SDO HMI 2014-08-06 18:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.52 | 22.55 | 3.22 | 16.06 | -21.05 | 157.08 | -37.44 | 127.63 | 0.7177 | 200.6 | 121.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.68 | -17.52 | 164.85 | -29.67 | 129.43 | 0.6133 | 521.0 | 583.2 | |
| 0.00 | 1.63 | 0.00 | 1.13 | -22.77 | 160.06 | -34.45 | 131.79 | 0.7019 | 700.0 | 591.2 | |
| 0.00 | 0.90 | 0.00 | 0.63 | -21.49 | 158.58 | -35.93 | 129.18 | 0.7067 | 430.0 | 370.0 | |
| 3.07 | 6.41 | 2.15 | 4.50 | -21.12 | 157.96 | -36.56 | 128.29 | 0.7101 | 749.6 | 542.9 | |
| 0.00 | 1.17 | 0.00 | 0.79 | -17.58 | 158.84 | -35.68 | 124.58 | 0.6776 | 682.0 | 474.7 | |
| 0.00 | 0.36 | 0.00 | 0.25 | -19.99 | 158.19 | -36.32 | 127.10 | 0.7002 | 462.0 | 442.0 | |
| 0.00 | 0.99 | 0.00 | 0.71 | -21.36 | 156.94 | -37.57 | 127.85 | 0.7214 | 404.0 | 343.9 | |
| 0.00 | 1.26 | 0.00 | 0.90 | -20.75 | 156.96 | -37.55 | 127.14 | 0.7173 | 519.0 | 475.6 | |
| 0.00 | 0.90 | 0.00 | 0.65 | -20.77 | 156.13 | -38.39 | 126.60 | 0.7255 | 461.0 | 345.1 | |
| 0.00 | 0.63 | 0.00 | 0.47 | -22.41 | 155.14 | -39.38 | 127.84 | 0.7450 | -428.0 | -492.0 | |
| 0.00 | 1.26 | 0.00 | 0.94 | -22.35 | 154.99 | -39.53 | 127.67 | 0.7460 | -444.0 | -368.5 | |
| 0.00 | 1.08 | 0.00 | 0.81 | -21.91 | 154.49 | -40.02 | 126.85 | 0.7478 | -507.0 | -395.0 | |
| 0.00 | 0.63 | 0.00 | 0.47 | -21.47 | 154.47 | -40.04 | 126.32 | 0.7454 | -618.0 | -534.3 | |
| 1.45 | 4.25 | 1.07 | 3.13 | -21.16 | 154.44 | -40.07 | 125.95 | 0.7439 | -691.4 | -604.7 | |
| 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. | |