SDO HMI 2014-03-14 08:11:44 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.57 | 120.79 | 39.64 | 107.00 | 11.29 | 9.95 | 53.16 | 288.84 | 0.8312 | -63.0 | -216.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.48 | 44.14 | 1.37 | 40.48 | 11.36 | 11.62 | 54.83 | 288.36 | 0.8465 | -420.2 | -454.9 | |
| 14.51 | -1.00 | 13.37 | -1.00 | 11.77 | 11.37 | 54.58 | 288.91 | 0.8454 | -568.5 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.93 | 10.24 | 10.43 | 53.64 | 287.47 | 0.8329 | 283.0 | 246.4 | |
| 0.00 | 1.48 | 0.00 | 1.32 | 10.52 | 10.45 | 53.66 | 287.78 | 0.8338 | 19.0 | 146.9 | |
| 0.00 | 0.35 | 0.00 | 0.31 | 11.29 | 10.66 | 53.86 | 288.60 | 0.8378 | -364.0 | -374.0 | |
| 2.43 | -1.00 | 2.20 | -1.00 | 12.10 | 10.63 | 53.84 | 289.54 | 0.8398 | -451.6 | 999999 | |
| 4.26 | 6.00 | 3.72 | 5.24 | 10.26 | 9.72 | 52.93 | 287.72 | 0.8264 | 431.0 | 185.9 | |
| 6.08 | 56.39 | 5.42 | 49.17 | 11.66 | 10.04 | 53.25 | 289.24 | 0.8332 | -665.1 | -199.3 | |
| 10.60 | -8.00 | 9.13 | -8.00 | 10.59 | 9.00 | 52.21 | 288.35 | 0.8206 | 658.2 | 999999 | |
| 2.87 | -8.00 | 2.47 | -8.00 | 10.98 | 8.85 | 52.06 | 288.86 | 0.8203 | 260.5 | 999999 | |
| 0.00 | 1.56 | 0.00 | 1.35 | 11.60 | 8.81 | 52.02 | 289.60 | 0.8218 | -458.0 | -369.0 | |
| 0.00 | 0.96 | 0.00 | 0.81 | 11.85 | 7.84 | 51.05 | 290.24 | 0.8134 | 167.0 | 176.4 | |
| 1.82 | 3.22 | 1.52 | 2.69 | 11.06 | 7.50 | 50.71 | 289.44 | 0.8077 | 508.4 | 394.3 | |
| 0.52 | 3.74 | 0.44 | 3.12 | 11.73 | 7.28 | 50.49 | 290.31 | 0.8077 | 507.5 | 459.4 | |
| 0.00 | 1.91 | 0.00 | 1.58 | 11.69 | 6.89 | 50.09 | 290.41 | 0.8037 | 428.0 | 390.4 | |
| 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. | |