Late 19th century navigational uncertainties and their influence on sea surface temperature estimates
Late 19th century navigational uncertainties and their influence on sea surface temperature estimates
Accurate estimates of historical changes in sea surface temperatures (SSTs) and their uncertainties are important for documenting and understanding historical changes in climate. A source of uncertainty that has not previously been quantified in historical SST estimates stems from position errors. A Bayesian inference framework is proposed for quantifying errors in reported positions and their implications on SST estimates. The analysis framework is applied to data from the International Comprehensive Ocean-Atmosphere Data Set (ICOADS3.0) in 1885, a time when astronomical and chronometer estimation of position was common but predated the use of radio signals. Focus is upon a subset of 943 ship tracks from ICOADS3.0 that report their position every two hours to a precision of 0.01∘ longitude and latitude. These data are interpreted as positions determined by dead reckoning that are periodically updated by celestial correction techniques. The posterior medians of uncertainties in celestial correction are 33.1 km (0.30∘ on the equator) in longitude and 24.4 km (0.22∘) in latitude, respectively. Celestial navigation uncertainties being smaller in latitude than longitude is qualitatively consistent with the relative difficulty of obtaining astronomical estimates. The posterior medians for two-hourly dead reckoning uncertainties are 19.2% for ship speed and 13.2∘ for ship heading, leading to random position uncertainties with median 0.18∘ (20 km on the equator) in longitude and 0.15∘ (17 km) in latitude. Reported ship tracks also contain systematic position uncertainties relating to precursor dead-reckoning positions not being updated after obtaining celestial position estimates, indicating that more accurate positions can be provided for SST observations. Finally, we translate position errors into SST uncertainties by sampling an ensemble of SSTs from the Multiscale Ultrahigh Resolution Sea Surface Temperature (MURSST) data set. Evolving technology for determining ship position, heterogeneous reporting and archiving of position information, and seasonal and spatial changes in navigational uncertainty and SST gradients together imply that accounting for positional error in SST estimates over the span of the instrumental record will require substantial additional effort.
22-40
Dai, Chenguang
cfa4fe97-558f-442c-9903-a5f5a1b86fe1
Chan, Duo
4c1278dc-7f39-4b67-b1cd-3f81f55f4906
Huybers, Peter
48e9a517-aa2a-40f1-96ef-06d76b19291c
Pillai, Natesh
e4bf6422-dbb2-4793-bd13-ba632017fbee
1 March 2021
Dai, Chenguang
cfa4fe97-558f-442c-9903-a5f5a1b86fe1
Chan, Duo
4c1278dc-7f39-4b67-b1cd-3f81f55f4906
Huybers, Peter
48e9a517-aa2a-40f1-96ef-06d76b19291c
Pillai, Natesh
e4bf6422-dbb2-4793-bd13-ba632017fbee
Dai, Chenguang, Chan, Duo, Huybers, Peter and Pillai, Natesh
(2021)
Late 19th century navigational uncertainties and their influence on sea surface temperature estimates.
The Annals of Applied Statistics, 15 (1), .
(doi:10.1214/20-AOAS1367).
Abstract
Accurate estimates of historical changes in sea surface temperatures (SSTs) and their uncertainties are important for documenting and understanding historical changes in climate. A source of uncertainty that has not previously been quantified in historical SST estimates stems from position errors. A Bayesian inference framework is proposed for quantifying errors in reported positions and their implications on SST estimates. The analysis framework is applied to data from the International Comprehensive Ocean-Atmosphere Data Set (ICOADS3.0) in 1885, a time when astronomical and chronometer estimation of position was common but predated the use of radio signals. Focus is upon a subset of 943 ship tracks from ICOADS3.0 that report their position every two hours to a precision of 0.01∘ longitude and latitude. These data are interpreted as positions determined by dead reckoning that are periodically updated by celestial correction techniques. The posterior medians of uncertainties in celestial correction are 33.1 km (0.30∘ on the equator) in longitude and 24.4 km (0.22∘) in latitude, respectively. Celestial navigation uncertainties being smaller in latitude than longitude is qualitatively consistent with the relative difficulty of obtaining astronomical estimates. The posterior medians for two-hourly dead reckoning uncertainties are 19.2% for ship speed and 13.2∘ for ship heading, leading to random position uncertainties with median 0.18∘ (20 km on the equator) in longitude and 0.15∘ (17 km) in latitude. Reported ship tracks also contain systematic position uncertainties relating to precursor dead-reckoning positions not being updated after obtaining celestial position estimates, indicating that more accurate positions can be provided for SST observations. Finally, we translate position errors into SST uncertainties by sampling an ensemble of SSTs from the Multiscale Ultrahigh Resolution Sea Surface Temperature (MURSST) data set. Evolving technology for determining ship position, heterogeneous reporting and archiving of position information, and seasonal and spatial changes in navigational uncertainty and SST gradients together imply that accounting for positional error in SST estimates over the span of the instrumental record will require substantial additional effort.
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Published date: 1 March 2021
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Local EPrints ID: 484278
URI: http://eprints.soton.ac.uk/id/eprint/484278
ISSN: 1932-6157
PURE UUID: 55dcb00a-f7ce-4db9-a92f-e7b60f665b9e
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Date deposited: 13 Nov 2023 18:56
Last modified: 18 Mar 2024 04:15
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Author:
Chenguang Dai
Author:
Duo Chan
Author:
Peter Huybers
Author:
Natesh Pillai
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