore W1712846871C105795698 @default.
• W1712846871 hasConceptScore W1712846871C116403925 @default.
• W1712846871 hasConceptScore W1712846871C121332964 @default.
• W1712846871 hasConceptScore W1712846871C121864883 @default.
• W1712846871 hasConceptScore W1712846871C145148216 @default.
• W1712846871 hasConceptScore W1712846871C156034889 @default.
• W1712846871 hasConceptScore W1712846871C19499675 @default.
• W1712846871 hasConceptScore W1712846871C198291218 @default.
• W1712846871 hasConceptScore W1712846871C30475298 @default.
• W1712846871 hasConceptScore W1712846871C33923547 @default.

• next