SDO HMI 2011-11-13 13:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.14 | 367.92 | 33.54 | 211.78 | 16.09 | 64.00 | 28.19 | 297.09 | 0.5120 | -875.8 | -356.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.20 | 355.20 | 0.70 | 204.73 | 15.99 | 64.81 | 29.00 | 296.28 | 0.5219 | -616.2 | -385.4 | |
| 0.86 | -1.00 | 0.50 | -1.00 | 15.42 | 64.37 | 28.56 | 295.55 | 0.5129 | -960.2 | 999999 | |
| 54.79 | -1.00 | 31.60 | -1.00 | 16.03 | 64.22 | 28.41 | 296.77 | 0.5142 | -1303.3 | 999999 | |
| 1.29 | -1.00 | 0.74 | -1.00 | 15.68 | 63.85 | 28.04 | 296.37 | 0.5073 | -1322.2 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.11 | 14.04 | 62.31 | 26.50 | 294.35 | 0.4772 | -898.0 | -767.2 | |
| 0.00 | 0.69 | 0.00 | 0.39 | 15.84 | 61.93 | 26.12 | 298.13 | 0.4823 | -243.0 | -172.8 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 18.06 | 59.85 | 24.04 | 304.20 | 0.4703 | 492.0 | 393.5 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 17.70 | 57.77 | 21.96 | 305.75 | 0.4408 | 851.0 | 630.6 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 16.49 | 56.98 | 21.18 | 304.24 | 0.4208 | 864.0 | 701.7 | |
| 0.00 | 1.29 | 0.00 | 0.71 | 18.37 | 56.81 | 21.01 | 308.16 | 0.4345 | 796.0 | 616.0 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 21.18 | 55.88 | 20.07 | 314.45 | 0.4502 | 915.0 | 721.3 | |
| 0.00 | 1.89 | 0.00 | 1.04 | 21.51 | 54.41 | 18.60 | 317.08 | 0.4376 | 849.0 | 643.8 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 20.92 | 54.16 | 18.36 | 316.44 | 0.4286 | 762.0 | 635.2 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 21.80 | 54.24 | 18.44 | 317.79 | 0.4389 | 638.0 | 457.0 | |
| 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. | |