SDO HMI 2011-11-28 12:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.51 | 98.15 | 33.50 | 134.84 | 7.64 | 129.76 | -68.88 | 82.29 | 0.9340 | -111.6 | -131.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.09 | 64.38 | 13.04 | 83.09 | 7.54 | 131.20 | -67.43 | 82.35 | 0.9253 | -594.7 | -271.0 | |
| 1.71 | -1.00 | 2.24 | -1.00 | 7.51 | 130.90 | -67.74 | 82.40 | 0.9273 | 175.9 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.98 | 7.28 | 130.00 | -68.64 | 82.67 | 0.9330 | -387.0 | -240.6 | |
| 0.00 | 1.80 | 0.00 | 2.40 | 5.62 | 130.40 | -68.24 | 84.45 | 0.9303 | -321.0 | -373.0 | |
| 0.00 | 1.03 | 0.00 | 1.44 | 7.18 | 129.36 | -69.28 | 82.80 | 0.9369 | -275.0 | -219.3 | |
| 1.03 | 2.48 | 1.48 | 3.56 | 7.80 | 128.79 | -69.85 | 82.15 | 0.9404 | -71.7 | -3.5 | |
| 2.31 | 3.76 | 3.28 | 5.36 | 6.93 | 129.01 | -69.63 | 83.07 | 0.9390 | -222.7 | -9.7 | |
| 0.94 | 1.88 | 1.39 | 2.77 | 8.11 | 128.31 | -70.33 | 81.83 | 0.9433 | -75.9 | 28.5 | |
| 0.85 | 1.62 | 1.25 | 2.36 | 7.34 | 128.52 | -70.12 | 82.64 | 0.9419 | 127.8 | 54.3 | |
| 0.00 | 1.03 | 0.00 | 1.52 | 7.58 | 128.25 | -70.39 | 82.40 | 0.9435 | 457.0 | 413.3 | |
| 0.85 | 5.64 | 1.30 | 8.55 | 8.58 | 127.75 | -70.89 | 81.35 | 0.9465 | 449.6 | 423.7 | |
| 3.59 | 7.27 | 5.89 | 11.91 | 8.19 | 126.18 | -72.45 | 81.80 | 0.9548 | 492.8 | 397.5 | |
| 2.14 | 5.81 | 3.63 | 9.90 | 7.91 | 125.60 | -73.04 | 82.11 | 0.9578 | 274.4 | 85.2 | |
| 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. | |