CAN ‘ORDINARY CONTRAILS’ CHANGE THE WEATHER ?
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Volume 98, Issue 10 (October 1970)
Article: pp. 745–748 | Abstract | PDF
Geophysical
Institute, University of Alaska, College, Alaska
DOI:
10.1175/1520-0493(1970)098<0745:OTPOWM>2.3.CO;2
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ABSTRACT
The possible
effect of contrails in modifying the weather is reconsidered in the light of
information obtained from ground-level contrails in Alaska. It appears likely
that inadvertent cloud seeding by jet aircraft may be of the same order of
magnitude as that attained in commercial cloud seeding operations. Further
investigation is needed; but in the meantime, the possibility of contrail
contamination should be kept in mind when evaluating the results of seeding
operations.
Article: pp. 496–508 | Abstract | PDF (1.01M)
Illinois
State Water Survey, Champaign 61820
(Manuscript received July 18, 1980, in
final form January 27, 1981)
DOI:
10.1175/1520-0450(1981)020<0496:MCSATT>2.0.CO;2
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ABSTRACT
Records of
monthly sky cover, sunshine and temperature for 1901–77 in a 10-state
midwestern area were analyzed on a temporal and spatial basis to discern
long-term trends and indications of shifts potentially due to added cirrus
generated by jet aircraft since about 1960. The skycover data show generally
long-term increasing frequencies of cloudy days and decreases in clear days
since 1901. Percent of possible sunshine also shows a decrease but to a lesser
extent than clear day frequencies. Changes have been greatest since the 1930's.
The greatest shifts to cloudier, less sunny conditions occurred since 1960 in
an east-west zone across southern Iowa-northern Missouri, northern two-thirds
of Illinois and Indiana, and extreme southern sections of Wisconsin and lower
Michigan, the area where commercial jet traffic has been greatest. The
long-term trends give evidence of natural climate changes, whereas the
localized shifts to more cloudiness in the central area since 1960 suggest
anomalous changes related to jet-induced cirrus. Months with moderated
temperatures (below average maximum and above average minimum) have increased
since 1960 in the central east-west zone and largely in summer and fall, the
seasons with the major shifts to cloudiness.
NATURAL AEROSOLS AND AIRCRAFT AEROSOL WX
ENGINEERING
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Title: |
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A possible change in cloud radiative forcing due to aircraft exhaust |
Authors: |
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Publication: |
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Geophysical Research Letters, Volume 25, Issue 10, p. 1673-1676 (GeoRL Homepage) |
Publication Date: |
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00/1998 |
Origin: |
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AGU Keywords: |
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Atmospheric Composition and Structure: Cloud physics and chemistry, Atmospheric Composition and Structure: Pollution-urban and regional, Meteorology and Atmospheric Dynamics: Radiative processes |
Abstract Copyright: |
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(c) 1998: American Geophysical |
DOI: |
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Bibliographic Code: |
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1998GeoRL..25.1673W |
Aircraft exhaust may reduce
the crystal size in natural cirrus. This work investigates the change in cloud
radiative forcing from such a size reduction by assuming a constant ice water
content. A 1-dim model with radiative properties that depend on the mean
crystal size is used to compute the radiative transfer for an atmospheric
column. The results show that the negative shortwave cloud forcing is enhanced
with smaller crystals as they mainly increase the reflectivity of clouds. The
change in the longwave cloud forcing is always positive although its magnitude
depends strongly on the ice water path. The weighted sum of SW and LW cloud
forcings depends on the mean crystal size, surface albedo and ice water
content. It appears that there is a range of diameters between 15 and 25 μm
where the response to a reduction in crystal size is fairly insensitive. Below
and above this range the change is negative or positive, respectively. In
regions of dense airtraffic the magnitude of the change in cloud forcing could
be on the order of 0.3 Wm-2 under the assumption of a 20% decrease
of the mean crystal size from about 30 μm to 24 μm. Aircraft exhaust thus has the potential to affect the climate but the
results should be taken with caution as they are based on parameterized optical
properties for cirrus clouds.
Article: pp. 301–309 | Abstract | PDF (1.24M)
a. Department
of Geography, Indiana University, Bloomington
b. Climate and Meteorology
Section, Illinois State Water Survey, Champaign, IL 61820.
DOI:
10.1175/1520-0477(1986)067<0301:JCACCA>2.0.CO;2
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ABSTRACT
The results
of a pilot study to assess the feasibility of documenting the occurrence of jet
contrails over the United States from high-resolution Defense Meteorological
Satellite Program (DMSP) imagery are presented. They are strongly positive,
suggesting that 1) contrails can be distinguished from natural cirrus on the
imagery; 2) contrails are consistently identifiable; 3) contrails often occur
in association with the natural cirrus and frequently spread, and 4) this
spreading could extend the accompanying natural cirrus shield. The analyses
also indicate that contrails tend to occur relatively frequently, that they
more often cluster in groups than appear singly, and that they seem to show a
preference for developing in (near) upper-tropospheric cold troughs
(ridgelines). It is accordingly suggested that DMSP imagery can provide a basis
for research into a contrail-cirrus-climate relationship.
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FEBRUARY 2002
AMERICAN
METEOROLOGICAL SOCIETY
|
CONTROLLING THE
GLOBAL WEATHER
BY
R
N. H
OFFMAN
AFFILIATION:
H
OFFMAN
—Atmospheric and
Environmental
Research, Inc.,
CORRESPONDING AUTHOR:
Ross N. Hoffman,
Atmospheric and
Environmental
Research, Inc.,
02421-3126
E-mail:
rhoffman@aer.com
In final form
©2002 American Meteorological Society
It had not been easy
to persuade the surviving superpowers to relinquish their orbital for-
tresses and to
hand them over to the Global Weather
Authority, in what was—if the meta-
phor could be
stretched that far—the last and most dramatic example of beating swords into
plowshares. Now
the lasers that had once threatened mankind directed their beams into care-
fully selected
portions of the atmosphere, or onto heat-absorbing target areas in remote re-
gions of the
earth. The energy they contained was trifling compared with that of the
smallest
storm; but so is
the energy of the falling stone that triggers an avalanche, or the single neu-
tron that starts
a chain reaction.—A
RTHUR
C. C
LARKE
,
Fountains
of
Technological advances over the next 30–50 years
may make it possible to control the
weather. If
we can, should we? Are “weather
wars” inevitable?
242
FEBRUARY 2002
The earth’s atmosphere has been hypothesized to be chaotic. Chaos
implies that there is a finite predictability time limit no matter how well the
atmosphere is observed and modelled. It is generally accepted that this limit
is typically 2 weeks for large-scale weather systems (Lorenz 1982),
although some situations may be more or less predictable, and smaller scales
are certainly less predictable. Chaos also implies sensitivity to small
perturbations. The most realistic numerical weather prediction (NWP) models are
very sensitive to initial conditions. It is therefore very likely that the
atmosphere is also extremely sensitive to small perturbations.
A series of such perturbations to the atmosphere might be devised to
effectively control the evolution of the atmosphere, if the atmosphere is
observed and modelled sufficiently well. We present system architecture to
control the global weather
that might be implemented within a few decades.
It is a dream of mankind to control the weather—not to make every day the
same, but to protect lives and property. We believe that this dream is in fact
a possibility. Just imagine: no droughts, no tornadoes, no snowstorms during
rush hour, etc.
We probably cannot eliminate hurricanes, but we might be able to control
the paths of hurricanes, and essentially prevent hurricanes from striking
population centres. Our goal is not to change the climate, but to control the
precise timing and paths of weather
systems. For ex-ample, eliminating hurricanes and the associated mix-
ing of the upper layers of the ocean would presumably change the climate
in many indirect ways. Because of the intensive coupling of the weather over
different regions of the globe, nothing short of control of the global weather
should be considered.
The nation that controls its own weather will necessarily control the
weather
of other nations. If there are several nations, each attempting to control the
weather over its territory, then each may operate at odds
with the others and “weather
wars” are conceivable.
An international weather
control treaty may be prudent now. In the future, an international agency may
be required so that weather
control is used “for the good of all.” Perhaps for the good of all is
unattainable. Any change to weather
will have both positive and negative effects. How can the interests of both the
“winners and losers” be accommodated?
OF course, weather always has both positive and
negative effects, and there are winners and losers now. In what follows we
present the underlying concepts for our approach and then outline the system
architecture of a controller for the global atmosphere, describing the
components of such a controller. Legal and ethical questions are only touched
on, and the issues of feasibility and cost–benefit trade-offs are only briefly
considered. Our proposed controller is similar in general to feedback control
systems common in many industrial processes; however, it is greatly complicated
by the number of degrees of freedom required to represent the atmosphere
adequately, the nonlinear nature of the governing equations, the paucity of
observations of the atmosphere, the difficulty of effecting control, and the
requirements that control be effected at significant time lags. However, the
existence of the technology to implement the weather controller is plausible at
the time range of 30–50 yr.
CHAOS, THE LIMITS OF
PREDICTABILITY,
AND IMPLICATIONS FOR
CONTROL.
Theoretical and model
studies have established that the dynamics governing the atmosphere can be
extremely sensitive to small changes in initial conditions (e.g., Rabier et al.
1996). Current operational practice at NWP centres illustrate this daily.
Examples summarized in what follows include data assimilation, generation of
ensembles, and targeted observations.
The key factor
enabling control of the weather
is that
the atmosphere is
sensitive to small perturbations.
That is, it is the
very instability of the atmosphere’s dy-
namics that makes
global weather
control a possibility.
Chaos causes extreme
sensitivity to initial condi-
tions. Although the
atmosphere, and indeed realistic
models of the
atmosphere, have not been proven to
be chaotic, the theory
of dynamical systems and chaos
provide a useful
background for this discussion. In a
realistic NWP model,
since small differences in ini-
tial conditions can
grow exponentially, small but cor-
rectly chosen
perturbations induce large changes in
the evolution of the
simulated weather.
Therefore we
hypothesize that as we
observe and predict the atmo-
sphere with more and
more accuracy, we will become
able to effect control
of the atmosphere with se-
quences of smaller and
smaller perturbations. Note
the basic difference
between predictability and con-
trol theory:
Predictability theory states that small dif-
ferences grow; control
theory states that a sequence
of small perturbations
can be used to track a desired
solution. By tracking
(i.e., following) a desired solu-
tion, our control
method may overcome differences
between model and
reality. We will expand and ex-
plain these basic
ideas in the following paragraphs.
The phase space
description of dynamical systems. The
evolution of dynamical
systems is conveniently dis-
cussed using the phase
space description of Poincaré
(Lorenz 1963). The
state of the system is specified by
n variables. For continuous systems, such as the at-
mosphere, we may first
approximate the continuous
system by
discretization and thereby obtain a large
number of coupled
nonlinear ordinary differential
equations. For a
physically realizable system, the col-
lection of feasible
points in the n-dimensional phase
space will be bounded.
For a single time, the
state of the system is repre-
sented by a single
point. As the system evolves, the
point representing the
system will in general describe
a curved line. This is
termed the trajectory. If the sys-
tem is in a stable
state, the trajectory is just the single
point. Small
perturbations about the point decay in
time toward the stable
point. A stable point is an
attractor. A stable
point is also a fixed point of the
system. There can be
unstable fixed points. Some tra-
jectories form closed
curves—these represent peri-
odic solutions.
For a realistic model
of the atmosphere with fixed
boundary conditions,
periodic solutions probably ex-
ist but are unstable.
There are many unstable periodic
solutions close to
chaotic attractors. Chaotic systems
are aperiodic, but
given enough time, return arbi-
trarily close to
points in the attractor. For the atmo-
sphere, the lack of
success for analog forecast tech-
niques suggests that
this return time is very long.
Chaotic systems.The strict definition of chaos describes
it as a behavior of
purely deterministic systems with
as few as three
components for a continuous phase
space flow (e.g.,
Lorenz 1963), or as few as a single
component for an
iterated mapping (e.g., Lorenz
1964). Chaotic systems
can appear to be random when
sampled at timescales
that are large compared to the
dynamical timescale.
The key characteristics associ-
ated with chaos are
that the system be bounded and
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possess at least one
positive Lyapunov exponent
(Lorenz 1965). A
positive Lyapunov exponent implies
average growth in the
associated direction that is ex-
ponential. Typically
in the phase space of such sys-
tems, a small initial
sphere of radiusε will over a short
time deform into an
ellipsoid. The axes of the ellip-
soid might be called
the finite time or local Lyapunov
directions, and the
ratio of these axes to ε might be
called the finite time
or local Lyapunov factors. As the
ellipsoid evolves it
tends to flatten parallel to the
attractor of the
system. Chaotic attractors are also
called strange
attractors. A characteristic of these
attractors is that
perturbations perpendicular to the
attractor collapse
exponentially, while perturbations
parallel to the
attractor grow exponentially.
It is for these
reasons that we say the small pertur-
bations can grow
exponentially. A randomly chosen
perturbation may be
decomposed into contributions
from the finite time
Lyapunov directions. Some, per-
haps most, will decay,
but the others will grow. The
perturbation may
therefore first decrease in size, be-
fore growing
explosively. A perturbation may also be
constructed which
projects only onto a particular
growing mode. Such a
perturbation will initially grow
exponentially.
The limits to
predictability. Since small
differences grow
rapidly in chaotic
systems, chaotic systems are diffi-
cult to predict.
Inevitably small errors will exist in our
specification of the
initial conditions. Further, errors
in model formulation
induce errors in the model state
at every model time
step. Although the magnitude of
the error may
initially decay with time, eventually
small errors will
begin to grow exponentially and
continue to do so
until they become large. It is gen-
erally accepted that
useful forecasts of the instanta-
neous weather
beyond 2–3 weeks are impossible
(Lorenz 1982; Simmons
et al. 1995).
For the atmosphere,
motions occur over a huge
spectrum of scales.
Smaller spatial scales have shorter
timescales. Errors in
the smallest scales will com-
pletely contaminate
those scales on the characteristic
timescale associated
with that spatial scale. These er-
rors will then induce
errors in the next larger scale
and so on (Lorenz
1969). In fluids, advection implies
that tiny errors on
the large scales will in turn cause
large errors on the
shortest scales. These interactions
lead to a finite
predictability time limit.
Control of chaotic
systems. Since chaos may appear
to
be random, control of
chaos might seem impossible.
But sensitivity to
initial conditions also implies sen-
sitivity to small
perturbations. As we have mentioned,
small perturbations in
some directions decay quickly,
but properly chosen
perturbations grow quickly.
Therefore a sequence
of very small amplitude but pre-
cisely chosen
perturbations will steer the chaotic sys-
tem within its
attractor. There have been many stud-
ies reported in the
literature that support this view
(Kapitaniak 1996). We
note two examples of the con-
trol of chaotic
systems.
The first is the
phenomena of resonance (Pecora and
Carroll 1990). Suppose
that there are two copies of
an evolving dynamical
system. Initially the two sys-
tem states are
arbitrarily different. One system evolves
freely but is
observed. In particular, one variable of
that system is
accurately observed. The correspond-
ing variable in the
second system is constantly reset
to the value observed
in the first system. Over time
all variables of the
second system approach the values
of the corresponding
variables in the first system. We
say that the second
system has become entrained by
the first system.
Second, within the
attractor of a chaotic system,
there are a multitude
of unstable periodic orbits.
Techniques to compute
these orbits are available.
Once the system is
close to one of these orbits, it is
possible to
continually follow the orbit by regularly
applying small
perturbations (Ott et al. 1990).
Control of realistic
atmospheric models. To control the
weather we must effect changes on timescales shorter
than those of the
examples of the previous section, and
to a system of huge
complexity. The numerical meth-
ods used must be
computationally feasible. The NWP
community has already
taken the first steps to con-
trol large dynamical
systems. One current NWP data
assimilation practice,
called 4DVAR, finds the small-
est perturbation at
the start of each data assimilation
period, which grows to
best fit all the available data,
thereby demonstrating
the practical control of large-
scale realistic
systems. Current 4DVAR practice finds
the smallest global
perturbation, as measured by the
a priori or background
error covariances, but it should
be possible to modify
4DVAR to find the smallest lo-
cal perturbation or
the smallest perturbation of a par-
ticular type. This
method is described further in the
section about data
assimilation systems. Further, some
other current NWP
technology may be adapted to de-
termine the optimal
perturbations to effect control.
These techniques are
described in what follows.
S
INGULAR VECTORS
.Singular vectors are
the fastest grow-
ing perturbations
about a given model forecast over
a finite time
interval, say 24 or 72 h, with respect to a
particular measure of
difference. (For example, the
244
FEBRUARY 2002
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size of the
perturbation might be taken to be its en-
ergy.) Singular
vectors are currently calculated opera-
tionally at the
European Centre for Medium-Range
Weather Forecasts (ECMWF) for the purpose of en-
semble forecasting
(Molteni et al. 1996). In principle,
ensemble forecasting
introduces equally likely small
perturbations in the
initial conditions of each en-
semble member. In
practice, because each of the fore-
casts within the
ensemble is computationally expen-
sive, only
perturbations that are rapidly growing are
included. The growth
rates of these perturbations are
explosive—24-h
amplification factors of 10–20 are
reported for
large-scale calculations with limited
physics, and much
larger amplification factors are
expected when smaller
scales and moist physics are
included. A basic
version of control can be effected
by calculating the
leading singular vectors, determin-
ing if a positive or
negative perturbation along one of
these modes would
produce a desired result, and then
introducing that
perturbation, if it was feasible.
T
ARGETED OBSERVATIONS
. During the last
decade there
has been considerable
research on targeted observa-
tions (Lorenz and
Emanuel 1998; Bergot et al. 1999;
Bishop and Toth 1999).
Given a current forecast of
some storm of
interest, we can backtrack from the
forecast to find that
region of the initial state that, if
better observed, would
improve the forecast of that
storm. The theory and
methodology of this approach
have advanced
sufficiently so that actual trials were
undertaken for several
field experiments including the
Fronts and Atlantic
Storm-Track Experiment
(FASTEX; Joly et al.
1997), the North Pacific Experi-
ment (NORPEX; Langland
et al. 1999), and the 1999
Winter Storms
Reconnaissance Program (WSRP 99;
Bergot et al. 1999).
This technology can be
adapted to calculate the
optimal perturbation.
Determining where to target
observations is
related to the problem of determin-
ing where to introduce
perturbations to effect a cer-
tain change in the
forecast. In both cases we are opti-
mizing a figure of
merit or objective function that is
calculated in terms of
the forecast with respect to
some change in the
initial conditions. Note that the
figure of merit can
include both costs and benefits.
THE GLOBAL WEATHER CONTROL SYS-
TEM. The global weather control (GWC) system we
envision is a feedback
control system, made complicated
by a number of
factors. These include the following:
• The number of
degrees of freedom required to
represent the
atmosphere adequately.
• The nonlinear nature
of the governing equations.
The atmosphere is
nonlinear and sometimes dis-
continuous. For
example, clouds have sharp edges.
• The paucity and
inaccuracy of observations of the
atmosphere. Satellites
provide a huge volume of
information. However
this information is not al-
ways in the right
place, accurate enough, or of the
right type.
• The control must be
effected at significant time lags
to minimize the size
of the perturbations, yet the
system is inherently
unpredictable at long lead times.
• The difficulty of
effecting control. The control
mechanisms do not yet
exist. The ideal perturba-
tions, while small in
amplitude, may be large in
scale.
• The ambiguous nature
of the figure of merit. For
inhabitants of
cane threat to that
city may take precedence over
all else. But in
general attempting to satisfy mul-
tiple objectives may
result in conflicts.
The GWC system is
sketched in Fig. 1. The “con-
troller” and “random
effects” perturb the system state.
The controller must
therefore compete with random
effects. However the
controller perturbations are de-
signed to grow, while
the random effects perturba-
tions tend to decay.
The “governing equations” ad-
vance the system from
time t
n
to time t
n+1
. If we
eliminate the
“observations” and controller elements
in this figure we have
a sketch showing how a NWP
model approximates the
atmosphere. On the other
hand, if we remove
only the random effects element,
we have a sketch of a
system that must be simulated
within the controller
element in order to estimate the
system state and then
the optimal perturbations. Note
the various noise
sources: The observations are inex-
act, the perturbations
are effected with some inaccura-
cies, the model
introduces further errors. The statistics
of these errors are
also inexact and must be estimated
empirically (from the
time history of the differences
between short-term
forecasts and observations).
Cost–benefit
trade-offs. Controlling
small-scale phe-
nomena will not be
cost effective. Certainly we want
to control destructive
tornadoes, but the time- and
space scales are so
fine that this may be impossible on
an individual basis.
It may be more effective to elimi-
nate the large-scale
conditions leading to the forma-
tion of tornadoes. In
general, theoretical predictabil-
ity studies (Lorenz
1969) suggest that doubling the
resolution of the
observations will only increase pre-
dictability by an
amount similar in magnitude to the
timescale of the
motions of the smallest resolved phe-
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nomena. For example,
since the timescale for the evo-
lution of a thunderstorm
is smaller than 1 h, observ-
ing details of
individual thunderstorms will improve
predictability by no
more than 1 h. Effecting control
at very large scales
may not be cost effective either.
The largest spatial
scales have the largest “inertia.”
These scales have the
longest associated timescales and
the greatest part of
the energy (Nastrom et al. 1984).
The GWC system will be
subject to optimization
itself. Our control of
the weather
will increase as we
increase the skill of
the NWP models, the accuracy of
the observations, and
the size of the controlling per-
turbations. All three
facets of the problem require re-
sources. A
cost–benefit analysis will balance resources
devoted to remote
sensing, computer power, and per-
turbations. As
advances in the supporting disciplines
accumulate, the
optimal point will shift, become fea-
sible, and eventually
become economically sensible.
Enabling technology.Implementation of the overall sys-
tem architecture will
require major advances in many
disciplines. Here we
discuss the required discoveries
and refinements.
Although it is difficult to predict the
pace of technological
advance, the control of the
weather is a plausible outcome of advances in various
fields over the time
span of a few decades.
N
UMERICAL WEATHER PREDICTION
. NWP is now a mature
science (Kalnay et al.
1998). Advances in computer
power will enable the
refinement of NWP. Current
high-resolution
mesoscale models point the way for
advances in global
models. In early NWP models,
many physical
processes were either removed by
filtering
approximations or modeled by parameteri-
zations. As NWP models
evolve, more and more of
the physics of the
atmosphere are resolved explicitly.
A recent report (ECMWF
1999) makes estimates
of the spatial
resolving power of NWP models over
the next decade. In
summary, this report predicts
horizontal resolution
increasing from the current 60
to 15 km by 2008.
Extrapolating for another 30 yr sug-
gests global
resolution of approximately 250 m.
(Currently vertical
resolution is much finer than hori-
zontal resolution, but
at the much higher future hori-
zontal resolution, the
same scale will be appropriate
for both horizontal
and vertical resolution in the tro-
posphere. This would
allow even higher resolution
than our simple
extrapolation would suggest.)
D
ATA ASSIMILATION SYSTEMS
. Data assimilation
systems
estimate the state of
the atmosphere given limited
observations and an
imperfect model of the evolution
of the atmosphere.
This problem is complicated by the
paucity of
observations, the huge number of degrees
of freedom needed to
specify the atmosphere, and
the extreme
nonlinearity of the governing equa-
tions. The data
assimilation system is a key part of
the controller of Fig.
1—the data assimilation pro-
vides estimates of the
current state of the atmo-
sphere.
The current state of
the art is 4DVAR or four-
dimensional
variational data assimilation. Opera-
tional 4DVAR assumes a
perfect model over short
time periods (6 or 24
h) and finds the initial condi-
tion at the start of
the period that best fits all avail-
able observations
during the period (e.g., Thépaut
et al. 1993). [This
optimization is made efficient by
the adjoint technique.
In practical implementations,
the adjoint model
performs a backward in time in-
tegration of the
sensitivity of the objective function
to the model state
(Courtier 1997).] Because the
NWP model is used to
extrapolate the initial condi-
tions, the 4DVAR
solution is necessarily dynamically
consistent. The end
point of the solution from the
previous period is
called the background and is used
as a special type of
observation. The error structure
of the background is
necessarily complex but has a
greatly simplified
representation in current versions
of 4DVAR. In the near
future we expect to see
higher resolution used
in 4DVAR in line with in-
creases in resolution
in NWP models, better esti-
mates of the
background error statistics, and a con-
vergence to the Kalman
filter methodology (Todling
and Cohn 1994;
Houtekamer and Mitchell 1998).
S
ATELLITE REMOTE SENSING
. Satellites observe
the at-
mosphere and the
earth’s surface with global cover-
age, rapid refresh,
and high horizontal resolution in vis-
F
IG
.1. Schematic
global weather
controller flow chart.
246
FEBRUARY 2002
|
ible, infrared, and
microwave spectral domains.
Sensors currently
being prepared for launch have
very high spectral
resolution, which in turn will pro-
duce higher vertical
resolution for the retrieved tem-
perature and moisture
profiles. Advances are ex-
pected in terms of
higher resolution, greater numbers
of satellites, and
higher accuracy in the future. Ac-
tive sensors, such as
the Tropical Rainfall Measuring
Mission (TRMM)
precipitation radar, may be used
more in the future.
The ability to collect
observations from space cur-
rently outstrips our
ability to use these data in global
NWP. Typically, the
observations are thinned to re-
duce resolution and
quantity. This will be more of a
problem with higher
spectral resolution sensors.
However, advances in
computing power and data as-
similation techniques
will improve this situation.
PERTURBATIONS
. Everything mankind does that can be
controlled may be considered a source of perturba-
tions. Here we mention a few possibilities:
• Aircraft
produce contrails. Contrails are essentially
cirrus
clouds and influence both the solar and ther-
mal
radiation (Poellot et al. 1999). Slight variations
in
the timing, levels, and routes of aircraft would
produce
perturbations (Murcray 1970).
• Solar
reflectors, in low earth orbit, capable of vary-
ing
orientation, would produce bright spots on the
night
side, and shadows on the day side, thereby
changing
the heating of the atmosphere. First
steps
have already been taken. However, the lat-
est
Russian experiment, named Znamya 2.5, failed
to
unfurl a 25-m diameter thin sheet mirror in
space
in February 1999 (Beatty 1999). In the fu-
ture
inflatable structures may be used (Dornheim
1999).
•
Solar-powered generators in geostationary orbit
have
been suggested as a low-cost energy source.
A
concern is that losses from the microwave down-
link
would be a heat source (
spatial
area and timing of the downlink were con-
trolled
this would be a source of perturbations. In
addition,
tuning of the microwave downlink fre-
quency
would control the height in the atmosphere
of
the energy deposition.
• An
enormous grid of fans that doubled as wind
turbines
might transfer atmospheric momentum
in
the form of electric energy.
To be effective the individual actions must be co-
ordinated, so that the total perturbation is one
that
produces a desired effect. This may be difficult.
COMPUTER TECHNOLOGY
. Computer processing capabil-
ity has been increasing exponentially. The require-
ments of GWC are truly staggering, but global NWP
models at the subkilometer scale seem attainable in
the
30–50 yr time frame, if the pace of advances in
com-
puter technology can be maintained. (If computer
power doubles every year, then after 30 yr it will
have
increased 1 billion times.) However, current
estimates
suggest that
growth of chip functionality as well as the
exponen-
tial growth of the cost of chip fabrication
facilities will
encounter physical obstacles around 2012 (Birnbaum
and Williams 2000). Potential breakthroughs in
nano-
technology, quantum devices, or in other areas will
be
needed.
SYSTEM INTEGRATION
.The GWC system is a megasystem.
Development of tools and methodologies for
megasystems engineering is driven by recent defense
and aerospace projects, such as the space shuttle,
the
strategic defense initiative (SDI), etc. In some
ways
the GWC system is analogous to SDI. Both require
huge real-time data gathering, prediction, and com-
mand capabilities. For GWC the problem is more
complex, but the timescale is more relaxed and
there
is no active opposing intelligence.
Concluding remarks:
The next step.The next step should
involve demonstration
tests in simulation. We suggest
a focus on the
hurricane problem. This problem is
both important and
feasible. Controlling the path of
hurricanes will be a
first-order priority of GWC. A hur-
ricane track is
largely determined by winds of the
large-scale
environment. Reasonable forecasts of hur-
ricane tracks can be
made without modeling the in-
ternal dynamics of the
hurricane. Recent studies have
examined the
sensitivity of such a model to changes
in initial conditions
(Aberson and Franklin 1999;
Cheung and Chan 1999).
For the demonstration
tests, we would be con-
cerned only with the
forecasting and control of the
hurricane tracks. For
this purpose our “NWP” model
could be a simple
quasigeostropic model. The hurri-
cane could be modeled as
a vertical tracer. A plausible
control mechanism
would be localized height pertur-
bations. The goal
would be to protect the Gulf and
East Coast populations
centers. This setup is feasible
and capable of
exploring some of the issues related to
the practicality of
global weather
control and to quan-
tify, albeit in a
limited context, the required resources
to effect GWC. Of
course application to real hurricanes
will require a model
that faithfully predicts hurricane
tracks.
247
FEBRUARY 2002
AMERICAN
METEOROLOGICAL SOCIETY
|
On a personal note, I
first put the main ideas ex-
pressed here on paper
in the fall of 1977 as part of a
potential thesis
proposal. My advisor, E. N. Lorenz,
commented that this
was an interesting idea but too
risky for a thesis
topic. Control of the global atmo-
sphere is still a
risky research topic, but there have
been substantial
technological advances in many of
the supporting
disciplines—computers, models, re-
mote sensing, etc. We
believe there is a good reason
to pursue this
research now.
The concept of global weather
control raises a host
of sociological,
ecological, and political issues. These
issues will only
receive proper attention when global
weather control seems plausible. The questions raised
in these arenas will
not be easy to resolve, and progress
is likely to be slow
compared to the advance of tech-
nology. Therefore, it
seems important to demonstrate
this plausibility now,
long before technology advances
to the point of
potential implementation, in order to
motivate a thorough
discussion of whether or not, and
if so, to what extent
and under what circumstances
we actually do wish to
control the weather.
ACKNOWLEDGMENTS.
I have benefitted from
com-
ments on this
paper by R. Rosen, K. Emanuel, J. Hansen,
R. Anthes, and
an anonymous reviewer. This work was sup-
ported in part
by the NASA Institute for Advanced Con-
cepts (NIAC)
through a grant from the Universities Space
Research
Association (USRA).
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Hello, A. Joly, and S. Malardel, 1999: Adap-
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and R. S. Williams, 2000: Physics and
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and Z. Toth, 1999: Ensemble transforma-
tion and
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W., and J. C. L. Chan, 1999: Ensemble
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1997: Variational methods. J. Meteor. Soc.
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O., and H. L. Mitchell, 1998: Data as-
similation
using an ensemble Kalman filter tech-
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Joly, A., and
Coauthors, 1997: The fronts and
stormtrack
experiment (FASTEX): Scientific objec-
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experimental design. Bull. Amer. Meteor.
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Kalnay, E., S.
J. Lord, and R. D. McPherson, 1998: Matu-
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Optical properties of
contrail-induced cirrus: discussion of unusual halo
phenomena.
Photographs of a 120
degrees parhelion and a 22 degrees parhelion within persistent contrails are
presented. These phenomena result from hexagonal plate-shaped ice crystals
oriented horizontally with diameters between 300 mum and 2 mm. From our
observations and reinvestigation of previous reports, we conclude that a subset
of the population in persistent contrails can consist of highly regular,
oriented, hexagonal plates or columns comparable to the most regular crystals
in natural cirrus clouds. This is explained by measured ambient humidities
below the formation conditions of natural cirrus. The resulting strong
azimuthal variability of the scattering phase function impacts the radiative
transfer through persistent contrails.
PMID: 18253447 [PubMed -
in process]
Applied
Physics Laboratory, The Johns Hopkins University, Silver Spring, Md. 20910
(Manuscript received November 6, 1973)
DOI: 10.1175/1520-0450(1974)013<0563:MCSOBR>2.0.CO;2
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ABSTRACT
An unusual
case of multiple streamers or filaments with the characteristic mare's tail
pattern in vertical section has been observed by radar where the generating
elements were condensation trails laid by high-altitude aircraft. The contrails
were laid perpendicular to the wind and as they drifted a multitude of
streamers formed along each trail. The streamers extended from 9 km to the
ground. Numerous contrails were observed, each of which produced a sheet of
streamers. RHI and PPI photographs at X and S band taken over a 2-hr period
show the three-dimensional shape of the streamers due to the wind shear.
Doppler measurements were also taken. The resulting velocity spectra are very
narrow indicating little or no turbulence. Reflectivity factors were measured
at various altitudes and show a decrease in reflectivity with distance from the
generating line. Fall velocities based on the slopes of the streamer patterns
varied from 0.4 to 1.4 m sec−1. In general, the characteristics of the
precipitation streamers were quite similar to those previously measured in
naturally occurring cloud forms such as cirrus uncinus.
Authors: Fichter, Christine; Marquart, Susanne; Sausen,
Source: Meteorologische
Zeitschrift, Volume 14, Number 4, August 2005 , pp. 563-572(10)
Publisher: E. Schweizerbart'sche
Verlagsbuchhandlung
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Abstract:
Within the framework of the European Fifth Framework
Project TRADEOFF, the impact of changing cruise altitudes on contrail coverage
and corresponding radiative forcing was investigated. On the basis of the
reference year 1992, a series of aircraft emissions inventories with changed
flight altitudes was prepared. These emission scenarios provide flown
distances, fuel consumption and NOx emissions on a three-dimensional grid. The vertical
resolution of these inventories was significantly increased over that used in
former inventories. With a downshift of cruise altitude by 2000 ft(Throughout
this paper we denote flight levels in ft. 2000 ft convert to approximately 610
m.), 4000 ft, and 6000 ft global annual mean contrail coverage is reduced in an
approximately linear manner, reaching a maximum decrease of almost 45 % for a
6000 ft lower cruise altitude. Contrary to this, a slight increase by 6 % of
global annual mean contrail coverage resulted for a 2000 ft higher maximum
flight altitude. Relative changes of corresponding radiative forcing were shown
to be very similar to those of contrail coverage. For changes in contrail
coverage and radiative forcing associated with changes in flight altitudes, a
strong seasonal and regional variability was found. This study only considers
contrail radiative forcing. Trade-offs from other aviation related radiative
impacts, e.g., from CO2 or O3, have not been studied.
Document Type: Research article
DOI: 10.1127/0941-2948/2005/0048
People who read this article also read...
Effects of aircraft emissions on ozone, cirrus clouds,
and global climate
BUT SOME CONTRAILS ARE MORE THAN JUST CONTRAILS !!!
STORMS WITHOUT LIGHTNING \: EXPLANATION
CHAFF
CLOUDS
Article: pp. 302–314 | Full
Text | PDF
(1.53M)
NOAA, Environmental Research Laboratories,
National Severe Storms Laboratory, Norman, Oklahoma
(Manuscript received February 5, 1996, in
final form July 22, 1996)
DOI:
10.1175/1520-0450(1997)036<0302:ICSWLO>2.0.CO;2
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ABSTRACT
On 20/21 August
1993, deep convective storms occurred across much of Arizona, except for the
southwestern quarter of the state. Several storms were quite severe, producing
downbursts and extensive wind damage in the greater Phoenix area during the
late afternoon and evening. The most severe convective storms occurred from
0000 to 0230 UTC 21 August and were noteworthy in that, except for the first
reported severe thunderstorm, there was almost no cloud-to-ground (CG)
lightning observed during their life cycles. Other intense storms on this day,
particularly early storms to the south of Phoenix and those occurring over
mountainous terrain to the north and east of Phoenix, were prolific producers
of CG lightning. Radar data for an 8-h period (2000 UTC 20 August–0400 UTC 21
August) indicated that 88 convective cells having maximum reflectivities
greater than 55 dBZ and persisting longer than 25 min occurred within
a 200-km range of Phoenix. Of these cells, 30 were identified as
“low-lightning” storms, that is, cells having three or fewer detected CG
strikes during their entire radar-detected life cycle. The region within which
the low-lightning storms were occurring spread to the north and east during the
analysis period.
Examination of the
reflectivity structure of the storms using operational Doppler radar data from
Phoenix, and of the supportive environment using upper-air sounding data taken
at Luke Air Force Base just northwest of Phoenix, revealed no apparent physical
reasons for the distinct difference in observed cloud-to-ground lightning
character between the storms in and to the west of the immediate Phoenix area
versus those to the north, east, and south. However, the radar data do reveal
that several extensive clouds of chaff initiated over flight-restricted
military ranges to the southwest of Phoenix. The prevailing flow advected the
chaff clouds to the north and east. Convective storms that occurred in the area
likely affected by the dispersing chaff clouds were characterized by little or
no CG lightning.
Field studies in
the 1970s demonstrated that chaff injected into building thunderstorms markedly
decreased CG lightning strikes. There are no data available regarding either
the in-cloud lightning character of storms on this day or the technical
specifications of the chaff being used in military aircraft anti–electronic
warfare systems. However, it is hypothesized that this case of severe, but
low-lightning, convective storms resulted from inadvertent lightning
suppression over south-central Arizona due to an extended period of numerous
chaff releases over the military ranges.
RADAR
CHAFF USES AND TESTS
Article: pp. 1101–1125 | Abstract
| PDF
(1.83M)
Institute of Atmospheric Sciences, South
Dakota School of Mines and Technology, Rapid City 57701
(Manuscript received January 24, 1980, in
final form June 7, 1980)
DOI:
10.1175/1520-0450(1980)019<1101:CSEIAD>2.0.CO;2
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ABSTRACT
A two-dimensional,
slab-symmetric, time-dependent cloud model has been devised to simulate deep
convection in the atmosphere. The dynamics and thermodynamics of deep
convection are prescribed and the microphysics of the liquid phase is
parameterized. Within this framework, the electrical nature of the atmosphere
has been added. Small positive and negative ions as well as the charge
associated with rain and cloud particles are included. The electrical
properties are allowed full interaction with the hydrodynamic properties of the
model. Charge is transported by conduction, convection and turbulent diffusion,
and free ions interact with hydrometeors through conduction, diffusion and
evaporation. A separation probability is specified for cloud and raindrops
colliding in the electric field allowing for charge transfer by the
polarization mechanism. Similarly, the charge on cloud droplets is transferred
to raindrops during coalescence.
The formulation
for the simulation of the chaff seeding process is then developed. An initial
distribution of chaff fibers is devised allowing for the introduction of a
prescribed amount of chaff at any time and altitude. Transport of the chaff
fibers in the wind field is accounted for and ion production by chaff in the
electric field is parameterized. Five cases, a control case and four seeding
cases, are examined to explore the effect of the chaff ions on the electrical
properties of the cloud.
The control case
(case 1) is reviewed showing its basic dynamical, microphysical and electrical
nature. The chaff seeding experiments are then discussed with the seeding
altitudes, times and the amount of chaff dispensed differentiating the four
cases.
It is found that
chaff seeding at a rate of 4 kg km−1, which yields an initial
maximum concentration of 8.66 × 10−8 kg m−3,
attains a reduction in the electric field strength within the cloud in two
ways. In a direct manner, the chaff ions reduce the charge on the hydrometeors
by conduction and diffusion. In an indirect manner, the reduction of charge on
the hydrometeors in one region is seen to reduce the electric field in other
regions, thereby reducing the efficiency of the polarization mechanism there,
and subsequently reducing the amount of charge separated. Comparison of an
early and late seeding case reveals that the initial effect of the chaff ions
is different, but that after a short time the effects become comparable and the
final result of the two cases is nearly identical. This suggests that as long
as the chaff fibers penetrate the active portions of the cloud, the exact
seeding time is of little consequence. Finally, it is suggested that chaff
seeding may be useful in discriminating between inductive and non-inductive
charge separation mechanisms.
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Radar remote sensing of the clear atmosphere—Review
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Army Evaluation of
JP-8 and Diesel Fuel Exposed to Anti-Detonation Material Filler (ADMF) for
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