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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
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.
1932-6157
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
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), 22-40. (doi:10.1214/20-AOAS1367).

Record type: Article

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

Identifiers

Local EPrints ID: 484278
URI: http://eprints.soton.ac.uk/id/eprint/484278
ISSN: 1932-6157
PURE UUID: 55dcb00a-f7ce-4db9-a92f-e7b60f665b9e
ORCID for Duo Chan: ORCID iD orcid.org/0000-0002-8573-5115

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Date deposited: 13 Nov 2023 18:56
Last modified: 18 Mar 2024 04:15

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Contributors

Author: Chenguang Dai
Author: Duo Chan ORCID iD
Author: Peter Huybers
Author: Natesh Pillai

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