SDO HMI 2014-11-15 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.24 | 100.40 | 33.95 | 128.25 | 13.92 | 15.62 | 67.15 | 283.93 | 0.9228 | -335.9 | -135.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.85 | 22.54 | 7.95 | 30.70 | 13.16 | 17.17 | 68.69 | 283.02 | 0.9327 | -458.0 | -121.3 | |
| 0.00 | 1.46 | 0.00 | 1.87 | 12.92 | 15.79 | 67.31 | 282.82 | 0.9239 | -450.0 | -363.8 | |
| 3.35 | 44.99 | 4.38 | 58.45 | 14.06 | 16.22 | 67.74 | 284.03 | 0.9270 | 40.5 | -20.1 | |
| 5.08 | 14.88 | 6.43 | 18.77 | 13.42 | 15.51 | 67.04 | 283.37 | 0.9223 | -553.9 | -472.3 | |
| 10.84 | -3.00 | 14.00 | -3.00 | 14.28 | 15.95 | 67.48 | 284.29 | 0.9254 | -502.0 | 999999 | |
| 0.00 | 4.13 | 0.00 | 5.11 | 14.06 | 14.87 | 66.39 | 284.10 | 0.9182 | -478.0 | -447.6 | |
| 0.00 | 2.15 | 0.00 | 2.58 | 15.17 | 13.93 | 65.46 | 285.38 | 0.9123 | -601.0 | -539.2 | |
| 0.43 | 1.81 | 0.47 | 1.96 | 14.83 | 11.12 | 62.64 | 285.22 | 0.8917 | -510.4 | -473.8 | |
| 0.00 | 0.86 | 0.00 | 0.92 | 14.24 | 10.69 | 62.21 | 284.59 | 0.8880 | 302.0 | 251.6 | |
| 0.00 | 0.26 | 0.00 | 0.28 | 14.39 | 10.76 | 62.28 | 284.76 | 0.8887 | 253.0 | 245.3 | |
| 0.69 | 4.22 | 0.72 | 4.44 | 13.90 | 10.19 | 61.72 | 284.25 | 0.8839 | 536.8 | 310.0 | |
| 0.00 | 1.12 | 0.00 | 1.12 | 13.84 | 8.58 | 60.11 | 284.32 | 0.8708 | 165.0 | 214.2 | |
| 0.00 | 0.26 | 0.00 | 0.26 | 13.85 | 8.28 | 59.81 | 284.37 | 0.8683 | 441.0 | 399.0 | |
| 0.00 | 1.03 | 0.00 | 1.12 | 19.96 | 10.71 | 62.24 | 291.00 | 0.8928 | -377.0 | -309.1 | |
| 0.00 | 0.69 | 0.00 | 0.67 | 20.48 | 6.56 | 58.09 | 292.23 | 0.8611 | 399.0 | 362.8 | |
| 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. | |