SDO HMI 2014-10-13 05:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.44 | 0.00 | 11.77 | 14.31 | 58.07 | 34.41 | 286.66 | 0.5723 | 212.7 | 208.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.78 | 14.70 | 67.13 | 43.48 | 285.03 | 0.6915 | -551.0 | -473.5 | |
| 0.00 | 0.96 | 0.00 | 0.65 | 11.44 | 66.38 | 42.72 | 280.37 | 0.6784 | -522.0 | -447.4 | |
| 0.00 | 1.05 | 0.00 | 0.70 | 12.36 | 66.18 | 42.53 | 281.76 | 0.6768 | -489.0 | -424.3 | |
| 0.00 | 0.96 | 0.00 | 0.60 | 13.33 | 60.25 | 36.60 | 284.26 | 0.6009 | 656.0 | 509.3 | |
| 0.00 | 1.05 | 0.00 | 0.67 | 20.49 | 61.17 | 37.52 | 295.35 | 0.6335 | -421.0 | -331.1 | |
| 0.00 | 0.88 | 0.00 | 0.54 | 16.36 | 59.04 | 35.39 | 289.62 | 0.5922 | -748.0 | -677.2 | |
| 0.00 | 1.58 | 0.00 | 0.96 | 16.66 | 58.15 | 34.50 | 290.45 | 0.5813 | -86.0 | -132.6 | |
| 0.00 | 0.70 | 0.00 | 0.41 | 12.76 | 56.05 | 32.40 | 284.31 | 0.5415 | 494.0 | 427.9 | |
| 0.00 | 1.84 | 0.00 | 1.08 | 13.47 | 55.79 | 32.14 | 285.69 | 0.5395 | 442.0 | 407.0 | |
| 0.00 | 1.66 | 0.00 | 0.98 | 13.33 | 55.66 | 32.01 | 285.47 | 0.5373 | 686.0 | 555.4 | |
| 0.00 | 1.66 | 0.00 | 0.97 | 13.52 | 55.40 | 31.75 | 285.92 | 0.5341 | 870.0 | 692.4 | |
| 0.00 | 2.89 | 0.00 | 1.68 | 13.77 | 54.86 | 31.21 | 286.55 | 0.5271 | 700.0 | 601.6 | |
| 0.00 | 0.44 | 0.00 | 0.25 | 14.09 | 54.41 | 30.75 | 287.33 | 0.5216 | 754.0 | 638.2 | |
| 0.00 | 1.58 | 0.00 | 0.91 | 13.73 | 54.35 | 30.70 | 286.67 | 0.5198 | 709.0 | 537.6 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 15.52 | 50.86 | 27.21 | 291.80 | 0.4765 | 697.0 | 542.2 | |
| 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. | |