SDO HMI 2014-02-27 11:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.76 | 38.21 | 6.53 | 33.09 | 15.99 | 102.36 | -50.53 | 64.74 | 0.8222 | -207.4 | -170.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.62 | 13.14 | 105.38 | -47.50 | 66.80 | 0.7835 | 551.0 | 513.1 | |
| 5.17 | 11.21 | 4.33 | 9.38 | 16.19 | 103.98 | -48.91 | 63.84 | 0.8087 | -655.2 | -516.6 | |
| 1.21 | -2.00 | 1.01 | -2.00 | 15.89 | 104.07 | -48.81 | 64.13 | 0.8066 | -695.4 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.81 | 17.26 | 103.61 | -49.28 | 62.79 | 0.8161 | -482.0 | -330.5 | |
| 0.86 | 3.10 | 0.73 | 2.63 | 16.18 | 103.41 | -49.48 | 64.10 | 0.8138 | -201.6 | -148.2 | |
| 0.00 | 6.38 | 0.00 | 5.39 | 15.80 | 103.39 | -49.49 | 64.54 | 0.8125 | -447.0 | -365.0 | |
| 0.00 | 1.12 | 0.00 | 0.94 | 15.45 | 103.41 | -49.47 | 64.94 | 0.8110 | -333.0 | -407.7 | |
| 0.00 | 2.33 | 0.00 | 2.05 | 16.53 | 101.87 | -51.01 | 64.36 | 0.8288 | 637.0 | 476.4 | |
| 0.52 | 3.97 | 0.46 | 3.52 | 16.17 | 101.31 | -51.58 | 64.99 | 0.8325 | -610.7 | -573.4 | |
| 0.00 | 2.76 | 0.00 | 2.48 | 15.86 | 100.67 | -52.22 | 65.60 | 0.8370 | -345.0 | -266.2 | |
| 0.00 | 1.81 | 0.00 | 1.61 | 14.78 | 100.65 | -52.24 | 66.83 | 0.8337 | 633.0 | 533.1 | |
| 0.00 | 1.47 | 0.00 | 1.37 | 15.96 | 99.08 | -53.81 | 66.10 | 0.8508 | -217.0 | -245.1 | |
| 0.00 | 1.47 | 0.00 | 1.43 | 16.87 | 97.73 | -55.15 | 65.60 | 0.8645 | 561.0 | 549.6 | |
| 0.00 | 0.86 | 0.00 | 0.86 | 15.71 | 96.63 | -56.26 | 67.25 | 0.8700 | 384.0 | 322.8 | |
| 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. | |