Pressure Pattern
Weather maps on TV and the Internet often show a surface
high (as opposed to high pressure aloft in the troposphere) with
an "H". Technically this is not surface pressure, but rather what the
pressure would be if the pressure at the surface was reduced to
sea level.
Pressure at the Earth's surface varies
with elevation over topography (lower pressure at higher elevations).
If a map actually showed surface pressure it would look a lot
like a topograpical map, and we wouldn't be able to pick out areas of
low and high pressure due to weather. Since our focus is on the
weather, we want to see pressure patterns due to high and low pressure
systems (not due to elevation changes). To overcome this, we calculate
what the surface pressure would be if we were down at sea
level. The result is a nice looking map of high and low pressure (Fig.
5ei.6). This is known as sea level pressure (SLP) or mean sea level
pressure (MSLP).
Pressure is shown on these maps with isobars.
Fig. 5ei.5 - Examples of surface high pressure
on a weather map. The contours are isobars (explained below). The
arrows show the direction of airflow in a clockwise direction around
the high. (Credit: Stull)
Isobars are
lines, or contours, connecting
locations that have the same pressure.
Isobars can be used to indicate high pressure centres and low
pressure centres. Both highs and lows are surrounded by concentric
isobar circles, which represent a maximum or minimum
in pressure, respectively. A high is a maximum in pressure
(Fig. 5ei.5a above), and the isobars around a high indicate that if you
travel in any direction away from the high, you will find
decreasing pressure values. To think of it in the reverse sense, if you
travel towards the high from any direction, pressure will
increase as you approach the high centre. This is just like on a
topographic map where the lines of constant elevation can show a
mountain peak, which is an elevation maximum. The opposite is true for
low pressure centres: the values of the isobars they decrease towards
the centre. We will discuss this more later.
It's also possible to have high pressure ridges
and low pressure troughs. Fig. 5ei.5b above shows a
high pressure ridge. The centre, or axis,
of the
ridge is indicated by a squiggly line. Ridges are areas of relatively
high pressure that extend out from high pressure centres. In a ridge,
the isobars do not form a closed circle, but rather partially enclose
values of higher pressure. If you travel away from a ridge in most
directions, pressure will decrease, but not in all directions. If you
travel along a ridge towards the high pressure centre it's
connected to, pressure will increase towards the high pressure centre.
They are visible on pressure maps as "kinks" in the isobars pointing
away from the high pressure centre. On a topographical
map, pressure
ridge is equivalent to a mountain ridge.
Recommended - watch this video: How to Read Temperature Maps.
Let's take a look at a real-world sea level pressure map:
Fig. 5ei.6 - A sea level pressure (SLP,
contoured) weather map for a summer's day over North America. (Credit:
West)
On some maps highs are marked with an "H" and lows are marked
with
an "L". Not all contours are labelled with values, so it can sometimes
be difficult to infer whether SLP values are increasing or decreasing
towards the closed circles that indicate the high and low centres.
With practice highs and lows will become easier to identify.
As an example, let's look at the high over northwestern North
America in
Fig. 5ei.6 above. Its centre is the highest pressure in the region. If
you
were to travel away from it in any direction, you'd encounter lower
pressure values. Now let's look at the high pressure ridge extending
northwest from the high. If you approach the ridge axis (squiggly line)
from the southwest or northeast (perpendicular to the axis), pressure
values
increase towards it. However, if you travel northwards along
the ridge, pressure values increase towards the high pressure centre.
There
is usually a scarcity of precipitation around a high pressure (not
shown on above figure), which can also help identify highs vs. lows.
Weather Conditions - The "why"
Let's bring it full circle now — why does high pressure bring
good weather?
Winds diverge away from the centre of high pressure, flowing
from higher to lower pressure. Due to the Coriolis effect, which turns
winds to the right (in the northern hemisphere), the wind spirals
outward in a clockwise circulation (Figs. 5ei.5a and 5ei.7). Pressure
differences are typically fairly weak under high pressure, so
winds tend to be lighter. This is important for snow sports,
as these
low winds can make for ideal ski conditions at the resort. In the
backcountry, where you're often far from shelter, low wind conditions
are even more important to safe travel.
Fig. 5ei.7 - Wind flow around a high pressure
system. Diverging at the low levels, spiralling out in a clockwise
direction due to the coriolis force, and subsiding from aloft. (Credit:
COMET/UCAR)
As winds diverge away from the centre of the surface high
pressure, compensating air sinks downward from aloft to fill
the void. When air travels downward in the
atmosphere, it becomes warmer and drier. For this
reason, high pressure systems are typically associated with
dry conditions, clearer skies, and a lack of precipitation.
Fig. 5ei.8 - Typical high pressure conditions
showing early morning blue sky and alpenglow over Cloudraker Mountain,
BC. (Credit: West)
Fig. 5ei.9 - Typical high pressure conditions
showing high wispy cirrus clouds over Mount Hood, OR, USA. Good
visibility and low winds are perhaps most critical to skiers on high,
isolated peaks, like volcanoes. (Credit: West)
High pressure, however, also carries with it some weather
hazards. First, with sun and warmth come sunburn, sweating, and
dehydration. It's important to cover up when it's sunny, especially
while skiing.
Insolation (not to be
confused with insulation, which is very different) is
a convenient term that refers to incoming solar radiation. It
includes all types of radiation from the sun. However, we're concerned
with just two types here: visible light and ultraviolet (UV) radiation.
Recall that pressure decreases with height in the atmosphere
because there's less air above you the higher you go. This means that
when you're at a high elevation in the mountains, there's less
atmosphere above you to absorb the insolation. At 3,000 m (~10,000 ft)
altitude, there's about 30% less atmospheric protection above you.
Further, snow can reflect more than 90% of light, which means
you get hit with most of the insolation again after it
reflects off the snow. It's best to cover up as much as possible, and
where you're not covered, apply (and reapply) high-SPF sunscreen. This
is especially important after about mid-February when the sun is
stronger.
Fig. 5ei.10 - Two examples of poor sun
protection during spring/summer skiing. As shown in the second picture,
covering yourself also protects against snow rash (spring/summer snow
is very abrasive). Left: Sessioning a kicker at Alta, UT, USA. Right:
Crashing on a summer snowfield on Mount Washington, NH, USA. (Credit:
West)
In the spring, ski tourers and mountaineers often wear a glacier or sun hat
with built-in sun protection. Perhaps even more important are special glacier glasses — sunglasses that
are very dark, and have side, top, and bottom protection to protect
your eyes from exposure to insolation (Fig. 5.ei.11). Insolation (and
that reflected off the snow) is strong enough at this time of year that
some skiers put sunscreen on the inside of their nostrils, and
sometimes get sunburn on the roof of their mouth! Glacier glasses
protect against the very real danger of snow
blindness. This is a temporarily debilitating blindness, a
very real danger on a mountain with hazards where navigation is
paramount to survival.
Fig. 5ei.11 - An example of good sun protection
coverage on Mount Skook Jim, Stein Valley, BC. (Credit: West)
High pressure does not guarantee nice weather. Occasionally
there can be strong
winds during a period of high pressure. These may be due to
pressure differences associated with an
approaching low pressure system, or due to local terrain-driven
effects. We'll cover some of these later.
Increasing high clouds (with the approach of a low pressure
system) can lead to flat light,
where the clouds
diffuse the light, and the snow surface no longer has any definition.
You'll know it when it happens. You may not be able to tell downhill
sections of the slope from flat or uphill areas. You might get caught
off guard by a mogul, bump, or gully. It's best to exercise caution and
slow, safe skiing under these conditions. Lastly, high pressure is
sometimes associated with very cold air temperatures, especially in
valleys, along with
valley clouds and fog. We'll cover this later as well.