Planetary Radiation Budgets - ceres

Planetary Radiation Budgets - ceres Planetary Radiation Budgets - ceres

ceres.larc.nasa.gov
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17.02.2015 Views

Each radiance measured (e.g. from A or N) is a single sample of directions (q S ; q v , f v ) contributing to the fluxes emerging at those points. The flux measured with WFOV results from radiances from points N, A, P, P’, etc. each with its set of angles, each more or less representative of the flux emerging at those points. P A CERES STM 23-25 Sept. 2003 N P’ R. Kandel & M. Viollier Planetary Radiation Budgets 6 CERES STM 23-25 Sept. 2003 R. Kandel & M. Viollier Planetary Radiation Budgets 6

Replacing the satellite by a much more remote observer, say on another planet – It’s the same problem Observer P A N Observed planet CERES STM 23-25 Sept. 2003 P’ R. Kandel & M. Viollier Planetary Radiation Budgets 6 CERES STM 23-25 Sept. 2003 R. Kandel & M. Viollier Planetary Radiation Budgets 7

Each radiance measured (e.g. from A or N) is a<br />

single sample of directions (q S ; q v , f v ) contributing to<br />

the fluxes emerging at those points.<br />

The flux measured<br />

with WFOV results<br />

from radiances from<br />

points N, A, P, P’, etc.<br />

each with its set of<br />

angles, each more or<br />

less representative of<br />

the flux emerging at<br />

those points.<br />

P<br />

A<br />

CERES STM<br />

23-25 Sept. 2003<br />

N<br />

P’<br />

R. Kandel & M. Viollier<br />

<strong>Planetary</strong> <strong>Radiation</strong> <strong>Budgets</strong><br />

6<br />

CERES STM<br />

23-25 Sept. 2003<br />

R. Kandel & M. Viollier<br />

<strong>Planetary</strong> <strong>Radiation</strong> <strong>Budgets</strong><br />

6

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