The chief purpose of the present survey is to look into further into the association between entire ozone ( TOZ ) and 11-year solar rhythm ( SC ) , during the period 1979 - 2010 by using satellite observations of TOZ and impulse flux ( MF ) . A positive correlativity between the one-year mean entire ozone ( TOZ ) over both hemispheres and macula figure ( SN ) is found. On the contrary, concentrating on the January and February mean monthly TOZ fluctuations from the equator to the high latitudes, of the Northern Hemisphere no association between TOZ and SN is derived. It is attributed to the being of the quasi-biennial-oscillation ( QBO ) and the El Ni & A ; ntilde ; o-Southern oscillation ( ENSO ) in TOZ clip series, . However, when sing TOZ over the zonary agencies centred at 17.5 & A ; deg ; N and 27.5 & A ; deg ; N and SN during the old ages of the east stage of QBO in the equatorial zonary air current at 50hPa, a important correlativity between TOZ and SN reveals. These findings are of important importance because solar radiation is a major driving force of the clime system.
Several surveies have shown that fluctuations in the 11-year solar irradiance and subsequent UV soaking up by ozone cause alterations in temperature and air current in the upper stratosphere ( Crooks and Gray, 2005 ; Alexandris et Al. 1999 ; Kondratyev and Varotsos 1996 ; Katsambas et Al. 1997 ) . These comparatively weak direct alterations could change the upward extension of planetary-scale moving ridges and lead to an indirect feedback on the lower ambiance through a alteration of the stratospheric mean circulation - Brewer- Dobson circulation ( Gernandt et al. 1995 ; Kodera and Kuroda, 2002 ; Tzanis and Varotsos, 2008 ; Cracknell and Varotsos 1994, 1995 ; Efstathiou et al. , 2003 ; Gernandt et al. , 1995 ; Varotsos, 2002, 2005 ; Varotsos et Al. 1994 ; Varotsos 1989, 2004 )
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Matthes et Al. ( 2010 ) indicated that the one-year mean solar response in temperature and ozone in the upper stratosphere is in qualitative understanding with other mold and experimental surveies and does non depend on the presence of the imposed quasi-biennial oscillation ( QBO ) of equatorial air current. However, the solar response in the center to take down stratosphere differs significantly for the two QBO stages. During solar maxima a weaker Brewer-Dobson circulation with comparative downwelling, warming, and enhanced ozone occurs in the tropical lower stratosphere during QBO east conditions, while a stronger circulation, chilling, and decreased ozone exists during QBO west conditions. During QBO east, the combination of production and advection resulted in the net ozone addition, whereas during QBO west, the effects cancel each other and consequence in small net ozone alterations. Matthes et Al. ( 2010 ) showed besides that during Southern Hemisphere ( SH ) tardily winter to early spring, the solar response at polar latitudes switches mark between the two QBO stages and qualitatively confirms observations and other recent theoretical account surveies.
Lu et Al. ( 2009 ) proposed some penetrations on the QBO modulated 11-year solar rhythm signals in Northern Hemisphere ( NH ) winter temperature and zonary air current. They used day-to-day ERA-40 Reanalysis and ECMWF Operational information for the period of 1958-2006 in order to analyze the seasonal development of the QBO-solar rhythm relationship at assorted force per unit area degrees up to the stratopause. The consequences showed that the solar signals in the NH winter extratropics are so QBO-phase dependant, traveling poleward and downward as winter progresses with a faster descent rate under westerly QBO than under eastern QBO. In the stratosphere, the signals seemed to be extremely important in late January to early March and have a life p of ?30-50 yearss. Under western QBO, the stratospheric solar signals clearly lead and connected to those in the troposphere in late March and early April where they have a life p of ?10 yearss.
Sitnov ( 2009 ) utilizing entire ozone informations obtained in the period of 1957 - 2007 at 10 ground-based European Stationss, investigated the effects of the QBO and 11-year solar rhythm, attesting in entire column ozone. In this work, it was derived that solar activity modulates the stage of the QBO consequence so that the quasi-biennial entire ozone signals during solar upper limit and solar lower limit are about in opposite stage. It was besides demonstrated that stray under lasting conditions of solar lower limit or solar upper limit the QBO effects in entire ozone have the clip graduated table of about 20 months.
Titova and Karol ( 2010 ) holding applied the method of discriminant analysis to the TOMS informations of satellite sounding of the entire ozone content ( TOC ) in the March months of 1979-2008, attempted to do a new estimation of the TOC field variableness in the Northern Hemisphere and inter-longitudinal regularities of its alterations under the action of climatic variableness. The effects of temperature fluctuations in the polar stratosphere, El Ni & A ; ntilde ; o -Southern Oscillation ( ENSO ) and QBO seemed to be comparable and make 80 DU in some parts. Titova and Karol ( 2010 ) besides proposed that the parts of TOC fluctuations and their location and dimensions change depending on the stages of QBO, AO, and ENSO. Three parts of increased TOC-over Europe, Eastern Siberia, and the Pacific Ocean-are formed in old ages with a warm stratosphere. A counterbalancing TOC lessening takes topographic point in the Torrid Zones and over Greenland. In the old ages of El Ni & A ; ntilde ; O and the eastern QBO stage, the TOC increases over Europe and drops over the cardinal Pacific, every bit good as to the South from 45 & A ; deg ; N.
Ziemke et Al. ( 2010 ) established an ENSO index utilizing column ozone informations measured in tropical latitudes from Nimbus 7 TOMS, Earth Probe TOMS, NOAA SBUV, and Aura OMI orbiter instruments. This index, which covered a clip period from 1979 to the present, was defined as the Ozone ENSO Index ( OEI ) and it was the first developed from atmospheric hint gas measurings. OEI was constructed by first averaging monthly average column ozone over two wide parts in the western and eastern Pacific and taking their difference. The combined Aura OMI and MLS ozone informations confirmed that zonary variableness in entire column ozone in the Torrid Zones caused by ENSO events lies about wholly in the troposphere. As a consequence, OEI can be derived straight from entire column ozone alternatively of tropospheric column ozone. For clear-sky ozone measurements a +1 K alteration in Nino 3.4 index corresponds to +2.9DU ( Dobson Unit ) alteration in OEI, while a +1 hPa alteration in Southern Oscillation index coincides with a ?1.7DU alteration in the OEI. For ozone measurings under all cloud conditions these Numberss are +2.4DU and ?1.4DU, severally.
Soukharev ( 1997 ) analyzing the monthly agencies of entire ozone, in months January to March between 1973 - 1995 on five Stationss in Northeastern Europe, indicated statistically important correlativities between the fluctuations of entire ozone in February and, partly, in March, and the SN during the different stages of QBO. Similar correspondence was established between the index of stratospheric circulation and SN sing the QBO stage. Based on the obtained correlativities between the interannual fluctuations of ozone and stratospheric circulation index, Soukharev concluded that a connexion between solar rhythm - QBO - ozone occurs through the kineticss of stratospheric circulation.
Varotsos ( 1989 ) analyzing the planetary TOZ, during the period 1958-1984, suggested that there was non any apparent connexion between TOZ and 10.7 centimeter solar flux ( F10.7 ) . However, when the informations were separated harmonizing to the E or west stage of QBO in the equatorial stratosphere, it was derived that entire ozone was positively correlated ( anticorrelated ) with the solar rhythm, during the West ( east ) stage of QBO.
The chief purpose of this work is to research farther the association between TOZ and solar activity, from the equator to the high latitudes in both Hemispheres over the last three solar rhythms.
Datas and analysis
QBO informations used in the present paper were calculated at the NOAA Earth System Research Laboratory-Physical Science Division ( NOAA/ESRL-PSD ) from the zonary norm of the 30mb zonary air current at the equator. Those informations were computed from the NCEP/NCAR
Additionally, the average monthly macula Numberss ( SN ) derived from the datasets of the National Geophysical Data Center ( NGDC ) , during the period January 1749 - October 2009, were employed.
TOZ informations set, was obtained from Nimbus-7, Meteor-3, and Earth Probe Total Ozone Mapping Spectrometer ( TOMS ) and Ozone Monitoring Instrument ( OMI ) , covering the period 1979-2010 ( with measuring spreads for several months of the old ages 1994, 1995 and 1996 ) .
Momentum Flux ( MF ) measurings between 45 & A ; deg ; N and 75 & A ; deg ; N, through 1979 - 2010, obtained by the National Aeronautics and Space Administration Goddard Space Flight Center, were besides used.
Finally, Ozone ENSO index ( OEI ) measurings obtained by the National Aeronautics and Space Administration Goddard Space Flight Center, Code 613.3 Chemistry and Dynamics Branch, in the Torrid Zones during 1979 - 2010, were employed ( Ziemke et al. , 2010 ) .
All clip series presented in this survey were normalized ( the long-run mean subtracted and so devided by the standard divergence ) and detrended.
Discussion and Consequences
Several surveies argued that when the solar UV radiation is stronger, more ozone via the photolysis of O2 would be formed in the upper stratosphere, so that the maximal ozone degree would happen at the maximal solar activity. Very late, Haigh et Al. ( 2010 ) have noticed that during the worsening stage of the most recent '11-year ' solar rhythm ( occurred during 2002-2009 ) there was a four to six times larger diminution in UV than would hold been predicted on the footing of our old apprehension. Haigh et Al. ( 2010 ) suggested that this decrease was partly compensated in the entire solar end product by an addition in radiation at seeable wavelengths. More unusually, they have besides showed that these spectral alterations appear to hold led to a important diminution from 2004 to 2007 in stratospheric ozone below an height of 45 kilometers, with an addition above this height.
Therefore, it is interesting to re-visit the probe of the influence of the solar activity to the column ozone variableness on a planetary and hemispheric footing.
The entire ozone and solar rhythm on a planetary and hemispheric footing
Along the lines above the 11-year solar rhythm and the TOZ one-year average fluctuations over the Earth, the NH and the SH, during the last solar rhythms are shown in Figure cubic decimeter ( a ) , ( B ) , ( degree Celsius ) , severally. Inspection of Figure 1 shows that an evident solar rhythm is outstanding in the TOZ information. To quantify this association the correlativity coefficients were calculated and derived statistically important ( at 95 % assurance degree ) by utilizing the non-parametric Spearman method.
Figure 1. Annual average TOZ and macula figure ( as a placeholder for the 11-year solar rhythm ) over ( a ) the Earth, ( B ) the northern hemisphere, ( degree Celsius ) the southern hemisphere, during 1979 - 2010. TOZ and SN clip series have been normalized and detrended.
This in-phase March of TOZ and solar activity is non surprising and it is rather consistent with the current apprehension about the solar forcing in TOZ kineticss. Harmonizing to this, the upper stratospheric ozone response ( 2-3 % between solar lower limit and solar upper limit ) is a direct radiative consequence of warming and photochemistry. The lower stratospheric solar rhythm in tropical ozone appears to be caused indirectly through a dynamical response to solar ultraviolet fluctuations. However, the beginning of such a dynamical response to the solar rhythm is non to the full understood ( WMO 2010 ) .
The entire ozone on the wintertime Northern Hemisphere and solar rhythm
To acquire a better apprehension of the afore-mentioned dynamical TOZ response, the probe of the plausible relationship between TOZ and solar activity would be performed at the wintertime government of the ambiance. Of class, during winter months, the solar rhythm signal is weak compared to big atmospheric fluctuations and the signal is hence more hard to pull out ( Labitzke and new wave Loon, 1988 ) . In an effort to farther research this job, the fluctuations of the average TOZ over the NH during January/February and the corresponding SN values during the period 1979 - 2010 are plotted in Figure 2 ( a ) .
Figure 2. ( a ) ( Jan+Feb ) /2 TOZ and SN over the northern hemisphere, during 1979 - 2010. ( B ) The running correlativities ( Rhode Island ) for twelvemonth I between the equatorial zonary air current at 50 hPa and the average TOZ for January and February. TOZ and SN clip series have been normalized and detrended.
The decision drawn from Figure 1 ( a ) is that a quasi-periodic constituent ( 2- 4 year ) in the Northern Hemispheric TOZ clip series reduces unusually the above mentioned correlativity between TOZ and SN fluctuations. To look into whether this taint of the association of the TOZ and SN fluctuations by the QBO is a map of the solar activity the method of running correlativities was employed ( Kodera ( 1993 ) . The consequences obtained are shown in Figure 2 ( B ) where the running correlativities ( Rhode Island ) for twelvemonth I between the equatorial zonary air current at 50 hPa and the average TOZ for January and February do non demo an 11-y signal ( figure 2b ) . Therefore, the above-said taint by the QBO of equatorial air current, is independent of the solar rhythm, upseting any evident association between TOZ and SN.
The latitudinal dependance of the association between the wintertime TOZ and solar rhythm at the Northern Hemisphere
Next, the probe of the possible association between the TOZ and SN is explored as a map of latitude. In this respect, Haigh ( 1994 ) have reported that due to the seasonality, the stratospheric ozone alterations due to solar flux fluctuation are largest at center to high latitudes in the winter hemisphere. Figure 3 ( a-f ) present the January / February mean TOZ and SN from the equator to the high latitudes, during 1979 - 2010. All these figures do non demo any evident correlativity between TOZ and solar activity, due to the taint by the quasi-periodic oscillations ( QBO and ENSO ) in the TOZ clip series.
Figure 3. ( Jan+Feb ) /2 TOZ and SN at ( a ) 7.5 & A ; deg ; N, ( B ) 17.5 & A ; deg ; N, ( degree Celsius ) 27.5 & A ; deg ; N, ( vitamin D ) 37.5 & A ; deg ; N, ( vitamin E ) 47.5 & A ; deg ; N, ( degree Fahrenheit ) 57.5 & A ; deg ; N, during 1979 - 2010. All clip series have been normalized and detrended.
However, the solar response in the winter entire ozone at 17.5 & A ; deg ; N and 27.5 & A ; deg ; N seemed to differ significantly under the two QBO stages.
Other surveies have besides identified solar influences on the strength and extent of the Walker circulation, that is a cell circulation in the zonal and perpendicular waies in the tropical troposphere caused by differences in heat distribution between ocean and land. Meehl et Al. ( 2008 ) and vanLoon et Al. ( 2007 ) showed a strengthening of the Walker circulation, at peak old ages of the 11-year solar rhythm, It should be reminded that when the Walker cell weakens or contraries, an El Ni & A ; ntilde ; o consequences, and when Walker cell becomes strong causes a La Ni & A ; ntilde ; a.
The association between the wintertime TOZ and solar rhythm at the Northern tropics ; the function of the QBO and ENSO
In the followers, the January and February mean TOZ and SN informations were grouped harmonizing to the QBO stages of the equatorial zonary air current at 50hPa and were plotted against the OEI at 17.5 & A ; deg ; N and 27.5 & A ; deg ; N ( figure 4a-d ) .
During the west stage of QBO, a statistically important anticorrelation between TOZ and OEI clip series is evident, ensuing in a quasi periodic constituent that coincides with ENSO ( Ziemke et al. 2010 ) and causes no correlativity between TOZ and SN. On the other manus, during the east stage of QBO, TOZ clip series exhibits the 11-year signal.
Figure 4. ( Jan+Feb ) /2 TOZ and SN at 17.5 & A ; deg ; N during ( a ) the west stage of QBO and ( B ) the east stage of QBO.
( Jan+Feb ) /2 TOZ and SN at 27.5 & A ; deg ; N during ( degree Celsius ) the west stage of QBO and ( vitamin D ) the east stage of QBO. The dotted lines present the OEI through 1979 - 2010 in the West and east stages of QBO. All clip series have been normalized and detrended.
In the undermentioned, figure 5 ( a ) presents the February mean TOZ and SN at 17.5 & A ; deg ; N, during 1979-2010, while figures 5 ( B ) , ( degree Celsius ) show the February TOZ and macula figure when the informations were grouped in the West and east stage of QBO, severally. Inspection of these figures shows an evident correlativity between TOZ and the 11-year solar rhythm, during QBO east ( statistically important correlativity at 95 % assurance degree ) . The ENSO constituent is noticeable one time more in the TOZ clip series when the informations were grouped in the west stage of QBO and is anticorrelated with OEI ( figure 5 ( B ) ) .
Figure 5. February average TOZ and SN at 17.5 & A ; deg ; N, through 1979-2010 ( a ) independently of the QBO stages, ( B ) for the western stages of QBO and ( degree Celsius ) for the eastern stages of QBO. The thin line with the symbol ten, in ( a ) , corresponds to the smoothened clip series of the February mean TOZ. All clip series have been normalized and detrended.
Figure 6. ( a ) February mean TOZ at 17.5 & A ; deg ; N against equatorial zonary air current at 50hPa, ( B ) temporal development of QBO upper limit and lower limit, during 1979 - 2010. All clip series have been normalized and detrended.
To analyze farther the part of the QBO in the equatorial zonary air current at 50 hPa to the association between the February TOZ at 17.5 & A ; deg ; N and OEI the figure 6 ( a ) is shown.. Figure 6a shows the statistically important anticorrelation between OEI and TOZ, but no any association of TOZ with QBO. The latter can likely be explained by the fact that TOZ exhibits OEI and it is modulated by the temporal development of QBO upper limit and lower limit. To give an penetration to it Figure 6 ( B ) depicts the temporal development of the difference between consecutive QBO upper limit and [ ( soap ( i+1 ) - soap ( I ) ] and the temporal development of the difference between consecutive QBO lower limit [ min ( i+1 ) - min ( I ) ] for twelvemonth ( I ) . Both the differences in the consecutive upper limit and the differences in the consecutive lower limit of QBO demonstrate the ENSO signal.
The association between the wintertime TOZ and solar rhythm at the Northern high latitudes ; the function of the QBO and ENSO
Finally, in order to research the function of the atmospheric kineticss to the relationship between the TOZ and solar rhythm the interannual variableness of the February mean impulse flux ( MF ) between 45 & A ; deg ; N and 75 & A ; deg ; N at 50hPa, during 1979 - 2010 was studied. , . Figure 7 ( a ) depicts the clip series of MF and SN for February, while figures 7b, degree Celsius show the impulse flux and macula figure when the informations were grouped harmonizing to the QBO stage. Harmonizing to Figure 1 ( degree Celsius ) , during the old ages of the east stage of QBO an evident anticorrelation between MF and the 11-year solar rhythm is observed. A plausible account is the fact that in winter months, the polar whirl is sensitive to equatorial air current. In this context, Salby and Callaghan ( 2000 ) have found that alterations in the polar-night whirl are consistent with the solar signature observed in wintertime records of polar temperature that have been stratified harmonizing to the QBO of equatorial air current.
Figure 7. February average MF and SN between 45 & A ; deg ; N and 75 & A ; deg ; N, through 1979-2010 ( a ) independently of the QBO stages, ( B ) for the western stages of QBO and ( degree Celsius ) for the eastern stages of QBO. All clip series have been normalized and detrended.
Another decision drawn from Figure 7 is that the increased dynamical variableness occurs during the west stage of the equatorial QBO and the winter whirl is significantly weakened during solar upper limit and western stage of the quasi-biennial oscillation.
In this survey, a statistically important correlativity was derived between the one-year mean TOZ and SN over the Earth, the northern and the southern hemisphere, through 1979 - 2010. The evident 11-year signals in TOZ were obtained without any grouping of ozone informations harmonizing to the QBO stages of equatorial air current. Furthermore, sing the January and February mean TOZ and SN over the NH, an obvious quasi-periodic constituent was seen in the TOZ clip series, cut downing perceptibly the above mentioned correlativity between TOZ and 11-year solar rhythm. No evident correlativity was besides derived analyzing the January and February mean TOZ and SN from the equator to the high latitudes, due to the quasi-periodic constituent in the TOZ clip series, caused likely by the quasi-periodic oscillations.
Concentrating on the January and February mean TOZ and SN at 17.5 & A ; deg ; N and 27.5 & A ; deg ; N, TOZ clip series revealed an 11-year signal during the eastern QBO stages and an ENSO signal during the western QBO stages. The correlativity between TOZ and the 11-year solar rhythm, in the east stage of QBO becomes higher for February.
Finally, analyzing the February mean MF between 45 & A ; deg ; N and 75 & A ; deg ; N at 50hPa, during 1979 - 2010, eastern stages of QBO seemed to do an obvious anticorrelation between MF and the 11-year solar rhythm.
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