SDO HMI 2014-10-13 18:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.44 | 338.12 | 57.46 | 329.66 | -8.96 | 318.91 | -57.61 | 104.19 | 0.8600 | 543.1 | 208.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.38 | 288.91 | 20.44 | 265.32 | -8.58 | 321.10 | -55.42 | 104.26 | 0.8421 | 995.9 | 246.9 | |
| 23.25 | -1.00 | 21.41 | -1.00 | -9.18 | 320.91 | -55.61 | 104.90 | 0.8451 | 833.3 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.95 | -7.41 | 321.08 | -55.44 | 102.90 | 0.8400 | 94.0 | 107.4 | |
| 6.56 | -1.00 | 6.07 | -1.00 | -8.86 | 320.66 | -55.86 | 104.47 | 0.8467 | 614.9 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.80 | -9.95 | 314.09 | -62.43 | 104.11 | 0.9021 | -477.0 | -430.8 | |
| 0.00 | 1.49 | 0.00 | 1.68 | -8.55 | 314.01 | -62.51 | 102.56 | 0.9006 | -580.0 | -494.5 | |
| 0.00 | 0.96 | 0.00 | 1.15 | -10.18 | 312.65 | -63.87 | 104.04 | 0.9126 | -456.0 | -396.6 | |
| 0.00 | 0.26 | 0.00 | 0.31 | -10.03 | 312.64 | -63.88 | 103.87 | 0.9125 | -406.0 | -351.7 | |
| 0.00 | 0.52 | 0.00 | 0.64 | -10.15 | 312.38 | -64.14 | 103.95 | 0.9144 | -308.0 | -274.0 | |
| 0.00 | 1.31 | 0.00 | 1.70 | -9.28 | 310.53 | -65.99 | 102.64 | 0.9256 | -457.0 | -329.2 | |
| 0.00 | 1.75 | 0.00 | 2.28 | -9.17 | 310.34 | -66.18 | 102.49 | 0.9267 | -541.0 | -411.1 | |
| 5.24 | 21.85 | 6.86 | 28.82 | -8.91 | 310.21 | -66.31 | 102.19 | 0.9272 | -370.0 | 109.3 | |
| 2.01 | 17.92 | 2.68 | 24.11 | -9.74 | 309.89 | -66.63 | 103.01 | 0.9302 | -241.6 | 142.9 | |
| 0.00 | 1.40 | 0.00 | 1.90 | -9.30 | 309.36 | -67.16 | 102.44 | 0.9329 | 482.0 | 453.5 | |
| 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. | |