SwePub
Sök i SwePub databas

  form:Ext_t

Träfflista för sökning "WFRF:(Johnson W. N.) ;lar1:(ltu)"

form:Search_simp_t: WFRF:(Johnson W. N.) > swepub_uni:Ltu_t

  • navigation:Result_t 1-2 navigation:of_t 2
hitlist:Modify_result_t
   
hitlist:Enumeration_thitlist:Reference_thitlist:Reference_picture_thitlist:Find_Mark_t
1.
  •  
2.
  • Lasue, J., et al. (creator_code:aut_t)
  • Martian Eolian Dust Probed by ChemCam
  • 2018
  • record:In_t: Geophysical Research Letters. - : John Wiley & Sons. - 0094-8276 .- 1944-8007. ; 45:20, s. 10968-10977
  • swepub:Mat_article_t (swepub:level_refereed_t)abstract
    • The ubiquitous eolian dust on Mars plays important roles in the current sedimentary and atmospheric processes of the planet. The ChemCam instrument retrieves a consistent eolian dust composition at the submillimeter scale from every first laser shot on Mars targets. Its composition presents significant differences with the Aeolis Palus soils and the Bagnold dunes as it contains lower CaO and higher SiO2. The dust FeO and TiO2contents are also higher, probably associated with nanophase oxide components. The dust spectra show the presence of volatile elements (S and Cl), and the hydrogen content is similar to Bagnold sands but lower than Aeolis Palus soils. Consequently, the dust may be a contributor to the amorphous component of soils, but differences in composition indicate that the two materials are not equivalent.
  •  
Skapa referenser, mejla, bekava och länka
  • navigation:Result_t 1-2 navigation:of_t 2

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt tools:Close_t

tools:Permalink_label_t