SDO HMI 2014-03-14 18:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.49 | 146.80 | 42.40 | 152.19 | 11.24 | 10.25 | 58.85 | 287.02 | 0.8794 | 8.0 | -220.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.89 | 76.57 | 17.18 | 82.42 | 11.71 | 11.57 | 60.17 | 287.16 | 0.8909 | -702.3 | -340.3 | |
| 0.00 | 1.30 | 0.00 | 1.36 | 10.41 | 10.76 | 59.36 | 285.95 | 0.8821 | 221.0 | 150.0 | |
| 0.00 | 0.43 | 0.00 | 0.46 | 11.99 | 11.00 | 59.60 | 287.62 | 0.8871 | -427.0 | -395.8 | |
| 0.00 | 1.13 | 0.00 | 1.20 | 12.17 | 10.95 | 59.54 | 287.84 | 0.8871 | -521.0 | -444.6 | |
| 1.13 | -1.00 | 1.18 | -1.00 | 11.50 | 10.53 | 59.12 | 287.22 | 0.8824 | -825.0 | 999999 | |
| 1.39 | 4.17 | 1.39 | 4.19 | 10.30 | 9.50 | 58.09 | 286.19 | 0.8717 | 319.3 | 184.7 | |
| 1.39 | 7.21 | 1.43 | 7.37 | 11.59 | 9.91 | 58.50 | 287.50 | 0.8777 | -615.5 | -543.9 | |
| 0.00 | 0.87 | 0.00 | 0.87 | 10.68 | 9.26 | 57.86 | 286.67 | 0.8706 | 289.0 | 254.3 | |
| 0.95 | 49.48 | 0.96 | 48.96 | 11.40 | 9.26 | 57.85 | 287.47 | 0.8721 | -601.6 | -29.0 | |
| 3.21 | -9.00 | 3.17 | -9.00 | 10.33 | 8.87 | 57.47 | 286.39 | 0.8666 | 592.4 | 999999 | |
| 15.97 | -9.00 | 15.60 | -9.00 | 10.47 | 8.46 | 57.06 | 286.67 | 0.8635 | 735.1 | 999999 | |
| 0.69 | 1.39 | 0.68 | 1.36 | 11.72 | 8.23 | 56.82 | 288.14 | 0.8644 | 219.2 | 178.5 | |
| 0.00 | 0.43 | 0.00 | 0.41 | 10.82 | 7.40 | 56.00 | 287.38 | 0.8553 | 582.0 | 532.0 | |
| 0.00 | 0.69 | 0.00 | 0.66 | 11.23 | 7.41 | 56.01 | 287.84 | 0.8564 | 441.0 | 357.0 | |
| 0.87 | 3.13 | 0.81 | 2.93 | 11.25 | 6.77 | 55.36 | 288.07 | 0.8509 | 448.2 | 394.3 | |
| 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. | |