SDO HMI 2014-09-13 18:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.23 | 93.52 | 14.53 | 51.60 | -15.67 | 65.32 | 12.90 | 209.01 | 0.4448 | 512.8 | 368.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.38 | 4.98 | 1.88 | 2.77 | -15.81 | 66.86 | 14.44 | 211.76 | 0.4576 | 922.4 | 705.8 | |
| 0.00 | 1.51 | 0.00 | 0.84 | -16.44 | 66.81 | 14.39 | 210.95 | 0.4654 | 737.0 | 623.1 | |
| 2.22 | 3.91 | 1.24 | 2.17 | -15.83 | 66.48 | 14.05 | 211.05 | 0.4548 | 939.8 | 672.3 | |
| 6.76 | 68.81 | 3.74 | 37.99 | -15.66 | 66.21 | 13.78 | 210.76 | 0.4503 | 983.9 | 521.2 | |
| 0.00 | 1.87 | 0.00 | 1.04 | -16.22 | 66.21 | 13.79 | 210.13 | 0.4578 | 798.0 | 629.2 | |
| 5.78 | -4.00 | 3.20 | -4.00 | -15.56 | 66.00 | 13.58 | 210.52 | 0.4473 | 1075.8 | 999999 | |
| 5.96 | -4.00 | 3.29 | -4.00 | -15.35 | 65.80 | 13.38 | 210.37 | 0.4430 | 1285.5 | 999999 | |
| 2.13 | -4.00 | 1.18 | -4.00 | -15.55 | 65.71 | 13.29 | 209.99 | 0.4449 | 1038.5 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.69 | -15.94 | 65.71 | 13.29 | 209.53 | 0.4502 | 593.0 | 512.9 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -16.99 | 61.89 | 9.46 | 201.06 | 0.4395 | -712.0 | -626.7 | |
| 0.00 | 1.24 | 0.00 | 0.69 | -17.08 | 61.76 | 9.34 | 200.73 | 0.4402 | -770.0 | -689.1 | |
| 0.00 | 1.07 | 0.00 | 0.57 | -12.68 | 61.30 | 8.87 | 203.94 | 0.3724 | 460.0 | 442.7 | |
| 0.00 | 1.16 | 0.00 | 0.62 | -12.99 | 60.93 | 8.51 | 202.73 | 0.3747 | -665.0 | -409.5 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -18.87 | 59.57 | 7.15 | 195.02 | 0.4563 | -842.0 | -681.6 | |
| 0.00 | 2.04 | 0.00 | 1.11 | -16.66 | 58.69 | 6.27 | 194.51 | 0.4192 | -744.0 | -677.3 | |
| 0.00 | 2.13 | 0.00 | 1.16 | -16.59 | 58.50 | 6.08 | 194.13 | 0.4174 | -567.0 | -510.8 | |
| 0.00 | 1.60 | 0.00 | 0.87 | -16.46 | 58.21 | 5.79 | 193.56 | 0.4142 | -673.0 | -524.1 | |
| 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. | |