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  • 1
    In: Journal of Atmospheric and Oceanic Technology, American Meteorological Society, Vol. 15, No. 3 ( 1998-06), p. 687-696
    Type of Medium: Online Resource
    ISSN: 0739-0572 , 1520-0426
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 1998
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  • 2
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 103, No. D14 ( 1998-07-27), p. 17149-17161
    Abstract: Detection of long‐term, linear trends is affected by a number of factors, including the size of trend to be detected, the time span of available data, and the magnitude of variability and autocorrelation of the noise in the data. The number of years of data necessary to detect a trend is strongly dependent on, and increases with, the magnitude of variance (σ N 2 ) and autocorrelation coefficient (ϕ) of the noise. For a typical range of values of σ N 2 and ϕ the number of years of data needed to detect a trend of 5%/decade can vary from ∼10 to 〉 20 years, implying that in choosing sites to detect trends some locations are likely to be more efficient and cost‐effective than others. Additionally, some environmental variables allow for an earlier detection of trends than other variables because of their low variability and autocorrelation. The detection of trends can be confounded when sudden changes occur in the data, such as when an instrument is changed or a volcano erupts. Sudden level shifts in data sets, whether due to artificial sources, such as changes in instrumentation or site location, or natural sources, such as volcanic eruptions or local changes to the environment, can strongly impact the number of years necessary to detect a given trend, increasing the number of years by as much as 50% or more. This paper provides formulae for estimating the number of years necessary to detect trends, along with the estimates of the impact of interventions on trend detection. The uncertainty associated with these estimates is also explored. The results presented are relevant for a variety of practical decisions in managing a monitoring station, such as whether to move an instrument, change monitoring protocols in the middle of a long‐term monitoring program, or try to reduce uncertainty in the measurements by improved calibration techniques. The results are also useful for establishing reasonable expectations for trend detection and can be helpful in selecting sites and environmental variables for the detection of trends. An important implication of these results is that it will take several decades of high‐quality data to detect the trends likely to occur in nature.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1998
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Atmospheres Vol. 102, No. D7 ( 1997-04-20), p. 8737-8754
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 102, No. D7 ( 1997-04-20), p. 8737-8754
    Abstract: Surface ultraviolet (UV) radiation measurements from the Robertson‐Berger (RB) meter network and existing documentation of these data were examined to determine long‐term variations of UV. RB meter data from 14 sites in the United States were analyzed for trends over the period 1974–1991. A more in‐depth analysis of the RB meter data, including the use of supporting geophysical data, was carried out for four of the locations. Results based on analysis of data from the 14 sites show a significant negative trend of the order of −6% per decade overall, reasonably consistent with annual trends obtained by Scotto et al . [1988] using similar data for the period 1974–1985. However, when allowance is made for mean level shifts in the data for several of the stations around 1979, which may be due to calibration and other instrument‐related problems, the resulting overall trend is found to be of the order of +2% per decade and not statistically significant. An additional trend analysis using only RB meter data since 1979 at the 14 sites is also performed and leads to overall trend results similar to those from the analysis which allows for mean level shifts in the data. The more detailed analysis of data from four of the stations for the period 1979–1991 is performed to investigate the extent to which the trend behavior in the RB meter measurements can be explained by the behavior of other geophysical quantities such as cloudiness and total ozone. In particular, radiative transfer model‐based calculations of ultraviolet irradiance based on satellite data from the total ozone mapping spectrometer are compared with the RB meter measurements to help explain their behavior. Generally, inconsistencies are found between the trend behavior in RB meter measurements and radiative transfer calculations, with the RB data showing substantial downward movement relative to the calculations for three of the four sites. Significant evidence exists to indicate that problems with the network render the existing RB meter measurements unreliable for long‐term trend detection. Different reasonable treatments of the data result in dramatically different trend results. Without further information, the data, by themselves, do not allow for definitive trend analysis results.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1984
    In:  Journal of Geophysical Research: Atmospheres Vol. 89, No. D3 ( 1984-06-20), p. 4833-4840
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 89, No. D3 ( 1984-06-20), p. 4833-4840
    Abstract: A statistical analysis of stratospheric ozone profile data from the Umkehr method is considered for the detection of trends which may be associated with the release of chlorofluoromethanes (CFMs), where possible effects of atmospheric aerosols on the Umkehr measurements are also taken into account. In the statistical trend analysis, time series models have been estimated using monthly averages of Umkehr data over the past 15 to 20 years through 1980 at each of 13 Umkehr stations and at each of the five highest Umkehr layers, 5–9, which cover an altitude range of approximately 24–48 km. The time series regression models incorporate seasonal, trend, and noise factors and an additional factor to explicitly account for the effects of atmospheric aerosols on the Umkehr measurements. At each Umkehr station, the explanatory series used in the statistical model to account for the aerosol effect is a 5 month running average of the monthly atmospheric transmission data at Mauna Loa, Hawaii, the only long running aerosol data available. A random effects model is used to combine the 13 individual station trend estimates from the time series models to form an overall estimate of trend for each Umkehr layer. The analysis indicates statistically significant trends in the upper Umkehr layers 7 and 8 of the order of −0.2 to −0.3% per year over the period 1970–1980, with little trend in the lower layers 5 and 6. The results of the estimation of trends as well as aerosol effects for the Umkehr data are compared with recent corresponding theoretical predictions.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1984
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  • 5
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 105, No. D17 ( 2000-09-16), p. 22201-22210
    Abstract: International agreements for the limitation of ozone‐depleting substances have already resulted in decreases in concentrations of some of these chemicals in the troposphere. Full compliance and understanding of all factors contributing to ozone depletion are still uncertain; however, reasonable expectations are for a gradual recovery of the ozone layer over the next 50 years. Because of the complexity of the processes involved in ozone depletion, it is crucial to detect not just a decrease in ozone‐depleting substances but also a recovery in the ozone layer. The recovery is likely to be detected in some areas sooner than others because of natural variability in ozone concentrations. On the basis of both the magnitude and autocorrelation of the noise from Nimbus 7 Total Ozone Mapping Spectrometer ozone measurements, estimates of the time required to detect a fixed trend in ozone at various locations around the world are presented. Predictions from the Goddard Space Flight Center (GSFC) two‐dimensional chemical model are used to estimate the time required to detect predicted trends in different areas of the world. The analysis is based on our current understanding of ozone chemistry, full compliance with the Montreal Protocol and its amendments, and no intervening factors, such as major volcanic eruptions or enhanced stratospheric cooling. The results indicate that recovery of total column ozone is likely to be detected earliest in the Southern Hemisphere near New Zealand, southern Africa, and southern South America and that the range of time expected to detect recovery for most regions of the world is between 15 and 45 years. Should the recovery be slower than predicted by the GSFC model, owing, for instance, to the effect of greenhouse gas emissions, or should measurement sites be perturbed, even longer times would be needed for detection.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2000
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  • 6
    Online Resource
    Online Resource
    American Meteorological Society ; 2000
    In:  Bulletin of the American Meteorological Society Vol. 81, No. 10 ( 2000-10), p. 2341-2357
    In: Bulletin of the American Meteorological Society, American Meteorological Society, Vol. 81, No. 10 ( 2000-10), p. 2341-2357
    Type of Medium: Online Resource
    ISSN: 0003-0007 , 1520-0477
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 2000
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  • 7
    In: Journal of Applied Meteorology, American Meteorological Society, Vol. 42, No. 2 ( 2003-02), p. 266-278
    Type of Medium: Online Resource
    ISSN: 0894-8763 , 1520-0450
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 2003
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  • 8
    In: Bulletin of the American Meteorological Society, American Meteorological Society, Vol. 99, No. 5 ( 2018-05), p. 975-1001
    Abstract: Forecasts by mid-2015 for a strong El Niño during winter 2015/16 presented an exceptional scientific opportunity to accelerate advances in understanding and predictions of an extreme climate event and its impacts while the event was ongoing . Seizing this opportunity, the National Oceanic and Atmospheric Administration (NOAA) initiated an El Niño Rapid Response (ENRR), conducting the first field campaign to obtain intensive atmospheric observations over the tropical Pacific during El Niño. The overarching ENRR goal was to determine the atmospheric response to El Niño and the implications for predicting extratropical storms and U.S. West Coast rainfall. The field campaign observations extended from the central tropical Pacific to the West Coast, with a primary focus on the initial tropical atmospheric response that links El Niño to its global impacts. NOAA deployed its Gulfstream-IV (G-IV) aircraft to obtain observations around organized tropical convection and poleward convective outflow near the heart of El Niño. Additional tropical Pacific observations were obtained by radiosondes launched from Kiritimati , Kiribati, and the NOAA ship Ronald H. Brown , and in the eastern North Pacific by the National Aeronautics and Space Administration (NASA) Global Hawk unmanned aerial system. These observations were all transmitted in real time for use in operational prediction models. An X-band radar installed in Santa Clara, California, helped characterize precipitation distributions. This suite supported an end-to-end capability extending from tropical Pacific processes to West Coast impacts. The ENRR observations were used during the event in operational predictions. They now provide an unprecedented dataset for further research to improve understanding and predictions of El Niño and its impacts.
    Type of Medium: Online Resource
    ISSN: 0003-0007 , 1520-0477
    Language: Unknown
    Publisher: American Meteorological Society
    Publication Date: 2018
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  • 9
    Online Resource
    Online Resource
    American Association for the Advancement of Science (AAAS) ; 1978
    In:  Science Vol. 202, No. 4367 ( 1978-11-03), p. 513-515
    In: Science, American Association for the Advancement of Science (AAAS), Vol. 202, No. 4367 ( 1978-11-03), p. 513-515
    Type of Medium: Online Resource
    ISSN: 0036-8075 , 1095-9203
    RVK:
    RVK:
    Language: English
    Publisher: American Association for the Advancement of Science (AAAS)
    Publication Date: 1978
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  • 10
    Online Resource
    Online Resource
    American Meteorological Society ; 1999
    In:  Journal of Atmospheric and Oceanic Technology Vol. 16, No. 11 ( 1999-11), p. 1736-1752
    In: Journal of Atmospheric and Oceanic Technology, American Meteorological Society, Vol. 16, No. 11 ( 1999-11), p. 1736-1752
    Type of Medium: Online Resource
    ISSN: 0739-0572 , 1520-0426
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 1999
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