Back to Thermal Lore : Article series.
Thermal Lore - Part 1
by Dennis Pagen (copyright © 2002), published in USHPA’s publication “Paragliding” November 2002.
All illustrations and figures are from USHPA.
Soaring pilots live and dream under the thrall
of thermals. Sure, ridge lift lets us zoom around and play local hero, waves
are a gift from the gods and convergence is a magic carpet when you find it.
But only thermals are consistently present and readily exploitable by even
newly fledged novice pilots. Thermals are intriguing because they are mostly
invisible and they can take us to dizzying heights, in some cases higher than
big brother wants our tender wings to go.
Another aspect of thermals is that they
reward the development of certain skills, but involve an element of dumb luck.
Just as with fishing or picking up a new romance at a party, you can never be
100% sure about what you’re going to come up with when you go trolling. It is
that element of expectation and surprise that adds spice to the endeavor. With
thermals, we cast our net based on knowledge and how much height we have to
spend, then hope for the best. The fact that it so often pays off is a tribute
to our glider’s performance, the wealth of knowledge that has accumulated in
the flying community and the abundant lift that nature affords. Many of us wish
that fishing for seafood or mates had such a high rate of return.
This series of articles is intended to
illuminate the many aspects and peculiar behavior of those elusive entities we
know as thermals. The idea is to promote better flying through knowledge.
Hopefully pilots of all skill levels will find some nuggets to carry with them
into the wild blue yonder. My approach will be to try to avoid too much
technical detail, but offer references for those who wish to delve deeper. I
believe this format is appropriate for the vast majority of pilots, since much
of thermal flying is (and should be) intuitive. But we do need a solid
groundwork on which to let our intuitive nature roam free.
Much of what we discuss will come from
conversations with the world’s top pilots, but also an important source has
been research papers written on micrometeorology. These papers most notably
appear in the OSTIV publications, which is dedicated to the technical aspects
of soaring (sailplanes). In the last decade or so there has been much interest
in micrometeorology because of the development of drones, surveillance aircraft
and other small flying objects. I’m dubious about the uses of these craft, but
grateful for the advancement in understanding.
In the course of this series we will visit
the subjects of thermal development, shapes, behavior, types and ways to
exploit them. We will also look at special thermal situations such as the cause
of cloud suck, the “dead zone,” high-pressure thermals, East and West
differences and inversion encounters. Hopefully we will touch on some of the
very core material that will make each of us a better thermal pilot, or at
least informed enough to know why we hit the ground while others are scribing
taunting zeros high over our heads.
Without going deeper into matters such as lapse
rate and insolation right now, let’s look at the broad picture of how a thermal
day develops. Most of us know that the air mass sitting over our area must be
relatively unstable for thermals to exist in abundance or usable form. What we
mean by unstable is a certain temperature change in the air with changing
altitude. On an unstable day, thermals rise spontaneously once solar heating
gets underway and heats the surface adequately. Here’s the sequence:
1) The
sun’s energy, in the form of visible light and ultraviolet radiation, mostly
passes through the atmosphere and strikes the ground. The solid molecules on
the ground catch the solar radiation and convert it to molecular vibrations and
much longer wavelengths — infrared. We detect vibrations and infrared radiation
as heat, and so does the overlying air. It is the transfer of heat from the sun
to the ground and then to the air that allows the creation, birth and growth of
thermals. Thus, solar energy gives rise to all life, including thermals that
are born in the heat of the day.
2) In the
morning, as the air overlying the surface gets heated, not much happens as a
thin layer thickens and grows warmer. A slight sloshing around may occur here
and there, but no real thermal activity happens until suddenly, all heaven
breaks loose — thermals happen everywhere. What’s going on here? The answer is
that ground inversions stop the release of thermals until they have penetrated
to the top of the inversion (we’ll discuss the nature of inversions in a later
part). However, once this penetration occurs, the thermal release comes all of
a sudden and from widespread sources.
3) The
abundant release of thermals may continue for half an hour or so, then
frequently it shuts down for a spell before thermals reappear in earnest. After
that, a more sparse but regular production of thermals occurs. This is when the
thermal day sets in properly and we are apt to be successful when we cast our
fate to the wind. The mechanism that causes the thermal production pause, then
the more regular succession of thermals is as follows: The warming ground in
the morning heats a large area (almost the entire layer) of air over the
surface. Thus, there is a large reservoir of warm air to go up as thermals. But
this air can’t release because of the ground inversion. When the bonds of the
inversion are broken, the thermals release with a vengeance. These early
thermals may not be all that strong because the sun isn’t yet beaming down all
that hard, but they come in rapid succession and often are fairly continuous streams as the warm air on the ground
seeks restitution aloft.
But
when the warm air is depleted, it has been replaced by cooler air from aloft
that takes time to heat. So we have a pause. In addition, without the presence
of the widespread ground inversion, the thermals that do build can release when
they grow to a certain size, or they are induced to do so by triggering
mechanisms. The most common triggers are downdrafts impelled by the rise of
other thermals in the area. Thus, we have a picture of a steady-state growth
and release of thermals as long as the sun’s heat continues in sufficient
strength. The size of the thermals depends on (among other things) how long
they sit on the ground and grow before release. The initial release, then pause
in thermal production, is often seen in the ridge and valley systems in the
eastern U.S.
4) As the
day progresses, thermals tend to climb higher and peak in strength just a bit
after the peak solar heating. Then they dwindle in strength and frequency but
still retain their maximum height. Finally, only a few anemic old-maid thermals
rise as the sun wanes and our soaring prospects dim. In the end, only dreams of
the day’s glory remain unless special situations occur that continue to result
in the artificial release of heat from the surface. (The artificial matters may
be buildings with internal heat sources, fires or water heated by some means
other than the sun’s rays.)
5) As
evening falls, the moon rules and the earth loses what it has taken from the
sun. The heat re‑radiates off as infrared, and this effect sustains the
warmth of the air for a while, but with no new solar heat to tickle the earth’s
surface, the surroundings soon grow colder. Then, the air stills, chills, and a
ground inversion layer develops. This layer thickens throughout the night until
the sun again peeks over the peaks and warming begins again. The cycle is
complete.
Ground
inversions can be anything from a few feet to a few thousand feet in thickness
in extreme cases. The thickest inversions occur in deep valleys in desert
conditions. The reason for this situation is that desert conditions result in
rapid and extensive radiation of heat from the surface because of the clear,
dry air, and thus a much colder overlying layer. The high mountains surrounding
the valleys drain these layers of cold air down into the valleys all night long
until a blanket of cold air is pooled deeply in quiet repose.
The thicker the ground inversion layer in a
given area, the longer it takes to reach trigger temperature, which is where
thermals break through the inversion in the morning. However, in desert
conditions the sun’s heating is comparatively more intense, so trigger
temperature is reached relatively sooner than in humid areas. In addition,
thicker inversions often result in a longer initial release of thermals, and in
this case there may be no pause between initial release and the onset of
regular thermal production. The reason for this latter factor is that the
thermals developing in a thick inversion are already rising high enough to
promote the vigorous downdrafts that can trigger other thermals building on the
ground. Thus, once the thermals begin their initial rise to full potential, the
process continues unabated. This situation is often noticed in the Owens Valley
and the Alps.
There
are a number of factors that affect thermal strength. These are in two main
categories: the temperature profile of the air and the intensity of the solar
heating. Let’s look at the heating factor first.
The more readily a surface on the ground is
heated, the more it imparts this heat to the overlying air. Thus, we should
expect to get good thermals above such surfaces. Take a barefoot walk across
the landscape on a sunny day and see what you feel. Did your feet get burned on
that blacktop? Did you enjoy the cool of the grass? How about the medium heat
of bare dirt or fields in crops? We know from experience and common sense that
the surfaces that heat most are more likely to produce the best thermals. But
we also know that no surface stands alone. Everything is affected by everything
else surrounding it, because the atmosphere is a dynamic system. It is moving
and three dimensional, so sometimes an area that would normally be excellent
for thermal production is constantly being swept with cooler winds or stable
air and thus does not live up to its potential. One such situation is beach
areas. We have all burnt our feet on those littoral sands, but beaches are
rarely great thermal producers because the constant inflow of the cool, stable
sea breeze attenuates the effects of the heated surface.
A big factor in intensity of heating is the
humidity in the air. When the atmosphere is dry, the solar influx goes right to
the ground with nearly its full power. But in humid conditions, a good portion
of the solar radiation gets scattered by the suspended water molecules, so the
air itself takes up heat and less is available to heat the surface. You might
think, “That’s okay, what we want is heated air and we just bypass the surface
exchange in this situation.” Unfortunately, that’s not true. What happens in
the case of humid air is that the sun’s beaming heat is scattered deeply
throughout the air’s layers, so we don’t have the potentially unstable
situation of a warm blob at the bottom of cooler overlying air pressing down.
In fact, the hot, humid, summer doldrums are what we Eastern pilots dread,
because the few thermals that do develop are weak. In the case mentioned here
it should be apparent that there are many factors that affect both the amount
of surface heating and the lapse rate.
Two more factors that affect the solar
heating of the surface are the sun’s position and the amount of cloud cover. We
acquire an almost unconscious knowledge of the sun’s diurnal variation. We all
know that only mad Englishmen and dogs go out in the heat of the day in the
heart of Africa. So we know that the peak heating at the peak of the day
provides peak thermal production. But put a little fudge factor in there
because there is a lag in the whole process, so peak thermal production usually
occurs a half hour to an hour after maximum sun height. Speaking of sun height,
we should all be aware that June 21, when the sun is at its peak height, and
December 21 when it is at its low point, are the acme and nadir of thermal
production, all other factors being equal.
Clouds affect solar heating of the surface
and thus thermal production simply by blocking the sun’s rays and scattering or
absorbing the energy. Cumulus clouds denote thermals rising, so we are happy to
see them around as long as they don’t throw a wet blanket on our fun by
overdeveloping into sunshine-robbing shrouds. Clouds in general reduce the
strength of thermals, as well as their abundance. They also alter thermal
behavior. A broad, weak, stratus cover may make the day less punctuated with
thermal exclamation points, but also make the thermals more regular as the
thermals spend more time building on the ground and are less interrupted by
vigorous, cool downdrafts. We’ve also seen it happen that the approach of a
stratus layer is accompanied by pre-frontal unstable air, so the thermals
actually get stronger even as the solar insolation weakens. So, you can never
talk absolutes in this game, which is what makes it a game in the first place.
This
article speaks mostly in generalities in order to set the stage for our later
discoveries. However, we can still glean a few straws of learning from the
general discussion. Perhaps the main point to recognize is that at many sites
it is a normal process for the first thermals of the day to happen in the
morning, anywhere from 10:00 am to
11:59 am. Then, after a flurry of
thermal activity, things die down and nobody stays up until a bit later when
the thermal day begins in earnest. It is important to recognize this
occurrence, because you don’t want to be the early bird who gets to be in the
landing field feeling like a worm. Learn to understand the behavior of your own
site(s) in this regard. Does it happen nearly every good thermal day? Does it
never happen? What are the conditions when it does happen? (Hint: Clear nights
with little upper wind, so a deep ground inversion forms. Note that these are
the same conditions conducive to dew and frost formation.)
Once you have figured out your sites, carry
your newfound awareness with you when you visit other sites. As you gain
knowledge and experience you will perhaps be able to predict thermal behavior
at other sites. It is this type of understanding that helps create great
pilots, for after all, a great pilot is just like you and me but with more
skill, more knowledge and more luck. I just wish there were some way to work on
the luck factor.
We
bypassed the discussion of lapse rates to avoid over-complicating this first
installment. But next time we will give the subject its due, because it is
important to the understanding of how thermals really work. For more
information on the matter of solar heating, and thus thermal production daily
variation, see Understanding the Sky,
beginning on page 189.