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Proceedings of ERAD (2002): 295–298 c Copernicus GmbH 2002 ERAD 2002 The measured kinetic energy of hailstone by radar and hailpads N. Pavlovic Berdon and M. Miladinovic Republic Hydrometeorological Institute of Serbia, Kneza Viseslava 66, 11 000 Belgrade, Republic Yugoslavia Abstract. In this paper we compared hailstone kinetic en- ergy measured by hailpads and weather radar over seeded and unseeded territory. Isocontures of radars reflectivity measured in db (each step of 10 db ) transformed in dbz, vere used. Horizontal cross – section of the cloud was measured at the level of 0 C isoterm, over two hailpads networks for the purpose of comparison. The agreement of kinetic energy of hailstone measured by radar and hailpads is 92% in aver- age for selected data. 1 Introduction A hailpad network has been working in the two province Bosna and Pocerina during the period 15 May – 15 August 1985. One network consists of 49 hailpads distributed homo- geneously in an area of 500 km 2 . The detailed description of the network, the calibration and the analyses of the pads, as well as some of the results obtained have already been pub- lished (Pavlovic Berdon, 1999). The protected area refers to the Pocerina territory, and un protected area is the terri- tory of Bosna. The hailstorms over our territory frequently come from west and northwest direction, and because of that, the hailpad network on the unprotected territory is located in front of the protected area. The other reason is to protect this area against agent contamination. These two areas were hail- pads are located, are climatologically similar and relatively near in order to compare the relative data. The experiment with hailpads network on two different ar- eas was established to verify to hail suppression efficiency. 2 Instruments and methods The experiment with hailpads was to identify the differences in hail kinetic energy and hailstone spectra on protected and Correspondence to: N. Pavlovic Berdon ([email protected]) 45 0 20’ N 43 0 52’ N 20 0 56’ E 19 0 16’ E Fig. 1. The location of radars. non-protected areas being the estimation of the hail suppres- sion effects. In this paper S-band radar and hailpad data are compared over the both territory. Republic Hydrometeorogical Service of Serbia started its hail suppression activity in Serbia from 1967. year. During 1985. the hail suppression system covered 96% ( 37 610 km 2 of the agricultural area in Serbia (except the north part called Vojvodina). There was a network of 13 hail suppression cen- ters equipped with MITSUBISHI RC-34A weather radars. There were 1415 launching stations on the protected area, from which hail suppression rockets were launched, depend- ing on radar and aerological criteria. We used hail suppres- sion rockets with vertical range of 8 km, and 5 km, which carried 20% AgI seeding material having the efficiency of 10 12 –10 13 of active particles, per gram of Silver Iodide, and the quantity of 400 g of agent. The hailpads consist of a foam rubber plate. The dimen- sions of the pads are 0.20 m × 0.20 m × 0.02 m. The hail-

Proceedings of ERAD (2002): 295–298 ERAD 2002Fig. 5. POCERINA, Kinetic energy (J/m2) measured by the hail-pads on 17 July 1985. hailpad data were analyzed later on, and compared

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Page 1: Proceedings of ERAD (2002): 295–298 ERAD 2002Fig. 5. POCERINA, Kinetic energy (J/m2) measured by the hail-pads on 17 July 1985. hailpad data were analyzed later on, and compared

Proceedings of ERAD (2002): 295–298c© Copernicus GmbH 2002 ERAD 2002

The measured kinetic energy of hailstone by radar and hailpads

N. Pavlovic Berdon and M. Miladinovic

Republic Hydrometeorological Institute of Serbia, Kneza Viseslava 66, 11 000 Belgrade, Republic Yugoslavia

Abstract. In this paper we compared hailstone kinetic en-ergy measured by hailpads and weather radar over seededand unseeded territory. Isocontures of radars reflectivitymeasured in db (each step of 10 db ) transformed in dbz, vereused. Horizontal cross – section of the cloud was measuredat the level of 0◦ C isoterm, over two hailpads networks forthe purpose of comparison. The agreement of kinetic energyof hailstone measured by radar and hailpads is 92% in aver-age for selected data.

1 Introduction

A hailpad network has been working in the two provinceBosna and Pocerina during the period 15 May – 15 August1985. One network consists of 49 hailpads distributed homo-geneously in an area of 500 km2. The detailed description ofthe network, the calibration and the analyses of the pads, aswell as some of the results obtained have already been pub-lished (Pavlovic Berdon, 1999). The protected area refersto the Pocerina territory, and un protected area is the terri-tory of Bosna. The hailstorms over our territory frequentlycome from west and northwest direction, and because of that,the hailpad network on the unprotected territory is located infront of the protected area. The other reason is to protect thisarea against agent contamination. These two areas were hail-pads are located, are climatologically similar and relativelynear in order to compare the relative data.

The experiment with hailpads network on two different ar-eas was established to verify to hail suppression efficiency.

2 Instruments and methods

The experiment with hailpads was to identify the differencesin hail kinetic energy and hailstone spectra on protected and

Correspondence to:N. Pavlovic Berdon([email protected])

6

APPENDIX A

Fig. 1. The location of radars

Fig. 2. BOSNA, Kinetic energy ( J/m2) measured by the hailpads 08.06.1985.

45020’ N

51

52

53

54

55

56

57

58

59

60

61

62

63

64

6566

67 68

69

70

71

72

73

75

76

77

78

7980

81

82

83

84

85

86

87

8889

90

91

92

9394

95

96

97

98

9944030’ N

19016’ E

43052’ N

20056’ E19016’ E

44030’ N

18056’ E

44057’ N

Fig. 1. The location of radars.

non-protected areas being the estimation of the hail suppres-sion effects. In this paper S-band radar and hailpad data arecompared over the both territory.

Republic Hydrometeorogical Service of Serbia started itshail suppression activity in Serbia from 1967. year. During1985. the hail suppression system covered 96% ( 37 610 km2

of the agricultural area in Serbia (except the north part calledVojvodina). There was a network of 13 hail suppression cen-ters equipped with MITSUBISHI RC-34A weather radars.There were 1415 launching stations on the protected area,from which hail suppression rockets were launched, depend-ing on radar and aerological criteria. We used hail suppres-sion rockets with vertical range of 8 km, and 5 km, whichcarried 20% AgI seeding material having the efficiency of1012–1013 of active particles, per gram of Silver Iodide, andthe quantity of 400 g of agent.

The hailpads consist of a foam rubber plate. The dimen-sions of the pads are 0.20 m× 0.20 m× 0.02 m. The hail-

Page 2: Proceedings of ERAD (2002): 295–298 ERAD 2002Fig. 5. POCERINA, Kinetic energy (J/m2) measured by the hail-pads on 17 July 1985. hailpad data were analyzed later on, and compared

296 N. Pavlovic Berdon and M. Miladinovic: The measured kinetic energy of hailstone by radar and hailpads

6

APPENDIX A

Fig. 1. The location of radars

Fig. 2. BOSNA, Kinetic energy ( J/m2) measured by the hailpads 08.06.1985.

45020’ N

51

52

53

54

55

56

57

58

59

60

61

62

63

64

6566

67 68

69

70

71

72

73

75

76

77

78

7980

81

82

83

84

85

86

87

8889

90

91

92

9394

95

96

97

98

9944030’ N

19016’ E

43052’ N

20056’ E19016’ E

44030’ N

18056’ E

44057’ N

Fig. 2. BOSNA, Kinetic energy (J/m2) measured by the hailpads on8 June 1985.

7

Fig. 3. BOSNA, Kinetic energy (J/m2) measured by the hailpads 23.06.1985.

Fig. 4. BOSNA, Kinetic energy(J/m2) measured by the hailpads 17.07.1985.

51

52

53

54

55

56

57

58

59

60

61

62

63

64

6566

67 68

69

70

71

72

73

75

76

77

78

7980

81

82

83

84

85

86

87

8889

90

91

92

9394

95

96

97

98

99

51

52

53

54

55

56

57

58

59

60

61

62

63

64

6566

67 68

69

70

71

72

73

75

76

77

78

7980

81

82

83

84

85

86

87

8889

90

91

92

9394

95

96

97

98

99

44057’N

19016’E

44030’N

18056’E

44057’N

19016’E

18056’E

44030’N

Fig. 3. BOSNA, Kinetic energy (J/m2) measured by the hailpads on23 June 1985.

pads are installed on a pole 1m above the ground. The kineticenergy E (J/m2) measured by a hailpad is obtained from thenumber of hailstonesni (m−2) in the diameter intervals∆Di

with mean diameterDi (mm) according to

E = 4, 58× 10−6

p∑i=1

niD4i

where indexp denotes the number of diameter intervals used.The global kinetic energy Eg of a hailfell is defined as thesum of all the kinetic energies measured by hailpads hit byone hailfell. In hailpad network at each point, besides thehailpads, there were rain gauges and observers in order torecord rainfall and hailstones on the ground, as well the timeof occurence of these events quantities and intensities. The

7

Fig. 3. BOSNA, Kinetic energy (J/m2) measured by the hailpads 23.06.1985.

Fig. 4. BOSNA, Kinetic energy(J/m2) measured by the hailpads 17.07.1985.

51

52

53

54

55

56

57

58

59

60

61

62

63

64

6566

67 68

69

70

71

72

73

75

76

77

78

7980

81

82

83

84

85

86

87

8889

90

91

92

9394

95

96

97

98

99

51

52

53

54

55

56

57

58

59

60

61

62

63

64

6566

67 68

69

70

71

72

73

75

76

77

78

7980

81

82

83

84

85

86

87

8889

90

91

92

9394

95

96

97

98

99

44057’N

19016’E

44030’N

18056’E

44057’N

19016’E

18056’E

44030’N

Fig. 4. BOSNA, Kinetic energy (J/m2) measured by the hailpads on17 July 1985.

8

Fig. 5. POCERINA, Kinetic energy (J/m2)measured by the hailpads 17.07.1985.

Fig. 6. BOSNA, Radars reflectivity in db 08.06.1985.

44029’N

44046’ N

19029’ E

19049 E

1

2

3

4

5

6

7

89

10

11

12

13

1415

16

17

18

19

20

21

22

23

24

25

26

27

28

29

30

31

32

33

34

35

36

37

38

39

40

41

43

44

45

46

47

48

42

49

44057’N 19016’E

18056’E

44030’N

Fig. 5. POCERINA, Kinetic energy (J/m2) measured by the hail-pads on 17 July 1985.

hailpad data were analyzed later on, and compared with radardata.

In this project we have weather radar MITSUBISHI RC-34A production in solid state tehnology S-band. It is usedfor the detection hail clouds. It is equipped with PPI,RHIand A/R displays indicating angular and vertical cut and thetarget distance for the amplitude of reflcted signals. It hasseveral types of light markers and operational ranges. Thebeam width is 2 degrades, output power 400 kW, anntenarotation speed is 6 revolutions per minute, ranges are 25, 50,100 and 250 km and the azimuth, elevation and range readoutis digital.

In this project we used 3 radars lounted at the Vljevo,

Page 3: Proceedings of ERAD (2002): 295–298 ERAD 2002Fig. 5. POCERINA, Kinetic energy (J/m2) measured by the hail-pads on 17 July 1985. hailpad data were analyzed later on, and compared

N. Pavlovic Berdon and M. Miladinovic: The measured kinetic energy of hailstone by radar and hailpads 297

8

Fig. 5. POCERINA, Kinetic energy (J/m2)measured by the hailpads 17.07.1985.

Fig. 6. BOSNA, Radars reflectivity in db 08.06.1985.

44029’N

44046’ N

19029’ E

19049 E

1

2

3

4

5

6

7

89

10

11

12

13

1415

16

17

18

19

20

21

22

23

24

25

26

27

28

29

30

31

32

33

34

35

36

37

38

39

40

41

43

44

45

46

47

48

42

49

44057’N 19016’E

18056’E

44030’N

Fig. 6. BOSNA, Radars reflectivity in db on 8 June 1985.

Fig. 7. BOSNA, Radars reflectivity in db on 23 June 1985.

Bukulja and Uzice and the largest distances between theradar and a pad was less than 40 km (Fig. 1).

Radar charts were made mannually and cloud crosssectins were given at the level of 0◦ C isotherm hight.

The Ze value of the corresponding PPI element was dis-plaed in digital form end manualy drawing togedther withthe stopped isoecho contours on the PPI screen on times per3 min. The radar reflectivity values are transformed into ki-netic energies by means of empirical Z-E realations optainedfrom measured time-resolved hailstone spectra (Table 1).

9

Fig. 7. BOSNA, Radars reflectivity in db 23.06.1985.

Fig. 8. BOSNA, Radars reflectivity in db 17. 07.1985.

44057’N

19016’E

18056’E

44030’N

44057’N

19016’E

18056’E

44030’N

Fig. 8. BOSNA, Radars reflectivity in db on 17 July 1985.

10

Fig. 9. POCERINA, Radars reflectivity in db 17. 07.1985.

440 46’N

190 29’E

440 29N 190 49 E

Fig. 9. POCERINA, Radars reflectivity in db on 17 July 1985.

3 Results

The analyses performed in this paper is the first attempt todeal with kinetic energy of hail measured by radar in ourcountry. The data of four severe hailstorms (8 June, 23 Juneand 17 July 1985) are studied and the following results areobtained: the agreement of data in space, time and the valuesof kinetic energy of halifells. The agreement in space andtime we can see from the Figs. 2 to 9. The Figs. 2 to 5 showkinetic energy calculated by hailpads. On Figs. 6 to 9 weshow the radar reflectivity in db for the same data.

Page 4: Proceedings of ERAD (2002): 295–298 ERAD 2002Fig. 5. POCERINA, Kinetic energy (J/m2) measured by the hail-pads on 17 July 1985. hailpad data were analyzed later on, and compared

298 N. Pavlovic Berdon and M. Miladinovic: The measured kinetic energy of hailstone by radar and hailpads

Table 1. Comparison of hailpad and radar data

BOSNA

data km2 t (min) Eg (106jM−2) >dbz Ec (106Jm−2) Eg/Ec(%)

08 June 1985 4.52 5 2,432.79 45 2,768.25 88%23 June 1985 1.39 3 604.62 55 602.85 100%17 July 1985 3.77 4 2,078.28 55 2,184.34 95%

POCERINA

17 July 1985 11.10 2 1,904.67 55 1,607.61 84%

4 Conclusion

In Table 1 we can see the values of kinetic energy calculatedby radars measurements and by hailpads data which show theagreements of data in 92%.

We are sure that if we analyzed the more number of datait will be possible find to the boundary between rain and hailmeasured by radar reflectivity. This is significant as a crite-rion for successful treatment of hail of clouds. Determinationof kinetic energy of hilstone is also important in objective an-alyzes of plant damage degree.

References

Federer B., Waldvogel A., Schmid, W., Hampel F., SchweingruberStahel, W., Mezeix, J.F., Doras, N., and Vento D.: First rezult ofGrossversuch IV, 755–762, 1981.

Waldvogel, A., Schmid, W., and Federer, B., The kinetic energy ofhailfalls. Part I: Hailstone Spectra, J. Appl. Meteor., 17, 515–520,1978.

Waldvogel, A., Federer, B., Schmid, W., and Mezeix, J.F.: The ki-netic energy of hailfalls. Part II: radar and hailpads, J. Appl. Me-teor., 17, 1680–1693, 1978.

Pavlovic Berdon, N.: The kinetic energy of hailfalls measured byhailpads, 1999.