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Part I: Impac<strong>ts</strong> of Climate-related Geo<strong>en</strong>gineering on Biological Diversity<br />

For the above reason (and because of ocean acidification effec<strong>ts</strong>), it is important that SRM should not be regarded<br />

as an alternative to strong emission reductions, in order to stabilize, and preferably reduce, the levels of gre<strong>en</strong>house<br />

gases in the atmosphere. SRM might, however, be considered as a supplem<strong>en</strong>tary action.<br />

4.2 POTENTIAL IMPACTS OF SRM ON BIODIVERSITY AT THE TECHNIQUE-SPECIFIC LEVEL<br />

Thus far, this chapter has addressed the g<strong>en</strong>eral effec<strong>ts</strong> of space- or atmospheric-based SRM on biodiversity, based<br />

on uniform dimming; as noted, such a change in the Earth’s radiative <strong>en</strong>ergy budget may not be achievable in<br />

practice. Below, the pot<strong>en</strong>tial b<strong>en</strong>efi<strong>ts</strong> and drawbacks associated with three specific techniques—stratospheric<br />

aerosol injection, cloud bright<strong>en</strong>ing and surface albedo <strong>en</strong>hancem<strong>en</strong>t—are considered, on the basis that these are<br />

the options most frequ<strong>en</strong>tly proposed, and are each theoretically capable of counteracting either all or most of the<br />

radiative forcing from gre<strong>en</strong>house gases.212 Important technique-specific considerations include the height above<br />

the Earth’s surface where the sunlight reflection occurs, and whether there may be additional physico-chemical<br />

interactions. The pot<strong>en</strong>tial positive and negative impac<strong>ts</strong> of space-based reflectors213, 214, 215 are expected to be<br />

similar to those theoretically indicated by models for uniform-dimming SRM described above.<br />

4.2.1 Pot<strong>en</strong>tial impac<strong>ts</strong> on biodiversity of stratospheric aerosol injection<br />

In addition to the positive and negative impac<strong>ts</strong> of idealised SRM already described, the climatic effec<strong>ts</strong> of<br />

geo<strong>en</strong>gineered stratospheric sulphate aerosol will dep<strong>en</strong>d on where (injection altitude and locality) and how<br />

(injection technique and timing) this technique is deployed, with significant effec<strong>ts</strong> of both factors on aerosol<br />

microphysics and behaviour, including the radius, radiative impact and longevity of the aerosols.216 Furthermore,<br />

this proposed technique could affect precipitation acidity, stratospheric ozone depletion, and the overall quantity<br />

and quality of light reaching the biosphere, with subsequ<strong>en</strong>t effec<strong>ts</strong> on biodiversity and ecosystem services. Some,<br />

but not all, of these unint<strong>en</strong>ded negative impac<strong>ts</strong> might be avoided if aerosols other than sulphates were to be used<br />

for this approach. Other particles that have be<strong>en</strong> suggested include electrostatic or magnetic nano-particles,217<br />

pot<strong>en</strong>tially with relatively long atmospheric lifetimes; there is also the possibility of designing a particle with<br />

specific attributes.218 However, they might bring with them their own particular risks—together with additional<br />

public acceptability issues.<br />

Increased precipitation acidity<br />

Use of sulphate aerosols for SRM would, to some degree, increase the acidity of precipitation (“acid rain”), with<br />

consequ<strong>en</strong>t impac<strong>ts</strong> on ecosystems. However, the size of this effect is considered to be small, since the quantities<br />

of sulphur estimated to be needed for this form of SRM are ≤10% of the curr<strong>en</strong>t global deposition, and possibly<br />

as little as 1%.219 Furthermore, sulphur deposition would be more widely distributed than is curr<strong>en</strong>tly the case<br />

from anthropog<strong>en</strong>ic sulphur emissions, and buffering processes mean than ocean acidification is unlikely to be<br />

significantly wors<strong>en</strong>ed.220<br />

212 Vaughan & L<strong>en</strong>ton (2011).<br />

213 Seifritz (1989).<br />

214 Angel (2006).<br />

215 McInnes (2010).<br />

216 Niemeier et al. (2011).<br />

217 Keith (2010).<br />

218 Oral pres<strong>en</strong>tation by B<strong>en</strong> Kravitz at Planet under Pressure confer<strong>en</strong>ce, London, 27 March 2012.<br />

219 Kravitz et al. (2009).<br />

220 Hunter et al. (2011).<br />

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