SDO HMI 2014-05-18 07:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.03 | 272.77 | 31.10 | 213.87 | -13.52 | 229.30 | 50.12 | 254.20 | 0.7769 | 240.3 | 238.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.27 | 0.00 | 0.31 | -12.52 | 243.15 | 63.97 | 257.20 | 0.9014 | 254.0 | 256.0 | |
| 0.00 | 0.99 | 0.00 | 0.88 | -7.33 | 235.34 | 56.16 | 262.72 | 0.8326 | 351.0 | 290.0 | |
| 0.00 | 1.44 | 0.00 | 1.31 | -13.66 | 235.87 | 56.69 | 255.20 | 0.8420 | 342.0 | 396.1 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -14.64 | 235.62 | 56.43 | 254.01 | 0.8407 | 465.0 | 417.0 | |
| 0.00 | 0.63 | 0.00 | 0.57 | -15.33 | 235.55 | 56.37 | 253.19 | 0.8410 | 477.0 | 410.9 | |
| 23.47 | 235.33 | 18.76 | 187.08 | -12.96 | 230.37 | 51.18 | 255.28 | 0.7873 | 924.5 | 337.2 | |
| 15.56 | -6.00 | 12.34 | -6.00 | -13.47 | 229.87 | 50.69 | 254.55 | 0.7829 | 885.8 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.75 | -11.29 | 228.19 | 49.01 | 257.08 | 0.7617 | -308.0 | -254.5 | |
| 0.00 | 1.80 | 0.00 | 1.36 | -11.24 | 228.04 | 48.85 | 257.13 | 0.7599 | -446.0 | -333.9 | |
| 0.00 | 1.17 | 0.00 | 0.89 | -11.49 | 227.90 | 48.72 | 256.78 | 0.7588 | -450.0 | -426.7 | |
| 0.00 | 0.63 | 0.00 | 0.47 | -10.79 | 227.61 | 48.42 | 257.66 | 0.7545 | -570.0 | -453.1 | |
| 0.00 | 1.53 | 0.00 | 1.15 | -11.46 | 227.66 | 48.48 | 256.77 | 0.7561 | -669.0 | -556.0 | |
| 0.00 | 1.35 | 0.00 | 1.01 | -11.65 | 227.52 | 48.34 | 256.50 | 0.7547 | -500.0 | -419.7 | |
| 0.00 | 1.53 | 0.00 | 1.13 | -12.38 | 226.72 | 47.53 | 255.39 | 0.7468 | -572.0 | -381.4 | |
| 0.00 | 0.63 | 0.00 | 0.47 | -15.17 | 226.21 | 47.02 | 251.60 | 0.7465 | -370.0 | -365.0 | |
| 0.00 | 1.44 | 0.00 | 1.06 | -15.27 | 225.91 | 46.73 | 251.39 | 0.7434 | -509.0 | -334.5 | |
| 0.00 | 0.90 | 0.00 | 0.65 | -12.99 | 224.86 | 45.68 | 254.20 | 0.7268 | -568.0 | -443.6 | |
| 0.00 | 1.35 | 0.00 | 0.95 | -14.14 | 223.72 | 44.53 | 252.35 | 0.7159 | -613.0 | -540.9 | |
| 0.00 | 0.90 | 0.00 | 0.62 | -12.64 | 222.89 | 43.71 | 254.23 | 0.7029 | -609.0 | -522.5 | |
| 0.00 | 1.53 | 0.00 | 1.06 | -15.36 | 222.45 | 43.27 | 250.32 | 0.7043 | -550.0 | -414.2 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -13.90 | 222.06 | 42.87 | 252.24 | 0.6958 | -594.0 | -502.8 | |
| 0.00 | 1.62 | 0.00 | 1.12 | -15.55 | 222.29 | 43.10 | 250.00 | 0.7028 | -722.0 | -539.3 | |
| 0.00 | 1.26 | 0.00 | 0.88 | -18.71 | 221.84 | 42.66 | 245.49 | 0.7076 | -644.0 | -567.5 | |
| 0.00 | 0.99 | 0.00 | 0.68 | -20.57 | 220.27 | 41.08 | 242.32 | 0.6970 | -626.0 | -478.1 | |
| 0.00 | 0.90 | 0.00 | 0.62 | -21.24 | 220.36 | 41.18 | 241.45 | 0.7009 | -475.0 | -364.8 | |
| 0.00 | 1.08 | 0.00 | 0.74 | -21.25 | 220.11 | 40.92 | 241.33 | 0.6981 | -322.0 | -378.8 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -21.54 | 220.03 | 40.85 | 240.90 | 0.6985 | -620.0 | -533.2 | |
| 0.00 | 1.17 | 0.00 | 0.77 | -21.27 | 216.49 | 37.31 | 239.50 | 0.6578 | -518.0 | -395.5 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -22.28 | 216.14 | 36.96 | 237.89 | 0.6590 | -547.0 | -507.6 | |
| 0.00 | 1.26 | 0.00 | 0.83 | -22.44 | 216.11 | 36.92 | 237.65 | 0.6596 | -556.0 | -407.1 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -21.73 | 215.89 | 36.71 | 238.52 | 0.6534 | -794.0 | -625.3 | |
| 0.00 | 2.34 | 0.00 | 1.52 | -21.58 | 215.73 | 36.54 | 238.64 | 0.6506 | -814.0 | -654.6 | |
| 0.00 | 1.26 | 0.00 | 0.81 | -21.26 | 215.27 | 36.09 | 238.83 | 0.6438 | -695.0 | -543.8 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -17.43 | 209.50 | 30.31 | 241.06 | 0.5524 | 538.0 | 476.8 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -23.60 | 200.11 | 20.93 | 221.84 | 0.4926 | -635.0 | -537.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |