SDO HMI 2014-01-13 03:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.23 | 186.69 | 23.05 | 95.19 | -17.95 | 30.21 | 0.41 | 181.65 | 0.2377 | 411.4 | 46.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.60 | -15.34 | 33.12 | 3.32 | 196.35 | 0.1996 | 765.0 | 609.4 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -18.54 | 32.34 | 2.54 | 189.72 | 0.2498 | 675.0 | 603.5 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -18.33 | 32.30 | 2.50 | 189.74 | 0.2462 | 851.0 | 580.0 | |
| 3.32 | 108.12 | 1.69 | 55.14 | -18.15 | 31.49 | 1.69 | 186.72 | 0.2412 | 1073.9 | 400.0 | |
| 28.05 | -4.00 | 14.30 | -4.00 | -17.96 | 31.31 | 1.51 | 186.07 | 0.2377 | 1199.0 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -17.24 | 30.44 | 0.64 | 182.73 | 0.2242 | 712.0 | 426.6 | |
| 0.00 | 3.74 | 0.00 | 1.91 | -18.30 | 30.28 | 0.48 | 181.91 | 0.2422 | 588.0 | 637.7 | |
| 0.00 | 4.17 | 0.00 | 2.12 | -18.00 | 30.19 | 0.39 | 181.58 | 0.2370 | 843.0 | 473.8 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -18.18 | 29.10 | -0.69 | 177.24 | 0.2403 | -950.0 | -792.3 | |
| 0.60 | 3.49 | 0.30 | 1.78 | -18.33 | 28.89 | -0.91 | 176.42 | 0.2430 | -1133.9 | -882.9 | |
| 1.53 | 60.61 | 0.78 | 30.90 | -17.75 | 28.39 | -1.40 | 174.25 | 0.2339 | -1138.9 | -583.5 | |
| 10.54 | -11.00 | 5.37 | -11.00 | -17.90 | 28.15 | -1.65 | 173.31 | 0.2369 | -1253.8 | 999999 | |
| 1.19 | -11.00 | 0.61 | -11.00 | -18.11 | 27.99 | -1.81 | 172.80 | 0.2408 | -944.9 | 999999 | |
| 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. | |