SDO HMI 2014-08-21 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.30 | 36.45 | 5.37 | 29.59 | 15.35 | 53.91 | 52.72 | 284.18 | 0.7919 | 54.0 | -0.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.05 | 6.03 | 3.66 | 5.45 | 14.72 | 58.58 | 57.39 | 283.10 | 0.8386 | -632.3 | -451.1 | |
| 0.00 | 1.89 | 0.00 | 1.70 | 14.27 | 58.40 | 57.21 | 282.57 | 0.8368 | -598.0 | -506.6 | |
| 0.00 | 2.34 | 0.00 | 2.09 | 14.12 | 58.10 | 56.91 | 282.39 | 0.8341 | -37.0 | -91.8 | |
| 0.00 | 1.17 | 0.00 | 0.97 | 14.03 | 55.18 | 53.99 | 282.37 | 0.8057 | 332.0 | 261.5 | |
| 0.00 | 1.44 | 0.00 | 1.20 | 15.27 | 55.26 | 54.07 | 283.90 | 0.8069 | -501.0 | -379.8 | |
| 0.00 | 0.81 | 0.00 | 0.68 | 16.43 | 55.45 | 54.26 | 285.34 | 0.8095 | -473.0 | -443.1 | |
| 0.00 | 5.67 | 0.00 | 4.66 | 16.05 | 54.59 | 53.40 | 284.92 | 0.8007 | -783.0 | -677.5 | |
| 0.00 | 0.90 | 0.00 | 0.69 | 14.62 | 51.18 | 49.99 | 283.35 | 0.7640 | 501.0 | 471.7 | |
| 0.00 | 1.89 | 0.00 | 1.46 | 15.93 | 51.47 | 50.28 | 285.04 | 0.7681 | 442.0 | 337.6 | |
| 0.00 | 0.90 | 0.00 | 0.69 | 15.01 | 51.01 | 49.82 | 283.87 | 0.7624 | 573.0 | 525.6 | |
| 1.26 | 3.33 | 0.97 | 2.55 | 15.80 | 51.22 | 50.04 | 284.88 | 0.7654 | 704.5 | 497.5 | |
| 0.00 | 1.08 | 0.00 | 0.82 | 15.12 | 50.80 | 49.62 | 284.04 | 0.7602 | 427.0 | 441.2 | |
| 0.00 | 0.72 | 0.00 | 0.54 | 15.01 | 50.38 | 49.19 | 283.92 | 0.7555 | 473.0 | 508.8 | |
| 0.00 | 1.08 | 0.00 | 0.81 | 14.54 | 50.00 | 48.81 | 283.34 | 0.7509 | 629.0 | 575.2 | |
| 0.00 | 0.90 | 0.00 | 0.67 | 15.04 | 49.96 | 48.77 | 284.01 | 0.7508 | 330.0 | 378.1 | |
| 0.00 | 0.63 | 0.00 | 0.47 | 16.55 | 50.16 | 48.97 | 285.99 | 0.7545 | 396.0 | 372.7 | |
| 0.99 | 4.59 | 0.74 | 3.42 | 16.19 | 49.61 | 48.42 | 285.58 | 0.7480 | 713.6 | 638.5 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 17.70 | 42.81 | 41.62 | 288.86 | 0.6710 | 492.0 | 400.0 | |
| 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. | |