SDO HMI 2011-11-28 11:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.84 | 155.98 | 16.95 | 88.52 | 17.75 | 223.69 | 24.51 | 305.89 | 0.4898 | -596.9 | -357.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.48 | 11.37 | 225.34 | 26.16 | 292.38 | 0.4694 | 665.0 | 509.7 | |
| 0.00 | 1.71 | 0.00 | 0.98 | 16.59 | 225.72 | 26.53 | 301.93 | 0.5065 | 764.0 | 538.3 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 17.16 | 224.36 | 25.17 | 304.19 | 0.4934 | -187.0 | -196.3 | |
| 10.26 | 135.19 | 5.85 | 76.84 | 17.74 | 224.27 | 25.09 | 305.30 | 0.4968 | -985.7 | -441.2 | |
| 0.00 | 2.05 | 0.00 | 1.16 | 17.35 | 223.94 | 24.76 | 304.93 | 0.4896 | -638.0 | -556.5 | |
| 19.24 | -4.00 | 10.91 | -4.00 | 18.03 | 223.49 | 24.31 | 306.58 | 0.4895 | -1167.0 | 999999 | |
| 0.00 | 2.74 | 0.00 | 1.53 | 15.79 | 222.99 | 23.80 | 303.07 | 0.4653 | 249.0 | 66.8 | |
| 0.00 | 1.97 | 0.00 | 1.10 | 15.58 | 222.89 | 23.71 | 302.76 | 0.4625 | 524.0 | 445.2 | |
| 0.00 | 5.81 | 0.00 | 3.25 | 16.25 | 222.77 | 23.59 | 304.15 | 0.4662 | 213.0 | 102.9 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 15.33 | 222.53 | 23.34 | 302.67 | 0.4559 | 929.0 | 829.4 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 15.65 | 221.83 | 22.65 | 304.02 | 0.4492 | 829.0 | 732.4 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 20.31 | 222.44 | 23.26 | 311.55 | 0.4969 | -570.0 | -402.9 | |
| 0.34 | 1.37 | 0.19 | 0.77 | 19.97 | 221.60 | 22.42 | 311.98 | 0.4842 | -808.5 | -664.1 | |
| 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. | |