SDO HMI 2011-11-14 02:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.99 | 346.28 | 31.07 | 214.66 | 16.40 | 63.54 | 34.91 | 293.80 | 0.6033 | -843.0 | -349.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 0.99 | 18.39 | 65.59 | 36.95 | 295.76 | 0.6357 | -688.0 | -522.8 | |
| 48.44 | 326.15 | 30.12 | 202.73 | 16.04 | 64.05 | 35.41 | 292.86 | 0.6067 | -1215.4 | -373.1 | |
| 1.55 | -2.00 | 0.95 | -2.00 | 15.66 | 63.48 | 34.85 | 292.52 | 0.5978 | -1093.0 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.68 | 14.86 | 62.66 | 34.02 | 291.60 | 0.5839 | -707.0 | -627.2 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 19.51 | 58.82 | 30.19 | 301.53 | 0.5582 | 674.0 | 519.9 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 19.94 | 58.73 | 30.10 | 302.30 | 0.5598 | 552.0 | 452.4 | |
| 0.00 | 1.38 | 0.00 | 0.81 | 17.95 | 58.05 | 29.41 | 299.50 | 0.5389 | 511.0 | 464.4 | |
| 0.00 | 3.18 | 0.00 | 1.85 | 18.22 | 56.89 | 28.25 | 300.84 | 0.5257 | 819.0 | 682.2 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 21.35 | 56.20 | 27.56 | 306.62 | 0.5390 | 688.0 | 576.8 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 21.42 | 54.53 | 25.90 | 308.27 | 0.5200 | 732.0 | 572.8 | |
| 0.00 | 1.29 | 0.00 | 0.76 | 22.99 | 54.71 | 26.07 | 310.59 | 0.5349 | 607.0 | 436.4 | |
| 0.00 | 1.72 | 0.00 | 1.01 | 26.14 | 52.21 | 23.57 | 317.87 | 0.5373 | -743.0 | -528.8 | |
| 0.00 | 2.49 | 0.00 | 1.47 | 29.34 | 49.49 | 20.85 | 325.21 | 0.5460 | -609.0 | -431.9 | |
| 0.00 | 1.38 | 0.00 | 0.81 | 29.61 | 49.08 | 20.44 | 326.04 | 0.5456 | -607.0 | -511.7 | |
| 0.00 | 2.15 | 0.00 | 1.26 | 29.12 | 48.68 | 20.04 | 325.94 | 0.5368 | -734.0 | -542.6 | |
| 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. | |