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Galloper Wind Farm Project - National Infrastructure Planning

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2842_SLVIA<br />

81<br />

east-southeast sector of the horizon line by a total of approximately 7.5°.<br />

Whilst this will result in a discernible difference to the horizon line view in<br />

the immediate proximity of the GGOWF, from this distance, the proximity of<br />

the WTGs of the existing GGOWF and the proposed GWF means they will be<br />

perceived as a single distant feature on the horizon line rather a than a series<br />

of disparate elements. As such, the additional WTGs of the proposed GWF<br />

will not alter the existing character of seaward views, nor will they<br />

fundamentally change any of the key elements within the existing view. The<br />

magnitude of operational effect on the existing seaward view illustrated in<br />

the photographic panorama is judged, therefore, to be Low to Negligible. The<br />

sensitivity of the viewpoint is judged to be High. The overall significance of<br />

operational effect is assessed as Minor.<br />

Viewpoint 6 Shingle Street near Martello Tower<br />

7.3.19. See wireframe and photomontage views (Figures 2842/WF/06 and<br />

2842/PM/06).<br />

Proposed View<br />

7.3.20. When visibility is good, the WTGs of the proposed GWF will be seen in the<br />

east-southeast sector of the horizon line overlapping with the WTGs of the<br />

GGOWF and extending an additional 3° further to the north and an<br />

additional 1° further to the south than the existing 35° spread of the GGOWF.<br />

Many of the proposed WTGs will appear clustered in the northern portion of<br />

the WTG arrangement, to the east of the GGOWF. The remainder of the<br />

proposed WTGs will appear relatively evenly interspersed amongst the<br />

WTGs of the existing GGOWF. The proposed WTGs will appear relatively<br />

recessive in the view relative to the WTGs of the GGOWF due to their greater<br />

distance from the viewpoint and, as such, will not markedly increase the<br />

apparent density of the WTGs of the GGOWF. When visibility is very good,<br />

the London Array wind farm will be visible in the southern sector of the<br />

horizon line view with approximately a 23° of visual separation from the<br />

southernmost WTG of the proposed GWF.<br />

Magnitude and Significance of Operational Effect<br />

7.3.21. The proposed GWF will increase the overall spread of WTGs visible on the<br />

distant horizon line by 4° when visibility is good. Whilst this will result in a<br />

slightly discernible difference in views towards the horizon line in the<br />

immediate proximity of the GGOWF, from this distance the WTGs the<br />

existing GGOWF and proposed GWF will still read as a single distant feature<br />

on the horizon line. When visibility is very good, the proposed WTGs will<br />

reduce the existing degree of visual separation between the London Array<br />

wind farm and the GGOWF by 1°. The London Array wind farm and the

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