There’s not that much ground-based astronomy in UV, relative to optical and IR 
astronomy.

Impact on optical astronomy is straightforward; if you lose 5% of the direct 
light, you need 5% longer integration time to get same number of photons.

Impact on IR astronomy is less obvious, as limited by the background from the 
sky, which depends on water vapour and temperature through the atmospheric 
column (with most telescopes being at 14000’ or so).  Shouldn’t be hard to 
estimate, I’ve never gotten someone interested enough to do the calculations 
but I could try again (my other job is being on the design team for the Thirty 
Meter Telescope).

I did ask people whether they noted anything after Pinatubo, and the answer I 
got was no… that doesn’t mean there wasn’t an effect, but it wasn’t something 
that the astronomy community by and large remembered.

From: [email protected] <[email protected]> On 
Behalf Of Russell Seitz
Sent: Sunday, April 7, 2019 9:31 AM
To: geoengineering <[email protected]>
Subject: [geo] Re: SRM optical impacts

Why would  reductions  in the  downwelling tropospheric light flux increase any 
of the above?    I'd instead  ask instrumental  astromomers what they think SO2 
scattering would do in the UV , as they have a lot to lose from  scattered 
light, which can  cost them contrast and  degrade the signal to noise ratio in 
interferometry and spectroscopy.

Try the Magellan and OWL teams

On Wednesday, April 3, 2019 at 7:47:35 AM UTC-4, Andrew Lockley wrote:
Has there been any investigation of SRM effects on vision? Eg perceived glare, 
macular degeneration, corneal sunburn, vision development in infants, object 
recognition when driving (and their equivalent in animals)?

Andrew Lockley
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