SDO HMI 2011-10-14 06:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.44 | 98.29 | 12.97 | 54.35 | 19.86 | 98.18 | 22.93 | 304.18 | 0.4448 | -297.3 | -252.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.27 | 5.60 | 1.27 | 3.12 | 20.19 | 99.44 | 24.19 | 303.49 | 0.4630 | -762.5 | -619.4 | |
| 9.97 | 59.82 | 5.54 | 33.22 | 19.52 | 99.09 | 23.84 | 302.53 | 0.4537 | -1079.7 | -393.6 | |
| 0.00 | 2.10 | 0.00 | 1.17 | 20.08 | 99.00 | 23.75 | 303.71 | 0.4566 | -802.0 | -721.0 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 19.93 | 98.84 | 23.59 | 303.58 | 0.4534 | -853.0 | -709.9 | |
| 4.64 | -2.00 | 2.57 | -2.00 | 19.54 | 98.74 | 23.49 | 302.89 | 0.4493 | -1042.3 | 999999 | |
| 0.00 | 2.62 | 0.00 | 1.45 | 19.83 | 98.34 | 23.09 | 303.88 | 0.4462 | -980.0 | -851.3 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 19.48 | 97.91 | 22.65 | 303.61 | 0.4379 | -748.0 | -623.2 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 18.48 | 97.32 | 22.07 | 302.17 | 0.4228 | 626.0 | 478.9 | |
| 0.00 | 4.02 | 0.00 | 2.20 | 19.77 | 96.71 | 21.46 | 305.49 | 0.4247 | -719.0 | -661.2 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 21.15 | 96.30 | 21.05 | 308.72 | 0.4311 | 405.0 | 388.3 | |
| 6.56 | 13.12 | 3.59 | 7.18 | 21.03 | 96.04 | 20.79 | 308.81 | 0.4269 | 949.3 | 607.7 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 20.38 | 95.95 | 20.70 | 307.64 | 0.4201 | 776.0 | 637.8 | |
| 0.00 | 2.45 | 0.00 | 1.32 | 20.40 | 94.62 | 19.37 | 309.35 | 0.4038 | 1087.0 | 888.4 | |
| 0.00 | 2.27 | 0.00 | 1.23 | 20.66 | 94.19 | 18.93 | 310.48 | 0.4009 | 600.0 | 417.2 | |
| 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. | |