SDO HMI 2014-08-14 10:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.21 | 349.23 | 42.52 | 225.96 | 14.66 | 133.03 | 39.87 | 284.88 | 0.6436 | -479.6 | -242.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.34 | 301.64 | 32.42 | 198.02 | 15.33 | 134.10 | 40.93 | 285.81 | 0.6590 | -1212.4 | -347.2 | |
| 3.52 | -1.00 | 2.29 | -1.00 | 14.93 | 133.67 | 40.51 | 285.28 | 0.6529 | -1025.2 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.09 | 10.94 | 128.28 | 35.12 | 279.67 | 0.5751 | 620.0 | 408.3 | |
| 0.00 | 1.98 | 0.00 | 1.20 | 12.70 | 127.97 | 34.81 | 282.79 | 0.5732 | 731.0 | 589.8 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 9.85 | 126.64 | 33.48 | 277.91 | 0.5508 | 512.0 | 485.9 | |
| 0.00 | 1.53 | 0.00 | 0.91 | 9.87 | 126.35 | 33.19 | 277.97 | 0.5466 | 693.0 | 522.5 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 9.33 | 126.21 | 33.05 | 276.99 | 0.5443 | 680.0 | 510.0 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 9.62 | 125.99 | 32.83 | 277.54 | 0.5412 | 587.0 | 610.9 | |
| 0.63 | 1.44 | 0.37 | 0.84 | 9.58 | 125.51 | 32.35 | 277.53 | 0.5342 | 907.4 | 775.8 | |
| 0.63 | 28.14 | 0.37 | 16.48 | 10.65 | 125.63 | 32.47 | 279.50 | 0.5370 | 721.7 | 654.7 | |
| 12.09 | -10.00 | 7.07 | -10.00 | 10.07 | 125.49 | 32.33 | 278.45 | 0.5344 | 991.0 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.74 | 9.44 | 125.34 | 32.18 | 277.27 | 0.5318 | 742.0 | 645.5 | |
| 0.00 | 6.22 | 0.00 | 3.62 | 9.22 | 124.99 | 31.83 | 276.88 | 0.5265 | 881.0 | 660.4 | |
| 0.00 | 1.44 | 0.00 | 0.84 | 10.71 | 125.16 | 32.00 | 279.68 | 0.5303 | 760.0 | 610.8 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 11.34 | 123.71 | 30.55 | 281.17 | 0.5100 | 63.0 | 141.7 | |
| 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. | |