Skip to main content

Table 5 Observational parameters (Y 1–Y 11) used for dust retrieval

From: Feasibility of retrieving dust properties and total column water vapor from solar spectra measured using a lander camera on Mars

Parameter (Y)

Relationship with measured quantities

Y 1

D 0

P 1

DSR(λ 0)

Y 2

D C

P 2/P 3

DSR(λ B )/DSR(λ R )

Y 3

A C

P 5/P 9

SSR(λ B , χ A )/SSR(λ R , χ A )

Y 4

A B

P 5/P 4

SSR(λ B , χ A )/SSR(λ B , χ 0)

Y 5

A R

P 9/P 8

SSR(λ R , χ A )/SSR(λ R , χ 0)

Y 6

F C

P 6/P 10

SSR(λ B , χ F )/SSR(λ R , χ F )

Y 7

F B

P 6/P 4

SSR(λ B , χ F )/SSR(λ B , χ 0)

Y 8

F R

P 10/P 8

SSR(λ R , χ F )/SSR(λ R , χ 0)

Y 9

B C

P 7/P 11

SSR(λ B , χ B )/SSR(λ R , χ B )

Y 10

B B

P 7/P 4

SSR(λ B , χ B )/SSR(λ B , χ 0)

Y 11

B R

P 11/P 8

SSR(λ R , χ B )/SSR(λ R , χ 0)