SDO HMI 2014-04-15 23:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81.81 | 263.22 | 40.63 | 130.84 | -9.47 | 244.99 | -1.52 | 163.92 | 0.0814 | 390.9 | 67.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.65 | 0.00 | 1.32 | -9.40 | 247.99 | 1.47 | 200.75 | 0.0718 | 308.0 | 218.8 | |
| 43.43 | 95.35 | 21.56 | 47.33 | -9.22 | 247.41 | 0.89 | 193.56 | 0.0658 | 1197.1 | 391.6 | |
| 0.00 | 1.42 | 0.00 | 0.71 | -11.93 | 247.13 | 0.62 | 185.45 | 0.1119 | 968.0 | 800.8 | |
| 1.59 | 6.01 | 0.79 | 2.99 | -10.00 | 246.86 | 0.34 | 184.36 | 0.0779 | 921.7 | 787.0 | |
| 0.00 | 1.33 | 0.00 | 0.66 | -8.64 | 246.74 | 0.22 | 184.08 | 0.0541 | 811.0 | 681.7 | |
| 0.00 | 3.01 | 0.00 | 1.49 | -8.49 | 246.37 | -0.14 | 177.24 | 0.0514 | 186.0 | 241.8 | |
| 0.71 | 8.67 | 0.35 | 4.30 | -8.19 | 246.22 | -0.29 | 173.68 | 0.0463 | 939.1 | 587.4 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -10.09 | 245.97 | -0.54 | 173.26 | 0.0798 | -815.0 | -595.0 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -10.36 | 245.88 | -0.63 | 172.57 | 0.0847 | -797.0 | -616.7 | |
| 0.00 | 1.15 | 0.00 | 0.57 | -10.66 | 245.76 | -0.76 | 171.67 | 0.0902 | 870.0 | 668.4 | |
| 0.53 | 1.68 | 0.26 | 0.84 | -10.72 | 245.60 | -0.91 | 170.14 | 0.0917 | 1026.7 | 836.2 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -10.21 | 245.36 | -1.15 | 166.25 | 0.0837 | 700.0 | 577.1 | |
| 1.42 | 3.63 | 0.70 | 1.80 | -9.97 | 245.06 | -1.46 | 161.92 | 0.0811 | -614.6 | -243.7 | |
| 0.97 | 5.13 | 0.48 | 2.55 | -8.58 | 245.06 | -1.45 | 154.57 | 0.0585 | -1066.5 | -781.9 | |
| 0.53 | 4.51 | 0.26 | 2.24 | -8.49 | 244.79 | -1.72 | 149.77 | 0.0594 | -1089.8 | -828.6 | |
| 0.00 | 2.30 | 0.00 | 1.14 | -10.60 | 244.69 | -1.83 | 160.34 | 0.0936 | -939.0 | -620.4 | |
| 1.33 | 2.56 | 0.66 | 1.27 | -9.42 | 244.51 | -2.00 | 152.87 | 0.0760 | -1125.6 | -915.9 | |
| 0.00 | 1.59 | 0.00 | 0.79 | -9.81 | 244.20 | -2.31 | 151.80 | 0.0845 | -995.0 | -794.7 | |
| 2.65 | 5.75 | 1.32 | 2.86 | -10.57 | 244.17 | -2.35 | 155.21 | 0.0965 | -1100.3 | -793.3 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -8.82 | 243.88 | -2.64 | 141.31 | 0.0731 | -923.0 | -636.7 | |
| 3.36 | 6.01 | 1.67 | 2.99 | -10.50 | 243.74 | -2.78 | 151.07 | 0.0989 | -1126.2 | -760.4 | |
| 0.00 | 4.25 | 0.00 | 2.11 | -10.68 | 243.46 | -3.05 | 149.62 | 0.1040 | -875.0 | -721.4 | |
| 0.00 | 1.33 | 0.00 | 0.66 | -8.87 | 243.42 | -3.10 | 137.31 | 0.0791 | 752.0 | 463.7 | |
| 10.79 | 14.51 | 5.36 | 7.20 | -8.33 | 243.39 | -3.12 | 131.93 | 0.0728 | 1092.2 | 697.9 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -9.11 | 243.39 | -3.13 | 139.02 | 0.0826 | -794.0 | -544.1 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -10.38 | 242.88 | -3.63 | 143.45 | 0.1051 | -759.0 | -587.5 | |
| 0.00 | 0.80 | 0.00 | 0.40 | -10.59 | 242.60 | -3.91 | 142.61 | 0.1109 | -771.0 | -609.7 | |
| 1.59 | 53.51 | 0.79 | 26.64 | -9.26 | 242.56 | -3.95 | 133.52 | 0.0943 | 782.4 | -105.2 | |
| 2.65 | -28.00 | 1.32 | -28.00 | -9.95 | 242.55 | -3.96 | 138.41 | 0.1030 | -1081.6 | 999999 | |
| 5.57 | 21.14 | 2.78 | 10.54 | -10.37 | 242.30 | -4.21 | 139.30 | 0.1114 | -1103.7 | -187.1 | |
| 4.69 | -28.00 | 2.33 | -28.00 | -9.50 | 242.25 | -4.26 | 133.19 | 0.1010 | 1009.1 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -12.79 | 242.14 | -4.38 | 149.43 | 0.1470 | 688.0 | 602.8 | |
| 0.00 | 3.89 | 0.00 | 1.94 | -9.10 | 242.07 | -4.44 | 129.04 | 0.0989 | 982.0 | 651.2 | |
| 0.00 | 1.15 | 0.00 | 0.57 | -10.52 | 241.99 | -4.52 | 138.18 | 0.1168 | 5.0 | 5.5 | |
| 0.00 | 1.86 | 0.00 | 0.93 | -9.74 | 241.88 | -4.63 | 132.53 | 0.1085 | 691.0 | 575.6 | |
| 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. | |