SDO HMI 2014-08-24 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.93 | 105.14 | 31.61 | 146.71 | -4.57 | 33.36 | 68.53 | 262.40 | 0.9369 | 313.1 | 255.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.98 | 83.56 | 3.00 | 120.30 | -4.35 | 34.97 | 70.13 | 262.91 | 0.9464 | -17.5 | 414.4 | |
| 0.00 | 0.81 | 0.00 | 1.23 | -5.74 | 34.77 | 69.93 | 261.42 | 0.9466 | 35.0 | 13.7 | |
| 0.00 | 0.27 | 0.00 | 0.41 | -5.26 | 34.64 | 69.81 | 261.90 | 0.9454 | 149.0 | 81.7 | |
| 0.00 | 0.63 | 0.00 | 0.93 | -5.08 | 34.42 | 69.58 | 262.05 | 0.9440 | 157.0 | 100.6 | |
| 0.00 | 0.27 | 0.00 | 0.42 | -7.54 | 35.08 | 70.24 | 259.60 | 0.9499 | 101.0 | 166.3 | |
| 18.51 | -1.00 | 26.84 | -1.00 | -4.66 | 33.97 | 69.14 | 262.42 | 0.9410 | 555.2 | 999999 | |
| 0.63 | 2.16 | 0.81 | 2.77 | -4.36 | 31.38 | 66.55 | 262.28 | 0.9247 | -145.7 | -122.6 | |
| 0.00 | 0.99 | 0.00 | 1.25 | -4.18 | 30.89 | 66.06 | 262.39 | 0.9213 | -314.0 | -289.2 | |
| 0.00 | 1.26 | 0.00 | 1.51 | -4.05 | 29.68 | 64.85 | 262.32 | 0.9128 | -305.0 | -235.1 | |
| 0.00 | 10.87 | 0.00 | 12.82 | -3.75 | 29.21 | 64.38 | 262.56 | 0.9091 | -650.0 | -468.1 | |
| 0.81 | 2.16 | 0.96 | 2.55 | -4.24 | 29.21 | 64.38 | 262.02 | 0.9097 | -413.9 | -360.5 | |
| 0.00 | 1.89 | 0.00 | 2.24 | -5.58 | 29.03 | 64.19 | 260.54 | 0.9101 | -459.0 | -314.2 | |
| 0.00 | 0.27 | 0.00 | 0.28 | -7.11 | 24.93 | 60.09 | 257.98 | 0.8814 | -334.0 | -277.7 | |
| 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. | |