SDO HMI 2014-03-14 03:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.80 | 61.85 | 18.06 | 51.07 | 11.44 | 9.74 | 50.10 | 290.13 | 0.8030 | -17.3 | -227.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.69 | 3.56 | 0.60 | 3.05 | 11.52 | 11.33 | 51.70 | 289.63 | 0.8187 | -362.6 | -336.8 | |
| 3.21 | 18.07 | 2.74 | 15.29 | 11.79 | 10.91 | 51.28 | 290.10 | 0.8155 | -588.9 | -513.9 | |
| 5.04 | -2.00 | 4.25 | -2.00 | 11.96 | 10.42 | 50.79 | 290.48 | 0.8114 | -582.1 | 999999 | |
| 2.78 | 3.91 | 2.28 | 3.21 | 10.28 | 9.77 | 50.14 | 288.72 | 0.7998 | 485.8 | 318.8 | |
| 0.00 | 1.30 | 0.00 | 1.08 | 10.84 | 9.81 | 50.18 | 289.38 | 0.8019 | -314.0 | -260.1 | |
| 3.04 | 14.94 | 2.52 | 12.26 | 11.67 | 9.68 | 50.04 | 290.42 | 0.8033 | -601.6 | -430.0 | |
| 0.61 | 1.74 | 0.49 | 1.41 | 10.54 | 9.27 | 49.64 | 289.22 | 0.7956 | 609.7 | 528.1 | |
| 0.00 | 1.39 | 0.00 | 1.14 | 11.30 | 9.44 | 49.81 | 290.07 | 0.7998 | -450.0 | -427.5 | |
| 4.43 | 9.47 | 3.60 | 7.71 | 10.78 | 9.18 | 49.55 | 289.54 | 0.7955 | 619.3 | 142.0 | |
| 2.00 | 3.73 | 1.58 | 2.95 | 11.25 | 7.66 | 48.03 | 290.72 | 0.7819 | 363.9 | 320.5 | |
| 0.00 | 1.30 | 0.00 | 1.04 | 12.09 | 7.86 | 48.23 | 291.64 | 0.7869 | 175.0 | 85.7 | |
| 0.00 | 1.13 | 0.00 | 0.90 | 11.93 | 7.59 | 47.96 | 291.57 | 0.7837 | 277.0 | 256.2 | |
| 0.00 | 0.96 | 0.00 | 0.76 | 11.77 | 7.46 | 47.83 | 291.42 | 0.7817 | 468.0 | 424.9 | |
| 0.00 | 0.35 | 0.00 | 0.27 | 11.89 | 7.08 | 47.45 | 291.72 | 0.7783 | 411.0 | 360.8 | |
| 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. | |