SDO HMI 2014-03-12 20:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.40 | 37.29 | 14.77 | 53.93 | -18.54 | 47.89 | 71.23 | 252.82 | 0.9404 | -69.8 | -28.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.78 | 4.34 | 1.33 | 7.39 | -18.18 | 51.22 | 74.56 | 253.12 | 0.9583 | -50.2 | 24.5 | |
| 1.04 | 3.30 | 1.62 | 5.13 | -16.90 | 49.38 | 72.72 | 254.54 | 0.9493 | 328.5 | 211.5 | |
| 0.95 | 3.38 | 1.57 | 5.59 | -18.25 | 50.60 | 73.94 | 253.07 | 0.9553 | 410.3 | 347.9 | |
| 0.00 | 0.69 | 0.00 | 1.04 | -18.06 | 48.55 | 71.89 | 253.34 | 0.9447 | 272.0 | 253.1 | |
| 0.00 | 1.21 | 0.00 | 1.82 | -18.39 | 48.68 | 72.02 | 252.99 | 0.9453 | 302.0 | 286.8 | |
| 0.00 | 0.95 | 0.00 | 1.38 | -17.61 | 47.82 | 71.16 | 253.83 | 0.9407 | 438.0 | 390.2 | |
| 0.00 | 1.39 | 0.00 | 2.08 | -18.62 | 48.61 | 71.94 | 252.75 | 0.9449 | 257.0 | 228.2 | |
| 0.00 | 0.78 | 0.00 | 1.11 | -19.15 | 47.55 | 70.89 | 252.20 | 0.9390 | -159.0 | -172.7 | |
| 0.00 | 1.47 | 0.00 | 1.95 | -18.15 | 45.87 | 69.21 | 253.29 | 0.9291 | 360.0 | 298.9 | |
| 2.34 | 4.25 | 3.12 | 5.67 | -18.48 | 45.98 | 69.32 | 252.93 | 0.9298 | -188.6 | -54.2 | |
| 1.91 | 3.21 | 2.64 | 4.44 | -19.69 | 46.94 | 70.28 | 251.63 | 0.9355 | -233.2 | -111.9 | |
| 0.00 | 1.13 | 0.00 | 1.53 | -19.41 | 46.38 | 69.72 | 251.93 | 0.9322 | -315.0 | -361.1 | |
| 1.99 | 11.19 | 2.66 | 14.80 | -19.23 | 46.03 | 69.37 | 252.13 | 0.9301 | -565.8 | -454.2 | |
| 1.39 | -13.00 | 1.83 | -13.00 | -18.98 | 45.71 | 69.05 | 252.39 | 0.9281 | -587.8 | 999999 | |
| 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. | |