EXPLORING the ROLE of SUB-MICRON-SIZED DUST GRAINS in the ATMOSPHERES of RED L0-L6 DWARFS

Keyphrases

• Dust Haze 100%
• L Dwarfs 75%
• Submicron 50%
• Particle Size Distribution 50%
• Brown Dwarfs 50%
• Dust Grains 50%
• Atmosphere Model 50%
• Upper Atmosphere 25%
• Small Particles 25%
• Column Density 25%
• Near-infrared 25%
• Reddening 25%
• Markov Chain Monte Carlo Methods 25%
• Silicate Grains 25%
• Dust Cloud 25%
• Large Grain 25%
• Mie Theory 25%
• Field L 25%
• Distribution Density 25%

Physics

• L Dwarf Stars 100%
• Planetary Atmosphere 66%
• Particle Size Distribution 66%
• Brown Dwarf 66%
• Near Infrared 33%
• Markov Chain Monte Carlo 33%
• Upper Atmosphere 33%
• Mie Scattering 33%
• Silicate Grains 33%
• Monte Carlo Method 33%

Earth and Planetary Sciences

• Planetary Atmosphere 100%
• Particle Size Distribution 100%
• Upper Atmosphere 50%
• Silicate 50%
• Markov Chain Monte Carlo 50%
• Mie Scattering 50%