SDO HMI 2011-07-15 14:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.38 | 290.26 | 27.22 | 160.61 | 16.50 | 169.32 | -23.78 | 60.71 | 0.4448 | -757.4 | -349.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.60 | 20.02 | 173.12 | -19.97 | 49.44 | 0.4242 | -845.0 | -739.6 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 19.13 | 171.75 | -21.34 | 52.87 | 0.4330 | -590.0 | -482.7 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 15.63 | 172.11 | -20.98 | 59.80 | 0.4007 | -828.0 | -611.2 | |
| 49.38 | 276.10 | 27.22 | 152.29 | 16.28 | 169.57 | -23.53 | 60.93 | 0.4402 | -1186.4 | -380.3 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 18.47 | 168.52 | -24.57 | 57.55 | 0.4693 | -689.0 | -564.4 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 16.53 | 168.49 | -24.61 | 61.38 | 0.4566 | 163.0 | 117.7 | |
| 0.00 | 0.45 | 0.00 | 0.26 | 20.86 | 166.75 | -26.34 | 54.87 | 0.5090 | 603.0 | 517.2 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 22.18 | 165.05 | -28.05 | 54.15 | 0.5393 | 791.0 | 675.0 | |
| 0.00 | 1.18 | 0.00 | 0.71 | 22.72 | 163.11 | -29.99 | 54.83 | 0.5660 | 731.0 | 613.2 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 19.74 | 163.70 | -29.40 | 59.26 | 0.5396 | 611.0 | 504.7 | |
| 0.00 | 1.27 | 0.00 | 0.77 | 23.09 | 162.44 | -30.65 | 54.77 | 0.5763 | 630.0 | 464.8 | |
| 0.00 | 1.09 | 0.00 | 0.68 | 23.05 | 159.75 | -33.34 | 56.70 | 0.6073 | 551.0 | 454.5 | |
| 0.00 | 1.63 | 0.00 | 1.01 | 21.24 | 159.65 | -33.45 | 59.51 | 0.5983 | 97.0 | 188.5 | |
| 0.00 | 1.09 | 0.00 | 0.72 | 24.55 | 155.30 | -37.80 | 57.15 | 0.6659 | 607.0 | 556.3 | |
| 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. | |