Madison
Chaos and Complex Systems Seminar
Spring 2006 Seminars
All seminars are Tuesday at 12:05 pm in 4274 Chamberlin except as
noted.
Short List
- Jan 17, 2006 - Clint Sprott, Physics
- Jan 24, 2006 - Cristie Hurd,
Zoology
- Jan 31, 2006 - David Hsu, Neurology
- Feb 7, 2006 - Gheorghe Craciun, Mathematics and
Biomolecular Chemistry
- Feb 14, 2006 - Jon Martin, AOS
- Feb 21, 2006 - Nancy Mathews, Gaylord Nelson Institute for
Environmental Studies
- Feb 28, 2006 - Bob Aune, Space Science and Engineering Center
- Mar 7, 2006 - David Houghton, AOS
- Mar 14, 2006 - NO SEMINAR (spring break)
- Mar 21, 2006 - Steve Vavrus, Gaylord Nelson Institute for
Environmental Studies
- Mar 28, 2006 - Karen Holden, La Follette School of Public Affairs
- Apr 4, 2006 - Michael Newton, Statistics
- Apr 11, 2006 - Christopher
Watts, University of New Mexico
- Apr 18, 2006 - Jonathan Patz, Gaylord Nelson Institute for
Environmental Studies
- Apr 25, 2006 - Jim Reardon, Physics
- May 2, 2006 - Mike Brown,
Swarthmore College
Join us for lunch during the summer on the Union Terrace at noon each
Tuesday,
starting May 9th!
Abstracts
January 17, 2006
Is global warming for real?
Clint Sprott, UW Department of Physics
Probably, but if you're a skeptic, this talk will not likely convince
you. What I will do is use Clay's ice core data and John Magnuson's
Lake Mendota ice cover data from last semester in a case study of
various time-series analysis techniques, both linear and nonlinear. I
will show the limitations and weaknesses of the various techniques and
the wide variety of predictions that they make. I will show the chaotic
output of an artificial neural network trained on the data and
demonstrate a new computer program that others can use to make
time-series forecasts in fields as diverse as meteorology,
ecology, and finance. Finally, I will make a prediction of when the ice
will thaw on Lake Mendota this year.
This talk is available as a PowerPoint
Presentation.
January 24, 2006
Investigating the dynamics of complex systems through the power law distributions they
generate
Cristie Hurd, UW Department of Zoology
What do sand pile avalanches, earthquakes, stock market crashes, hits
on Internet sites, extinctions of species, and social insect foragers
have in common? All belong to complex systems characterized by a
stable, scale-free distribution of event sizes. Though orders of
magnitude less frequent, the sheer size of the most extreme events
dramatically alters the system’s behavior. In some systems the
consequences can be devastating. One example is the death toll from
Pakistan’s earthquake last October. In other systems the self-similar
distribution may indicate that the system has self-organized to an
optimal trade-off between efficiency of energy flow through the system
and system robustness. Current ideas on the emergence and
classification of complex systems characterized by a power law
distribution of event sizes will be discussed. Data on the allocation
of labor in a social insect colony will be presented as an example of a
scale-free system.
January 31, 2006
Brain waves on potential energy surfaces: relating
particle dynamics to brain state
David Hsu, UW Department of Neurology
Abstract: A working brain emits electromagnetic
fields which can be
detected at the scalp with electroencephalograms (EEG). Since the
invention of human EEG techniques in 1924, we’ve learned, on a
phenomenological level, that certain waveforms of the brain represent
an awake and alert state, other forms represent different levels of
sleep, and yet others represent epileptic seizures. Here we show
how
to go beyond a phenomenological description, by regarding EEG output as
the coordinates of a hypothetical particle. The hypothetical
particle
“moves on” an effective potential energy surface. By extracting
pieces
of this potential energy surface from real EEG data, we find that
seizure onset is associated with escape of the hypothetical particle
from potential energy wells and crossings of potential energy
barriers. This picture of a hypothetical particle moving on a
potential energy surface allows us to ask new kinds of questions about
brain states and changes in brain state. We discuss this
particle-on-a-potential-energy-surface model in relation to chaos
theory and persistent reports of widespread oscillations seen on
different types of brain wave recordings.
February 7, 2006
Switch-like behavior in biochemical reaction networks
Gheorghe Craciun, UW Departments of Mathematics and
Biomolecular Chemistry
Gene regulatory networks,
metabolic and signaling networks in
cells can be regarded as dynamical systems obeying mass-action chemical kinetics. These systems are
usually high-dimensional, nonlinear,
and depend on many unknown parameters. In general, chemical systems are capable of
arbitrarily complex behavior, but, on the
other hand, the range of possible dynamic behavior is often limited or even uniquely determined by
the network structure. We will show
that reaction diagrams, similar to those that biochemists usually draw, carry subtle information
that relates the reaction network's
topology with its capacity to exhibit switch-like behavior. We will also discuss implications for
the interpretation of experiments
in cell biology.
February 14, 2006
Thoughts on communicating global changes issues
Jon Martin, UW Department of Atmospheric and Oceanic Sciences
Study of global climate change has
become a major endeavor in the atmospheric and oceanic sciences within
the last
25 years. Given the considerable
potential for societal impact from global climate change, the
atmospheric
sciences have been increasingly called upon for sound, reasoned
guidance in the
shaping of public policy. Unfortunately,
the public policy arena is unfamiliar ground for most scientists and is
significantly
influenced by politics. Consequently,
the central issues in climate change science are often obfuscated by
political
rhetoric. This circumstance compels the
scientific community to not only continue the basic scientific research
on
global change, but to also identify means by which the complicated
interplay
between physical processes and boundary conditions in the climate
system can be
explained, in their essence, to non-experts.
In this talk I suggest a baseball analogy that may provide an
example of
the extreme sensitivity of complicated systems to small changes in
boundary
conditions.
February 21, 2006
Role of deer behavior in transmission of CWD prions
Nancy Mathews, Gaylord Nelson Institute for Environmental
Studies
Chronic wasting disease (CWD), an infectious and fatal disease of white-tailed deer, was first detected
in south-central Wisconsin in 2001.
Understanding movements of deer is an essential aspect of modeling CWD transmission and for managing the
disease in the wild. Home range sizes of
individual female deer and social groups are a result of individual movement, social interactions, and
behavioral responses to habitat characteristics.
While there is substantial evidence that home range size is influenced by factors such as sex,
age, body weight, and season, the influence
of deer density, harvest, and landscape pattern is not as well understood. My students and I examined
individual and social group home range
sizes, and movement patterns in relation to habitat fragmentation (forest edge density and the ratio of
agriculture to forest), local deer density,
and deer harvest intensity. Forest edge density, the only predictor of home range size for both
individual females and social groups, was
inversely related to home range size. Further, forest edge density was greater within natal gestation home
ranges of yearling male dispersers than non-dispersers,
but there were no differences in year, the ratio of agriculture to forest, deer density,
or harvest intensity. Perhaps the most
significant finding of the research, however, is preliminary evidence suggesting that clusters of infected
deer may be more linked to geographic location
than to deer density. This suggests the potential existence of hotspots of environmental
contamination. I will discuss the implications of direct transmission among deer,
verses indirect transmission through environmental
contamination, and how this might affect future management.
February 28, 2006
Improving short-term numerical weather forecasts using observation from
satellites
Robert Aune, NOAA's Advanced Satellite Products
Branch, UW Madison
Computer models that generate forecasts of
future atmospheric states (1-3 days) have evolved into highly complex
systems
over the past 30 years. Increases in
computer power allow modelers to include additional realism in their
models
with the goal of improving forecast accuracy.
Changes to any forecast model must be objectively validated against
measured atmospheric parameters.
Historically this has been accomplished using point-source observations
with poor spatial and temporal coverage.
In the late 1980's scientists at the Cooperative Institute for
Meteorological Satellite Studies (CIMSS), began using observations from
geostationary satellites to validate numerical models. What
resulted was the CIMSS Regional
Assimilation System (CRAS), a forecast model unique in that its
development was
guided by validation against truth as viewed by satellites. I
will present a summary of numerical weather
prediction concepts, focusing on limitations set by non-linearity,
error growth
and predictability. I will conclude with a brief history of
the
CRAS forecast model and how satellite observations were used to improve
its
accuracy. Real-time CRAS forecasts can
be viewed at http://cimss.ssec.wisc.edu/model/daily/daily.html
March 7, 2006
The N-dimensions of global climate change “complexity”
David Houghton, UW Department of Atmospheric and Oceanic Sciences
A broad overview of the climate change issue reveals the complexity of
the physical system that must be considered and the long list of
uncertainties facing those trying to make predictions for the future. I
share my perceptions arising from writing an education text on this
subject and making many presentations to public groups. The relevant
physical system includes the land, air, oceans, and biosphere
(including most importantly – people). Science hurdles include both
observing the system and predicting its changes. It is shown how
uncertainties build on each other so that predictions for future
climate conditions for local communities along with resulting impacts
can be considered still to be quite uncertain. Examples of these
uncertainties document the “complexity” of the system and the
challenges to both the scientific community and the world community.
March 21, 2006
The role of terrestrial snow
cover in the climate system
Steve Vavrus, Gaylord Nelson Institute for Environmental Studies
Snow cover is known to exert a strong influence on the overlying
atmosphere and underlying soil, but quantifying this impact is
difficult. Besides its well-accepted ability to cool locally,
snow cover can also force climate remotely in complex ways by inducing
changes in the atmospheric circulation. Most research on the
impact of snow cover has focused on the regional rather than global
scale. By contrast, this study investigates the global impact of
terrestrial snow cover in the present climate by comparing a pair of
numerical climate model simulations run with prognostic snow cover
(control case) and with all snow cover on land eliminated
(NOSNOWCOVER). In this experiment all snowfall over land was
converted into liquid water upon reaching the surface. Compared
with the control run, NOSNOWCOVER produces mean-annual surface air
temperatures up to 5 K higher over northern North America and Eurasia
and 8 to 9 K greater in these regions during winter. The
global-mean warming of 0.8 K in NOSNOWCOVER is 1/3 as large as the
model’s response to a doubling of carbon dioxide and larger than the
observed warming trend since accurate measurements began in the late
19th century. This pronounced surface heating propagates
throughout the atmosphere, causing changes in circulation patterns
aloft. Despite the large atmospheric warming, the absence of an
insulating snow pack causes soil temperatures in NOSNOWCOVER to fall
throughout northern Asia and Canada, including extreme wintertime
cooling of more than 20 K in Siberia and a 5 to 10o
equatorward expansion of simulated permafrost. The absence of
local melt-water percolation causes significantly drier soils over
northern boreal regions and a consequent decrease in cloudiness.
The removal of snow cover also drastically affects extreme weather in
middle latitudes. Extreme cold-air outbreaks (CAOs), defined
relative to the control simulation, essentially disappear in
NOSNOWCOVER. The loss of CAOs appears to stem from both the local
effect of eliminating the chilling influence of snow cover in
mid-latitudes and a remote effect over CAO source regions in the
Arctic, where –40oC air masses are unable to form in
NOSNOWCOVER.
March 28, 2006
Social Security--in chaos or all as predicted?
Karen Holden, La Follette School of Public Affairs
It is often argued that the U.S. Old Age Security, Disability and
Health Insurance (OASDHI) program--known as "Social Security"--is
unsustainable due to the underlying characteristics of the program and
economic changes that were unpredicted by its framers. This seminar
attempts to clarify the purpose and nature of the program and what
exactly was expected by the framers of the program (who were actually
surprisingly close in predicting today's current beneficiary to worker
ratios). It will review what are the data being presented to the public
on the financial status of Social Security, why we uniquely have
long-term projections of OASDI (in contrast to most other government
programs), and what are the issues being raised in current discussions
of Social Security reform. Even though OASDI may no longer be a major
public policy initiative of the White House, the issues and discussions
do continue among economists and policy makers. What are they saying
about the future? What can the audience at the seminar expect to see
over their lifetime? I won't answer that question, but hopefully
after the seminar you may be a bit more informed in shaping your own
expectations.
April 4, 2006
On polyclonality of intestinal tumors: statistical and biological
analysis indicates short range interaction of initiated clones.
Michael Newton, UW Department of Statistics
The working hypothesis in cancer research is that cells within a tumor
have descended from a single initiated aberrant cell. In contrast to
this clonality hypothesis, data have emerged which support the
polyclonality of intestinal tumors. I will discuss statistical and
biological aspects of polyclonality from a recent study of mouse
aggregation chimeras. Three important issues are: (1) Random collision:
Is it possible that observed polyclonality can be explained by the
chance proximity of initiated clones? A hypothesis test is derived
using some classical results from stochastic geometry. (2) What is the
spatial extent of interaction among initiated clones? Techniques from
Bayesian image analysis are used to combine image data on the chimeric
patch structure of the intestinal wall with tumor count data. (3) What
fraction of tumors are polyclonal? The lower bound proposed by Novelli
and colleagues is shown to be flawed owing to a misinterpretation of
conditional probability.
This is a joint project with A. Thliveris, R. Halberg, L. Clipson, R.
Sullivan and W. F. Dove from the McArdle Laboratory, and S. Stanhope
from Statistics.
This talk is available in PDF format.
April 11, 2006
Heating the solar corona: A hot topic in plasma astrophysics
Christopher Watts, Electrical
& Computer Engineering, University of New Mexico
The surface or photosphere
of the sun is a blackbody with a
temperature of about 7500° C, and
the basic mechanism that heats the sun, nuclear
fusion, is well understood. However, there
is a disconcerting paradox: The temperature of the solar atmosphere or corona
starts to rise away from the
surface to about 1,000,000° C. It's like
walking away from a fire S<caron> and you suddenly feel hotter. The energy that heats the
corona is almost certainly
stored in the magnetic field of the
sun. There are two main competing models for how this energy is released: 1)
Magnetic waves and 2) Tearing
and reconnection of the magnetic field.
Both models are probably valid in different
regimes. In this talk, I will present an
overview of the coronal heating paradox and the two heating models. Then I'll talk
about current research by plasma
physicists, using both remote
observations and laboratory simulations, focused
on substantiating these models.
April 18, 2006
Complexity in disease emergence from global climate
and ecological change
Jonathan Patz, Gaylord Nelson Institute for
Environmental Studies
Health effects of global climate and ecological change will
come via multiple exposure pathways, many of which are complex and non
linear. Climate-related health outcomes,
for example, heat-related mortality or morbidity, air pollution-related
illnesses, and infectious diseases may also be exacerbated by
concomitant
landscape changes that influence local climate.
Every environmental perturbation impacts the ecological balance
and context
within which disease manifests itself within populations.
These changes affect the hosts or vectors of
disease and the pathogens and parasites that breed, develop, and
transmit
disease. In addition to climate change,
landscape impacts such as deforestation, human settlement sprawl,
industrial
development, road construction (e.g., linear disturbances), large water
control
projects (e.g., dams, canals, and irrigation systems, reservoirs) have
been
accompanied by the spread of pathogens into new areas. For example, the
competence of different anopheline mosquitoes to transmit malaria
varies
between species, and anopheline species occupy a variety of ecological
niches.
Moreover, biological systems (e.g, mosquitoes and disease-causing
agents
within) can amplify the effects of subtle environmental and climatic
changes. These complexities of disease
risk stemming from global environmental change will be presented.
April 25, 2006
Central force motion and the physics of running
Jim Reardon, UW Department of Physics
The motion of a human runner is complex yet also familiar. In
this talk I discuss a
mathematical "toy model" of running humans that is founded on four observations of
runners: all successful runners have a
cadence above 180 steps per minute; the resultant ground force during stance phase passes through the
runner's center of gravity; heel
strike is much more energetically costly than leg swing; and energy cost is proportional to the
time integral of muscle tension. At
issue is the optimal solution of the "runner's dilemma": should one run so that one's center of
gravity stays at a constant height above
the ground, or should one try to minimize one's ground contact time? Implications of the toy model
for real-world training will also
be discussed.
May 2, 2006
Self-organization in magnetized plasmas
Michael Brown, Swarthmore College
It is a common process in the universe for plasma and magnetic fields
to evolve together in a turbulent way but then rapidly relax to simple,
self-organized structures. Solar flares erupt from the photosphere
tangled and chaotic, but via a process called magnetic reconnection,
they relax and straighten. This process releases energy in the form of
superheated plasma and rapidly flowing jets. On a much larger scale
(millions of light years), galactic disks collapse, rapidly shedding
angular momentum and in the process generate extended, magnetized jets
along their axes. On human scales, laboratory experiments are underway
seeking self-organized magnetic structures that would be suitable
“bottles’’ for a fusion reactor. We present recent experimental results
from the merger of two rings of hot, magnetized plasma in the
Swarthmore Spheromak Experiment (SSX). During the merging process, the
plasma self-organizes to generate a single, large scale (r = 0.2 m, L =
0.6 m), three-dimensional magnetic structure called a field-reversed
configuration (FRC). The rate at which the merging proceeds is
governed locally by magnetic reconnection in which magnetic fields
associated with each ring become shared. The magnetic reconnection rate
is fast and fully three-dimensional. Magnetic
reconnection converts magnetic energy to heat (up to Te ~ 106 K),
energetic particles (Ei
> 100 eV), and flow (up to 100 km/s). See http://plasma.physics.swarthmore.edu/selforg/index.html
for more information.