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Volumn 316, Issue 5821, 2007, Pages 92-95

Subsurface radar sounding of the south polar layered deposits of Mars

(24)  Plaut, Jeffrey J a   Picardi, Giovanni b   Safaeinili, Ali a   Ivanov, Anton B a   Milkovich, Sarah M a   Cicchetti, Andrea b   Kofman, Wlodek c   Mouginot, Jérémie c   Farrell, William M d   Phillips, Roger J e   Clifford, Stephen M f   Frigeri, Alessandro g   Orosei, Roberto h   Federico, Costanzo g   Williams, Iwan P i   Gurnett, Donald A j   Nielsen, Erling k   Hagfors, Tor k   Heggy, Essam f   Stofan, Ellen R l   more..

h INAF   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

ICE THICKNESS; IONOSPHERE; MAPPING; MARS; RADAR; TOPOGRAPHY;

EID: 34147097407     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1139672     Document Type: Article
Times cited : (302)

References (23)
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    • Loss tangent in this context is defined as (ε″/ε′) where ε″and ε′ are the imaginary and real parts, respectively, of the complex dielectric permittivity
    • Loss tangent in this context is defined as (ε″/ε′) where ε″and ε′ are the imaginary and real parts, respectively, of the complex dielectric permittivity.
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    • We used the natural-neighbor interpolation as implemented in the ArcMap GIS software from ESRI (Redlands, CA, The interpolation applies a weighted moving average and is a preferred method for irregularly distributed data sets 16
    • We used the natural-neighbor interpolation as implemented in the ArcMap GIS software from ESRI (Redlands, CA). The interpolation applies a weighted moving average and is a preferred method for irregularly distributed data sets (16).
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    • The error on this estimate includes a 10% uncertainty in refractive index and an additional factor due to gaps in coverage and detectability of the basal interface
    • The error on this estimate includes a 10% uncertainty in refractive index and an additional factor due to gaps in coverage and detectability of the basal interface.
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    • The authors acknowledge the support of the space agencies of Italy (Agenzia Spaziale Italiana, the United States (NASA, and Europe (European Space Agency) for the operations of MARSIS and Mars Express. We thank Y. Gim for clutter simulation. Some of the research described in this publication was carried out at the Jet Propulsion Laboratory, California Institute of Technology
    • The authors acknowledge the support of the space agencies of Italy (Agenzia Spaziale Italiana), the United States (NASA), and Europe (European Space Agency) for the operations of MARSIS and Mars Express. We thank Y. Gim for clutter simulation. Some of the research described in this publication was carried out at the Jet Propulsion Laboratory, California Institute of Technology.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.