Paramecia are single-celled microorganisms that can be found in freshwater ponds and other standing water. Aside from the amoeba, the paramecia are probably the most widely known protozoan because of their interesting slipper shape and the fact that they are generally taught in school biology classes as a typical representative of the ciliates.

Like most other ciliates, Paramecia are fairly large for one-celled creatures. At between about 100 to 200 micrometers long, they can almost be seen without a microscope. They are fun to watch under low-power magnification because of their graceful swimming habit and the way they react to obstacles in their path. Long and streamlined, the paramecium glides through the water while twirling around its long axis. When a barrier is encountered, the paramecium reverses motion, swings around to a different angle and then moves forward again. This trial and error strategy is repeated until the paramecium has maneuvered around the obstacle. Just how the paramecium can coordinate the movements of their thousands of individual cilia to accomplish this locomotion, obstacle avoidance and feeding behaviour has yet to be explained.

These ciliates are also interesting in how they reproduce. They have two means of reproduction. One is simple cell division (binary fission or mitosis), where one cell splits itself up into two identical daughter cells. The other reproductive mechanism is conjugation, in which two paramecia come into contact and exchange genetic material in a fairly complex process.

There are several species of paramecia. Most of them don't have many noticeable differences from the others, but one, P. Bursaria, is both strikingly different and very interesting as well. Bursaria are green. That's not because they contain chloroplasts like Euglena or the plants, but because their cells are filled with chlorella, which live inside the paramecia as endosymbiotes.

Domain: Eukarya
Kingdom: Protista
Subkingdom: Protozoa
Phylum: Ciliata (Ciliaphora)
Class: Nassophorea
Subclass: Nassoporia
Order: Peniculida

Peak-to-Peak Dynamics (PPD) is a particular form of deterministic chaos, where, from a n-th order continuous-time dynamical system, the amplitude and time of occurrence of the next peak of its output variable can be predicted from information concerning at most two previous peaks.

Simple PPD have been discovered by famous metheorologist Edward Lorenz in his pioneering 1963 paper on chaos.. Later, PPD have been noticed by various researchers in some fields, like ecology, bio & electrochemistry, physics and electronics.

E.g., remarkably irregular peaks characterize the dynamics of many plant and animal populations. As such peaks are often associated with undesirable consequences (e.g., pest outbreaks, epidemics, forest fires), the forecast of the intensity of a forthcoming peak is a problem of major concern, and has been shown to be most often predictable from the previous peaks, through the analysis of both, simulations of related mathematical models and of some of the longest and most celebrated ecological time series.

Basics

After a transient, any deterministic, dissipative, nonlinear dynamical system settles on an attractor (an equilibrium, a limit cycle, a torus or, most famously, a strange attractor) and remains there forever if it's not perturbed. Some insights about the attractor can be obtained, even in the absence of a formal mathematical model, if a single variable y of time t has been recorded for a "sufficiently long" period, provided that the system was on the attractor. In particular, you can extract from the record all the peaks (i.e., extreme occurrences) of the variable and plot them one peak against the previous one, sequentially, thus obtaining a set of points called Peak-to-Peak Map (PPM), or sometimes also called next-amplitude map, next-maximum map, or, originally, Lorenz map.

If the dynamical regime is periodic (i.e., the system's attractor is a cycle) and there are k peaks per period, the PPM's composed simply of k distinct points. By contrast, if the regime is quasi-periodic (i.e., the system's attractor is a torus) or chaotic (i.e., the system's attractor is a strange attractor), the points on the PPM are all distinct and sometimes display filiform geometries - the points lie on a closed regular curve when there's quasi-periodicity (corresponding to a slice of a torus), roughly on one or more curves¹, when there's low dimensional chaos, and form a cloud-like set when there's high dimensional chaos.

When the PPM is filiform - i.e., when the system's attractor is low-dimensional -, the intensity of the forthcoming peak and its time of occurrence can be predicted with remarkable accuracy from the current peak, when we say the PPD are simple, or from the current + the previous peaks, when we say the PPD are complex (in other words, the forecast of the next peak based solely on the current peak would be ambiguous).

When the set of extracted extreme occurrences is filiform, it can be approximated by a set of curves called Peak-to-Peak Skeleton (PPS), described by a k-value function that can be interpreted as follows: Given a certain peak, the next one's approximately one of the k elements of the function set. When k=1 the PPS is called simple, as well as the underlying PPD. In case the PPD are complex, the extra information needed to accomplish the task (i.e., to forecast the next peak) is a "surrogate" information of the previous peak (i.e., not the previous peak itself), namely knowing if the previous peak was "small" or "large". E.g, in a specific study on plankton-fish interactions it has been shown that the next peak of "young of the year" planktivorous fish, that systematically occurs every year during the summer, can be forecasted on the basis of the current peak + the month during which the previous peak occurred (i.e., the exact date of the occurrence of the previous peak's not needed).

Practical Uses

Once PPD have been identified, the underlying dynamical system (often attached to a model composed by n differential equations) can be described by a very simple reduced order model involving only the peaks of the variable of concern or the corresponding occurrence times.

Identification of attractors

The identification of the attractor of a dynamical system from the observations of a single variable is a problem of major concern, which is usually solved through relatively complex techniques. By contrast, peak-to-peak analysis (i.e., the determination of the PPM associated with a recorded time series) is an almost trivial task that can be even performed by hand. This is also an effective tool for discovering if the dynamics within the attractor can be described by a one-dimensional map. I.e., before performing any analysis of a recorded time series, it's worth extracting its PPM to check if it's really justified to proceed further with more sophisticated (i.e., costly) methods.

Next peak forecast

Although, in theory, forecasting the output peak and the time of occurrence of this peak use equivalent schemes, in practice there's no real equivalence, because the peak amplitude can be known for higher or lower precision than the time of occurrence. E.g., in many ecosystems the time of occurrence of recurrent extreme episodes is well known, while the severity of each episode can be hardly evaluated.

Controlling PPD

In many real-world problems, the peaks of the output variable are associated with high costs, so that it's natural to refer to a reduced order model and formulate an optimal control problem involving only the peaks, their times of occurrences, and the control efforts. Actually, when the peaks are the most crucial episodes, the only available information on the past history of the system are often the times of occurrence of the last peak, fortunately exactly what's needed to forecast the next peak or to exert the control action suggested by the reduced order model.

Challenges

The problem that certainly deserves more attention is the identifiability of PPD from the all-around, real-world, "noisy" field/experimental data, since the structure of the PPM is sensitive to high frequency measurement errors. Of course, this can be somewhat compensated by "filtering" the data before extracting the peaks. General and effective counter-measures to this problem seems to be hard to discover, but the challenge's worth trying. Alternatively, the study of particular cases has been illuminating and suggested how to circumvent particular obstacles. Meanwhile, it seems appropriate to make a combined use of data and models, where a naïve way of proceeding is to use the supporting model only for a qualitative consistency check and/or for a calibration of the simulated PPM with the data. This is certainly justified if the aim is to build an operational forecasting technique based only on information on past peaks.

¹ These PPMs would be thinner if the measurement error, inevitably present during experiments/recordings, would have been smaller.

There's a persistent quasiscientific myth that glass is actually a supercooled, superviscous liquid or fluid. Tour guides in historic churches and other old buildings will often point out that the panes in the windows are thicker at the bottom than the top, "because they've flowed ever-so-slowly downwards over the years." But it turns out this isn't quite true.

Glass is actually an "amorphous solid". It has no crystalline structure, and it does not undergo a normal phase change as most materials (such as water, and metals) do. (Another amorphous solid is rubber.) Nevertheless, the molecules in room-temperature glass are rigidly bound to each other, and there's no evidence that they flow, even after hundreds or thousands of years.

So what about those old windowpanes that are thicker at the bottom? Well, until recently, there wasn't a good way of making perfectly flat, smooth glass for windows. For example, the "crown glass" technique (used since medieval times) involved blowing, flattening, and then spinning what became a large disc of glass, slightly thicker at the outer edge due to centrifugal force. These irregularities obviously persisted even after you cut smaller square panes out of the large discs. Windowmakers tended to mount panes with the thicker edge down -- they looked better that way -- but what this means is that the bottoms had always been thicker; they didn't sag over the years. And sometimes you can find old panes that are thicker at one side, or at the top, because they happened to be installed that way, and this is a pretty good proof that the thick-at-the-bottom panes aren't that way due to "flow".

Sources:
http://math.ucr.edu/home/baez/physics/General/Glass/glass.html
http://dwb.unl.edu/Teacher/NSF/C01/C01Links/www.ualberta.ca/~bderksen/windowpane.html

(P.S. There is at least one example of a superviscous "liquid" that takes years to flow -- pitch. If you do a web search for "pitch drop experiment" you can find pictures of a funnel full of pitch at the University of Queensland that has dribbled out just eight drops in over seventy years.)