These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
5. Distinct Mineralogy and Age of Individual Lava Flows in Atla Regio, Venus Derived From Magellan Radar Emissivity. Brossier J; Gilmore MS; Toner K; Stein AJ J Geophys Res Planets; 2021 Mar; 126(3):. PubMed ID: 33959469 [TBL] [Abstract][Full Text] [Related]
6. Deriving iron contents from past and future Venus surface spectra with new high-temperature laboratory emissivity data. Helbert J; Maturilli A; Dyar MD; Alemanno G Sci Adv; 2021 Jan; 7(3):. PubMed ID: 33523894 [TBL] [Abstract][Full Text] [Related]
7. H2O-H2SO4 system in Venus' clouds and OCS, CO, and H2SO4 profiles in Venus' troposphere. Krasnopolsky VA; Pollack JB Icarus; 1994 May; 109(1):58-78. PubMed ID: 11539137 [TBL] [Abstract][Full Text] [Related]
8. Visible-near infrared point spectrometry of drill core samples from Río Tinto, Spain: results from the 2005 Mars Astrobiology Research and Technology Experiment (MARTE) drilling exercise. Sutter B; Brown AJ; Stoker CR Astrobiology; 2008 Oct; 8(5):1049-60. PubMed ID: 19105759 [TBL] [Abstract][Full Text] [Related]
10. A Hyperspectral Imaging Approach for Classifying Geographical Origins of Rhizoma Atractylodis Macrocephalae Using the Fusion of Spectrum-Image in VNIR and SWIR Ranges (VNIR-SWIR-FuSI). Ru C; Li Z; Tang R Sensors (Basel); 2019 May; 19(9):. PubMed ID: 31052476 [TBL] [Abstract][Full Text] [Related]
11. Magellan: electrical and physical properties of venus' surface. Tyler GL; Ford PG; Campbell DB; Elachi C; Pettengill GH; Simpson RA Science; 1991 Apr; 252(5003):265-70. PubMed ID: 17769273 [TBL] [Abstract][Full Text] [Related]
12. The complex relationship between olivine abundance and thermal inertia on Mars. Hanna RD; Hamilton VE; Putzig NE J Geophys Res Planets; 2016 Jul; 121(7):1293-1320. PubMed ID: 31007993 [TBL] [Abstract][Full Text] [Related]
13. [Study on the Characterization of VNIR-MIR Spectra and Prediction of Soil Organic Matter in Paddy Soil]. Chen SC; Peng J; Ji WJ; Zhou Y; He JX; Shi Z Guang Pu Xue Yu Guang Pu Fen Xi; 2016 Jun; 36(6):1712-6. PubMed ID: 30052377 [TBL] [Abstract][Full Text] [Related]
14. Olivine Dissolution in Seawater: Implications for CO Montserrat F; Renforth P; Hartmann J; Leermakers M; Knops P; Meysman FJ Environ Sci Technol; 2017 Apr; 51(7):3960-3972. PubMed ID: 28281750 [TBL] [Abstract][Full Text] [Related]
15. Red clays indicate sub-aerial exposure of the Rio Grande Rise during the Eocene volcanic episode. Srivastava P; J Murton B; Sant'Anna LG; Florindo F; Hassan MB; Taciro Mandacaru Guerra J; de Assis Janasi V; Jovane L Sci Rep; 2023 Nov; 13(1):19092. PubMed ID: 37925541 [TBL] [Abstract][Full Text] [Related]
16. Correlated compositional and mineralogical investigations at the Chang'e-3 landing site. Ling Z; Jolliff BL; Wang A; Li C; Liu J; Zhang J; Li B; Sun L; Chen J; Xiao L; Liu J; Ren X; Peng W; Wang H; Cui X; He Z; Wang J Nat Commun; 2015 Dec; 6():8880. PubMed ID: 26694712 [TBL] [Abstract][Full Text] [Related]
17. Time-resolved remote Raman study of minerals under supercritical CO2 and high temperatures relevant to Venus exploration. Sharma SK; Misra AK; Clegg SM; Barefield JE; Wiens RC; Acosta T Philos Trans A Math Phys Eng Sci; 2010 Jul; 368(1922):3167-91. PubMed ID: 20529953 [TBL] [Abstract][Full Text] [Related]
18. The color of the surface of venus. Pieters CM; Head JW; Pratt S; Patterson W; Garvin J; Barsukov VL; Basilevsky AT; Khodakovsky IL; Selivanov AS; Panfilov AS; Gektin YM; Narayeva YM Science; 1986 Dec; 234(4782):1379-83. PubMed ID: 17755059 [TBL] [Abstract][Full Text] [Related]