Hi All
A recent estimate of the climate problem is that a reduction of the solar input 
by 1.7 watts per square metre would give tolerable temperature conditions. This 
is 0.5% of the mean global 24 hour solar input. If marine cloud brightening was 
used for only 10% of the global surface an increase of reflectivity of 5% would 
be adequate.

The grey scale below has 20 bars ranging from black to white.  Most people need 
to see at least three bars to detect the direction of the gradient. This shows 
that ship tracks give a contrast change far higher than would be required for 
climate control and that we would need image processing of satellite images to 
detect that it been done.  There may be many tracks of which we are unaware.

[cid:[email protected]]

Stephen

Emeritus Professor of Engineering Design
School of Engineering
University of Edinburgh
Mayfield Road
Edinburgh EH9 3DW
Scotland
0131 650 5704 or 0131 662 1180
YouTube Jamie Taylor Power for Change







From: [email protected] <[email protected]> On 
Behalf Of Geoengineering News
Sent: 26 February 2023 09:59
To: [email protected]
Subject: [geo] An Optical Flow Approach to Tracking Ship Track Behavior Using 
GOES-R Satellite Imagery

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https://ieeexplore.ieee.org/document/9837429

Authors
Kelsie M. Larson, Lyndsay Shand , Andrea Staid, Skyler Gray, Erika L. Roesler, 
and Don Lyons

22 July 2022

Abstract:Ship emissions can form linear cloud structures, or ship tracks , when 
atmospheric water vapor condenses on aerosols in the ship exhaust. These 
structures are of interest because they are observable and traceable examples 
of MCB, a mechanism that has been studied as a potential approach for solar 
climate intervention. Ship tracks can be observed throughout the diurnal cycle 
via space-borne assets like the advanced baseline imagers on the national 
oceanic and atmospheric administration geostationary operational environmental 
satellites, the GOES-R series. Due to complex atmospheric dynamics, it can be 
difficult to track these aerosol perturbations over space and time to precisely 
characterize how long a single emission source can significantly contribute to 
indirect radiative forcing. We propose an optical flow approach to estimate the 
trajectories of ship-emitted aerosols after they begin mixing with low boundary 
layer clouds using GOES-17 satellite imagery. Most optical flow estimation 
methods have only been used to estimate large scale atmospheric motion. We 
demonstrate the ability of our approach to precisely isolate the movement of 
ship tracks in low-lying clouds from the movement of large swaths of high 
clouds that often dominate the scene. This efficient approach shows that ship 
tracks persist as visible, linear features beyond 9 h and sometimes longer than 
24 h.
[Fig. 1. - These figures show the result of the optical flow method applied to 
a manually-selected local cloud region, starting with an intersection of two 
ship tracks on June 17, 2019, at 07:02 UTC (a) and stepping forward in time, 
with snapshots shown at 6 (b), 12 (c), and 18 (d) hr later. The tracking 
algorithm is able to follow the movement of the cloud region well, and the 
tracks are still clearly visible 18 hr later. The center location of these 
images is $33^{\circ }$27’02.0”N $138^{\circ 
}$06’11.9”W.]<https://ieeexplore.ieee.org/mediastore_new/IEEE/content/media/4609443/9656571/9837429/shand1-3193024-large.gif>

Fig. 1.

These figures show the result of the optical flow method applied to a 
manually-selected local cloud region, starting with an intersection of two ship 
tracks on June 17, 2019, at 07:02 UTC (a) and stepping forward in time, with 
snapshots shown at 6 (b), 12 (c), and 18 (d) hr later. The tracking algorithm 
is able to follow the movement of the cloud region well, and the tracks are 
still clearly visible 18 hr later.

Source: IEEE Xplore

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