Rotational Raman scattering in the Earth's atmosphere ... - SRON
Rotational Raman scattering in the Earth's atmosphere ... - SRON
Rotational Raman scattering in the Earth's atmosphere ... - SRON
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Retrieval of cloud properties from NUV, VIS and NIR 103<br />
prom<strong>in</strong>ent Fraunhofer l<strong>in</strong>es and weaker molecular <strong>scatter<strong>in</strong>g</strong> <strong>in</strong> <strong>the</strong>se spectral ranges.<br />
Figure 5.2: R<strong>in</strong>g spectra <strong>in</strong> <strong>the</strong> wavelength range 388–400 nm for a clear-sky observation (gray curve;<br />
f c =0, A s =0.05, surface pressure p s = 1013 hPa) and for two fully clouded observations (black curves;<br />
f c =1, τ c =40) with different cloud top height. Increas<strong>in</strong>g <strong>the</strong> cloud top height from 1.9 km (p c =800 hPa;<br />
dotted l<strong>in</strong>e) to 5.6 km altitude (p c = 500 hPa; black solid l<strong>in</strong>e) leads to a reduction of <strong>the</strong> R<strong>in</strong>g effect<br />
structures. We used <strong>the</strong> solar spectrum of Chance and Spurr [1997] as <strong>in</strong>put for our simulations.<br />
F<strong>in</strong>ally, sensitivity to clouds <strong>in</strong> <strong>the</strong> measurements is caused by molecular absorption l<strong>in</strong>es. The<br />
most prom<strong>in</strong>ent absorption feature of O 2 is located <strong>in</strong> <strong>the</strong> NIR w<strong>in</strong>dow. Ano<strong>the</strong>r significant, but<br />
much weaker absorption band is <strong>the</strong> O 2 -O 2 absorption band <strong>in</strong> <strong>the</strong> VIS w<strong>in</strong>dow. O<strong>the</strong>r absorption<br />
features <strong>in</strong> <strong>the</strong> NUV, VIS and NIR w<strong>in</strong>dows are of m<strong>in</strong>or importance for <strong>the</strong> sensitivity to clouds. A<br />
large part of <strong>the</strong> sensitivity to clouds arises from <strong>the</strong> shield<strong>in</strong>g effect of clouds; <strong>the</strong> vertical column<br />
of O 2 and O 2 -O 2 below <strong>the</strong> cloud is shielded and hence <strong>the</strong> depth of <strong>the</strong> O 2 and O 2 -O 2 absorption<br />
features are reduced, which can be used <strong>in</strong> a retrieval approach. At wavelengths with both strong and<br />
weak atmospheric absorption such as <strong>in</strong> <strong>the</strong> O 2 A band additional sensitivity of <strong>the</strong> measurement is<br />
obta<strong>in</strong>ed. The measured strong atmospheric absorption bands consist of <strong>the</strong> radiation that has been<br />
scattered back to <strong>the</strong> satellite at high altitudes, because <strong>in</strong>cident radiation cannot penetrate to lower<br />
altitudes due to absorption. The situation is different for wavelengths with weak or no atmospheric<br />
absorption. Here, <strong>the</strong> measured radiation travels all <strong>the</strong> way through <strong>the</strong> <strong>atmosphere</strong>, is reflected by<br />
<strong>the</strong> cloud, and subsequently scattered by <strong>the</strong> air molecules <strong>in</strong>to <strong>the</strong> satellite’s l<strong>in</strong>e of sight. Therefore<br />
<strong>the</strong> measurement is sensitive to radiation from any altitude. This results <strong>in</strong> a characteristic sensitivity<br />
of absorption bands such as <strong>the</strong> O 2 A band <strong>in</strong> reflectivity measurements to cloud properties which can<br />
be used <strong>in</strong> a retrieval approach.