SDO HMI 2014-04-13 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.09 | 435.29 | 33.75 | 225.95 | 11.61 | 274.75 | -0.39 | 1.13 | 0.3002 | -987.7 | -398.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.09 | 0.00 | 1.61 | 11.69 | 278.23 | 3.10 | 349.97 | 0.3051 | -769.0 | -672.8 | |
| 65.09 | 411.09 | 33.75 | 213.18 | 11.49 | 275.01 | -0.13 | 0.42 | 0.2974 | -1542.1 | -448.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 13.91 | 273.15 | -1.98 | 5.71 | 0.3391 | -865.0 | -685.4 | |
| 0.00 | 1.24 | 0.00 | 0.65 | 13.85 | 272.47 | -2.66 | 7.67 | 0.3394 | -697.0 | -597.4 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 13.62 | 272.38 | -2.75 | 8.02 | 0.3360 | -859.0 | -736.6 | |
| 0.00 | 1.15 | 0.00 | 0.61 | 14.38 | 269.60 | -5.53 | 15.21 | 0.3574 | 783.0 | 647.5 | |
| 0.00 | 2.21 | 0.00 | 1.17 | 14.55 | 269.41 | -5.72 | 15.58 | 0.3608 | 866.0 | 694.0 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 12.86 | 269.42 | -5.71 | 16.96 | 0.3341 | 749.0 | 630.5 | |
| 0.00 | 2.12 | 0.00 | 1.11 | 12.54 | 269.12 | -6.02 | 18.10 | 0.3307 | 855.0 | 745.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.71 | 268.81 | -6.33 | 18.81 | 0.3349 | 906.0 | 736.7 | |
| 0.00 | 3.89 | 0.00 | 2.06 | 14.34 | 268.30 | -6.84 | 18.62 | 0.3629 | 855.0 | 710.8 | |
| 0.00 | 1.59 | 0.00 | 0.84 | 13.79 | 268.25 | -6.89 | 19.25 | 0.3547 | 943.0 | 668.1 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 16.86 | 267.74 | -7.40 | 17.82 | 0.4044 | 686.0 | 564.2 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 16.08 | 267.67 | -7.46 | 18.60 | 0.3928 | 777.0 | 537.7 | |
| 0.00 | 1.50 | 0.00 | 0.80 | 14.16 | 267.33 | -7.80 | 21.21 | 0.3655 | 654.0 | 426.2 | |
| 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. | |