M P M P = 20 P - grc.nasa.gov€¦ · 0.00 0.70 0.90 1.45 1.75 Pplenum / PT local Q sonic 0.0 0.2...

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Page 1: M P M P = 20 P - grc.nasa.gov€¦ · 0.00 0.70 0.90 1.45 1.75 Pplenum / PT local Q sonic 0.0 0.2 0.4 0.6 0.8 1.0 0.0 0.2 0.4 0.6 0.8 1.0 0.50 Mlocal Mlocal PT local α = 20° P plenum

0.000.70

0.90

1.45

1.75

Pplenum / PT local

Qso

nic

0.0 0.2 0.4 0.6 0.8 1.00.0

0.2

0.4

0.6

0.8

1.0 0.50Mlocal

Mlocal PT local

α = 20° Pplenum

L / D = 2

0.8

1.9

= Mlocal

Pplenum / PT local

Qso

nic

0.0 0.2 0.4 0.6 0.8 1.00.0

0.2

0.4

0.6

0.8

1.0

Mlocal

0.80.91.01.11.21.31.41.51.61.71.81.9

Mlocal PT local

α = 90° Pplenum

L / D = 3

On Particle Gibbs Samplingmwl25/mcmski/slides/ss_mcmski14.pdf · 0.6 0.8 ACF X 0 multinomial residual systematic multi+BS 0 10 20 30 40 50 60 70 80 lag 0.0 0.2 0.4 0.6 0.8 ACF X 399

On Particle Gibbs Samplingmwl25/mcmski/slides/ss_mcmski14.pdf · 0.6 0.8 ACF X 0 multinomial residual systematic multi+BS 0 10 20 30 40 50 60 70 80 lag 0.0 0.2 0.4 0.6 0.8 ACF X 399

CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

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PageRank. s1s1 p 12 p 21 s2s2 s3s3 p 31 s4s4 p 41 p 34 p 42 p 13 x 1 = p 21 p 34 p 41 + p 34 p 42 p 21 + p 21 p 31 p 41 + p 31 p 42 p 21 / Σ x 2 = p 31.

PageRank. s1s1 p 12 p 21 s2s2 s3s3 p 31 s4s4 p 41 p 34 p 42 p 13 x 1 = p 21 p 34 p 41 + p 34 p 42 p 21 + p 21 p 31 p 41 + p 31 p 42 p 21 / Σ x 2 = p 31.

Proportional Navigation with Adaptive Terminal … 670.6 670.8 671 671.2 671.4 228 230 232 234 236 238 240 242 244 246 248-1-0.8-0.6-0.4-0.2 0 0.2 0.4 0.6 0.8 1 228 230 232 234 236

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Por que estudar o Sol? O SOL - Portal IAG · 2 σT 4 4πR p 2σ(fT p)4dp2 f - correção para o efeito estufa A – albedo (~0.4). Conexão o clima A cobertura de nuvens podem mudar.

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