Matches in SemOpenAlex for { <https://semopenalex.org/work/W3146537805> ?p ?o ?g. }
Showing items 1 to 65 of
65
with 100 items per page.
- W3146537805 abstract "The effect of the Martian crustal magnetic field is one of the hot topics of the study of Martian ionosphere.The studies on this topic are summarized in this paper.Main data of the Martian ionosphere were resulted from radio occultation experiments.According to the observations,the electron density scale height and the peak electron density of the Martian ionosphere are influenced by its crustal magnetic field.The strong horizontal magnetic field prevents the vertical diffusion of the plasma and makes the electron density scale height in the topside ionosphere close to that in the photo equilibrium region.In the cusp-like regions with strong vertical magnetic field,the enhanced vertical diffusion leads to a larger electron density scale height in the diffusion equilibrium region.The observation of radio occultation experiment onboard Mars Global Surveyor (MGS) showed that the averaged peak electron density observed in the southern hemisphere with strong crustal magnetic field was slightly larger than that in the northern hemisphere with weak crustal magnetic field.The Mars advanced radar for subsurface and ionosphere sounding (MARSIS) onboard Mars Express (MEX) was the first topside sounder to be used to observe Martian ionosphere.The MARSIS results confirmed that the enhancement of the peak electron density occurred in cusp-like regions with open field lines,and the amount of the enhancement was much larger than that observed by the radio occultation experiment.There are two possible mechanisms for the peak electron density enhancement in the cusp-like crustal magnetic field regions:One is the precipitation of the energetic particles and the other is the heating by the waves excited by plasma instabilities.It's difficult to determine which one is the key mechanism for the peak electron density enhancement.Based on these studies,several interesting problems on the Martian ionosphere and plasma environment are presented." @default.
- W3146537805 created "2021-04-13" @default.
- W3146537805 creator A5025639588 @default.
- W3146537805 date "2010-01-01" @default.
- W3146537805 modified "2023-09-28" @default.
- W3146537805 title "Effects of Martian crustal magnetic field on its ionosphere" @default.
- W3146537805 hasPublicationYear "2010" @default.
- W3146537805 type Work @default.
- W3146537805 sameAs 3146537805 @default.
- W3146537805 citedByCount "0" @default.
- W3146537805 crossrefType "journal-article" @default.
- W3146537805 hasAuthorship W3146537805A5025639588 @default.
- W3146537805 hasConcept C115260700 @default.
- W3146537805 hasConcept C116403925 @default.
- W3146537805 hasConcept C121332964 @default.
- W3146537805 hasConcept C125485243 @default.
- W3146537805 hasConcept C127313418 @default.
- W3146537805 hasConcept C147120987 @default.
- W3146537805 hasConcept C199635899 @default.
- W3146537805 hasConcept C2777034083 @default.
- W3146537805 hasConcept C2778600265 @default.
- W3146537805 hasConcept C2779271181 @default.
- W3146537805 hasConcept C62520636 @default.
- W3146537805 hasConcept C8058405 @default.
- W3146537805 hasConcept C83260615 @default.
- W3146537805 hasConcept C87355193 @default.
- W3146537805 hasConceptScore W3146537805C115260700 @default.
- W3146537805 hasConceptScore W3146537805C116403925 @default.
- W3146537805 hasConceptScore W3146537805C121332964 @default.
- W3146537805 hasConceptScore W3146537805C125485243 @default.
- W3146537805 hasConceptScore W3146537805C127313418 @default.
- W3146537805 hasConceptScore W3146537805C147120987 @default.
- W3146537805 hasConceptScore W3146537805C199635899 @default.
- W3146537805 hasConceptScore W3146537805C2777034083 @default.
- W3146537805 hasConceptScore W3146537805C2778600265 @default.
- W3146537805 hasConceptScore W3146537805C2779271181 @default.
- W3146537805 hasConceptScore W3146537805C62520636 @default.
- W3146537805 hasConceptScore W3146537805C8058405 @default.
- W3146537805 hasConceptScore W3146537805C83260615 @default.
- W3146537805 hasConceptScore W3146537805C87355193 @default.
- W3146537805 hasOpenAccess W3146537805 @default.
- W3146537805 hasRelatedWork W1584324561 @default.
- W3146537805 hasRelatedWork W1970491080 @default.
- W3146537805 hasRelatedWork W1978367474 @default.
- W3146537805 hasRelatedWork W1987787709 @default.
- W3146537805 hasRelatedWork W1988242208 @default.
- W3146537805 hasRelatedWork W1990280259 @default.
- W3146537805 hasRelatedWork W2013841217 @default.
- W3146537805 hasRelatedWork W2015683643 @default.
- W3146537805 hasRelatedWork W2026454154 @default.
- W3146537805 hasRelatedWork W2048184924 @default.
- W3146537805 hasRelatedWork W2053009243 @default.
- W3146537805 hasRelatedWork W2056708358 @default.
- W3146537805 hasRelatedWork W2078678232 @default.
- W3146537805 hasRelatedWork W2230546014 @default.
- W3146537805 hasRelatedWork W2378941059 @default.
- W3146537805 hasRelatedWork W3001598076 @default.
- W3146537805 hasRelatedWork W3035980057 @default.
- W3146537805 hasRelatedWork W3096231675 @default.
- W3146537805 hasRelatedWork W3156666935 @default.
- W3146537805 hasRelatedWork W3196350755 @default.
- W3146537805 isParatext "false" @default.
- W3146537805 isRetracted "false" @default.
- W3146537805 magId "3146537805" @default.
- W3146537805 workType "article" @default.