Unit 3 · Wind and dynamics

What makes the wind blow

Foundations · about 40 minutes · Published

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Air pressure
Key terms
Wind, Wind direction, Knot, Anemometer, Gust, Beaufort scale, ASOS, Pressure gradient force, Isobar, Coriolis effect, Coriolis parameter, Rossby number, Geostrophic wind, Gradient wind, Ageostrophic wind, Atmospheric boundary layer, Ekman spiral, Cross-isobar angle, Buys Ballot’s law, Low-level jet, Sea breeze, Land breeze, Valley wind, Mountain wind

Wind is air moving from high pressure toward low pressure, turned by the earth's rotation and slowed by the ground. Three forces decide its speed and direction: the pressure gradient force, the Coriolis effect and friction. This lesson takes each in turn and puts numbers on it from one real storm, the great Midwest cyclone of October 26, 2010, whose sea-level pressure fell below 960 hPa over northern Minnesota: its isobars, its surface winds at 477 airports and nine Great Lakes buoys, and the balloon winds above it. It ends with the daily cycle of the wind at Dodge City, Kansas, the local winds of coasts and valleys, and the strongest winds ever measured.

An orange airport windsock on a white and yellow pole against a blue sky with white clouds: the throat of the sock is filled with air and points into the wind, while its tail hangs down.
A windsock in a light breeze. The sock at Frankenmuth, Michigan (airport 66G), April 27, 2024. Its open throat turns to face the wind, so the sock points downwind. The Federal Aviation Administration's specification designs a windsock "to fully extend when exposed to a wind of 15 knots"; this one is filled only near the throat, in a wind well under that. Photo: Mrmanssss, Wikimedia Commons, CC0.[16][5]
In this lesson

What wind is

The American Meteorological Society defines wind as "air in motion relative to the surface of the earth." Because vertical motion is small near the ground, "meteorologists use the term to denote almost exclusively the horizontal component. Vertical winds are usually identified as such."[1] A wind has a speed and a direction, and the direction follows a convention that confuses nearly everyone at first: wind direction is "the direction from which the wind is blowing."[1] A north wind blows from the north toward the south. The World Meteorological Organization measures it "clockwise from geographical north, namely, true north," so 90° is an east wind, 180° a south wind and 270° a west wind.[4]

Speeds come in four units. US weather reports use the knot, one nautical mile per hour, which the AMS gives as "1.1508 statute miles (1.852 km) per hour or 1.687 ft (0.5144 m) per second."[1] Forecasts for the public use miles per hour, science uses meters per second, and most of the world's public forecasts use kilometers per hour.

UnitWhere it is usedIn knotsIn meters per second
Knot (kt)Observations, aviation, marine forecasts, upper-air charts10.5144
Meter per second (m/s)Science, the WMO, most of this lesson's arithmetic1.9441
Mile per hour (mph)US public forecasts and warnings0.8690.447
Kilometer per hour (km/h)Public forecasts in most other countries0.5400.278

Conversions from the AMS definition of the knot and the international mile. For quick work, a speed in meters per second doubles to roughly knots, and a speed in knots adds about 15 percent to become miles per hour.

How wind is measured

An anemometer is "the general name for instruments designed to measure either total wind speed or the speed of one or more linear components of the wind vector," and those in common meteorological use "include the cup, propeller, Pitot-tube, hot-wire or hot-film, and sonic anemometers."[1] Direction was traditionally read from a wind vane, whose end with "the greater resistance to the motion of air moves to the downwind position."[1]

Height matters, because wind speed increases rapidly with height near the ground. The ASOS User's Guide records that airport wind sensors were once exposed 20 feet up, and that federal siting standards now specify "a height of 10 meters (32.8 feet)," with "typical ASOS wind sensor heights" of "33 feet or 27 feet, depending on local site-specific restrictions."[2] The WMO's Beaufort equivalents below are likewise given "at a standard height of 10 m above open flat ground."[4] The guide describes the cup-and-vane sensor of the 1990s; the National Weather Service's current ASOS sensor page is headed "Ultrasonic Ice Free Wind Sensor," and the averaging it describes is the same.[3]

The reported wind
A 2-minute average. ASOS measures once a second, forms 5-second averages, and "every 5 seconds a running 2-minute average wind (direction and speed) is computed." A 2-minute average of 2 knots or less is reported as calm.[2]
Gusts
A gust is "a sudden, brief increase in the speed of the wind," usually lasting "less than 20 s."[1] ASOS reports the greatest 5-second average of the past 10 minutes when it beats the current 2-minute average by 3 knots or more and the lowest 5-second speed of the period by 10 knots or more. "The minimum gust speed reported by ASOS is 14 knots."[2]
Peak wind
"The greatest 5-second average wind exceeding 25 knots which has been observed since the previously scheduled hourly METAR," added to the hourly report as a remark.[2]
Direction
Reported to the nearest 10°, relative to true north in the coded report, "e.g., 274 degrees is reported as 270 degrees."[2] The coded group 24010G20KT reads 240° at 10 knots, gusting to 20.

The rest of the world averages differently. The WMO's guide asks that "wind speed and direction for synoptic reports should represent an average over 10 min," warns that "1 min 'averages' should be described as long gusts," and settles on a gust duration of about 3 seconds, long enough, it says, to "engulf structures of ordinary suburban/urban size."[4] A 2-minute US wind and a 10-minute wind from another country's station are not the same quantity, and the shorter average reads a little higher in gusty air.

0102030405010 am11 amNoon1 pm2 pm3 pm4 pmKnotsOctober 26, 2010, CDT
Table: the hourly reports (METAR), Minneapolis-St. Paul, October 26, 2010
Time, CDTDirection, degreesSpeed, knotsGust, knots
10:53 am2401624
11:53 am2301932
12:53 pm2402233
1:53 pm2402233
2:53 pm2402035
3:53 pm2302036
Six hours of wind, minute by minute. Minneapolis-St. Paul airport, 10 am to 4 pm CDT October 26, 2010, as the storm in this lesson passed to the north. Blue: the 2-minute average wind recorded each minute, mostly between 15 and 23 knots (the 10th and 90th percentiles) and 19.4 on average. Orange: the highest 5-second average in each minute, 25.9 knots on average and 39 knots at its peak, at 2:19 pm. The circles are the six hourly reports: the wind (open) and the gust (filled), from 16 knots gusting to 24 at 10:53 am to 20 gusting to 36 at 3:53 pm. The hourly report is a sample of one 2-minute average from each hour. Data from the Iowa Environmental Mesonet.[8]

The Beaufort scale

Before anemometers were common, wind was estimated by eye. The Beaufort scale is "a system of estimating and reporting wind speeds using a numerical scale ranging from 0 (calm) to 12 (hurricane)," invented "in the early nineteenth century by Admiral Beaufort of the British Navy and was originally based on the effects of various wind speeds on the amount of canvas that a full-rigged frigate of the period could carry."[1] Its governing form today is the WMO's table of wind speed equivalents, which the WMO guide gives for use "when the instrumentation is temporarily out of operation or when it is not provided."[4]

ForceDescriptionKnotsm/smphSpecification for estimating speed over land
0Calm<10 to 0.2<1Calm; smoke rises vertically
1Light air1 to 30.3 to 1.51 to 3Direction of wind shown by smoke drift but not by wind vanes
2Light breeze4 to 61.6 to 3.34 to 7Wind felt on face; leaves rustle; ordinary vanes moved by wind
3Gentle breeze7 to 103.4 to 5.48 to 12Leaves and small twigs in constant motion; wind extends light flag
4Moderate breeze11 to 165.5 to 7.913 to 18Raises dust and loose paper; small branches are moved
5Fresh breeze17 to 218.0 to 10.719 to 24Small trees in leaf begin to sway, crested wavelets form on inland waters
6Strong breeze22 to 2710.8 to 13.825 to 31Large branches in motion; whistling heard in telegraph wires; umbrellas used with difficulty
7Near gale28 to 3313.9 to 17.132 to 38Whole trees in motion; inconvenience felt when walking against the wind
8Gale34 to 4017.2 to 20.739 to 46Breaks twigs off trees; generally impedes progress
9Strong gale41 to 4720.8 to 24.447 to 54Slight structural damage occurs (chimney pots and slates removed)
10Storm48 to 5524.5 to 28.455 to 63Seldom experienced inland; trees uprooted; considerable structural damage occurs
11Violent storm56 to 6328.5 to 32.664 to 72Very rarely experienced; accompanied by widespread damage
12Hurricane64 and over32.7 and over73 and over

Speeds are the equivalents at 10 m above open flat ground, and the descriptions are the WMO's own, from Table 5.1 of its Guide to Instruments and Methods of Observation.[4] The Minneapolis wind in the figure above, 20 knots gusting to 36, was force 5 by its average and force 8 in its gusts.

A day with a tight gradient

The examples in the rest of this lesson come from one storm. A low tracked northeast from the Plains on October 25, 2010 and crossed Minnesota on the 26th. The National Weather Service office in Milwaukee recorded that it set Wisconsin's record low pressure, 961.3 millibars at Superior, and that "Bigfork had a minimum sea level pressure of 955.2 millibars (28.21") at 5:13 PM CDT," a Minnesota record.[11] The barograms of the same storm are in the air pressure lesson. In the North American Regional Reanalysis (NARR), the 32 km analysis used here, the center deepened from 980 hPa at 7 pm CDT on the 25th to 959 hPa at 10 pm on the 26th. Computed here.[7]

L9659689729769809849889929961000
Table: the plotted winds, 18 UTC October 26, 2010
StationDirection, degreesSpeed, knotsGust, knotsGeostrophic wind, knotsGeostrophic directionTurned toward low, degrees
45001 (buoy)10331374716259
45002 (buoy)2103241402111
45003 (buoy)13927335418041
45004 (buoy)11032405317060
45006 (buoy)194192430157-37
45007 (buoy)21730375426346
45008 (buoy)15125305119847
46D30035436633535
9V931032475332111
ABR29031466531323
AIG20023385224545
ANJ14020306218848
ATY28030447031131
AZO22031394426343
BBW3003039443033
BMI230275325828
BRD26017245629535
CAD2202533462277
CAV26028366327919
CCY25024316827020
CDJ2601427422699
CIN26026365428121
CKN31024305433727
CMX180152645170-10
CNK290243643288-2
COU2602133462644
CVG2401324432433
DAY230135524818
DBQ24023297026121
DKB23027405726535
DLH18019243720020
DTW2201851216-4
DVN24028375526121
EFT23026416926232
EGV20013214323232
ELO13018242918353
ENL22017224324828
ERY12020355418969
EVV2101226341131
FDY21016255923424
FFL25028364726313
FFX22035424625636
FNB280243442273-7
FRM27029417128414
FSD2903041552955
FWA24022304527131
GLR15023345519646
GPZ330416188
GRI28026384529717
GUS23023325928656
GYL24019317228646
HCO108445-5
HDE28027373829717
HUF24014233628343
ICL2702128432722
IIB25022356626616
IMT17012254821545
IND23019275532393
INL7011192212959
IRK24020284426727
IWD20017263022323
JKJ30033416731717
JXN23020304324111
LNK290183644286-4
LRJ2802741512877
LWD25017264627323
MBS17017264421444
MCI280122442270-10
MCK29021323830313
MHE29031434830616
MIW2602841632688
MML28039467029818
MOX28033456730727
MTO2401625632411
OLU2902534462911
ONA23010217426535
OTG27036436629323
OXV2603240522677
P53200224350195-5
PCZ20025306124949
PKD29023296031828
RCX20025305023333
RNH23026316827141
RRT301417247040
RYV21028366325949
SBM21035486025343
SDF24012194825616
SPI24024334525414
STC26022387929232
SUS2602737462600
TOB24033397327535
TQE2703039482788
UIN25023334426010
VOK23024406825525
VPZ23032455527747
Y7020018314224747
YKN28030445029212
The storm at 1 pm CDT, October 26, 2010. Sea-level pressure from NARR, isobars every 4 hPa, around a 965 hPa low over northern Minnesota. The barbs are the observed winds at the same hour, thinned so they do not overlap: orange at airports, blue at Great Lakes buoys. Each barb's shaft points toward the direction the wind blows from; a full feather is 10 knots, a half feather 5 and a pennant 50. The isobars are packed tightest from the Dakotas across southern Minnesota, where the winds blow across them toward the low. Pressure from NARR; winds from the Iowa Environmental Mesonet and the National Data Buoy Center.[7][8][10]

The map shows everything the next sections explain. The winds circle the low counterclockwise. They are strongest where the isobars are closest together. And none of them blows exactly along the isobars: every barb is turned some way toward the low. At Faith, South Dakota (D07) the wind was from 300° at 39 knots, gusting to 53. At Bismarck it gusted to 51 knots and at Fargo to 42.

The pressure gradient force

The pressure gradient force is "the force due to differences of pressure within a fluid mass."[1] Air with higher pressure on one side than the other is pushed toward the lower pressure, at right angles to the isobars. Per unit mass the force is

F = (1/ρ) Δp/Δn

where ρ is the air's density and Δp/Δn is how fast pressure changes across the isobars. In words: the closer the isobars, the harder the push, and the same pressure difference pushes thin air harder than dense air.

At Minneapolis-St. Paul at 1 pm on October 26 the analyzed sea-level pressure fell by 4.99 hPa per 100 km toward the low, about the spacing of the 4 hPa isobars on the map: one every 80 km. With the air's density from the airport's own pressure and temperature, 1.214 kg/m³, the force is

(1/1.214) × 499 Pa / 100,000 m = 0.0041 m/s²

That is small, four ten-thousandths of gravity, but it acts all the time. On its own it would take air from rest to 40 m/s (78 knots) in under three hours. Computed here. The vertical pressure gradient is vastly larger, "approximately 10,000 times greater than the horizontal component," in the AMS glossary's words, but it is balanced by gravity, as the air pressure lesson shows.[1] The wind is the response to the small horizontal remainder. Something must stop the air from accelerating without limit, and on the scale of weather maps that something is the earth's rotation.

The Coriolis effect

The earth turns once a day beneath the air. Seen from the ground, anything moving over it appears to be pushed sideways. The AMS defines the Coriolis force as "an apparent force on moving particles in a noninertial coordinate system," one "required if Newton's laws are to be applied in this system." It "acts as a deflecting force, normal to the velocity, to the right of the motion in the Northern Hemisphere and to the left in the Southern Hemisphere. It cannot alter the speed of the particle."[1]

A physical picture helps. Air at rest over Kansas is carried east by the earth's rotation at about 360 m/s, the speed of the ground at 39° N. If the air moves north, toward latitudes where the ground travels east more slowly, it keeps its eastward speed and runs ahead of the ground beneath it: seen from the ground, it turns right. Moving south, it arrives over faster ground, lags and again turns right. The same holds for eastward and westward motion through the centrifugal effect of the earth's spin, and the AMS's full expression covers every direction.

The horizontal Coriolis force per unit mass is fV, where V is the wind speed and f is the Coriolis parameter, "twice the component of the earth's angular velocity about the local vertical, 2Ω sinφ, where Ω is the angular speed of the earth and φ is the latitude."[1] The earth turns once a sidereal day, so Ω = 7.292 × 10⁻⁵ per second.

LatitudeCoriolis parameter f, per secondCoriolis force on a 20 m/s wind, m/s²Inertial period
0° (equator)00none
10°2.53 × 10⁻⁵0.0005168.9 h
20°4.99 × 10⁻⁵0.0010035.0 h
30°7.29 × 10⁻⁵0.0014623.9 h
40°9.38 × 10⁻⁵0.0018818.6 h
45°1.03 × 10⁻⁴0.0020616.9 h
50°1.12 × 10⁻⁴0.0022315.6 h
60°1.26 × 10⁻⁴0.0025313.8 h
90° (pole)1.46 × 10⁻⁴0.0029212.0 h

Computed here. The inertial period, 2π/f, is the time air set moving with nothing but the Coriolis force acting on it takes to turn a full circle, "with constant speed and a velocity vector that constantly veers to the right in the Northern Hemisphere."[1] At 45° that is 17 hours. The deflection is slow: over a few minutes it hardly shows, over a day it dominates. That is why it governs weather systems and not much smaller motions. The AMS makes the point: "its importance in any given atmospheric motion may be judged from the representative speed and duration of the motion."[1] The Rossby number, U/(fL), makes it exact: for a 10 m/s wind in a system 1,000 km across at 45° it is 0.1, and rotation rules; for the same wind in a thunderstorm 10 km across it is 10, and rotation hardly matters. Computed here.

It follows that the Coriolis effect does not decide which way a sink drains. Water moving 10 cm per second at 45° feels a Coriolis acceleration of 1.0 × 10⁻⁵ m/s², about one millionth of gravity, for the few seconds it takes to cross the basin. Computed here. Thomas Humphrey of the Exploratorium in San Francisco, answering the question for Scientific American, put it this way: "Coriolis acceleration at mid-latitudes is about one ten-millionth the acceleration of gravity. Because it is a very small acceleration, it needs a very long distance for it to produce an appreciable curvature ... A toilet or sink is just not large enough." The direction comes instead from the basin's shape and from currents left over from filling it, which "can take more than a day" to die away, in the words of the physicist Robert Ehrlich in the same article.[12]

Geostrophic balance

Put the two forces together. Air starts toward low pressure, the Coriolis force turns it to the right, and it keeps turning until the two forces point in opposite directions and cancel. The wind that results is the geostrophic wind, "that horizontal wind velocity for which the Coriolis acceleration exactly balances the horizontal pressure force." It "is thus directed along the contour lines on a constant-pressure surface (or along the isobars in a geopotential surface) with low elevations (or low pressure) to the left in the Northern Hemisphere and to the right in the Southern Hemisphere."[1]

Above the boundary layerTwo forces in balance996 hPa1000 hPa1004 hPa1008 hPaLow pressureHigh pressurePressure gradientCoriolisWindNear the groundFriction added996 hPa1000 hPa1004 hPa1008 hPaLow pressureHigh pressurePressure gradientCoriolisFrictionWind
The balance of forces, schematic. Left: above the boundary layer, the pressure gradient force toward low pressure and the Coriolis force at right angles to the wind balance, and the wind blows along the isobars with low pressure on its left. Right: near the ground, friction slows the wind and pulls back against it; the slower wind feels a weaker Coriolis force, which can no longer balance the pressure gradient force alone, and the wind turns across the isobars toward low pressure until the three forces cancel. Drawn here for a 30° turn.

Setting the two forces equal, fV = (1/ρ) Δp/Δn, gives the geostrophic speed at the surface:

Vg = (1/ρf) Δp/Δn

At Minneapolis at 1 pm on October 26, with f = 1.03 × 10⁻⁴ per second at 44.9° N, the 4.99 hPa per 100 km gradient gives a geostrophic wind of 39.9 m/s, 78 knots, from 280°. The airport measured 22 knots from 240°. The next sections account for the difference: over the ground the real wind is not geostrophic. Aloft, where friction is absent, it nearly is.

On a constant-pressure chart the same balance is written with the height of the pressure surface instead of pressure, which removes the density: Vg = (g/f) Δz/Δn, where Δz/Δn is the slope of the surface across its height contours. The air pressure lesson explains why those charts are drawn on pressure surfaces; this is the other reason. At Detroit at 7 am CDT on October 26, the 500 hPa surface fell 29.4 m per 100 km toward the west-northwest. With f = 9.89 × 10⁻⁵ per second at 42.7° N the geostrophic wind is 9.81 × 0.000294 / 0.0000989 = 29.2 m/s, 57 knots, from 211°. The Detroit balloon measured 57 knots from 220°. Computed here from NARR heights and the radiosonde report.[7][9]

534540546552558564570576582
Table: radiosonde winds at 500 hPa, 12 UTC October 26, 2010, and the geostrophic wind from the NARR heights
StationHeight, mDirectionSpeed, knotsGeostrophic, knotsGeostrophic direction
CWMJ5,6402652928256
CWPL5,5001652938174
CWSE5,390350101213
CYAH5,5402851413261
CYJT5,5802755343280
CYSA5,7102604960268
CYYE5,40032573272
CYYQ5,4102203424224
CYZT5,4202801115305
K1Y75,7802905349293
KABQ5,6402807988286
KABR5,2903201518318
KALY5,7102552532250
KAMA5,59028083117286
KAPG5,7402902731303
KAPX5,5702155245211
KBIS5,3003101813342
KBMX5,7902355255230
KBNA5,7202355864240
KBOI5,4702703631273
KBRO5,8502751813278
KBUF5,6802503039235
KCAR5,6102703331266
KCHH5,7302354636247
KCHS5,8302753227277
KCRP5,8402602343264
KDDC5,4702904970303
KDNR5,4803003538282
KDRT5,8102703850258
KDTX5,6302205757211
KDVN5,42021099101207
KEDW5,7503006766281
KEPZ5,7502856767282
KEYW5,8701401317155
KFFC5,8102454345233
KFGZ5,6902806475284
KFWD5,7302556793264
KGGW5,3503203229341
KGJT5,5002753753301
KGRB5,3801855573183
KGSO5,7802603536258
KGYX5,6902603541266
KIAD5,7502803232276
KIAG5,6822513035234
KILN5,6902305863228
KILX5,5302058495223
KINL5,3801703955149
KJAN5,7802355258246
KJAX5,8602552015224
KLBF5,3803105464317
KLKN5,5103003946283
KLMN5,52027065111272
KLZK5,6802407886246
KMAF5,7402706382274
KMFL5,88021058139
KMFR5,4902855459280
KMHX5,8102903229269
KMIA5,882211512144
KMPX5,3101553542169
KNGP5,8372582442265
KNIP5,8622572014221
KNKX5,8102854849281
KNQX5,8681381318154
KOAK5,6802907477285
KOAX5,3302953038274
KOKX5,7302052525239
KOTX5,42045125166
KOUN5,59026593143262
KPIT5,7102404152224
KREV5,5802958574286
KRIW5,4403102433282
KRNK5,7702604435239
KSGF5,530225102153235
KSHV5,7402556672261
KSIL5,8302453945245
KSLC5,4903003946290
KSLE5,4502852217292
KTBW5,870215813204
KTFX5,4103102935321
KTLH5,8502302422217
KTOP5,3802605269264
KTUS5,7702955650296
KUIL5,4403202018327
KUNR5,3603153054310
KVBG5,7702956964285
KWAL5,7602902933299
KXMR5,8801951112208
KYUM5,7802905350291
MDSD5,880320101561
MMAN5,8502752130231
MMGM5,8402752532274
MMLP5,88033091256
MMMZ5,870355162276
MMUN5,870165619207
MYNN5,87035097186
PANN5,400300811236
TXKF5,8702201212241
The 500 hPa surface at 7 am CDT, October 26, 2010. Height contours from NARR every 60 m, labeled in decameters (540 is 5,400 m), around a closed low over eastern North Dakota at 5,279 m. The barbs are the balloon winds measured at 500 hPa at the same hour. Almost every one blows along the contours, with lower heights on its left, and they are strongest where the contours are packed, across the West and from the Ohio Valley to the Northeast. Heights from NARR; winds from the Iowa Environmental Mesonet's radiosonde archive.[7][9]

Testing it against balloon winds

One station agreeing proves little, so every radiosonde wind at 500 and 300 hPa in the four soundings from 7 pm CDT October 25 to 7 am October 27 was set against the geostrophic wind computed from the NARR heights at the balloon's launch site. Of 652 usable winds (a measured speed of at least 10 knots and a geostrophic speed of at least 5 m/s), the median difference in direction was 8°, and 81 percent were within 20°. The median observed speed was 0.93 of the geostrophic. Computed here.[7][9]

Observed wind against geostrophic wind020406080100020406080100Observed by radiosonde, m/sGeostrophic, m/s
Table: observed radiosonde winds against the geostrophic and gradient winds, 500 and 300 hPa, October 26 and 27, 2010
FlowWindsObserved / geostrophic, medianObserved minus geostrophic, mean, m/sWinds with a gradient-wind solutionObserved / gradient, medianObserved minus gradient, mean, m/s
Cyclonic2900.87-6.02901.143.6
Anticyclonic1891.040.81020.81-5.0
Nearly straight1400.91-3.61400.95-2.2
How geostrophic is the wind aloft? Each dot is one balloon wind at 500 or 300 hPa, October 26 and 27, 2010, set against the geostrophic wind from the NARR height gradient at the launch site: 619 winds within 40° of the geostrophic direction. They cluster along the dashed line, where observed equals geostrophic. Dots are colored by the curvature of the height contours: blue where the flow curves cyclonically, around troughs and lows (radius under 2,500 km), orange where it curves anticyclonically, around ridges, gray where it is nearly straight. The blue dots fall mostly below the line. Computed here.[7][9]

The scatter has a pattern. In cyclonically curved flow, 290 winds, the median observed speed was 0.87 of geostrophic and the average shortfall 6.0 m/s. In anticyclonically curved flow, 189 winds, it was 1.04, slightly faster than geostrophic. In nearly straight flow, 140 winds, it was 0.91. Computed here. Curvature is the subject of the next section. The largest winds on the chart, up to 162 knots at 300 hPa over Grand Junction, Colorado, belong to the jet stream, the subject of the jet stream lesson.

Curved flow: the gradient wind

Air that follows curved isobars is changing direction, and changing direction takes a net force toward the center of the curve, the centripetal acceleration, "with magnitude V²/R, where V is the speed of the particle and R the radius of curvature of the path."[1] So in curved flow the pressure gradient and Coriolis forces cannot cancel exactly. The balanced wind in that case is the gradient wind: at such points "the Coriolis acceleration and the centripetal acceleration together exactly balance the horizontal pressure force," and "it follows that the cyclonic gradient speed is less than (and the anticyclonic gradient speed is greater than) the geostrophic wind speed for the same latitude and pressure force."[1]

Around a lowLPressure gradient force exceeds Coriolis;the wind is slower than geostrophicAround a highHCoriolis exceeds the pressure gradient force;the wind is faster than geostrophic
Why curvature changes the speed, schematic. Around a low (left), the net force toward the center is the pressure gradient force minus the Coriolis force, so the Coriolis force, and with it the wind, must be smaller than in straight flow. Around a high (right), the net inward force is the Coriolis force minus the pressure gradient force, so the Coriolis force, and the wind, must be larger. Northern Hemisphere; arrow lengths illustrative.

In symbols, for a radius of curvature R that is positive around a low, V²/R + fV = fVg. Around the October 2010 low the effect is large: at 300 km from the center at 45° N, a 40 m/s geostrophic wind corresponds to a gradient wind of 23 m/s. Computed here. That is part of why the winds near the center of a deep low are lighter than its packed isobars suggest.

The same equation sets a limit around highs. For anticyclonic flow it has a real solution only if the geostrophic wind is no more than fR/4, and the gradient wind then cannot exceed fR/2. At 40° N and 500 km from the center of a high, that caps the geostrophic wind at 11.7 m/s and the pressure gradient at about 1.3 hPa per 100 km. Computed here. This is why the isobars near the center of a high are always widely spaced and its winds light, while a low can have gradients many times steeper, like the 5 hPa per 100 km over Minnesota on October 26.

The balloon check shows both the idea and its limits. The measured winds were slower than geostrophic in cyclonic flow and slightly faster in anticyclonic flow, as the gradient wind requires. But the gradient wind computed from the curvature of the analyzed height contours overcorrected: in cyclonic flow the observed winds ran at a median of 1.14 times the computed gradient wind, and in anticyclonic flow 87 of the 189 winds sat where the contour curvature was too tight for any gradient-wind solution. Computed here. The equation needs the curvature of the air's path, as the AMS definition says, and in a moving weather system the paths of the air are straighter than the contours they cross. The waves themselves are the subject of the troughs, ridges and shortwaves lesson, and the spin of curved flow is the subject of the vorticity lesson.

Friction and the boundary layer

Near the ground the balance changes. The lowest part of the atmosphere is the atmospheric boundary layer, "the bottom layer of the troposphere that is in contact with the surface of the earth. It is often turbulent and is capped by a statically stable layer of air or temperature inversion." Its depth ranges "from tens of meters in strongly statically stable situations, to several kilometers in convective conditions over deserts."[1] The AMS calls its old name, the friction layer, "somewhat inappropriate": "in the real atmosphere, turbulent drag, rather than molecular friction, is responsible for reducing wind speeds in the boundary layer."[1] Turbulent eddies carry the slow air near the ground upward and the fast air above downward, and the net effect is a drag on the wind.

Drag slows the wind. A slower wind feels a weaker Coriolis force, which can no longer balance the pressure gradient force, and the wind turns toward low pressure until the pressure gradient, Coriolis and drag forces balance, as in the right half of the balance figure. The angle between the wind and the isobars is the cross-isobar angle, which the AMS notes is "most conspicuous within the friction layer where the wind often has a component from high to low pressure."[1] The classic theory is the Ekman spiral, under which "the wind blows across the isobars toward low pressure, at an angle that is a maximum at the surface and does not exceed 45°."[1] The AMS also cautions that the Ekman layer "is not observed in the earth's atmosphere" in its idealized form, because large eddies and a stable cap shape the real boundary layer.[1]

How large is the angle in fact? Pyykkö and Svensson, comparing climate models with a climatology from more than 800 radiosonde stations, note that the Ekman solution gives 45° "yet, using more realistic assumptions, this angle is found to be lower," that the observed angles form a distribution "quite broad" and skewed toward positive values, and that every model and reanalysis they tested turns the wind too little.[13] They also note that most such studies are over land "due to a lack of suitable observations" over the ocean.[13] The October 2010 storm offers a direct measurement over land and water at once: every airport report and Great Lakes buoy report from October 26 to 28 at the NARR analysis times, each compared with the geostrophic wind from the analyzed sea-level pressure at its site.

How far the wind turned from the geostrophic direction0%10%20%30%−60°−30°0°30°60°90°Degrees toward low pressureEkman theory's limit, 45°Turning over land by time of day0°10°20°30°40°50°Midnight4 am8 amNoon4 pm8 pmMidnightLocal time, CDT
Table: turning toward low pressure and speed as a fraction of geostrophic, October 26 to 28, 2010
GroupReportsMedian turning, degreesMiddle half, degreesMedian speed / geostrophic
All airports6,4973422 to 450.35
Great Lakes buoys1503319 to 460.50
Airports, 1 am CDT792380.29
Airports, 4 am CDT786380.30
Airports, 7 am CDT801370.32
Airports, 10 am CDT848300.34
Airports, 1 pm CDT850270.45
Airports, 4 pm CDT832300.47
Airports, 7 pm CDT801330.39
Airports, 10 pm CDT787360.33
How far the surface wind turned toward low pressure. Top: the angle between each observed wind and the geostrophic wind at the same place and hour, October 26 00 UTC to October 28 00 UTC, 2010. Airports (orange, 6,497 reports) had a median of 34° and a middle half from 22° to 45°; Great Lakes buoys (blue, 150 reports) a median of 33° and a middle half from 19° to 46°. Four percent of the airport winds were turned the other way. Bottom: the median airport angle at each analysis time: 38° from 1 to 4 am CDT, 27° at 1 pm; the dashed line is the buoys' median. Computed here from NARR, ASOS and NDBC data.[7][8][10]

Three results stand out. First, the turning is large: a median of 34° over land, not far below Ekman's 45° and well above what models produce, as Pyykkö and Svensson found. Second, the speed falls much further than the direction turns. The airport winds ran at a median of 0.35 of the geostrophic speed; the buoy winds at 0.50, because open water is far smoother than land. Some of the shortfall near the low is curvature, not friction; the rest is drag. Third, the turning followed the clock. At 1 pm, when sunshine stirred the boundary layer, the median angle over land was 27° and the speed 0.45 of geostrophic; at 1 and 4 am it was 38° and 0.29 to 0.30. The buoys, with 16 to 27 reports at each hour, showed no clear daily cycle. Computed here.

The difference between the real wind and the geostrophic wind has a name, the ageostrophic wind: "the vector difference between the real (or observed) wind and the geostrophic wind."[1] Near the ground it is large and points across the isobars toward low pressure. The same two numbers, turning and speed, explain the Minneapolis report. At 1 pm the geostrophic wind was 78 knots from 280°; the airport measured 22 knots from 240°, 40° toward the low at 0.28 of the geostrophic speed. At buoy 45007, in southern Lake Michigan, the wind was 30 knots from 217° against a geostrophic wind of 54 knots from 263°. Computed here.

The cross-isobar flow matters beyond the station plot. Summed around a low, it carries air inward, toward the center, in the lowest kilometer. That air has to go somewhere, and it rises; how rising air on a large scale is organized is the subject of the lesson on why air rises.

Buys Ballot's law

Geostrophic balance gives a rule that needs no instruments. The AMS states Buys Ballot's law: "if one stands with the back to the wind, the pressure to the left is lower than to the right in the Northern Hemisphere. In the Southern Hemisphere, the relation is reversed." It was "formulated in 1857 by the Dutch meteorologist Buys Ballot and is a qualitative statement of the geostrophic wind relation."[1] Near the ground, where the wind is turned toward low pressure, the low lies to the left and somewhat ahead. At Minneapolis at 1 pm on October 26 an observer with a back to the 240° wind faced east-northeast, 60°, and the low lay north-northwest, at a bearing of 342°: 78° to the left of straight ahead rather than the full 90°. Computed here.

Why afternoons are gusty

The turning angle's daily swing is one sign of a larger rhythm. Over land in fair weather, the AMS notes, the boundary layer "has a marked diurnal cycle. During daytime, a mixed layer of vigorous turbulence grows in depth"; near sunset "turbulence decays, leaving a residual layer," and at night its bottom "is transformed into a statically stable boundary layer by contact with the radiatively cooled surface."[1] By day the mixed layer stirs the momentum of the air a kilometer or more up down to the anemometer. At night the stable boundary layer cuts the ground off from the wind above it. The lapse rates and stability and inversions lessons treat the temperature side of the same cycle.

Average wind speed, knots05101520Midnight4 am8 amNoon4 pm8 pmMidnightShare of reports with a gust0%20%40%60%80%Midnight4 am8 amNoon4 pm8 pmMidnightLocal time, CDT
Table: Dodge City, Kansas, hourly reports, April 2024
Hour, CDTReportsAverage speed, knotsReports with a gustAverage gust when reported, knotsCalm reports
Midnight2910.121%28.73%
1 am2910.217%27.60%
2 am299.621%24.73%
3 am269.38%24.54%
4 am2710.215%27.54%
5 am2910.717%28.23%
6 am2910.414%31.00%
7 am2910.617%28.20%
8 am3011.230%25.90%
9 am3013.647%28.80%
10 am3016.053%30.30%
11 am2715.459%29.40%
Noon2516.468%27.60%
1 pm2916.276%27.80%
2 pm2716.581%27.90%
3 pm2715.670%28.40%
4 pm3014.973%27.53%
5 pm2716.070%28.80%
6 pm2815.364%26.60%
7 pm2814.239%28.40%
8 pm2910.621%28.20%
9 pm299.210%33.33%
10 pm299.914%30.80%
11 pm2910.417%30.27%
The daily cycle of the wind at Dodge City, Kansas, April 2024. Top: the average of the hourly 2-minute winds at each hour, from 9.2 knots at 9 pm to 16.5 knots at 2 pm CDT. Bottom: the share of hourly reports that carried a gust, from 81 percent at 2 pm to 8 percent at 3 am and 10 percent at 9 pm. 681 hourly reports, each placed at the nearest whole hour. Data from the Iowa Environmental Mesonet.[8]

The wind picks up between 8 and 10 am and drops between 7 and 9 pm, in the hours after sunrise and around sunset, when the mixed layer grows and dies. The gusts follow it more strongly still, because a gust is a parcel of faster air brought down by a turbulent eddy, and the eddies are strongest in the afternoon. The strongest gust of the month, 53 knots, came at 1:52 pm on April 6. Computed here.

At night the wind above does not stop; it speeds up. Cut off from the ground's drag, the air a few hundred meters up accelerates, often past its geostrophic speed, and over the Plains it becomes the low-level jet, which the AMS places in the lowest 2 to 3 km of the troposphere and which at night is "sometimes called a nocturnal jet."[1]

03006009001,2001,500010203040Height above the ground, mMedian wind speed, knots
Table: median wind speed by height above the ground, Dodge City soundings, April 2024, knots
Height, m7 am CDT7 pm CDT
012.015.0
10016.915.6
20020.915.4
30025.517.8
40028.417.9
50030.618.8
60026.117.8
80025.019.0
1,00022.119.0
1,20022.618.9
1,50022.417.9
Calm below, fast above. The median wind speed at each height in the lowest 1,500 m over Dodge City, from the balloons launched at 7 am and 7 pm CDT through April 2024, 31 of each. At 7 am the wind at the ground was 12 knots and 500 m up 31 knots; at 7 pm, while the day's mixing lingered, it was 15 knots at the ground and 18 to 19 knots from 500 m to 1,200 m. Radiosonde reports from the Iowa Environmental Mesonet, interpolated between reported levels.[9]

The morning profile is the decoupled night in one picture: the ground has lost its connection to the wind above, and the jet that formed overnight sits a few hundred meters up. Once the sun rebuilds the mixed layer, that faster air is mixed down, which is why a calm dawn on the Plains so often turns into a windy, gusty late morning.

Sea breezes and valley winds

The same forces drive small winds. Where land and water or mountains and valleys heat unevenly, they build small pressure differences a few kilometers to a few tens of kilometers across, and the air responds. Over such short distances and times the Coriolis force has too little time to act, so these winds blow more nearly straight from high to low pressure.

The strongest winds

RecordSpeedWhere and whenSource
Highest wind gust measured by an anemometer (also the tropical cyclone record)113.2 m/s (253 mph, 220 kt)Barrow Island, Australia, April 10, 1996WMO[6]
Highest gust, Northern and Western Hemispheres103.3 m/s (231 mph)Mount Washington, New Hampshire, April 12, 1934, at 1,856 mWMO[6]
Highest tornadic wind speed135 m/s (302 mph)Bridge Creek, Oklahoma, May 3, 1999WMO[6]
Strongest tropical cyclones by maximum sustained wind (tie)95 m/s (185 kt, 215 mph)Typhoon Nancy, September 12, 1961; Hurricane Patricia, October 23, 2015WMO[6]

The WMO's archive lists the Barrow Island gust both as its maximum gust and as the tropical cyclone record, and keeps the tornado figure as a separate category. The Mount Washington gust, set 62 years before Barrow Island's, remains the record for the Northern and Western Hemispheres. The October 2010 storm, for comparison, produced gusts of 53 and 54 knots (61 and 62 mph) at South Dakota airports in the reports used here: force 10 on the Beaufort scale, in wind driven by the pressure gradient of a cyclone over land. Computed here.

Reading the wind on a map

  1. Find the pressure pattern first. Winds circle lows counterclockwise and highs clockwise in the Northern Hemisphere, and blow hardest where the isobars or height contours are packed.
  2. Aloft, expect the wind along the contours. Above about a kilometer the wind is close to geostrophic: within 20° of the contours in four cases out of five in the balloon check here.
  3. At the surface, expect it turned toward the low and slowed. About 30° to 40° across the isobars over land, and at a third to a half of the geostrophic speed, less at night and more on a sunny afternoon.
  4. Around a deep low, expect less than the gradient suggests; around a high, a little more, but the gradient near a high is never steep.
  5. Read the direction as "from." A 240° wind comes from the southwest and blows toward the northeast.
  6. Compare averages with averages. A US 2-minute wind, a 10-minute wind from elsewhere and a gust are three different numbers.

Current winds at thousands of US stations are on the site's Observations page, and coastal and buoy winds are on Marine.

Check yourself

  1. A METAR reports 31025G38KT. Where is the wind coming from, how fast, and what does G38 mean?

    Answer

    From 310°, the northwest, at a 2-minute average of 25 knots, with a gust (the highest 5-second average in the past 10 minutes) of 38 knots. On the Beaufort scale that is force 6 by the average and force 8 in the gusts.

  2. Two maps show the same pressure gradient, 2 hPa per 100 km, one at 30° N and one at 60° N. Where is the geostrophic wind faster, and by how much?

    Answer

    At 30° N. The geostrophic speed is inversely proportional to f = 2Ω sin φ, and sin 30° is 0.5 against 0.87 for 60°, so the wind at 30° is about 1.7 times faster.

  3. Why is there no geostrophic wind at the equator?

    Answer

    The horizontal Coriolis force is fV, and f = 0 at the equator. Nothing can balance the pressure gradient force, so the wind there cannot settle into flow along the isobars; air moves more directly from high to low pressure.

  4. Why does the surface wind cross the isobars toward low pressure, while the wind at 500 hPa does not?

    Answer

    Turbulent drag near the ground slows the wind, which weakens the Coriolis force. With the Coriolis force too weak to balance the pressure gradient force alone, the wind turns toward low pressure until pressure gradient, Coriolis and drag balance. At 500 hPa drag is negligible and the wind is nearly geostrophic.

  5. On October 26, 2010, airport winds crossed the isobars at a median of 38° at 4 am and 27° at 1 pm. Why the difference?

    Answer

    In the afternoon, sunshine drives turbulent mixing through a deep boundary layer, bringing fast, less-turned air from above down to the surface. At night a stable layer cuts the ground off from the air above, and the surface wind is slower and turned further.

  6. Two systems have isobars equally spaced; one curves around a low, the other around a high. Which has the stronger wind?

    Answer

    The high. Around a low the net inward force is the pressure gradient force minus the Coriolis force, which makes the wind subgeostrophic; around a high it is the Coriolis force minus the pressure gradient force, which makes it supergeostrophic. The balloon winds in October 2010 ran at 0.87 of geostrophic in cyclonic flow and 1.04 in anticyclonic flow.

  7. Standing with your back to the wind in Chicago, where is the low?

    Answer

    To the left, by Buys Ballot's law, and somewhat ahead of straight left, because the surface wind is turned toward the low.

  8. A friend says the Coriolis effect makes toilets flush the other way in Australia. What is the size of the effect?

    Answer

    About a millionth of gravity for water moving 10 cm per second, far smaller than the effects of the bowl's shape and the jets that fill it. The Coriolis effect matters only for motions that are large and long-lived, like weather systems.

Video

The Coriolis effect and winds. Part three of the Met Office's series on the global circulation.[17]
The Coriolis effect in action. The Met Office.[18]
The Coriolis effect. MetLink, the Royal Meteorological Society's education service.[19]
Geostrophic wind and geostrophic balance. A lecture by Djordje Romanic.[20]

Methods

Pressure and heights are from the NCEP North American Regional Reanalysis, read from NOAA PSL over OPeNDAP on its 32.463 km Lambert conformal grid; the projection used for the maps and the gradients reproduces NARR's own latitude and longitude arrays to within 0.006 of a grid cell. Gradients are centered differences times the map factor, rotated to true north, and interpolated bilinearly to each station. Surface geostrophic winds use sea-level pressure (smoothed once with a 1-2-1 filter) and the density from each report's own pressure and temperature; winds aloft use the 500 and 300 hPa heights, smoothed twice, and contour curvature is the divergence of the unit normal to the height contours after twelve passes. Curvature classes: cyclonic above 0.4 and anticyclonic below −0.4 per 1,000 km. Surface reports are the ASOS routine reports of 13 states from ND to OH and KS to KY within 20 minutes before or 5 minutes after each 3-hourly analysis time, and the hourly NDBC reports of nine Great Lakes buoys (45001 to 45008 and 45012); a report enters the turning statistics if its wind is at least 5 knots and the geostrophic wind at least 5 m/s. Buoy winds are 8-minute averages from anemometers a few meters above the water, not the 2-minute 10 m winds of ASOS, which favors lower speeds on the buoys.[10] Radiosonde winds at 500 and 300 hPa are from IEM's archive, 00 and 12 UTC October 26 and 27, 2010, for winds of 10 knots or more where the geostrophic wind is at least 5 m/s; the figure omits the 33 whose direction differed from geostrophic by more than 40°. Gradient winds solve κV²/f + V − Vg = 0 with κ the contour curvature. Dodge City statistics use every routine report of April 2024 (CDT) and every 12 and 00 UTC sounding whose reported wind levels reach 1,500 m above the ground, interpolated in wind components. Coriolis values use Ω = 7.2921 × 10⁻⁵ per second. The code and data are in the site's repository, in scripts/learn/what-makes-the-wind-blow.mjs, scripts/learn/what-makes-the-wind-blow-fetch.mjs and scripts/learn/what-makes-the-wind-blow-data/. Map outlines are Natural Earth.[15]

Isobars, pressure surfaces and the storm's barograms are in Air pressure. The stable night and the mixed afternoon are in Lapse rates and stability, and the sea breeze's temperature contrast in Temperature and heat. Wind barbs on a sounding are read in How to read a skew-T. Unfamiliar terms are in the glossary.

Sources

Quotations are verbatim from the source named. Figures and numbers marked "computed here" are described under Methods.

  1. American Meteorological Society, Glossary of Meteorology, entries wind, wind direction, knot, gust, ageostrophic wind, anemometer, wind vane, Beaufort wind scale, pressure-gradient force, Coriolis force, Coriolis parameter, inertial oscillation, Rossby number, geostrophic wind, centripetal acceleration, gradient wind, atmospheric boundary layer, friction layer, cross-isobar angle, Ekman spiral, Ekman layer, Buys Ballot's law, low-level jet, sea breeze, land breeze, valley wind and mountain wind.
  2. National Weather Service, Automated Surface Observing System (ASOS) User's Guide, 1998, section 3.2, Wind.
  3. National Weather Service, ASOS wind sensor.
  4. World Meteorological Organization, Guide to Instruments and Methods of Observation (WMO-No. 8), Volume I, 2023 edition, Chapter 5, Measurement of surface wind, including Table 5.1, Wind speed equivalents.
  5. Federal Aviation Administration, Advisory Circular 150/5345-27F, Specification for Wind Cone Assemblies, 2021.
  6. World Meteorological Organization, World Weather and Climate Extremes Archive, Records of weather and climate extremes, as of January 30, 2024.
  7. F. Mesinger and coauthors, North American Regional Reanalysis, NCEP; data from NOAA Physical Sciences Laboratory, NCEP North American Regional Reanalysis: 3-hourly sea-level pressure (prmsl) and isobaric heights, October 2010.
  8. Iowa Environmental Mesonet, Iowa State University, ASOS-AWOS-METAR data download and one-minute ASOS data: 13 states, October 26 to 28, 2010; Minneapolis-St. Paul (MSP) one-minute data, October 26, 2010; Dodge City (DDC), April 2024.
  9. Iowa Environmental Mesonet, upper-air sounding archive: 500 and 300 hPa, 00 and 12 UTC October 26 and 27, 2010; Dodge City (DDC), April 2024.
  10. National Data Buoy Center, historical standard meteorological data, buoys 45001 to 45008 and 45012, 2010, and measurement descriptions.
  11. National Weather Service Milwaukee/Sullivan, Historic low pressure, October 26, 2010.
  12. Scientific American, Does water flowing down a drain spin in different directions depending on which hemisphere you're in?, January 28, 2001, answers by Fred W. Decker, Robert Ehrlich and Thomas Humphrey.
  13. Joakim Pyykkö and Gunilla Svensson, Wind Turning in the Planetary Boundary Layer in CMIP6 Models, Journal of Climate 36, 2023, 5727 to 5742.
  14. NOAA JetStream, The Sea Breeze.
  15. Natural Earth, 1:50m admin 1, states and provinces, with lakes, public domain.
  16. Mrmanssss, United States Airport Windsock at 66G Airport, Frankenmuth, MI, Wikimedia Commons, CC0.
  17. Met Office, What is global circulation? Part Three: The Coriolis effect and winds, YouTube (Met Office - Learn About Weather).
  18. Met Office, The Coriolis effect in action, YouTube (Met Office - Learn About Weather).
  19. Royal Meteorological Society, MetLink: The Coriolis Effect, YouTube.
  20. Djordje Romanic, Geostrophic Wind and Geostrophic Balance, YouTube.

Corrections: contact@weatherovertime.com.

Unit 3: Wind and dynamics

  1. What makes the wind blow

    Pressure gradient, Coriolis and friction, and why wind crosses the isobars near the ground.

    Foundations40 min
  2. The jet stream

    Where the jet stream comes from, how it moves, and what jet streaks do.

    Foundations40 min
  3. Troughs, ridges and shortwaves

    The waves in the upper-level flow and the weather under each part of them.

    Intermediate40 min
  4. Vorticity

    Spin in the atmosphere, from the jet stream down to the mesocyclone.

    Intermediate40 min
  5. Why air rises: lift on the large scale

    Divergence aloft, warm air advection and the quasi-geostrophic picture of ascent.

    Advanced40 min