881 to 890 of 2,089 Results
Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
Fixed Field Text Data - 3.5 MB -
MD5: bd4f8139d0f4706c45f2d22f23794936
|
Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
Fixed Field Text Data - 279.3 KB -
MD5: e02bec66a6541cbfd9abc1489215aa8d
|
Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
Fixed Field Text Data - 280.3 KB -
MD5: b5e6bdfc91ee6034d2de558077490f99
|
Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
Fixed Field Text Data - 370.4 KB -
MD5: 34c7334fc15f0ded585a9f273b644b0d
|
Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
Fixed Field Text Data - 371.1 KB -
MD5: e3ec8d3cd3f9af5057bf1cd11006d6d5
|
Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
Plain Text - 1.9 KB -
MD5: 21cf16b9db1045c188d87f2e81cc150c
|
Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
Unknown - 4.4 KB -
MD5: e571f1a4c6a5f6fea67b513211b3f4b6
|
Jul 20, 2021 - SEIS InSight
Khan, Amir; Ceylan, Savas; van Driel, Martin; Giardini, Domenico; Lognonné, Philippe; Samuel, Henri; Schmerr, Nicholas C.; Stähler, Simon C.; Duran, Andrea C.; Huang, Quancheng; Kim, Doyeon; Broquet, Adrien; Charalambous, Constantinos; Clinton, John F.; Davis, Paul M.; Drilleau, Mélanie; Karakostas, Foivos; Lekic, Vedran; McLennan, Scott M.; Maguire, Ross R.; Michaut, Chloé; Panning, Mark P.; Pike, William T.; Pinot, Baptiste; Plasman, Matthieu; Scholz, John-Robert; Widmer-Schnidrig, Rudolf; Spohn, Tilman; Smrekar, Suzanne E.; Banerdt, William B., 2021, "Upper mantle structure of Mars from InSight seismic data: Supplementary data", https://doi.org/10.18715/IPGP.2021.kpnr925g, IPGP Research Collection, V1
We provide two seismic velocity models that are characteristic of the inverted families of models shown in Khan et al. (2021) (cf. Fig.2A). The blue and red models correspond to models with lithospheric thicknesses in the range 400-500 km and 500-600 km (cf. Fig.2B of Khan et al.... |
Unknown - 5.7 KB -
MD5: 9afa2afede7ee31f40a02c0a1e93c18d
|
Adobe PDF - 78.2 KB -
MD5: 2041c1e235a3d4d1d361f00b926c25d3
|