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 |
| 77.36 | 315.47 | 80.65 | 321.98 | 5.33 | 11.37 | 59.96 | 280.16 | 0.8773 | 62.3 | 116.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.38 | 12.24 | 9.16 | 15.20 | 4.80 | 16.91 | 65.51 | 278.44 | 0.9185 | -454.8 | -273.8 | |
| 0.00 | 1.39 | 0.00 | 1.70 | 4.69 | 16.53 | 65.13 | 278.40 | 0.9157 | -615.0 | -484.9 | |
| 0.00 | 1.13 | 0.00 | 1.32 | 5.37 | 15.26 | 63.85 | 279.38 | 0.9076 | -176.0 | -159.0 | |
| 0.00 | 1.04 | 0.00 | 1.19 | 4.02 | 14.89 | 63.48 | 277.98 | 0.9032 | -582.0 | -506.0 | |
| 0.00 | 2.86 | 0.00 | 3.28 | 5.06 | 14.72 | 63.32 | 279.15 | 0.9033 | -617.0 | -454.9 | |
| 0.78 | 1.82 | 0.87 | 2.04 | 5.68 | 13.98 | 62.57 | 279.98 | 0.8987 | -364.3 | -320.8 | |
| 9.46 | 21.96 | 10.55 | 24.46 | 6.08 | 13.80 | 62.39 | 280.46 | 0.8979 | -468.5 | -208.2 | |
| 0.00 | 1.04 | 0.00 | 1.14 | 5.49 | 13.42 | 62.02 | 279.89 | 0.8942 | -424.0 | -455.6 | |
| 16.67 | 271.99 | 17.16 | 271.65 | 3.94 | 11.74 | 60.34 | 278.52 | 0.8785 | -625.8 | 173.3 | |
| 2.17 | -9.00 | 2.23 | -9.00 | 4.86 | 11.57 | 60.16 | 279.59 | 0.8785 | 94.8 | 999999 | |
| 1.74 | -9.00 | 1.77 | -9.00 | 4.51 | 11.39 | 59.99 | 279.23 | 0.8765 | -550.0 | 999999 | |
| 15.28 | -9.00 | 15.40 | -9.00 | 5.89 | 10.66 | 59.25 | 280.94 | 0.8727 | 668.1 | 999999 | |
| 1.39 | -9.00 | 1.40 | -9.00 | 6.31 | 10.62 | 59.21 | 281.43 | 0.8731 | 492.8 | 999999 | |
| 5.04 | -9.00 | 4.91 | -9.00 | 4.81 | 9.73 | 58.33 | 279.94 | 0.8630 | 667.4 | 999999 | |
| 17.45 | -9.00 | 17.20 | -9.00 | 6.31 | 9.80 | 58.40 | 281.62 | 0.8663 | 838.2 | 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. | |