30
C hapter 2 The precipitation in the country (India) is mainly in the form of rain fall though there is appreciable snowfall at high altitudes in the Himalayan range and most of the rivers in north India are perennial since they receive snow-melt in summer (when there is no rainfall). 2.1 TYPES OF PRECIPITATION The precipitation may be due to (i) Thermal convection (convectional precipitation)—This type of precipiation is in the form of local whirling thunder storms and is typical of the tropics. The air close to the warm earth gets heated and rises due to its low density, cools adiabatically to form a cauliflower shaped cloud, which finally bursts into a thunder storm. When accompanied by destructive winds, they are called ‘tornados’. (ii) Conflict between two air masses (frontal precipitation)—When two air masses due to contrasting temperatures and densities clash with each other, condensation and precipita- tion occur at the surface of contact, Fig. 2.1. This surface of contact is called a ‘front’ or ‘frontal surface’. If a cold air mass drives out a warm air mass’ it is called a ‘cold front’ and if a warm air mass replaces the retreating cold air mass, it is called a ‘warm front’. On the other hand, if the two air masses are drawn simultaneously towards a low pressure area, the front developed is stationary and is called a ‘stationary front’. Cold front causes intense precipitation on com- paratively small areas, while the precipitation due to warm front is less intense but is spread over a comparatively larger area. Cold fronts move faster than warm fronts and usually over- take them, the frontal surfaces of cold and warm air sliding against each other. This phenom- enon is called ‘occlusion’ and the resulting frontal surface is called an ‘occluded front’. (ii) Orographic lifting (orographic precipitation)—The mechanical lifting of moist air over mountain barriers, causes heavy precipitation on the windward side (Fig. 2.2). For exam- ple Cherrapunji in the Himalayan range and Agumbe in the western Ghats of south India get very heavy orographic precipitation of 1250 cm and 900 cm (average annual rainfall), respec- tively. (iv) Cyclonic (cyclonic precipitation)—This type of precipitation is due to lifting of moist air converging into a low pressure belt, i.e., due to pressure differences created by the unequal heating of the earth’s surface. Here the winds blow spirally inward counterclockwise in the northern hemisphere and clockwise in the southern hemisphere. There are two main types of cyclones—tropical cyclone (also called hurricane or typhoon) of comparatively small diameter of 300-1500 km causing high wind velocity and heavy precipitation, and the extra-tropical cyclone of large diameter up to 3000 km causing wide spread frontal type precipitation. 17 PRECIPITATION

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Page 1: Ch 2 Precipitation(Raghunath)

Chapter 2

The precipitation in the country (India) is mainly in the form of rain fall though there isappreciable snowfall at high altitudes in the Himalayan range and most of the rivers in northIndia are perennial since they receive snow-melt in summer (when there is no rainfall).

2.1 TYPES OF PRECIPITATION

The precipitation may be due to(i) Thermal convection (convectional precipitation)—This type of precipiation is in the

form of local whirling thunder storms and is typical of the tropics. The air close to the warmearth gets heated and rises due to its low density, cools adiabatically to form a cauliflowershaped cloud, which finally bursts into a thunder storm. When accompanied by destructivewinds, they are called ‘tornados’.

(ii) Conflict between two air masses (frontal precipitation)—When two air masses dueto contrasting temperatures and densities clash with each other, condensation and precipita-tion occur at the surface of contact, Fig. 2.1. This surface of contact is called a ‘front’ or ‘frontalsurface’. If a cold air mass drives out a warm air mass’ it is called a ‘cold front’ and if a warm airmass replaces the retreating cold air mass, it is called a ‘warm front’. On the other hand, if thetwo air masses are drawn simultaneously towards a low pressure area, the front developed isstationary and is called a ‘stationary front’. Cold front causes intense precipitation on com-paratively small areas, while the precipitation due to warm front is less intense but is spreadover a comparatively larger area. Cold fronts move faster than warm fronts and usually over-take them, the frontal surfaces of cold and warm air sliding against each other. This phenom-enon is called ‘occlusion’ and the resulting frontal surface is called an ‘occluded front’.

(ii) Orographic lifting (orographic precipitation)—The mechanical lifting of moist airover mountain barriers, causes heavy precipitation on the windward side (Fig. 2.2). For exam-ple Cherrapunji in the Himalayan range and Agumbe in the western Ghats of south India getvery heavy orographic precipitation of 1250 cm and 900 cm (average annual rainfall), respec-tively.

(iv) Cyclonic (cyclonic precipitation)—This type of precipitation is due to lifting of moistair converging into a low pressure belt, i.e., due to pressure differences created by the unequalheating of the earth’s surface. Here the winds blow spirally inward counterclockwise in thenorthern hemisphere and clockwise in the southern hemisphere. There are two main types ofcyclones—tropical cyclone (also called hurricane or typhoon) of comparatively small diameterof 300-1500 km causing high wind velocity and heavy precipitation, and the extra-tropicalcyclone of large diameter up to 3000 km causing wide spread frontal type precipitation.

17

PRECIPITATION

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18 HYDROLOGY

Frontal surfacecold air mass Warm air

mass

(a) Cold front (b) Warm front

Cold airmass

Frontal surface

Warm airmass

Warmair

Cold airColder air

(c) Stationary front

Low pressure

Fig. 2.1 Frontal precipitation

Sea

msl

Heavy rain

Windward(Seaward side)

Mountainousrange

Leeward(Landward) side

Rain-shadow area

Land

Fig. 2.2 Orographic precipitation

2.2 MEASUREMENT OF PRECIPITATION

Rainfall may be measured by a network of rain gauges which may either be of non-recording orrecording type.

50

Measuringjar (glass)

60 cm60 cm

20 cm20 cm

55 cm55 cm

25 cm25 cm

5 cmGL 5 cm5 cm

GL

Masonryfoundation block

60 cm × 60 cm × 60 cm

12.5 cm

Rim (30 cm above GL)

Metal casing

Funnel

Glass bottle(7.5-10 cm dia.)

Ground level

Fig. 2.3 Symon’s rain gauge

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The non-recording rain gauge used in India is the Symon’s rain gauge (Fig. 2.3). It con-sists of a funnel with a circular rim of 12.7 cm diameter and a glass bottle as a receiver. Thecylindrical metal casing is fixed vertically to the masonry foundation with the level rim 30.5cm above the ground surface. The rain falling into the funnel is collected in the receiver and ismeasured in a special measuring glass graduated in mm of rainfall; when full it can measure1.25 cm of rain.

The rainfall is measured every day at 08.30 hours IST. During heavy rains, it must bemeasured three or four times in the day, lest the receiver fill and overflow, but the last meas-urement should be at 08.30 hours IST and the sum total of all the measurements during theprevious 24 hours entered as the rainfall of the day in the register. Usually, rainfall measure-ments are made at 08.30 hr IST and sometimes at 17.30 hr IST also. Thus the non-recording orthe Symon’s rain gauge gives only the total depth of rainfall for the previous 24 hours (i.e.,daily rainfall) and does not give the intensity and duration of rainfall during different timeintervals of the day.

It is often desirable to protect the gauge from being damaged by cattle and for thispurpose a barbed wire fence may be erected around it.

Recording Rain GaugeThis is also called self-recording, automatic or integrating rain gauge. This type of rain gaugeFigs. 2.4, 2.5 and 2.6, has an automatic mechanical arrangement consisting of a clockwork, adrum with a graph paper fixed around it and a pencil point, which draws the mass curve ofrainfall Fig. 2.7. From this mass curve, the depth of rainfall in a given time, the rate or inten-sity of rainfall at any instant during a storm, time of onset and cessation of rainfall, can bedetermined. The gauge is installed on a concrete or masonry platform 45 cm square in theobservatory enclosure by the side of the ordinary rain gauge at a distance of 2-3 m from it. Thegauge is so installed that the rim of the funnel is horizontal and at a height of exactly 75 cmabove ground surface. The self-recording rain gauge is generally used in conjunction with anordinary rain gauge exposed close by, for use as standard, by means of which the readings ofthe recording rain gauge can be checked and if necessary adjusted.

30 cm

Receiver

FunnelTipping bucket

To recordingdevice

Measuring tube

Revolving drum(chart mounted)

Clock mechanism Pen

Springbalance

Catchbucket

Metal cover

Receivingfunnel

Fig. 2.4 Tipping bucket gauge Fig. 2.5 Weighing type rain gauge

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20 HYDROLOGY

There are three types of recording rain gauges—tipping bucket gauge, weighing gaugeand float gauge.

Tipping bucket rain gauge. This consists of a cylindrical receiver 30 cm diameterwith a funnel inside (Fig. 2.4). Just below the funnel a pair of tipping buckets is pivoted suchthat when one of the bucket receives a rainfall of 0.25 mm it tips and empties into a tankbelow, while the other bucket takes its position and the process is repeated. The tipping of thebucket actuates on electric circuit which causes a pen to move on a chart wrapped round adrum which revolves by a clock mechanism. This type cannot record snow.

Weighing type rain gauge. In this type of rain-gauge, when a certain weight of rain-fall is collected in a tank, which rests on a spring-lever balance, it makes a pen to move on achart wrapped round a clockdriven drum (Fig. 2.5). The rotation of the drum sets the timescale while the vertical motion of the pen records the cumulative precipitation.

Float type rain gauge. In this type, as the rain is collected in a float chamber, the floatmoves up which makes a pen to move on a chart wrapped round a clock driven drum (Fig. 2.6).When the float chamber fills up, the water siphons out automatically through a siphon tubekept in an interconnected siphon chamber. The clockwork revolves the drum once in 24 hours.The clock mechanism needs rewinding once in a week when the chart wrapped round thedrum is also replaced. This type of gauge is used by IMD.

203 cm203 cm

750 cm750 cm

Ring

Funnel

Base cover

Revolving drum(Clock-driven)Chart mountedPenClock mechanism

Float chamber

Float

Base

G.L.

SyphonSyphonchamber

Filter

Fig. 2.6 Float type rain gauge

The weighing and float type rain gauges can store a moderate snow fall which the op-erator can weigh or melt and record the equivalent depth of rain. The snow can be melted in

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PRECIPITATION 21

the gauge itself (as it gets collected there) by a heating system fitted to it or by placing in thegauge certain chemicals such as Calcium Chloride, ethylene glycol, etc.

2025303540

20151050

0 1 2 3 4 5 6 7 8Time (days)

Pen reversesdirection

Curve traced by pen ofself-recording rain gauge

Totalrainfall(cm)

Fig. 2.7 Mass curve of rainfall

China

Tibet

Pa

k

is

ta

n

25 cm

50 cm

75 cm

125 cm

190cm 190

cm1257550cm

25 cm50 cm

125 cm

125 cm115 cm

90 cm190 cm

190 cm

190cm

125 cm

125 cm

75cm

75cm75

cm

50 cm125

cm

190

250cm

300cm

50cm

50cm

75cm

75cm

125

cm

75cm

300cm

cm250

190125

Ar

ab

ia

ns

ea

Bay ofBengal

190 cm

250 cm 500 cm

375 cm

190cm

250

cm

Bangladesh

Burma

SriLanka

Indian ocean

Isohyetin cm(normal annual)

75cm

Fig. 2.8 Isohyetal map of India

Automatic-radio-reporting rain-gaugeThis type of raingauge is used in mountainous areas, which are not easily accessible to collectthe rainfall data manually. As in the tipping bucket gauge, when the buckets fill and tip, they

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22 HYDROLOGY

give electric pulses equal in number to the mm of rainfall collected which are coded into mes-sages and impressed on a transmitter during broadcast. At the receiving station, these codedsignals are picked up by UHF receiver. This type of raingauge was installed at the Koynahydro-electric project in June 1966 by IMD, Poona and is working satisfactorily.

2.3 RADARS

The application of radars in the study of storm mechanics, i.e. the areal extent, orientation andmovement of rain storms, is of great use. The radar signals reflected by the rain are helpful indetermining the magnitude of storm precipitation and its areal distribution. This method isusually used to supplement data obtained from a network of rain gauges. The IMD has a wellestablished radar network for the detection of thunder storms and six cyclone warning radars,on the east cost at Chennai, Kolkata, Paradeep, Vishakapatnam, Machalipatnam and Karaikal.See the picture given on facing page.

Location of rain-gauges—Rain-gauges must be so located as to avoid exposure to windeffect or interception by trees or buildings nearby.

The best location may be an open plane ground like an airport.The rainfall records are maintained by one or more of the following departments:

Indian Meteorological Department (IMD)Public Works Department (PWD)Agricultural DepartmentRevenue DepartmentForest Department, etc.

2.4 RAIN-GAUGE DENSITY

The following figures give a guideline as to the number of rain-gauges to be erected in agiven area or what is termed as ‘rain-gauge density’

Area Rain-gauge density

Plains 1 in 520 km2

Elevated regions 1 in 260-390 km2

Hilly and very heavy 1 in 130 Km2 preferably with 10% of the

rainfall areas rain-gauge stations equipped with the self

recording type

In India, on an average, there is 1 rain-gauge station for every 500 km2, while in moredeveloped countries, it is 1 stn. for 100 km2.

The length of record (i.e., the number of years) neeeded to obtain a stable frequencydistribution of rainfall may be recommended as follows:

Catchment layout: Islands Shore Plain Mountainousareas regions

No. of years: 30 40 40 50

The mean of yearly rainfall observed for a period of 35 consecutive years is called theaverage annual rainfall (a.a.r.) as used in India. The a.a.r. of a place depends upon: (i) distance

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(i) Station-year method—In this method, the records of two or more stations are com-bined into one long record provided station records are independent and the areas in which thestations are located are climatologically the same. The missing record at a station in a particu-lar year may be found by the ratio of averages or by graphical comparison. For example, in acertain year the total rainfall of station A is 75 cm and for the neighbouring station B, there isno record. But if the a.a.r. at A and B are 70 cm and 80 cm, respectively, the missing year’srainfall at B (say, PB) can be found by simple proportion as:

7570

= PB

80∴ PB = 85.7 cm

This result may again be checked with reference to another neighbouring station C.(ii) By simple proportion (normal ratio method)–This method is illustrated by the fol-

lowing example.Example 2.1 Rain-gauge station D was inoperative for part of a month during which a stormoccured. The storm rainfall recorded in the three surrounding stations A, B and C were 8.5, 6.7and 9.0 cm, respectively. If the a.a.r for the stations are 75, 84, 70 and 90 cm, respectively,estimate the storm rainfall at station D.Solution By equating the ratios of storm rainfall to the a.a.r. at each station, the storm rain-fall at station D (PD) is estimated as

8 575.

= 6 784

9 070 90

. .= = PD

� The average value of PD = 13

8 575

906 784

909 070

90. . .× + × + ×L

NMOQP = 9.65 cm

(iii) Double-mass analysis—The trend of the rainfall records at a station may slightlychange after some years due to a change in the environment (or exposure) of a station eitherdue to coming of a new building, fence, planting of trees or cutting of forest nearby, whichaffect the catch of the gauge due to change in the wind pattern or exposure. The consistency ofrecords at the station in question (say, X) is tested by a double mass curve by plottting thecumulative annual (or seasonal) rainfall at station X against the concurrent cumulative valuesof mean annual (or seasonal) rainfall for a group of surrounding stations, for the number ofyears of record (Fig. 2.9). From the plot, the year in which a change in regime (or environment)has occurred is indicated by the change in slope of the straight line plot. The rainfall recordsof the station x are adjusted by multiplying the recorded values of rainfall by the ratio of slopesof the straight lines before and after change in environment.Example 2.2 The annual rainfall at station X and the average annual rainfall at 18 surround-ing stations are given below. Check the consistency of the record at station X and determine theyear in which a change in regime has occurred. State how you are going to adjust the recordsfor the change in regime. Determine the a.a.r. for the period 1952-1970 for the changed regime.

Annual rainfall (cm)

Year Stn. X 18-stn. average

1952 30.5 22.8

1953 38.9 35.0

1954 43.7 30.2

1955 32.2 27.4

(contd.)...

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1956 27.4 25.2

1957 32.0 28.2

1958 49.3 36.1

1959 28.4 18.4

1960 24.6 25.1

1961 21.8 23.6

1962 28.2 33.3

1963 17.3 23.4

1964 22.3 36.0

1965 28.4 31.2

1966 24.1 23.1

1967 26.9 23.4

1968 20.6 23.1

1969 29.5 33.2

1970 28.4 26.4

Solution

Cumulative Annual rainfall (cm)

Year Stn. X 18-stn. average

1952 30.5 22.8

1953 69.4 57.8

1954 113.1 88.0

1955 145.3 115.4

1956 172.7 140.6

1957 204.7 168.8

1958 254.0 204.9

1959 282.4 233.3

1960 307.0 258.4

1961 328.8 282.0

1962 357.0 315.3

1963 374.3 338.7

1964 396.6 374.7

1965 425.0 405.9

1966 449.1 429.0

1967 476.0 452.4

1968 496.6 475.5

1969 526.1 508.7

1970 554.5 535.1

The above cumulative rainfalls are plotted as shown in Fig. 2.9. It can be seen from thefigure that there is a distinct change in slope in the year 1958, which indicates that a change inregime (exposure) has occurred in the year 1958. To make the records prior to 1958 comparable

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26 HYDROLOGY

with those after change in regime has occurred, the earlier records have to be adjusted bymultiplying by the ratio of slopes m2/m1 i.e., 0.9/1.25.

0 100 200 300 400 500 600

Cumulative annual rainfall-18 Stns. average, cm

Cum

ulat

ive

annu

alra

infa

llof

Stn

. X, c

m600

500

400

300

200

100

01952

1954

1956

1958

19601960

19621964

1966

1968

1970

2.5

2.5

1.8

1.8

22Change in regimeindicated in 1958

Adjustment of records

prior to1958 : 0.91.25

Slop

e=

=1.

25=

m 1

2.5

2

Slope

=

=0.

9=

m 2

1.8

2

Fig. 2.9 Double mass analysis Example 2.2

Cumulative rainfall 1958-1970= 554.5 – 204.7 = 349.8 cm

Cumulative rainfall 1952-1957adjusted for changed environment

= 204.7 × 0 9125

..

= 147.6 cm

Cumulative rainfall 1952-1970(for the current environment) = 497.4 cma.a.r. adjusted for the current regime

= 497.4 cm19 years

= 26.2 cm.

2.6 MEAN AREAL DEPTH OF PRECIPITATION (Pave)

Point rainfall—It is the rainfall at a single station. For small areas less than 50 km2, pointrainfall may be taken as the average depth over the area. In large areas, there will be a net-work of rain-gauge stations. As the rainfall over a large area is not uniform, the average depthof rainfall over the area is determined by one of the following three methods:

(i) Arithmetic average method—It is obtained by simply averaging arithmetically theamounts of rainfall at the individual rain-gauge stations in the area, i.e.,

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Pave = ΣPn

1 ...(2.1)

where Pave = average depth of rainfall over the areaΣP1 = sum of rainfall amounts at individual rain-gauge stations n = number of rain-gauge stations in the areaThis method is fast and simple and yields good estimates in flat country if the gauges

are uniformly distributed and the rainfall at different stations do not vary very widely fromthe mean. These limitations can be partially overcome if topographic influences and aerialrepresentativity are considered in the selection of gauge sites.

(ii) Thiessen polygon method—This method attempts to allow for non-uniform distribu-tion of gauges by providing a weighting factor for each gauge. The stations are plotted on abase map and are connected by straight lines. Perpendicular bisectors are drawn to the straightlines, joining adjacent stations to form polygons, known as Thiessen polygons (Fig. 2.10). Eachpolygon area is assumed to be influenced by the raingauge station inside it, i.e., if P1, P2, P3, ....are the rainfalls at the individual stations, and A1, A2, A3, .... are the areas of the polygonssurrounding these stations, (influence areas) respectively, the average depth of rainfall for theentire basin is given by

Pave = ΣΣA PA1 1

1...(2.2)

where ΣA1 = A = total area of the basin.The results obtained are usually more accurate than those obtained by simple arithme-

tic averaging. The gauges should be properly located over the catchment to get regular shapedpolygons. However, one of the serious limitations of the Thiessen method is its non-flexibilitysince a new Thiessen diagram has to be constructed every time if there is a change in theraingauge network.

(iii) The isohyetal method—In this method, the point rainfalls are plotted on a suitablebase map and the lines of equal rainfall (isohyets) are drawn giving consideration to orographiceffects and storm morphology, Fig. 2.11. The average rainfall between the succesive isohyetstaken as the average of the two isohyetal values are weighted with the area between theisohyets, added up and divided by the total area which gives the average depth of rainfall overthe entire basin, i.e.,

Pave = Σ

ΣA P

A1 2 1 2

1 2

− −

−...(2.3)

where A1–2 = area between the two successive isohyets P1 and P2

P1–2 = P P1 2

2+

ΣA1–2 = A = total area of the basin.This method if analysed properly gives the best results.

Example 2.3 Point rainfalls due to a storm at several rain-gauge stations in a basin areshown in Fig. 2.10. Determine the mean areal depth of rainfall over the basin by the threemethods.

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28 HYDROLOGY

Basin boundary

Thiessenpolygons

LG

D

H

K

M

NJ

I

E

F

C

A

O

B

Stn.

Fig. 2.10 Thiessen polygon method, Example 2.3

Solution (i) Arithmetic average method

Pave = ΣPn

1 =1331cm15 stn.

= 8.87 cm

ΣP1 = sum of the 15 station rainfalls.(ii) Thiessen polygon method—The Thiessen polygons are constructed as shown in

Fig. 2.10 and the polygonal areas are planimetered and the mean areal depth of rainfall isworked out below:

Station Rainfall Area of influen- Product (2) × (3) Mean arealrecorded, P1 tial polygon, A1 A1P1 depth of

(cm) (km2) (km2-cm) rainfall

1 2 3 4 5

A 8.8 570 5016

B 7.6 920 6992

C 10.8 720 7776

D 9.2 620 5704

E 13.8 520 7176

F 10.4 550 5720

G 8.5 400 3400

H 10.5 650 6825

I 11.2 500 5600

J 9.5 350 3325

K 7.8 520 4056L 5.2 250 1300M 5.6 350 1960

Pave = ΣΣA PA1 1

1

= 667147180

= 9.30 cm

(contd.)...

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N 6.8 100 680O 7.4 160 1184

Total 1331 cm 7180 km2 66714 km2-cm

n = 15 = ΣP1 = ΣA1 ΣA1P1

(iii) Isohyetal method—The isohyets are drawn as shown in Fig. 2.11 and the meanareal depth of rainfall is worked out below:

Zone Isohyets Mean isohyetal Area between Product Mean areal(cm) value, P1–2 isohyets, A1–2 (3) × (4) depth of

(cm) (km2) (km2-cm) rainfall(cm)

1 2 3 4 5 6

I <6 5.4 410 2214

II 6-8 7 900 6300

III 8-10 9 2850 25650

IV 10-12 11 1750 19250

V >12 12.8 720 9220

VI <8 7.5 550 4120

Total 7180 km2 66754 km2-cm= ΣA1–2 = ΣA1–2.P1–2

Example 2.3 (a) The area shown in Fig. P (2.3a) is composed of a square plus an equilateraltriangular plot of side 10 km. The annual precipitations at the rain-gauge stations located atthe four corners and centre of the square plot and apex of the traingular plot are indicated infigure. Find the mean precipitation over the area by Thiessen polygon method, and comparewith the arithmetic mean.Solution The Thiessen polygon is constructed by drawing perpendicular bisectors to the linesjoining the rain-gauge stations as shown in Fig. P (2.3a). The weighted mean precipitation iscomputed in the following table:

Area of square plot = 10 × 10 = 100 km2

Area of inner square plot = 10

2

10

2× = 50 km2

Difference = 50 km2

Area of each corner triangle in the square plot = 564 = 12.5 km2

13 area of the equilateral triangular plot = 1

3 ( 12 × 10 × 10 sin 60)

= 25

3 = 14.4 km2

Pave =

ΣΣ

A PA

1 2 1 2

1 2

− −

= 667547180

= 930 cm

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30 HYDROLOGY

VI

IIIIV

VIV

III

II

I

9.2 cm

8.8 cm 9.2 cmA D

C10.8 cm

12 cm12 cm

E

13.8 cm

H

10.5cm

11.2 cmI

9.5 cmJ

10cm

10cm

8cm

8cm

6cm

6cm6.8

N

M

5.6 cm5.6 cm

K7.8 cm

Basin boundary

10.4 cmF

10cm

10cm8

cm8

cm

7.6 cm

B

7.4 cmO

8.5 cm

GL

5.2 cm

Isohyetals

7.9 cm

P

F

Fig. 2.11 Isohyetal method, Example 2.3

10 km

60°10 km

D (80 cm)

F

(60 cm)

10 km

A (46 cm) 10 km B (65 cm)

45°

45°

Influence areas

10 km

E(70 cm)

C (76 cm)10 km

Fig. P(2.3a)

Station Area, A (km2) Precipitation A × P PaveP (cm) (km2-cm) (cm)

A (12.5 + 14.4) 46 1238

= 26.9

B 12.5 65 813

(contd.)...

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C 12.5 76 950 = Σ

ΣA PA.

D (12.5 + 14.4) 80 2152 = 9517143 2.

= 26.9 = 66.3 cmE 50 70 3500

F 14.4 60 864

n = 6 ΣA = 143.2 ΣP = 397 ΣA.P. = 9517

= 100 + 25 3as a check

Arithmetic mean = ΣPn

= 3976

= 66.17 cm

which compares fairly with the weighted mean.

2.7 OPTIMUM RAIN-GAUGE NETWORK DESIGN

The aim of the optimum rain-gauge network design is to obtain all quantitative data averagesand extremes that define the statistical distribution of the hydrometeorological elements, withsufficient accuracy for practical purposes. When the mean areal depth of rainfall is calculatedby the simple arithmetic average, the optimum number of rain-gauge stations to be estab-lished in a given basin is given by the equation (IS, 1968)

N = CpvF

HGIKJ

2

...(2.4)

where N = optimum number of raingauge stations to be established in the basinCv = Coefficient of variation of the rainfall of the existing rain gauge stations (say, n) p = desired degree of percentage error in the estimate of the average depth of rainfall

over the basin.The number of additional rain-gauge stations (N–n) should be distributed in the differ-

ent zones (caused by isohyets) in proportion to their areas, i.e., depending upon the spatialdistribution of the existing rain-gauge stations and the variability of the rainfall over thebasin.

Saturated Newtork DesignIf the project is very important, the rainfall has to be estimated with great accuracy; then anetwork of rain-gauge stations should be so set up that any addition of rain-gauge stations willnot appreciably alter the average depth of rainfall estimated. Such a network is referred to asa saturated network.Example 2.4 For the basin shown in Fig. 2.12, the normal annual rainfall depths recordedand the isohyetals are given. Determine the optimum number of rain-gauge stations to be estab-lished in the basin if it is desired to limit the error in the mean value of rainfall to 10%. Indicatehow you are going to distribute the additional rain-gauge stations required, if any. What is thepercentage accuracy of the existing network in the estimation of the average depth of rainfallover the basin ?

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32 HYDROLOGY

Solution

Station Normal annual Difference (Difference)2 Statistical parametersrainfall, x (cm) (x – x ) (x – x )2 x , σ, Cv

A 88 – 4.8 23.0 x = Σxn

= 4645

B 104 11.2 125.4 = 92.8 cm

C 138 45.2 2040.0 σ = Σ( )x x

n−−

2

1

D 78 – 14.8 219.0 = 3767 45 1

.− = 30.7

E 56 – 36.8 1360.0

n = 5 Σx = 464 Σ(x – x )2 = 3767.4 Cv = σx

= 30 792 8

.

. × 100

= 33.1%

VI

IIIIV

VIV

III

II

I

88 cmA

120 cm120 cm

C

138 cm

100cm

100cm

80cm

80cm

60cm

60cm

E

56 cm56 cm

D78 cm104 cm

B

100

cm10

0cm

80cm

80cm

Isohyetals

Basin boundary

Fig. 2.12 Isohyetal map, Example 2.4

Note: x = Arithmetic mean, σ = standard deviation.

The optimum number of rain-gauge stations to limit the error in the mean value ofrainfall to p = 10%.

N = CpvF

HGIKJ = F

HGIKJ

2 233 110

. = 11

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∴ Additional rain-gauge stations to be established = �N – n = 11 – 5 = 6The additional six raingauge stations have to be distributed in proportion to the areas

between the isohyetals as shown below:

Zone I II III IV V VI Total

Area (Km2) 410 900 2850 1750 720 550 7180

Area, as decimal 0.06 0.12 0.40 0.24 0.10 0.08 1.00

N × Area indecimal (N = 11) 0.66 1.32 4.4 2.64 1.1 0.88

Rounded as 1 1 4 3 1 1 11

Rain-gauges existing 1 1 1 1 1 – 5

Additional raingauges — — 3 2 — 1 6

These additional rain-gauges have to be spatially distributed between the differentisohyetals after considering the relative distances between rain-gauge stations, their accessi-bility, personnel required for making observations, discharge sites, etc.

The percentage error p in the estimation of average depth of rainfall in the existingnetwork,

p = C

Nv , putting N = n

P = 33 1

5

. = 14.8%

Or, the percentage accuracy = 85.2%

2.8 DEPTH-AREA-DURATION (DAD) CURVES

Rainfall rarely occurs uniformly over a large area; variations in intensity and total depth offall occur from the centres to the peripheries of storms. From Fig. 2.13 it can be seen that theaverage depth of rainfall decreases from the maximum as the area considered increases. Theaverage depths of rainfall are plotted against the areas up to the encompassing isohyets. Itmay be necessary in some cases to study alternative isohyetal maps to establish maximum 1-day, 2-day, 3 day (even up to 5-day) rainfall for various sizes of areas. If there are adequateself-recording stations, the incremental isohyetal maps can be prepared for the selected (orstandard) durations of storms, i.e., 6, 12, 18, 24, 30, 42, 48 hours etc.

Step-by-step procedure for drawing DAD curves:(i) Determine the day of greatest average rainfall, consecutive two days of greatest

average rainfall, and like that, up to consecutive five days.(ii) Plot a map of maximum 1-day rainfall and construct isohyets; similarly prepare

isohyetal maps for each of 2, 3, 4 and 5-day rainfall separately.(iii) The isohyetal map, say, for maximum 1-day rainfall, is divided into zones to repre-

sent the principal storm (rainfall) centres.

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34 HYDROLOGY

(iv) Starting with the storm centre in each zone, the area enclosed by each isohyet isplanimetered.

(v) The area between the two isohyets multiplied by the average of the two isohyetalvalues gives the incremental volume of rainfall.

(vi) The incremental volume added with the previous accumulated volume gives thetotal volume of rainfall.

(vii) The total volume of rainfall divided by the total area upto the encompassing isohyetgives the average depth of rainfall over that area.

(viii) The computations are made for each zone and the zonal values are then combinedfor areas enclosed by the common (or extending) isohyets.

(ix) The highest average depths for various areas are plotted and a smooth curve isdrawn. This is DAD curve for maximum 1-day rainfall.

(x) Similarly, DAD curves for other standard durations (of maximum 2, 3, 4 day etc. or6, 12, 18, 24 hours etc.) of rainfall are prepared.Example 2.5 An isohyetal pattern of critical consecutive 4-day storm is shown in Fig. 2.13.Prepare the DAD curve.

Rain-gauge stations

10 cm10 cm

15 cm15 cm

20 cm20 cm

25 cm25 cm

30cm

30cm

35cm

35cm

+B

Stormcentres

+A

505045454040

3535cmcm

30cm

30cm

25cm

25cm

20cm

20cm

15cm

15cm10

cm10

cm

Fig. 2.13 Isohyetal pattern of a 4-day storm, Example 2.5

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PRECIPITATION 35

Solution Computations to draw the DAD curves for a 4-day storm are made in Table 2.1.Table 2.1.Computation of DAD curve (4-day critical storm)

Storm Encom Area Isohyetal Average Area Incremen- Total Averagecentre passing enclosed range isohyetal between tal volume volume depth

isohyet (km2) (cm) value isohyets (cm.km2) (cm.km2) (8) ÷ (3)(cm) (1000) (cm) (km2) (1000) (1000) (cm)

(1000)

1 2 3 4 5 6 7 8 9

A 50 0.5 > 50 say, 55 0.5 27.5 27.5 5540 4 40–50 45 3.5 157.5 185.0 46.2535 7 35–40 37.5 3 112.5 297.5 42.530 29 30–35 32.5 22 715.0 1012.5 34.91

B 35 2 > 35 say, 37.5 2 75.0 75.0 37.530 9.5 30–35 32.5 7.5 244.0 319.0 33.6

A 25 82 25–30 27.5 43.5 1196.2 2527.8 30.8122 20–25 22.5 40 900 3427.8 28.1

15 156 15–20 17.5 34 595 4022.8 25.8236 10–15 12.5 80 1000 5022.8 21.3

Plot ‘col. (9) vs. col. (3)’ to get the DAD curve for the maximum 4-day critical storm, asshown in Fig. 2.14.

00

40 80 120 160 200 240 280

Area in (1000 km2)

Ave

rage

dept

hcm

10

20

30

40

50

60

4-day storm

Fig. 2.14 DAD-curve for 4-day storm, Example 2.5

Isohyetal patterns are drawn for the maximum 1-day, 2-day, 3-day and 4-day (consecu-tive) critical rainstorms that occurred during 13 to 16th July 1944 in the Narmada and Tapticatchments and the DAD curves are prepared as shown in Fig. 2.15. The characteristics ofheavy rainstorms that have occurred during the period 1930–68 in the Narmada and Taptibasins are given below:

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0 200 40 60 80 100Storm area (1000 km

2)

(a) Narmada basin

Ave

rage

dept

h(c

m)

50

40

30

50

20

10

0

3-day storm2-day storm

1-day storm

Storm area (1000 km2)

(b) Tapti basin

Ave

rage

dept

h(c

m)

0 20 40 60 100

60

50

40

30

20

10

0

3-day storm2-day storm1-day storm

Fig. 2.15 DAD-curves for Narmada & Tapti Basin for rainstorm of 4-6 August 1968

Year River basinMaximum depth of rainfall (cm)

1-day 2-day 3-day 4-day

13–16 Narmada 8.3 14.6 18.8 22.9July Tapti 6.3 9.9 11.2 15.21944

4–6 Narmada 7.6 14.5 17.4August Tapti 11.1 19.0 21.11968

8–9 Narmada 8.8 11.9September Tapti 4.7 7.51961

21–24 Narmada 4.1 7.4 10.4 12.9September Tapti 10.9 14.7 18.0 20.01945

17 Narmada 3.8

August Tapti 10.4

1944

2.9 GRAPHICAL REPRESENTATION OF RAINFALL

The variation of rainfall with respect to time may be shown graphically by (i) a hyetograph,and (ii) a mass curve.

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A hyetograph is a bar graph showing the intensity of rainfall with respect to time(Fig. 2.16) and is useful in determining the maximum intensities of rainfall during a particu-lar storm as is required in land drainage and design of culverts.

16

14

12

10

8

6

4

2

0

Inte

nsity

ofra

infa

lli (

cm/h

r)

00 30 60 90 120 150 180 210

Time t (min)

3.54.0

12.0 cm/hr

210-min. storm

8.5

4.5

3.0

Fig. 2.16 Hyetograph

A mass curve of rainfall (or precipitation) is a plot of cumulative depth of rainfall againsttime (Fig. 2.17). From the mass curve, the total depth of rainfall and intensity of rainfall at anyinstant of time can be found. The amount of rainfall for any increment of time is the differencebetween the ordinates at the beginning and end of the time increments, and the intensity ofrainfall at any time is the slope of the mass curve (i.e., i = ∆P/∆t) at that time. A mass curve ofrainfall is always a rising curve and may have some horizontal sections which indicates peri-ods of no rainfall. The mass curve for the design storm is generally obtained by maximising themass curves of the severe storms in the basin.

Cum

ulat

ive

rain

fall

P,cm

7

6

5

4

3

2

1

012 AM 4 8 12 PM 4 8 12 AM 4 8 12 PM

Time t, hr

Intensity, i =Ñ p

t

ÑÑtt

ÑpMass curve ofprecipitation

Ñ

Fig. 2.17 Mass curve of rainfall

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2.10 ANALYSIS OF RAINFALL DATA

Rainfall during a year or season (or a number of years) consists of several storms. The charac-teristics of a rainstorm are (i) intensity (cm/hr), (ii) duration (min, hr, or days), (iii) frequency(once in 5 years or once in 10, 20, 40, 60 or 100 years), and (iv) areal extent (i.e., area overwhich it is distributed).

Correlation of rainfall records—Suppose a number of years of rainfall records observedon recording and non-recording rain-gauges for a river basin are available; then it is possibleto correlate (i) the intensity and duration of storms, and (ii) the intensity, duration and fre-quency of storms.

If there are storms of different intensities and of various durations, then a relation maybe obtained by plotting the intensities (i, cm/hr) against durations (t, min, or hr) of the respec-tive storms either on the natural graph paper, or on a double log (log-log) paper, Fig. 2.18(a)and relations of the form given below may be obtained

(a) i = a

t b+ A.N. Talbot’s formula ...(2.5)

(for t = 5-120 min)

(b) i = k

tn ...(2.6)

(c) i = ktx ...(2.7)where t = duration of rainfall or its part, a, b, k, n and x are constants for a given region. Sincex is usually negative Eqs. (2.6) and (2.7) are same and are applicable for durations t > 2 hr. Bytaking logarithms on both sides of Eq. (2.7),

log i = log k + x log twhich is in the form of a straight line, i.e., if i and t are plotted on a log-log paper, the slope, ofthe straight line plot gives the constant x and the constant k can be determined as i = k whent = 1. Hence, the fitting equation for the rainfall data of the form of Eq. (2.7) can be determinedand similarly of the form of Eqs. (2.5) and (2.6).

On the other hand, if there are rainfall records for 30 to 40 years, the various stormsduring the period of record may be arranged in the descending order of their magnitude (ofmaximum depth or intensity). When arranged like this in the descending order, if there are atotal number of n items and the order number or rank of any particular storm (maximumdepth or intensity) is m, then the recurrence interval T (also known as the return period) of thestorm magnitude is given by one of the following equations:

(a) California method (1923), T = nm

....(2.8)

(b) Hazen’s method (1930), T = n

m − 12

...(2.9)

(c) Kimball’s method, (Weibull, 1939) T = n

m+ 1

...(2.10)

and the frequency F (expressed as per cent of time) of that storm magnitude (having recur-rence interval T) is given by

F = 1T

× 100% ...(2.11)

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PRECIPITATION 39

Natural paper

i = or i = ktxa

t + b

Time t (min or hr)

Inte

nsity

i(cm

/hr)

dydx

i = ktx

–x =dydx

Log-log paperi = k

Inte

nsity

i(cm

/hr)

Time t (min or hr)1

(a) Correlation of intensity and duration of storms

Inte

nsity

i(cm

/hr)

T = 15-yearT = 10-yearT = 5-yearT = 1-year

Naturalpaper

i =kT

t

x

e

Time t (min or hr) Time t (min or hr)

Inte

nsity

i(cm

/hr)

A : High intensity for short durationB : Low intensity for long duration

i = k

i1

Ñlog i Ñ

log t

A

x = log i

i2

1

i2

ÑÑlog ilog tlog ilog t

ÑÑ– e =– e =

One logcycle of T

One logcycle of T

Log-log paperLog-log paperi = kT

t

x

e

Dec

reas

ing

frequ

ency

T = 50-year

T = 20-yearT = 15-year

T = 15-yearT = 5-yearT = 5-yearT = 1-yearT = 1-year

B

(b) Correlation of intensity, duration and frequency of storms

1

Fig. 2.18 Correlation of storm characteristics

Values of precipitation plotted against the percentages of time give the ‘frquency curve’.All the three methods given above give very close results especially in the central part of thecurve and particularly if the number of items is large.

Recurrence interval is the average number of years during which a storm of given mag-nitude (maximum depth or intensity) may be expected to occur once, i.e., may be equalled orexceeded. Frequency F is the percentage of years during which a storm of given magnitudemay be equalled or exceeded. For example if a storm of a given magnitude is expected to occuronce in 20 years, then its recurrence interval T = 20 yr, and its frequency (probability ofexceedence) F = (1/20) 100 = 5%, i.e., frequency is the reciprocal (percent) of the recurrenceinterval.

The probability that a T-year strom and frequency FT

= ×FHG

IKJ

1100% may not occur in

any series of N years isP(N, 0) = (1 – F)N ...(2.12)

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40 HYDROLOGY

and that it may occur isPEx = 1 – (1 – F)N ...(2.12a)

where PEx = probability of occurrence of a T-year storm in N-years.The probability of a 20-year storm (i.e., T = 20, F = 5%) will not occur in the next 10 years

is (1 – 0.05)10 = 0.6 or 60% and the probability that the storm will occur (i.e., will be equalled orexceeded) in the next 10 years is 1 – 0.6 = 0.4 or 40% (percent chance).

See art. 8.5 (Encounter Probability), and Ex. 8.6 (a) and (b) (put storm depth instead offlood).

If the intensity-duration curves are plotted for various storms, for different recurrenceintervals, then a relation may be obtained of the form

i = kT

t

x

e ... Sherman ...(2.13)

where k, x and e are constants.‘i vs. t’ plotted on a natural graph paper for storms of different recurrence intervals

yields curves of the form shown in Fig. 2.18 (b), while on a log-log paper yields straight lineplots. By taking logarithms on both sides of Eq. (2.13),

log i = (log k + x log T) – e log twhich plots a straight line; k = i, when T and t are equal to 1. Writing for two values of T (forthe same t) :

log i1 = (log k + x log T1) – e log tlog i2 = (log k + x log T2) – e log t

Subtracting, log i1 – log i2 = x (log T1 – log T2)

or, x = ∆∆

loglog

iT

∴ x = charge in log i per log-cycle of T (for the same value of t)Again writing for two values of t (for the same T):

log i1 = (log k + x log T) – e log t1

log i2 = (log k + x log T) – e log t2

Subtracting log i1 – log i2 = – e(log t1 – log t2)

or –e = loglog

it

or e = – slope = ∆∆

loglog

it

∴ e = change in log i per log cycle of t (for the same value of T).The lines obtained for different frequencies (i.e., T values) may be taken as roughly

parallel for a particular basin though there may be variation in the slope ‘e’. Suppose, if a 1-year recurrence interval line is required, draw a line parallel to 10–year line, such that thedistance between them is the same as that between 5-year and 50-year line; similarly a 100-year line can be drawn parallel to the 10-year line keeping the same distance (i.e., distance perlog cycle of T). The value of i where the 1-year line intersects the unit time ordinate (i.e., t = 1min, say) gives the value of k. Thus all the constants of Eq. (2.13) can be determined from thelog-log plot of ‘i vs. t’ for different values of T, which requires a long record of rainfall data.Such a long record, will not usually be available for the specific design area and hence it

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becomes necessary to apply the intensity duration curves of some nearby rain gauge stationsand adjust for the local differences in climate due to difference in elevation, etc. Generally,high intensity precipitations can be expected only for short durations, and higher the intensityof storm, the lesser is its frequency.

The highest recorded intensities are of the order of 3.5 cm in a minute, 20 cm in 20 minand highest observed point annual rainfall of 26 m at Cherrapunji in Assam (India). It hasbeen observed that usually greater the intensity of rainfall, shorter the duration for which therainfall continues. For example, for upper Jhelum canals (India) maximum intensities are17.8 and 6.3 cm/hr for storms of 15 and 60 min respectively.Example 2.5 (a) In a Certain water shed, the rainfall mass curves were available for 30 (n)consecutive years. The most severe storms for each year were picked up and arranged in thedescending order (rank m). The mass curve for storms for three years are given below. Establish

a relation of the form i = kTt

x

e , by plotting on log-log graph paper.

Time(min) 5 10 15 30 60 90 120

Accumulated

depth (mm)

for m = 1 9 12 14 17 22 25 30

for m = 3 7 9 11 14 17 21 23

for m = 10 4 5 6 8 11 13 14

Solution

Time t (min) 5 10 15 30 60 90 120 T-yr = n

m+ 1

Intensity

i (mm/hr)

for m = 195

× 601210

× 60 56 34 22 16.6 1530 1

1+

~− 30 yr

= 108 = 72

for m = 375

× 60910

60× 44 28 14 14 11.530 1

3+ −~ 10 yr

= 84 = 54

for m = 1045

60× 510

60× 24 16 11 8.7 730 1

10+ −~ 3 yr

= 48 = 30

The intensity-duration curves (lines) are plotted on log-log paper (Fig. 2.18 (c)), whichyield straight lines nearby parallel. A straight line for T = 1 – yr is drawn parallel to the lineT = 10-yr at a distance equal to that between T = 30–yr and T = 3-yr. From the graph at T = 1-yr and t = 1 min, k = 103.

The slope of the lines, say for T = 30-yr is equal to the change in log i per log cycle of t,i.e., for t = 10 min and 100 min, slope = log 68 – log 17 = 1.8325 – 1.2304 = 0.6021 ~− 0.6 = e.

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400

200

100

80

50

30

20

10

8

654

1 10 1004

10

100

400

i = 103 T

t

0.34

0.6

Log-log paperLog-log paper

Log cycleof t

Log cycleof tÑ

log i = 0.6 = e

Log cycleof T, log i = 0.34 = x

T = 30 yr

6868

5555

3131

1717

T = 1 yr

Ñ

T = 3 yr

T & t= 1103 = K

T = 10 yr

t (min)

i(m

m/h

r)

Fig. 2.18. (c) Intensity-duration relationship, (Ex. 2.5 (a))

At t = 10 min, the change in log i per log cycle of T, i.e., between T = 3–yr and 30–yr lines(on the same vertical), log 68 – log 31 = 1.8325 – 1.4914 = 0.3411 ~− 0.34 = x.

Hence, the intensity-duration relationship for the watershed can be established as

i = 104 0.34

0.6T

tFor illustration, for the most severe storm (m = 1, T = 30–yr), at t = 60 min, i.e., after 1

hr of commencement of storm,

i = 103 30

60

0.34

0.6

( )

( ) = 28 mm/hr

which is very near to the observed value of 22 mm/hr.A more general Intensity-Duration–Frequency (IDF) relationship is of the form

Sherman i = KT

t a

x

n( )+ , i in cm/hr, t in min, T yr.

where K, x, a and n are constants for a given catchment. The rainfall records for about 30 to 50years of different intensities and durations on a basin can be analysed with their computedrecurrence interval (T). They can be plotted giving trial values of ‘a’ for the lines of best fit as

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shown in Fig. 2.18 (b). The values of a and n may be different for different lines of recurrenceinterval.

The constants can also be obtained by multiple regression model based on the principleof least squares and solutions can be obtained by computer-based numerical analysis; confi-dence intervals for the predictions can be developed.

Extreme point rainfall values of different durations and recurrence interval (returnperiod) have been evaluated by IMD and the ‘isopluvial maps’ (lines connecting equal depthsof rainfall) for the country prepared.Example 2.5 (b) A small water shed consists of 2 km2 of forest area (c = 0.1), 1.2 km2 of culti-vated area (c = 0.2) and 1 km2 under grass cover (c = 0.35). A water course falls by 20 m in alength of 2 km. The IDF relation for the area may be taken as

i = 80

12

0.2

0.5

Tt( )+

, i in cm/hr, t in min and T yr

Estimate the peak rate of runoff for a 25 yr frequency.Solution Time of concentration (in hr)

tc = 0.06628 L0.77 S–0.385, Kirpich’s formula, L in km

= 0.06628 × 20.77 20

2 1000

0.385

×FHG

IKJ

= 0.667 hr × 60 = 40 min.

i = ic when t = tc in the given IDF relation

∴ ic = 80 2540 12

0.2

0.5

×+( )

= 21.1 cm/hr

Qpeak = 2.78 C ic A, rational formula, CA = ΣCiAi

= 2.78 × 21.1 × (0.1 × 2 + 0.2 × 1.2 + 0.35 × 1) = 46.4 cumec

2.11 MEAN AND MEDIAN

The sum of all the items in a set divided by the number of items gives the mean value,i.e.,

x = Σxn

...(2.10)

where x = the mean valueΣx = sum of all the items n = total number of items.The magnitude of the item in a set such that half of the total number of items are larger

and half are smaller is called the median. The apparent median for the curve in Fig. 2.21 is theordinate corresponding to 50% of the years. The mean may be unduly influenced by a few largeor small values, which are not truly representative of the samples (items), whereas the medianis influenced mainly by the magnitude of the main part of intermediate values.

To find the median, the items are arranged in the ascending order; if the number ofitems is odd, the middle item gives the median; if the number of items is even, the average ofthe central two items gives the median.

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Example 2.6 The annual rainfall at a place for a period of 10 years from 1961 to 1970 arerespectively 30.3, 41.0, 33.5, 34.0, 33.3, 36.2, 33.6, 30.2, 35.5, 36.3. Determine the mean andmedian values of annual rainfall for the place.

Solution (i) Mean x = Σxn

= (30.3 + 41.0 + 33.5 + 34.0 + 33.3 + 36.2

+ 33.6 + 30.2 + 35.5 + 36.3)/10

= 343 9

10.

= 34.39 cm

(ii) Median: Arrange the samples in the ascending order 30.2, 30.3 33.3, 33.5, 33.6, 34.0,35.5, 36.2, 36.3, 41.0

No. of items = 10, i.e., even

∴ Median = 33 6 34 0

2. .+

= 33.8 cm

Note the difference between the mean and the median values. If 11 years of record, say1960 to 1970, had been given, the median would have been the sixth item (central value) whenarranged in the ascending order.

Example 2.7 The following are the rain gauge observations during a storm. Construct: (a)mass curve of precipitation, (b) hyetograph, (c) maximum intensity-duration curve and developa formula, and (d) maximum depth-duration curve.

Time since commencement Accumulatedof storm rainfall

(min) (cm)

5 0.1

10 0.2

15 0.8

20 1.5

25 1.8

30 2.0

35 2.5

40 2.7

45 2.9

50 3.1

Solution (a) Mass curve of precipitation. The plot of ‘accumulated rainfall (cm) vs. time(min)’ gives the ‘mass curve of rainfall’ Fig. 2.19 (a).

(b) Hyetograph. The intensity of rainfall at successive 5 min interval is calculated and abar-graph of ‘i (cm/hr) vs. t (min)’ is constructed; this depicts the variation of the intensity ofrainfall with respect to time and is called the ‘hyetograph; 2.19 (b).

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PRECIPITATION 45

Time, t Accumulated ∆ P in time Intensity,(min) rainfall ∆t = 5 min

i = ∆∆Pt

× 60

(cm) (cm) (cm/hr)

5 0.1 0.1 1.2

10 0.2 0.1 1.2

15 0.8 0.6 7.2

20 1.5 0.7 8.4

25 1.8 0.3 3.6

30 2.0 0.2 2.4

35 2.5 0.5 6.0

40 2.7 0.2 2.4

45 2.9 0.2 2.4

50 3.1 0.2 2.4

3.5

3.0

2.5

2.0

1.5

1.0

0.5

0

Tota

lrai

nfal

ldep

th(c

m)

mass curve traced byself-recording rain gauge

50-min storm

0 5 10 15 20 25 30 35 40 45 50 55 60

Time t (min)

Ñ pt

Ñi =

Ñt

Ñp

(a) Mass curve of precipitation

1.2 cm/hr

8.4 cm/hr

2.4 cm/hr

7.2

3.6

2.4

6.0

50-min storm

Area under the curvegives total precipitation (cm)

Inte

nsity

i(cm

/hr)

10

8

6

4

2

00 5 10 15 20 25 30 35 40 450 50

Time t (min)

(b) Hyetograph

Fig. 2.19 Graphs from recording rain-gauge data, Example 2.7

(c) Maximum depth–duration curve. By inspection of time (t) and accumulated rainfall(cm) the maximum rainfall depths during 5, 10, 15, 20, 25, 30, 35, 40, 45 and 50 min durations

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46 HYDROLOGY

are 0.7, 1.3, 1.6, 1.8, 2.3, 2.5, 2.7, 2.9, 3.0 and 3.1 cm respectively. The plot of the maximumrainfall depths against different durations on a log-log paper gives the maximum depth-dura-tion curve, which is a straight line, Fig. 2.20 (a).

i = 17

t0.375

b. Maximum intensity-duration curveb. Maximum intensity-duration curve

a. Maximum depth-duration curvea. Maximum depth-duration curve

k = 17

x = – 0.3750.75cm

Log-log paper

100

80

60

40

30

20

15

10

8

65

4

3

2

1.5

1

Inte

nsity

i(cm

/hr)

1 1.5 2 3 4 5 6 8 10 15 20 30 40 60 80 100

10

8

6

4

3

2

1.5

1

0.8

0.6

0.4

0.3

0.2

0.15

2.0 cm2.0 cm

0.1

Max

imum

dept

h(c

m)

Time t (min)

Slope

Fig. 2.20 Maximum depth-duration & intensity-duration curves (Example 2.7)

(d) Maximum intensity-duration curve. Corresponding to the maximum depths obtained

in (c) above, the corresponding maximum intensities can be obtained ∆∆Pt

× 60, i.e., 8.4, 7.8, 6.4,

5.4, 5.52, 5.0, 4.63, 4.35, 4.0 and 3.72 cm/hr, respectively. The plot of the maximum intensitiesagainst the different duration on a log-log paper gives the maximum intensity-duration curvewhich is a straight line, Fig. 2.20 (b).

The equation for the maximum itensity duration curve is of the form i = ktx

Slope of the straight line plot,

– x = dydx

= 0.75 cm2.00 cm = 0.375

k = 17 cm/hr when t = 1 minHence, the formula becomes

i = 170.375t

which can now be verified ast = 10 min, i = 7.2 cm/hrt = 40 min, i = 4.25 cm/hr

which agree with the observed data