SDO HMI 2014-01-10 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 |
| 26.59 | 65.67 | 19.85 | 49.04 | 16.79 | 25.04 | -44.26 | 63.26 | 0.7503 | 236.3 | 102.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.69 | 10.11 | 4.05 | 7.19 | 15.97 | 27.64 | -41.66 | 63.04 | 0.7194 | -768.3 | -500.5 | |
| 0.00 | 2.46 | 0.00 | 1.76 | 15.64 | 27.31 | -41.99 | 63.63 | 0.7215 | -399.0 | -431.6 | |
| 0.00 | 1.36 | 0.00 | 1.01 | 17.29 | 25.77 | -43.54 | 62.31 | 0.7451 | 686.0 | 521.8 | |
| 0.51 | 1.70 | 0.37 | 1.24 | 15.56 | 25.95 | -43.35 | 64.40 | 0.7357 | -515.2 | -420.9 | |
| 1.70 | 38.84 | 1.27 | 29.38 | 17.38 | 25.18 | -44.12 | 62.47 | 0.7516 | 797.4 | 491.4 | |
| 3.31 | -5.00 | 2.49 | -5.00 | 17.37 | 24.84 | -44.47 | 62.65 | 0.7550 | 768.5 | 999999 | |
| 0.00 | 2.38 | 0.00 | 1.77 | 15.90 | 24.75 | -44.55 | 64.52 | 0.7498 | -563.0 | -388.6 | |
| 13.43 | -5.00 | 10.20 | -5.00 | 17.33 | 24.28 | -45.02 | 62.96 | 0.7605 | 855.0 | 999999 | |
| 0.68 | 5.61 | 0.51 | 4.21 | 15.88 | 24.41 | -44.90 | 64.69 | 0.7533 | -692.2 | -594.5 | |
| 0.00 | 1.44 | 0.00 | 1.09 | 16.17 | 24.24 | -45.07 | 64.41 | 0.7562 | -344.0 | -262.4 | |
| 1.27 | -9.00 | 0.96 | -9.00 | 15.73 | 24.32 | -44.98 | 64.92 | 0.7536 | -669.2 | 999999 | |
| 0.00 | 0.76 | 0.00 | 0.59 | 16.92 | 23.70 | -45.60 | 63.72 | 0.7647 | 312.0 | 271.4 | |
| 0.00 | 0.59 | 0.00 | 0.45 | 14.50 | 23.57 | -45.74 | 66.79 | 0.7568 | 534.0 | 452.7 | |
| 0.00 | 0.42 | 0.00 | 0.35 | 17.77 | 19.73 | -49.57 | 64.36 | 0.8064 | -480.0 | -466.4 | |
| 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. | |