SDO HMI 2014-08-18 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.18 | 54.75 | 4.69 | 28.05 | -4.62 | 31.24 | -9.05 | 141.91 | 0.2533 | 423.0 | 541.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.95 | 33.33 | 2.52 | 16.98 | -4.27 | 32.64 | -7.65 | 145.15 | 0.2334 | 1111.9 | 770.2 | |
| 1.53 | -1.00 | 0.78 | -1.00 | -4.40 | 32.30 | -7.99 | 144.29 | 0.2385 | 923.7 | 999999 | |
| 1.08 | -1.00 | 0.55 | -1.00 | -4.22 | 32.24 | -8.05 | 143.63 | 0.2366 | 1066.8 | 999999 | |
| 0.00 | 5.22 | 0.00 | 2.67 | -4.35 | 31.93 | -8.36 | 142.91 | 0.2415 | 736.0 | 686.4 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -3.75 | 30.70 | -9.58 | 137.47 | 0.2469 | 973.0 | 757.8 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -4.65 | 30.66 | -9.63 | 139.69 | 0.2588 | 939.0 | 782.5 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -4.09 | 30.64 | -9.65 | 138.19 | 0.2519 | 841.0 | 710.8 | |
| 0.00 | 2.16 | 0.00 | 1.11 | -4.81 | 30.41 | -9.88 | 139.36 | 0.2636 | 735.0 | 624.6 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -4.03 | 30.42 | -9.87 | 137.40 | 0.2537 | 962.0 | 687.3 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -3.85 | 30.05 | -10.23 | 135.86 | 0.2557 | 864.0 | 714.4 | |
| 1.62 | 3.60 | 0.84 | 1.86 | -5.73 | 29.06 | -11.23 | 137.91 | 0.2903 | -942.4 | -721.8 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -4.43 | 29.02 | -11.27 | 134.62 | 0.2749 | -854.0 | -683.4 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -13.40 | 24.13 | -16.16 | 141.51 | 0.4369 | -744.0 | -510.7 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -1.78 | 23.58 | -16.71 | 116.60 | 0.3228 | -636.0 | -477.8 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -5.66 | 21.28 | -19.01 | 122.83 | 0.3873 | -496.0 | -422.8 | |
| 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. | |