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Table 1:

Properties of the observed H I halo clouds.
  $\upsilon _{\rm lsr}$ R z $N_{\rm HI}$ s D $ \Delta \upsilon_{1/2}$ $T_{\rm kin}$ $\langle n \rangle$ P $M_{H {\sc i}}$
  km s-1 kpc kpc 1018 cm-2 arcmin pc km s-1 K ${\rm cm^{-3}}$ K $~{\rm cm^{-3}}$ $M_{\odot}$
113.3+27.0 -40 10.5 1.8 16(2) 13 16(7) 7.0 1080(150) 0.33(0.15) 360(170) 25(22)
113.2+25.5 -32 10.0 1.4 6(1) 9 8(5) 4.0 350(90) 0.23(0.14) 80(50) 3(4)
116.2+23.6 -68 12.5 2.8 11(2) 25 51(17) 3.0 200(70) 0.07(0.03) 14(8) 120(80)
116.7+22.8 -81 14.5 3.5 25(3) 27 70(19) 5.1 570(110) 0.12(0.04) 68(26) 770(440)
116.5+21.4 -42 10.5 1.5 36(4) 13 14(6) 5.4 650(120) 0.70(0.30) 455(210) 45(39)
115.0+23.9 -84 14.5 3.9 15(3) 22 60(20) 3.3 240(70) 0.08(0.03) 19(7) 220(140)
115.4+22.4 -66 12.0 2.5 35(3) 18 34(12) 10.0 2200(220) 0.33(0.12) 730(275) 260(180)
117.3+24.0 -71 13.0 3.0 36(3) 27 58(18) 8.1 1440(170) 0.20(0.06) 290(90) 770(490)
118.0+24.6 -71 13.0 3.1 20(3) 18 40(15) 5.0 550(110) 0.16(0.07) 87(40) 200(150)
118.0+24.0 -72 13.0 3.0 74(4) 18 40(15) 21.1 9800(460) 0.60(0.22) 5800(2140) 750(550)
117.5+25.2 -74 13.0 3.0 60(4) 18 40(15) 11.6 2960(260) 0.48(0.18) 1449(550) 600(440)
114.5-15.9 -38 10.5 -1.0 10(2) 18 18(7) 4 350(90) 0.18(0.08) 62(31) 20(16)
113.6-12.4 -85 4.5 -1.9 16(2) 13 35(14) 4 350(90) 0.14(0.06) 50(25) 120(100)
113.0-12.4 -55 12.0 -1.2 41(3) 18 28(9) 6.7 990(150) 0.49(0.16) 470(170) 205(130)
113.0-13.0 -40 10.5 -0.9 28(3) 9 9(5) 4.4 425(100) 1.02(0.32) 435(170) 14(16)
113.3-14.1 -57 12.0 -1.3 39(4)     4.9 510(100)      
113.6-13.5 -50 11.5 -1.3 68(5)     7.0 1080(150)      
114.3+21.8 -75 13.5 3.0 7(-) 9 21(12)          
128.8-18.5 -58 14.0 -1.9 54(6)     4.8 510(100)      
131.0-19.2 -72 15.0 -2.8 49(5)     5.4 640(120)      
130.6-19.5 -68 14.0 -2.5 35(3)     6.0 780(130)      
112.1+27.3 -39 10.5 1.8 6(1) 9 10(6) 5.3 620(120) 0.20(0.12) 126(80) 4(5)
113.8+28.7 -69 12.5 3.6 9(2) 18 39(14) 6.0 790(130) 0.08(0.03) 61(25) 90(70)
112.4+29.9 -65 12.5 3.7 4(1) 9 20(11) 2.0 80(40) 0.07(0.04) 6(5) 11(13)
114.7+29.6 -89 15.0 5.4 19(3)     3.6 285(80)      

Notes.  $\upsilon _{\rm lsr}$  is the line of sight velocity in km s-1, R  is the Galactocentric distance. z is the height above mid-plane. $N_{\rm HI}$ is the H I column density. s is the measured angular diameter. D is the spatial diameter. $ \Delta \upsilon_{1/2}$ is the full width half maximum of the line width. $T_{\rm kin}$ the kinetic temperature. $\langle n \rangle$  the volume H I density. P is the pressure of the H I gas. $M_{H {\sc i}}$ the visible H I mass of the cloud.


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