SDO HMI 2014-05-18 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.25 | 240.25 | 41.25 | 128.58 | -16.58 | 194.78 | 17.24 | 228.75 | 0.3789 | 136.6 | 96.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.64 | -17.64 | 197.30 | 19.75 | 230.35 | 0.4201 | 805.0 | 567.5 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -16.80 | 196.40 | 18.86 | 230.76 | 0.4011 | 659.0 | 571.9 | |
| 30.12 | 113.29 | 16.29 | 61.26 | -17.34 | 196.05 | 18.51 | 229.19 | 0.4020 | 1155.4 | 389.9 | |
| 0.81 | -3.00 | 0.44 | -3.00 | -17.78 | 196.00 | 18.45 | 228.25 | 0.4057 | 870.1 | 999999 | |
| 3.42 | 10.34 | 1.84 | 5.56 | -16.43 | 195.66 | 18.12 | 230.45 | 0.3885 | 1085.2 | 806.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -16.56 | 195.41 | 17.86 | 229.81 | 0.3865 | 915.0 | 693.7 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -14.35 | 194.92 | 17.38 | 233.92 | 0.3595 | 888.0 | 694.2 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -15.10 | 194.95 | 17.40 | 232.26 | 0.3667 | 760.0 | 617.8 | |
| 0.81 | 6.74 | 0.43 | 3.61 | -16.41 | 194.93 | 17.39 | 229.39 | 0.3792 | 1144.2 | 784.3 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -15.51 | 194.78 | 17.24 | 231.11 | 0.3685 | 637.0 | 445.8 | |
| 0.81 | -9.00 | 0.43 | -9.00 | -16.60 | 194.78 | 17.24 | 228.77 | 0.3792 | 905.3 | 999999 | |
| 3.51 | 103.40 | 1.86 | 54.69 | -15.80 | 193.79 | 16.24 | 228.86 | 0.3589 | -969.1 | -492.6 | |
| 8.63 | -12.00 | 4.57 | -12.00 | -15.86 | 193.56 | 16.02 | 228.34 | 0.3568 | -902.5 | 999999 | |
| 13.13 | -12.00 | 6.95 | -12.00 | -16.05 | 193.12 | 15.58 | 227.15 | 0.3535 | -942.1 | 999999 | |
| 16.01 | -12.00 | 8.44 | -12.00 | -15.46 | 192.98 | 15.43 | 228.20 | 0.3455 | -1223.5 | 999999 | |
| 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. | |