SDO HMI 2011-07-01 11:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.08 | 42.07 | 8.19 | 21.45 | 15.87 | 23.61 | 3.57 | 344.26 | 0.2387 | 129.1 | 95.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.72 | 10.45 | 3.41 | 5.30 | 13.43 | 26.65 | 6.61 | 328.59 | 0.2159 | 1072.2 | 721.1 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 14.14 | 26.01 | 5.97 | 332.73 | 0.2211 | 697.0 | 549.4 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 15.68 | 25.13 | 5.09 | 338.92 | 0.2387 | -1005.0 | -786.1 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 16.08 | 25.14 | 5.10 | 339.50 | 0.2452 | -787.0 | -668.8 | |
| 1.82 | 3.63 | 0.93 | 1.86 | 16.34 | 24.99 | 4.95 | 340.43 | 0.2483 | -913.7 | -569.7 | |
| 1.91 | 2.73 | 0.97 | 1.39 | 15.52 | 24.46 | 4.42 | 341.27 | 0.2324 | -922.4 | -854.8 | |
| 0.00 | 2.00 | 0.00 | 1.01 | 14.50 | 24.37 | 4.34 | 340.04 | 0.2154 | -964.0 | -700.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.77 | 24.37 | 4.33 | 341.97 | 0.2359 | -925.0 | -690.8 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 16.53 | 23.59 | 3.55 | 345.88 | 0.2446 | -1000.0 | -702.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 18.33 | 21.44 | 1.41 | 355.01 | 0.2687 | -728.0 | -571.8 | |
| 0.00 | 1.64 | 0.00 | 0.84 | 17.42 | 21.28 | 1.24 | 355.31 | 0.2530 | 851.0 | 670.2 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 17.99 | 21.22 | 1.18 | 355.71 | 0.2625 | 469.0 | 256.5 | |
| 5.63 | 10.26 | 2.88 | 5.25 | 17.32 | 20.77 | 0.73 | 357.22 | 0.2509 | 1069.0 | 757.7 | |
| 0.00 | 3.00 | 0.00 | 1.54 | 17.73 | 20.54 | 0.50 | 358.13 | 0.2577 | 750.0 | 586.5 | |
| 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. | |