Neil R.P. Harris

Prof. Neil R.P. Harris

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Research Focus & Metrics

Academic Career Length

33Years (1994-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 May 2001 in Reviews of Geophysics
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Journal Article
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JSJ. Staehelin
J. Staehelin
NHNeil R.P. Harris
Neil R.P. Harris
CAC. Appenzeller
C. Appenzeller
JEJ. Eberhard
J. Eberhard

28 February 2004 in Geophysical Research Letters
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Journal Article
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MRM. Rex
M. Rex
RSR. J. Salawitch
R. J. Salawitch
PGP. von der Gathen
P. von der Gathen
NHNeil R.P. Harris
Neil R.P. Harris
MCM. P. Chipperfield
M. P. Chipperfield
BNB. Naujokat
B. Naujokat

14 September 2017 in Nature
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Journal Article
Open access
MCMartyn P. Chipperfield
Martyn P. Chipperfield
SBSlimane Bekki
Slimane Bekki
SDSandip Dhomse
Sandip Dhomse
NHNeil R.P. Harris
Neil R.P. Harris
BHBirgit Hassler
Birgit Hassler
MWMark Weber
Mark Weber
As a result of the 1987 Montreal Protocol and its amendments, the atmospheric loading of anthropogenic ozone-depleting substances is decreasing. Accordingly, the stratospheric ozone layer is expected to recover. However, short data records and atmospheric variability confound the search for early signs of recovery, and climate change is masking ozone recovery from ozone-depleting substances in some regions and will increasingly affect the extent of recovery. Here we discuss the nature and timescales of ozone recovery, and explore the extent to which it can be currently detected in different atmospheric regions.

11 September 2017 in Atmospheric Chemistry and Physics
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Journal Article
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WSWolfgang Steinbrecht
Wolfgang Steinbrecht
LFLucien Froidevaux
Lucien Froidevaux
RFRyan Fuller
Ryan Fuller
RWRay Wang
Ray Wang
JAJohn Anderson
John Anderson
FTFiona Tummon
Fiona Tummon
Ozone profile trends over the period 2000 to 2016 from several merged satellite ozone data sets and from ground-based data measured by four techniques at stations of the Network for the Detection of Atmospheric Composition Change indicate significant ozone increases in the upper stratosphere, between 35 and 48 km altitude (5 and 1 hPa). Near 2 hPa (42 km), ozone has been increasing by about 1.5 % per decade in the tropics (20° S to 20° N), and by 2 to 2.5 % per decade in the 35 to 60° latitude bands of both hemispheres. At levels below 35 km (5 hPa), 2000 to 2016 ozone trends are smaller and not statistically significant. The observed trend profiles are consistent with expectations from chemistry climate model simulations. This study confirms positive trends of upper stratospheric ozone already reported, e.g., in the WMO/UNEP Ozone Assessment 2014 or by Harris et al. (2015). Compared to those studies, three to four additional years of observations, updated and improved data sets with reduced drift, and the fact that nearly all individual data sets indicate ozone increase in the upper stratosphere, all give enhanced confidence. Uncertainties have been reduced, for example for the trend near 2 hPa in the 35 to 60° latitude bands from about ±5 % (2σ) in Harris et al. (2015) to less than ±2 % (2σ). Nevertheless, a thorough analysis of possible drifts and differences between various data sources is still required, as is a detailed attribution of the observed increases to declining ozone-depleting substances and to stratospheric cooling. Ongoing quality observations from multiple independent platforms are key for verifying that recovery of the ozone layer continues as expected.

7 September 2015 in Atmospheric Chemistry and Physics
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NHNeil R.P. Harris
Neil R.P. Harris
BHBirgit Hassler
Birgit Hassler
FTF. Tummon
F. Tummon
GBG. E. Bodeker
G. E. Bodeker
DHDaan Hubert
Daan Hubert
JZJ. M. Zawodny
J. M. Zawodny
Trends in the vertical distribution of ozone are reported and compared for a number of new and recently revised data sets. The amount of ozone-depleting compounds in the stratosphere (as measured by equivalent effective stratospheric chlorine – EESC) was maximised in the second half of the 1990s. We examine the periods before and after the peak to see if any change in trend is discernible in the ozone record that might be attributable to a change in the EESC trend, though no attribution is attempted. Prior to 1998, trends in the upper stratosphere (~ 45 km, 4 hPa) are found to be −5 to −10 % per decade at mid-latitudes and closer to −5 % per decade in the tropics. No trends are found in the mid-stratosphere (28 km, 30 hPa). Negative trends are seen in the lower stratosphere at mid-latitudes in both hemispheres and in the deep tropics. However, it is hard to be categorical about the trends in the lower stratosphere for three reasons: (i) there are fewer measurements, (ii) the data quality is poorer, and (iii) the measurements in the 1990s are perturbed by aerosols from the Mt Pinatubo eruption in 1991. These findings are similar to those reported previously even though the measurements for the main satellite and ground-based records have been revised. There is no sign of a continued negative trend in the upper stratosphere since 1998: instead there is a hint of an average positive trend of ~ 2 % per decade in mid-latitudes and ~ 3 % per decade in the tropics. The significance of these upward trends is investigated using different assumptions of the independence of the trend estimates found from different data sets. The averaged upward trends are significant if the trends derived from various data sets are assumed to be independent (as in Pawson et al., 2014) but are generally not significant if the trends are not independent. This occurs because many of the underlying measurement records are used in more than one merged data set. At this point it is not possible to say which assumption is best. Including an estimate of the drift of the overall ozone observing system decreases the significance of the trends. The significance will become clearer as (i) more years are added to the observational record, (ii) further improvements are made to the historic ozone record (e.g. through algorithm development), and (iii) the data merging techniques are refined, particularly through a more rigorous treatment of uncertainties.

1 October 1997 in Nature
Verified
Journal Article
Closed access
MRMarkus Rex
Markus Rex
NHNeil R.P. Harris
Neil R.P. Harris
PGPeter Von Der Gathen
Peter Von Der Gathen
RLRalph Lehmann
Ralph Lehmann
GBGeir O. Braathen
Geir O. Braathen
JWJohn Wenger
John Wenger