FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2018221443> ?p ?o ?g. }

• W2018221443 endingPage "575" @default.
• W2018221443 startingPage "557" @default.
• W2018221443 abstract "New insight into the seasonal, diurnal and spatial distribution of water vapor on Mars has been obtained from analyzing the spectra of the short-wavelength channel (SW) of the Planetary Fourier Spectrometer (PFS) onboard Mars Express. The processed dataset, recorded between January 2004 and April 2005, covers the seasons from LS=331° of Mars Year 26 to LS=196° of the following year. In this period the mean column density around vernal equinox was 8.2 pr. μm. The maximum values during northern summer were about 65 pr. μm, located around 75° N latitude with a longitudinally inhomogeneous distribution. Regarding the atmospheric transport, the majority of polar water vapor remains in the north polar region while only about a quarter is transported southward. Geographically there are two water vapor maxima visible, over Arabia Terra and the Tharsis plateau, that are most likely caused both by atmosphere–ground interaction and by atmospheric circulation. A comparison with other instruments generally shows a good agreement, only the SPICAM results are systematically lower. Compared to the results from the PFS long-wavelength channel the results of this work are slightly higher. A strong discrepancy is visible northward of about 50° N during the northern summer that is possibly explained by a non-uniform vertical H2O mixing. In particular, a confinement of the water to the lower few kilometers yields a much better agreement between the retrieved column densities of the two PFS channels." @default.
• W2018221443 created "2016-06-24" @default.
• W2018221443 creator A5014959032 @default.
• W2018221443 creator A5024778716 @default.
• W2018221443 creator A5031414738 @default.
• W2018221443 creator A5037035926 @default.
• W2018221443 creator A5044704721 @default.
• W2018221443 creator A5065036871 @default.
• W2018221443 creator A5087028059 @default.
• W2018221443 date "2008-06-01" @default.
• W2018221443 modified "2023-10-11" @default.
• W2018221443 title "Investigation of water vapor on Mars with PFS/SW of Mars Express" @default.
• W2018221443 cites W1964268965 @default.
• W2018221443 cites W1969495672 @default.
• W2018221443 cites W1972485123 @default.
• W2018221443 cites W1974704539 @default.
• W2018221443 cites W1977827704 @default.
• W2018221443 cites W1983079246 @default.
• W2018221443 cites W1986449672 @default.
• W2018221443 cites W1996813864 @default.
• W2018221443 cites W2003148180 @default.
• W2018221443 cites W2011951131 @default.
• W2018221443 cites W2012452586 @default.
• W2018221443 cites W2013339212 @default.
• W2018221443 cites W2016052612 @default.
• W2018221443 cites W2017566741 @default.
• W2018221443 cites W2020396568 @default.
• W2018221443 cites W2027276225 @default.
• W2018221443 cites W2030938175 @default.
• W2018221443 cites W2040471242 @default.
• W2018221443 cites W2040992156 @default.
• W2018221443 cites W2052898648 @default.
• W2018221443 cites W2060731099 @default.
• W2018221443 cites W2066537922 @default.
• W2018221443 cites W2074893756 @default.
• W2018221443 cites W2076178834 @default.
• W2018221443 cites W2077543585 @default.
• W2018221443 cites W2082123320 @default.
• W2018221443 cites W2083438663 @default.
• W2018221443 cites W2085076608 @default.
• W2018221443 cites W2086893183 @default.
• W2018221443 cites W2090137411 @default.
• W2018221443 cites W2092960892 @default.
• W2018221443 cites W2120973061 @default.
• W2018221443 cites W2135594129 @default.
• W2018221443 cites W2146441174 @default.
• W2018221443 cites W2171020757 @default.
• W2018221443 cites W4211105962 @default.
• W2018221443 cites W4247175323 @default.
• W2018221443 doi "https://doi.org/10.1016/j.icarus.2008.01.018" @default.
• W2018221443 hasPublicationYear "2008" @default.
• W2018221443 type Work @default.
• W2018221443 sameAs 2018221443 @default.
• W2018221443 citedByCount "44" @default.
• W2018221443 countsByYear W20182214432012 @default.
• W2018221443 countsByYear W20182214432013 @default.
• W2018221443 countsByYear W20182214432014 @default.
• W2018221443 countsByYear W20182214432015 @default.
• W2018221443 countsByYear W20182214432016 @default.
• W2018221443 countsByYear W20182214432017 @default.
• W2018221443 countsByYear W20182214432018 @default.
• W2018221443 countsByYear W20182214432019 @default.
• W2018221443 countsByYear W20182214432021 @default.
• W2018221443 countsByYear W20182214432022 @default.
• W2018221443 crossrefType "journal-article" @default.
• W2018221443 hasAuthorship W2018221443A5014959032 @default.
• W2018221443 hasAuthorship W2018221443A5024778716 @default.
• W2018221443 hasAuthorship W2018221443A5031414738 @default.
• W2018221443 hasAuthorship W2018221443A5037035926 @default.
• W2018221443 hasAuthorship W2018221443A5044704721 @default.
• W2018221443 hasAuthorship W2018221443A5065036871 @default.
• W2018221443 hasAuthorship W2018221443A5087028059 @default.
• W2018221443 hasBestOaLocation W20182214432 @default.
• W2018221443 hasConcept C121332964 @default.
• W2018221443 hasConcept C122523270 @default.
• W2018221443 hasConcept C127313418 @default.
• W2018221443 hasConcept C13280743 @default.
• W2018221443 hasConcept C134306372 @default.
• W2018221443 hasConcept C134920139 @default.
• W2018221443 hasConcept C147534773 @default.
• W2018221443 hasConcept C153294291 @default.
• W2018221443 hasConcept C18459110 @default.
• W2018221443 hasConcept C2778600265 @default.
• W2018221443 hasConcept C2780030769 @default.
• W2018221443 hasConcept C33923547 @default.
• W2018221443 hasConcept C39432304 @default.
• W2018221443 hasConcept C45095769 @default.
• W2018221443 hasConcept C65440619 @default.
• W2018221443 hasConcept C83260615 @default.
• W2018221443 hasConcept C87355193 @default.
• W2018221443 hasConcept C91586092 @default.
• W2018221443 hasConceptScore W2018221443C121332964 @default.
• W2018221443 hasConceptScore W2018221443C122523270 @default.
• W2018221443 hasConceptScore W2018221443C127313418 @default.
• W2018221443 hasConceptScore W2018221443C13280743 @default.
• W2018221443 hasConceptScore W2018221443C134306372 @default.
• W2018221443 hasConceptScore W2018221443C134920139 @default.
• W2018221443 hasConceptScore W2018221443C147534773 @default.

• next