SDO HMI 2014-08-08 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.08 | 14.79 | 1.04 | 12.11 | -6.44 | 228.44 | 51.01 | 256.88 | 0.7904 | 203.6 | 228.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.63 | 0.00 | 0.61 | -7.77 | 235.15 | 57.73 | 257.10 | 0.8615 | 364.0 | 336.7 | |
| 1.08 | 2.98 | 1.04 | 2.87 | -7.80 | 234.87 | 57.45 | 256.99 | 0.8592 | 588.4 | 493.1 | |
| 0.00 | 1.26 | 0.00 | 1.21 | -7.93 | 234.56 | 57.14 | 256.77 | 0.8567 | 515.0 | 452.9 | |
| 0.00 | 0.27 | 0.00 | 0.22 | -5.28 | 229.05 | 51.63 | 258.50 | 0.7989 | 519.0 | 550.0 | |
| 0.00 | 0.81 | 0.00 | 0.66 | -5.26 | 228.75 | 51.33 | 258.45 | 0.7957 | 481.0 | 401.1 | |
| 0.00 | 0.45 | 0.00 | 0.36 | -6.52 | 227.93 | 50.51 | 256.67 | 0.7902 | 358.0 | 291.6 | |
| 0.00 | 1.90 | 0.00 | 1.52 | -5.92 | 227.81 | 50.38 | 257.38 | 0.7874 | 623.0 | 503.3 | |
| 0.00 | 0.90 | 0.00 | 0.73 | -8.23 | 227.86 | 50.44 | 254.55 | 0.7939 | 383.0 | 337.7 | |
| 0.00 | 1.08 | 0.00 | 0.85 | -7.32 | 226.33 | 48.91 | 255.20 | 0.7755 | 626.0 | 519.8 | |
| 0.00 | 0.54 | 0.00 | 0.42 | -7.62 | 226.29 | 48.86 | 254.80 | 0.7758 | 611.0 | 549.5 | |
| 0.00 | 0.90 | 0.00 | 0.62 | -4.49 | 220.13 | 42.71 | 256.88 | 0.6966 | -540.0 | -439.0 | |
| 0.00 | 0.63 | 0.00 | 0.42 | -3.91 | 218.65 | 41.23 | 257.18 | 0.6766 | -537.0 | -487.3 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -3.97 | 218.09 | 40.66 | 256.91 | 0.6697 | -660.0 | -505.7 | |
| 0.00 | 1.45 | 0.00 | 0.96 | -2.94 | 218.03 | 40.61 | 258.38 | 0.6660 | -496.0 | -510.0 | |
| 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. | |