SDO HMI 2014-08-11 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.45 | 84.99 | 19.63 | 157.31 | 13.99 | 55.09 | -75.53 | 77.21 | 0.9628 | -195.7 | 27.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.02 | 40.79 | 15.07 | 61.22 | 13.77 | 58.87 | -71.75 | 77.62 | 0.9458 | -455.0 | -250.5 | |
| 1.44 | 6.14 | 2.25 | 9.64 | 13.45 | 58.18 | -72.44 | 77.93 | 0.9496 | -304.6 | -182.7 | |
| 0.00 | 1.17 | 0.00 | 1.97 | 12.31 | 56.86 | -73.75 | 79.07 | 0.9566 | -264.0 | -371.4 | |
| 0.00 | 0.90 | 0.00 | 1.52 | 12.12 | 56.78 | -73.83 | 79.26 | 0.9571 | -337.0 | -331.6 | |
| 0.00 | 1.35 | 0.00 | 2.43 | 12.72 | 55.72 | -74.90 | 78.58 | 0.9620 | -156.0 | -89.7 | |
| 0.00 | 4.78 | 0.00 | 9.40 | 13.76 | 54.10 | -76.52 | 77.40 | 0.9689 | 361.0 | 283.8 | |
| 0.00 | 0.27 | 0.00 | 0.48 | 11.91 | 55.77 | -74.85 | 79.42 | 0.9620 | -65.0 | -78.7 | |
| 0.99 | 20.85 | 2.31 | 49.08 | 14.47 | 51.61 | -79.01 | 76.54 | 0.9783 | 253.5 | 265.5 | |
| 0.00 | 3.43 | 0.00 | 9.07 | 15.25 | 50.07 | -80.54 | 75.64 | 0.9832 | 76.0 | -47.7 | |
| 0.00 | 1.26 | 0.00 | 2.90 | 13.97 | 51.93 | -78.69 | 77.07 | 0.9773 | 452.0 | 469.5 | |
| 0.00 | 1.35 | 0.00 | 3.09 | 13.79 | 51.99 | -78.63 | 77.26 | 0.9771 | 418.0 | 385.5 | |
| 0.00 | 0.99 | 0.00 | 2.57 | 14.31 | 50.41 | -80.21 | 76.62 | 0.9824 | 80.0 | 70.6 | |
| 0.00 | 0.81 | 0.00 | 1.81 | 12.71 | 52.45 | -78.17 | 78.39 | 0.9757 | 326.0 | 339.6 | |
| 0.00 | 0.90 | 0.00 | 2.13 | 12.84 | 51.65 | -78.96 | 78.20 | 0.9786 | 70.0 | 86.3 | |
| 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. | |