Rainfall and El Niño

Guest Post by Willis Eschenbach

In a recent post here on WattsUpWithThat, the claim was made that the El Nino influences rainfall. They showed a correlation between various historical proxies and El Nino/La Nina. So I thought I’d take a look at the modern correlation between rainfall and the El Nino. As a measurement of the El Niño, I’m using the Oceanic Nino Index (ONi).

So, what is the ONI when it’s at home? NOAA says:

Oceanic Nino Index

The Oceanic Nino Index (ONI) is one of the primary indices used to monitor the El Nino-Southern Oscillation (ENSO). The ONI is calculated by averaging sea surface temperature anomalies in an area of the east-central equatorial Pacific Ocean, which is called the Nino-3.4 region (5S to 5N; 170W to 120W). Also, a 3-month time average (running mean) is calculated in order to better isolate variability closely related to the ENSO phenomenon.

SOURCE

OK … although I don’t like the 3-month boxcar filter (running mean). It is known to do things like reverse the peaks and valleys of a dataset, and is a horrible choice. So I’ve used the un-averaged version of the ONI

Now, I’ve written about the relationship between temperature and rainfall before, in “Cooling and Warming, Clouds and Thunderstorms” and in “How Thunderstorms Beat The Heat” The TLDR version is that over the ocean, where most of the rain falls, the rainfall amounts go up with increasing temperature. The evaporation of the water to make rain is one of the major mechanisms that keeps the ocean from overheating.

But I digress, I’m here to discuss the El Niño and the Oceanic Nino Index. The paper made a curious claim, that La Nina conditions were wetter, and El Nino conditions were dryer. Here’s the graphic from their paper:

(a) Flores LLPC1 record. (b) Marine foraminifera δ18Osw (ref. 5) and (c) terrestrial δDleaf-wax (ref. 6) records recovered from marine sediment cores located in the Makassar Strait on the Sulawesi margin. (d) δ18O of lake sediment calcite in Laguna Pumacocha in the central Peruvian Andes (proxy for the strength of the South American summer monsoon)44. (e) Speleothem δ18O record from Cascayunga cave in northeast Peru46. (f) δDleaf-wax record from Washington Island in the central equatorial Pacific8. (g) Red-colour intensity from Laguna Pallcacocha, southern Ecuador47. (h) Percent sand in El Junco lake, Galápagos Islands10. For clarity, all records have been converted to standard (z) scores with blue indicating wetter conditions (a–f) or heavier precipitation events (g–h) and vice versa for red. Vertical bars indicate the approximate timing of the MCA (yellow), LIA (blue) and CWP (pink) in Flores.
(a) Flores LLPC1 record. (b) Marine foraminifera δ18Osw (ref. 5) and (c) terrestrial δDleaf-wax (ref. 6) records recovered from marine sediment cores located in the Makassar Strait on the Sulawesi margin. (d) δ18O of lake sediment calcite in Laguna Pumacocha in the central Peruvian Andes (proxy for the strength of the South American summer monsoon)44. (e) Speleothem δ18O record from Cascayunga cave in northeast Peru46. (f) δDleaf-wax record from Washington Island in the central equatorial Pacific8. (g) Red-colour intensity from Laguna Pallcacocha, southern Ecuador47. (h) Percent sand in El Junco lake, Galápagos Islands10. For clarity, all records have been converted to standard (z) scores with blue indicating wetter conditions (a–f) or heavier precipitation events (g–h) and vice versa for red. Vertical bars indicate the approximate timing of the MCA (yellow), LIA (blue) and CWP (pink) in Flores.

Figure 1, with Original Caption

Now I was born yesterday, but having lived in the South Pacific I do know that there is no general rainfall rule for El Nino and La Nina. Some places like Southern California get wetter in an El Nino year, and some places like Australia get drier. So I found it odd that they identified “wetter” with La Nina and “drier” with El Nino. I thought I’d look at the correlation between the amount of rainfall and the Oceanic Nino Index (ONI). Figure 2 shows that result. A positive correlation (yellow to red) means that a high ONI index (El Nino condition) is accompanied by increased rain. A negative correlation (green and blue), on the other hand, means the opposite—there is less rain during El Nino conditions. The correlation (both positive and negative) with rainfall is at a maximum three months after the change in the ONI.

correlation rainfall and oniFigure 2. Correlation of the monthly Oceanic Nino Index (ONI) with the amount of monthly rainfall, 2000-2015. Red box shows the area which is represented by the ONI. Red/white circles show the locations of the proxies shown in Figure 1.

This shows what I started out by saying, which was that an El Nino increases the rain in Southern California and decreases the rain in Australia. In other words, we cannot say “Wet/La Niña-like” or “Dry/El Niño-like” as the authors do.

It also shows the idiosyncratic and convoluted nature of the area of positive and negative correlation. For example, the ONI is generally positive correlated with the northern hemisphere rainfall, and negatively correlated with southern hemisphere rainfall.

Now, the authors of the study say:

The composite record shows pronounced shifts in monsoon rainfall that are antiphased with precipitation records for East Asia and the central-eastern equatorial Pacific. These meridional and zonal patterns are best explained by a poleward expansion of the Australasian Intertropical Convergence Zone and weakening of the Pacific Walker circulation (PWC) between ~1000 and 1500 CE.

I see no need to invoke any such special mechanisms to explain rainfall shifts that are “antiphased” to rainfall shifts in other areas. From an examination of Figure 2 above, such antiphasing is the rule rather than the exception. In La Niña times California gets drier, Australia gets wetter, and the world goes on.

Regards to all on a sunny evening,

w.

My Usual Request: Misunderstandings can be avoided. If you disagree with me or anyone, please quote the exact words you disagree with, so we can all understand the exact nature of your objections. I can defend my own words. I cannot defend someone else’s interpretation of some unidentified words of mine.

My Other Request: If you believe that e.g. I’m using the wrong method or the wrong dataset, please educate me and others by demonstrating the proper use of the right method or the right dataset. Simply claiming I’m wrong about methods doesn’t advance the discussion unless you can point us to the right way to do it.

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Latitude
June 11, 2016 8:08 am

Here’s the graphic from their paper:
====
Honest question….
On their graphic, they have boxed in the LIA…..
…but according to their graphic, the LIA does not end a little past 1800
Their own graphic shows the LIA ending around 1950
First they claim when the LIA ended…
…and then blame all of the recovery after that on man’s fault

BFL
June 11, 2016 9:02 am

Would there be different/more noticeable conditions such as rain/dry during the change over between the two since that (perhaps) is when the cold/warm air masses react together more often?

K. Kilty
June 11, 2016 9:12 am

In looking back at the effects of El Nino since 1946 I was surprised that I could not find a consistent effect on precipitation in Northern Colorado/Southern Wyoming. Some El Ninos leave this area wet and sometimes dry–no clear pattern. During this most recent event I think I observed what explains this. During this recent El Nino we experienced a persistent northerly flow over Wyoming and Colorado in which the clash of warm/cold air occurred over the border region (from the I-70 corridor to I-80). Thus, Northern Wyoming was cold and dry, the border region wet and cold, and southern Colorado/northern New Mexico was dry and warm–the boundary between regimes being quite abrupt. Depending on circumstances, perhaps El Nino strength or location E/W in the Pacific, this pattern might shift north or south.

Reply to  K. Kilty
June 11, 2016 11:09 am

The patterns can move hundreds of kms from event to event. The general pattern is still there but it might have shifted by a few hundred kms north south east west.

John Harmsworth
June 11, 2016 10:17 am

I believe I read somethng on this site a few weeks ago that might be relevant. If I remember accurately the post said that in some el nino years the mass of warm surface water doesn’t make it all the way to the coast and as a result the rain tends to fall off or near the coast rather than more inland.
Obviously there are other major weather systems that interact but the el nino/LA Nina systems are beginning to be better understood and provide a good starting point for untangling the fantastic intricacies of global weather. Heat goes in at the tropics and drives a chaotic process in three dimensions while finding its way upward, poleward and back out.
Climate scientists should pull the plug on computer models and do some basic work on the slightly simpler subsystems.

June 11, 2016 11:26 am

A running mean does more than just distort locally. The “irregularities” it is used to suppress are not noise but information. More specifically, the sharp “noise” peaks it wipes out are the ENSO oscillation, manifesting itself as El Nino peaks with La Nina valleys in between. People simply don’t think about that because “out of sight, out of mind.” applies. It never occurs to them to ask why the entire hundred fifty year global temperature graph is covered by shark teeth spaced five years apart. I had a few things to say about that in a comment I attached to their paper.

June 11, 2016 2:52 pm

Does not El Nino happen at different times of the year?The impact of each occurance must have to take account of this.

June 11, 2016 3:22 pm

Wills wrote, “The paper made a curious claim, that La Nina conditions were wetter, and El Nino conditions were dryer.” I don’t agree! The figure Willis labeled as Figure 1 (it’s actually Figure 4) only shows that, for the locations indicated, La Niñas tend to be wetter.
Nick Stokes pointed out correctly that their real Figure 1 shows that the authors were well aware of the fact that Los Niños make it drier some places and wetter other places. They are not claiming that there is less rain globally.
Willis missed the whole point of the paper, which is that the paleoclimate record shows that there are large climate fluctuations that occur on century time scales and which can effect global temperature. In the discussion at the end of the paper the authors state, “Our analysis of multicentury hydroclimate variability suggests that projections of tropical rainfall patterns, and global temperature extremes, will remain uncertain until paleoclimate records and models consistently capture the lower-frequency variability, and associated feedbacks, in the tropical Pacific.”
This implies that it is possible that all, or almost all, of the current warming (mild though it is) could be due to low-frequency variability that climate models do not capture. I think that’s an important finding, although it’s not the first paper to show such evidence.

June 11, 2016 5:15 pm

The whole thing is now a funding vehicle with advanced running gear to the1982/3 model.
Previously El Nino only referred to the Australian dry season which encompassed autumn through early spring. It was only called off-on at the end of any given year and there was no such thing as an El Nino summer, nor an El Nino for New Zealand, North America or Britain – in fact it only drove to Peru!
The Mustang GT350 is not the old ’82 Cortina.
The latest El Nino model purrs along at a billion dollars a day; with sea-level stabilisers, a global-warming gearbox and a climate-change clutch. It is fuelled by alarmism, driven by politicians and self-adjusts to inflation.

dlb
June 11, 2016 5:46 pm

From Lu et al 2007 http://dx.doi.org/10.1175/JCLI4227.1 “The ENSO events generally do not impact the tropical total rainfall, but rather induce significant anomalies with opposite signs over tropical land and ocean”
hence:
Boening et al 2012 DOI: 10.1029/2012GL053055 “ Global mean sea level (GMSL) dropped by 5 mm between the beginning of 2010 and mid 2011”, “This temporary shift of water from the ocean to land is closely related to the transition from El Niño conditions in 2009/10 to a strong 2010/11 La Niña, which affected precipitation patterns world-wide.”
and
http://www.drroyspencer.com/2016/03/record-rainy-cloudy-humid-february-over-the-oceans/

Carla
June 11, 2016 6:34 pm

In La Niña times California gets drier, Australia gets wetter, and the world goes on.
Regards to all on a sunny evening,
w.
—————————————————–
Enjoy the sunny evening.
For our viewing pleasure tonight, a cloud, that is being called, “da mutter ship.”
http://www.spaceweather.com/images2016/11jun16/lenticular.png
Larger version available at http://www.spaceweather.com .
THE ‘MOTHERSHIP’ OVER MT. TOM: On the evening of June 9th, a spectacular array of UFO-shaped clouds appeared above California’s Eastern Sierra mountain range. The display was a sensation on social media as people in nearby valleys began posting pictures of the sunset-colored armada. One photographer, however, was in the mountains; ultrarunner Jeff Kozak of Bishop CA captured this edge-on view from 11,100 feet:
http://www.spaceweather.com/images2016/11jun16/lenticular.png
I was topping out on Morgan Pass at sunset when I looked south to see what I thought was The Mothership hovering over Mt Tom!” says Kozak.
In fact, it was a lenticular cloud. Lenticular clouds form downwind of mountain ranges where the air organizes itself into starship-sized waves. Although they appear stationary, moist air is constantly moving through them, condensing at the apex of the wave. Wind scults the clouds into giant saucers and voilà–spaceships in the sky.
Larger version available at http://www.spaceweather.com .
Note: Still looking for a rotation mechanism, as one of the contributing mechanisms, for ENSO changes.
1972-1980 9 Leap seconds added.
1980-1990 7 ” ” ”
1990-2000 6 ” ” ”
2000-2010 2 ” ” ” (1 in ’05’ and 1 in ’08’)
2010-2016 2 ” ” ” (1 in ’12’ and 1 in ’15’)
Earth was in a slowdown period before 1990’s. Since 1990’s has gathered some momentum.
Taken from: THE IERS BULLETIN C
AND THE PREDICTION OF LEAP SECONDS D. Gambis and the IERS Bulletin C notices given at their website.

JFD
June 11, 2016 7:22 pm

Vuk, posted a pretty good reference to the variability of El Nino impacts around the world. I have correlated it for many decades for the Gulf Coast and far West Texas.

Editor
June 12, 2016 2:30 am

Thanks Willis. Very interesting, very informative (as usual). I had always thought of El Nino patterns as being East-West. Now I see they are North-South.

June 12, 2016 5:22 pm

An ocean driven climate cycles of about 1000 years duration is shown convincingly in the linked study. This study shows an oscillation of about 1000 years wavelength. There appear to be approximately 500 year periods of alternate warm/cold and wet/dry conditions. The oscillation is a Lorenz type butterfly wing oscillator / attractor which alternately hangs in one of two states, or wings – the el nino dominated and the la nina dominated.
https://en.m.wikipedia.org/wiki/Lorenz_system
What is interesting is that these Lorenz millenial oscillations are in different phase in different places. Inter hemispheric bipolar seesawing is evident. The paleo records seem to fall into three categories:
1. North hemisphere like:
Flores, Sulawesi; Warm/dry in MWP, cool/wet in LIA.
2. Southern Hemisphere like:
Galapagos; Cool/wet during MWP, warm/dry in LIA.
3. Chaotically switching between NH and SH regimes: Peru, Ecuador

1sky1
Reply to  Willis Eschenbach
June 13, 2016 1:25 pm

An 11-yr MA will NOT produce any “significant reversal” of the sunspot series itself, whose narrow-band power spectrum is peaked right around 11yrs. Your Parana example shows such reversal only for the RESIDUALS of several prior operations, whose spectrum is peaked apparently at somewhat higher frequencies.
The polarity reversal problem can occur only when there’s significant spectral content at the side-bands of the MA filter. Sadly, “climate scientists” are seldom aware of the spectral structure of the signals they write about and concern themselves only with the MA’s obliteration of signal components corresponding to the length of the MA.

1sky1
Reply to  1sky1
June 14, 2016 3:26 pm

Willis:
By cherry-picking the oldest, pre-Maunder segment of the sunspot series, you’ve managed to show some small, out-of-phase oscillations in the 11-yr MA output. But this is obviously the result of abnormally short cycles in this–the most unreliable–segment of the record. You will not find consistently noteworthy reversals in the more reliable, post-Maunder segment of the record, especially if a ~10.6yr MA is employed on the MONTHLY data. (That is not to say that small wiggles will not be encountered after that periodicity is zeroed out by the MA.) Before claiming I’m 100% wrong, you should at least show the complete smoothed record and recognize that the wiggle polarity is critically dependent upon which side of the first zero in the frequency response of the MA do the sunspot frequencies lie. Having used MAs extensively as a tool for removing periodicities and all their harmonics, I’m 100% confident in that matter.

1sky1
Reply to  1sky1
June 14, 2016 6:04 pm

Willis:
My memory lapse about the name of the minimum in the early 19-th century (Dalton) scarcely affects the fact that the data is unreliable until ca. 1820 and has features not seen afterward. Nor does that alter the analytic fact that phase reversal can occur only when there is significant spectral content at frequencies HIGHER then the first zero of the frequency response, which is always equal to 1/T, where T is the duration of the MA. You are badly mistaken that it results from periods very near T, because those periods are almost entirely reduced to zero amplitude. And my reference to consistently noteworthy reversals was in anticipation of your examining the monthly series with a 127-month MA, which produces a reversal of direction every time that the difference between the current point and that 128 months ago changes sign. Had you done that examination, my meaning would be clear.

robinedwards36
Reply to  1sky1
June 15, 2016 2:38 am

Following all this lively stuff on smoothing, with strongly held opinions that do not sit well together, is it not fairly clear that the science of “smoothing” is less than settled? some interesting technical aspects have been discussed quite heatedly in this thread, though I don’t recall seeing anything on the problem of starting and end points of time series.
Some postings recommend what seems to me to be rather obvious – to avoid “smoothing” and to use original observations to support ones ideas, or hopes, rather than simply discard, to a greater or lesser extent, observations that do not run in good (sequential) accord with other related observations.
Clearly, careful scrutiny of recorded observations is essential. There are several reasons why. The primary one is a technical mistake in the technology. The next most likely one (in my experimental experience) is digit transposition, like 27 instead of 72. This would probably be rather obvious to the careful experimentalist, but 56 and 65 rather less so.
I think that we have to take it as read that mistakes – and in the case of climate, deliberate ones – could occur, but that we just do not know for certain where they are.
In my analyses I avoid smoothing the original data, unless simply to replicate what others have done and thus assure myself that I am examining the same published data. Unless one knows otherwise an observation is an observation and deserves respect. The diagrams that I produce, always using the original data, but cannot publish here, disclose (I think) features of complex time series that are not apparent to most people who scrutinise the same data, but which I believe are pertinent to the understanding of what can be expected from careful time series analyses of climate related data, and what can not. The important one in my opinion is that climate time series should /never/ be extrapolated beyond very few (perhaps 3) time steps. You can never be sure about what might happen!
At the final stage of many data analyses – climate in particular – smoothing in the form of fitting a (linear?) model is unavoidable, if simply to pre-digest very complex information into something that can be handled by the primitive digestive systems that are typical of the MSM and politicians, before they spew out their heavy type headlines to the general public.
I’m learning interesting stuff from this thread. Let’s keep it running!

1sky1
Reply to  1sky1
June 15, 2016 4:38 pm

robin:
The question whether to “smooth” or otherwise filter data is inextricably
related to the intrinsic nature of the data and the purpose thereof. If
the data contain no extraneous, confounding signal components and
demonstrate a high S/N ratio, there is no reason to filter. But that is
seldom the case with real-world geophysical data, where several unrelated
physical processes are often at play and the observations may be very
noisy. Indeed, very much different physical processes are found in
different frequency ranges of the power density spectrum of sea-surface
elevation, where sea level changes, tidal variations, long waves and
sea-swell superimpose upon each other. Frequency discrimination filtering
is often required to isolate the signal of interest in the time domain. And
even when there are no confounding components, strong high-frequency
fluctuations or noise can usefully reduced by judicious smoothing. (See,
e.g.,http://www.sidc.be/silso/dayssnplot.)
Instrument response characteristics usually smooth the highest frequencies.
Sunspot data are gathered daily, but are usually decimated into monthly or
yearly averages by simply subsampling corresponding MAs. Ironically, these
smoothings are ignored by those who preach the naïve mantra of: “NEVER
analyze smoothed data,” while manifesting little comprehension of the
spectral structure of the signal or the effects of noise. One can, of
course, resort to purely spectral techniques of analysis upon the raw data, but there is little demonstrated such proficiency in climate science, where presentation of results and of signal relationships is almost always done exlusively in the time domain. Nevertheless, the key to proper analysis of filtered data lies in fully comprehending the effects of the over-all frequency response.

1sky1
Reply to  1sky1
June 15, 2016 5:27 pm

Willis:
Instead of presuming to know the quirks of my memory, you should examine your own. At the outset I wrote about not producing any “significant reversal” of the sunspot series. You now claim, that I simply said “would not have a reversal”–without any qualification. This after I took pains to explain exactly when a reversal CAN take place. And then you dismiss that mathematically proven explanation as “hogwash.” Ironically, you then have the temerity to turn around and resort to that same explanation, but in different words, as your very own. Finally, only the tendentiously blind would claim that the 127-month smoothed series doesn’t show any, albeit tiny, reversals beyond those seen in the 11-year smoothing.
Such high-school polemical tactics are no substitute for producing the ENTIRE post-Dalton record of the 127-month smoothing., or for comprehending indisputable analytic facts. I’ll try to find more time tomorrow to explain what that smoothing really shows.

1sky1
Reply to  1sky1
June 16, 2016 4:44 pm

Despite the ability of the negative side-bands of the frequency response of
moving averages to invert the polarity of certain frequency components,
there are strong clues that something else is happening with the smoothed
sunspot data.
The first and strongest clue is the lack of any consistency of appearance of
out-of-phase wiggles. Even in Willis’ cherry-picked stretches of record,
and contrary to his earlier claim that “the 11-year running mean totally
reverses the peaks and valleys of the sunspot data,” they appear primarily
over the troughs of the unsmoothed data, often without corresponding
inversion under the peaks. No linear filter can produce such disparate
response at peaks and troughs. Furthermore, it’s apparent (particularly in
the monthly data) that the timing of actual reversal is not exactly
coincident with the troughs. Since no MA can change the phase relationship
by any amount other than 180 degrees, this points elsewhere than simple
inversion of appreciably higher-frequency signal components.
This suspicion is only reinforced by noting that some of the wiggles seem to
exceed ~10% of the original wave-height of the data, despite the analytic
fact that the amplitude response stays below 0.1 at all frequencies within
10% of the first zero of the M-point MA response function
H(f)= sin(M*pi*f)/(M*sin(pi*f)) for normalized frequency f 0.01 can produce a “beat frequency” matching the
visible centennial-scale grouping of Schwabe cycles and their attendant
minima.
What seems to explain the wiggles more convincingly is the persistent asymmetry of the Schwabe cycle, with more rapid rises than falls. Such asymmetry necessitates that there be significant spectral components well out-of-phase with the peak of the waveform. Also, the asymmetric shallowing of the troughs relative to the peaks requires net positive contributions from components concealed from the eye in the original data. They emerge into view, however, as a feature of the well-known Gibbs phenomenon when the major components of the Schwabe cycle are annihilated by the near-zero response of the MA. That inherent aspect of Fourier composition is notorious for producing features not at all visible in data.
I’ll conclude my comments tomorrow.

1sky1
Reply to  1sky1
June 16, 2016 4:46 pm

My comment disappeared again.

1sky1
Reply to  1sky1
June 17, 2016 3:45 pm

Failure to comprehend the essentials of the Fourier composition of signals
and noise leads to much confusion about the effects of smoothing,
particularly by MAs. The Slutsky effect, which is related to the Gibbs
phenomenon, is frequently misinterpreted by signal-analysis novices as
producing spurious features not at all present in the data. In fact, the
output of all filters is a strictly deterministic product of the data. In
the case of linear filters, the frequency of all components is unchanged;
only their and amplitude and phase are changed by the (generally complex)
frequency response function.
This should put to rest Willis’ ludicrous notion that “a smoother (such as
the 11-year running mean that they used on the Parana data above) merely
redistributes the energy present in the signal. A filter, on the other
hand, actually removes energy from the signal.” He then comes to the
multiply wrong conclusion: “The net result is that we end up with some of
the frequency data aliased into the average as amplitude data.” In fact,
there is no inherent difference between MAs and other low-pass filters other than
their frequency responses.
Certainly, MAs are far removed from ideal, positive definite low-pass
filters. But obtaining the latter (e.g., binomial filters) requires far
longer convolution kernels, with attendant greater loss of output to end
effects, to achieve the same frequency cut-off. Similarly greater losses
are incurred when cascading MAs to minimize the side-band ripples. MAs are
best viewed as simple, first-cut low-pass filters. Where they excel,
however, is in totally annihilating strictly T-periodic components by
virtue of their exact zero-response at 1/T and all higher harmonics.
They are thus the filters of choice in eliminating diurnal and annual
cycles.
Despite the negative side-bands of frequency response, the efficacy of
removing the 11-yr Schwabe cycle to reveal otherwise hidden
lower-frequency components is apparent at a glance in all of Wiilis’ figures
presented here. While railing against presumed, but unproven, inversions of
the Schwabe cycle by the 11-year MA, he totally fails to recognize tbat it’s not for that narrow-band cycle, but for these wide-band, lower-frequency components of the sunspot record that the authors of the paper claim high correlation with Parana River flow. That makes for a polemical tempest in a teapot, rather than credible geophysics.

1sky1
Reply to  1sky1
June 17, 2016 5:06 pm

Moderator:
Your delayed posting of my comment at 4:44pm yesterday deleted the following passage immediately after the phrase “frequency <= 0.5" on the previous line : "It can be shown that there's simply too little spectral content in the sunspot series beyond such a narrow frequency interval (centered at ~10.6yrs) to produce such strong wiggles by inversion consistently. Indeed,…" Please rectify this meaning-destroying elision.

1sky1
Reply to  1sky1
June 18, 2016 1:44 pm

Instead of simply inserting the passage I indicated in my comment to the Moderator yesterday, the third paragraph of my June 16 4:44pm comment was mangled even further. In its entirety, that paragraph should read:
“This suspicion is only reinforced by noting that some of the wiggles seem to
exceed ~10% of the original wave-height of the data, despite the analytic
fact that the amplitude response stays below 0.1 at all frequencies within
10% of the first zero of the M-point MA response function
H(f)= sin(M*pi*f)/(M*sin(pi*f)) for normalized frequency f 0.01 can produce a “beat frequency” matching the
visible centennial-scale grouping of Schwabe cycles and their attendant
minima.”.

1sky1
Reply to  1sky1
June 18, 2016 1:48 pm

Try again to post the original third paragraph:
This suspicion is only reinforced by noting that some of the wiggles seem to
exceed ~10% of the original wave-height of the data, despite the analytic
fact that the amplitude response stays below 0.1 at all frequencies within
10% of the first zero of the M-point MA response function
H(f)= sin(M*pi*f)/(M*sin(pi*f)) for normalized frequency f 0.01 can produce a “beat frequency” matching the
visible centennial-scale grouping of Schwabe cycles and their attendant
minima.

1sky1
Reply to  1sky1
June 18, 2016 1:53 pm

The persistent mangling is bizarre! Let’s try posting again, but with the line contining the formula placed at the end here.This suspicion is only reinforced by noting that some of the wiggles seem to
exceed ~10% of the original wave-height of the data, despite the analytic
fact that the amplitude response stays below 0.1 at all frequencies within
10% of the first zero of the M-point MA response function
It can be shown that there’s simply too little spectral content in the
sunspot series beyond such a narrow frequency interval (centered at
~10.6yrs) to produce such strong wiggles by inversion consistently. Indeed,
no frequency separation > 0.01 can produce a “beat frequency” matching the
visible centennial-scale grouping of Schwabe cycles and their attendant
minima.
H(f) = sin(M*pi*f)/(M*sin(pi*f)) for normalized frequency f <= 0.5

1sky1
Reply to  1sky1
June 18, 2016 1:58 pm

The third try seems to the charm. It’s astonishing how WordPress can mangle a comment containing a separate line of mathematical formula.

1sky1
Reply to  Willis Eschenbach
June 13, 2016 1:28 pm

Why has my response disappeared without a trace?

1sky1
Reply to  Willis Eschenbach
June 13, 2016 5:10 pm

Don’t have time to replicate my original response. Suffice it to say that an 11-yr MA does NOT produce “significant reversal of oscillations” in sunspot data, which has a narrow-band power spectrum concentrated near 11 years. Your Parana examples apply the MA not to sunspot data, but to RESIDUALS, whose spectrum obviously contains higher-frequency content. Furthermore, MJO is a high-frequency oscillation which doesn’t even dominate the atmospheric record, let alone the Oceanic Nino Index, whose very wide-band spectrum is peaked near 5.5 yrs. A 3-month seasonal data smoothing does negligible harm in examining relationships to ENSO.

1sky1
Reply to  Willis Eschenbach
June 13, 2016 5:16 pm

My abbreviated duplicate response of a few minutes ago has likewise disappeared. I won’t waste any more time in the face of such pitiful evasions.

James at 48
June 13, 2016 10:25 am

ENSO during positive PDO seems to behave more reliably than ENSO during a negative PDO.