SDO HMI 2014-12-03 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.37 | 135.26 | 39.50 | 114.63 | -16.12 | 125.01 | 52.15 | 249.39 | 0.8120 | 120.3 | 21.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.02 | 10.93 | 1.00 | 10.62 | -15.23 | 131.05 | 58.19 | 251.87 | 0.8648 | 467.7 | 421.3 | |
| 3.50 | -1.00 | 3.39 | -1.00 | -15.10 | 130.65 | 57.78 | 251.94 | 0.8612 | 609.0 | 999999 | |
| 4.87 | 54.83 | 4.27 | 47.39 | -15.27 | 126.76 | 53.89 | 250.90 | 0.8270 | -856.2 | -119.4 | |
| 0.00 | 1.28 | 0.00 | 1.12 | -16.01 | 126.68 | 53.81 | 250.01 | 0.8277 | -153.0 | -159.7 | |
| 7.09 | -3.00 | 6.09 | -3.00 | -14.93 | 126.01 | 53.15 | 251.14 | 0.8193 | 608.0 | 999999 | |
| 2.73 | -3.00 | 2.34 | -3.00 | -14.53 | 125.87 | 53.01 | 251.59 | 0.8171 | 653.3 | 999999 | |
| 3.16 | -3.00 | 2.69 | -3.00 | -14.68 | 125.62 | 52.75 | 251.35 | 0.8150 | 706.0 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.94 | -14.92 | 125.55 | 52.68 | 251.03 | 0.8148 | 273.0 | 379.1 | |
| 0.00 | 1.11 | 0.00 | 0.94 | -14.73 | 125.18 | 52.32 | 251.17 | 0.8109 | 719.0 | 688.5 | |
| 2.31 | 3.84 | 1.94 | 3.23 | -15.38 | 125.00 | 52.14 | 250.35 | 0.8106 | 529.4 | 465.4 | |
| 7.86 | 12.04 | 6.69 | 10.25 | -17.29 | 125.07 | 52.21 | 248.06 | 0.8156 | 603.1 | 428.4 | |
| 0.00 | 0.77 | 0.00 | 0.63 | -15.06 | 124.05 | 51.18 | 250.49 | 0.8005 | 552.0 | 538.0 | |
| 0.00 | 0.85 | 0.00 | 0.72 | -17.54 | 124.61 | 51.75 | 247.64 | 0.8119 | 431.0 | 402.5 | |
| 0.00 | 1.02 | 0.00 | 0.83 | -15.02 | 123.11 | 50.25 | 250.28 | 0.7911 | -163.0 | -188.9 | |
| 1.28 | 4.10 | 1.04 | 3.32 | -15.94 | 123.08 | 50.22 | 249.14 | 0.7930 | -647.9 | -456.3 | |
| 1.71 | 4.87 | 1.37 | 3.91 | -15.72 | 122.82 | 49.95 | 249.33 | 0.7898 | -639.0 | -461.1 | |
| 0.00 | 1.28 | 0.00 | 1.03 | -16.00 | 122.72 | 49.85 | 248.96 | 0.7895 | -616.0 | -556.9 | |
| 0.00 | 0.85 | 0.00 | 0.69 | -16.40 | 122.81 | 49.94 | 248.49 | 0.7915 | -78.0 | -155.3 | |
| 0.00 | 0.68 | 0.00 | 0.56 | -17.61 | 123.11 | 50.24 | 247.10 | 0.7977 | 394.0 | 475.4 | |
| 0.85 | 6.66 | 0.71 | 5.52 | -19.53 | 123.35 | 50.48 | 244.87 | 0.8053 | 720.1 | 447.8 | |
| 1.45 | 2.82 | 1.19 | 2.30 | -18.61 | 122.82 | 49.95 | 245.80 | 0.7976 | 495.8 | 402.0 | |
| 0.00 | 1.37 | 0.00 | 1.13 | -19.71 | 123.23 | 50.36 | 244.61 | 0.8047 | 221.0 | 340.4 | |
| 0.00 | 2.39 | 0.00 | 1.92 | -17.58 | 122.32 | 49.45 | 246.90 | 0.7898 | -203.0 | -192.6 | |
| 8.54 | 13.07 | 6.78 | 10.38 | -17.41 | 121.74 | 48.87 | 246.91 | 0.7836 | -707.3 | -515.1 | |
| 0.00 | 2.05 | 0.00 | 1.60 | -16.79 | 121.05 | 48.18 | 247.47 | 0.7748 | 513.0 | 421.8 | |
| 0.00 | 1.79 | 0.00 | 1.44 | -19.23 | 121.95 | 49.09 | 244.76 | 0.7911 | 624.0 | 488.5 | |
| 0.00 | 0.43 | 0.00 | 0.34 | -18.44 | 121.08 | 48.21 | 245.43 | 0.7800 | 428.0 | 421.0 | |
| 0.00 | 0.77 | 0.00 | 0.61 | -19.47 | 121.10 | 48.23 | 244.17 | 0.7835 | 341.0 | 418.2 | |
| 0.00 | 1.02 | 0.00 | 0.81 | -19.63 | 121.11 | 48.25 | 243.98 | 0.7842 | 676.0 | 634.6 | |
| 0.00 | 0.77 | 0.00 | 0.57 | -20.00 | 117.41 | 44.54 | 242.06 | 0.7484 | -601.0 | -517.4 | |
| 0.00 | 0.68 | 0.00 | 0.48 | -16.64 | 115.48 | 42.62 | 245.60 | 0.7147 | -449.0 | -384.2 | |
| 0.00 | 0.60 | 0.00 | 0.44 | -20.44 | 116.64 | 43.77 | 241.17 | 0.7423 | -443.0 | -372.7 | |
| 0.00 | 0.43 | 0.00 | 0.31 | -19.39 | 116.19 | 43.32 | 242.30 | 0.7333 | -647.0 | -621.6 | |
| 0.00 | 0.85 | 0.00 | 0.60 | -16.85 | 115.04 | 42.17 | 245.13 | 0.7106 | -363.0 | -409.2 | |
| 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. | |