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ao - ForOT Optical Turbulence Forecasts

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WAVEFRONT DISTURBANCE BY REFRACTIVE INDEX (n) CHANGES<br />

∆y<br />

d<br />

n 2<br />

n 1<br />

Sea Level<br />

RH = 1<br />

∆x = (n 2 -n 1 )*d<br />

∆φ = ∆x/λ<br />

∆x<br />

NOTE: ∆x , dx/dy (tilt) and<br />

d 2 x/dy 2 (curvature)<br />

are achromatic if<br />

n is λ-independent<br />

CIRCLES: RH = 1 AIR<br />

Cerro Paranal<br />

RH = 0<br />

RADIO<br />

WAVES<br />

R.J. Mather, 2004<br />

ANOMALOUS DISPERSION EFFECTS<br />

J H K L M<br />

NOTE:<br />

(i) in general refractive index is function of<br />

temperature & water vapor (RH)<br />

(ii) in optical/IR water vapor has little effect;<br />

T (⇒ P & density) variations dominate seeing.<br />

(iii) in radio & far-IR astronomy water vapor<br />

variations dominate “seeing”<br />

(iv) anomalous dispersion effects occur mostly<br />

outside atmospheric transmission windows;<br />

they have minor effects on n variations<br />

(and do not “compensate seeing” as I had hoped many years ago)

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