SDO HMI 2014-11-27 19:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.36 | 385.55 | 41.85 | 233.55 | 16.12 | 110.31 | -32.32 | 63.23 | 0.5771 | -930.3 | -296.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.39 | 368.77 | 40.66 | 222.57 | 16.09 | 110.63 | -32.00 | 63.11 | 0.5730 | -1355.5 | -343.4 | |
| 1.97 | -1.00 | 1.19 | -1.00 | 16.64 | 110.31 | -32.32 | 62.43 | 0.5801 | -743.4 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 16.52 | 107.88 | -34.74 | 64.04 | 0.6099 | -550.0 | -408.3 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 16.85 | 107.17 | -35.45 | 63.93 | 0.6203 | 176.0 | 289.9 | |
| 0.00 | 1.97 | 0.00 | 1.24 | 16.63 | 107.03 | -35.60 | 64.33 | 0.6211 | 801.0 | 698.8 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 16.24 | 105.34 | -37.28 | 65.76 | 0.6401 | 832.0 | 677.5 | |
| 0.00 | 1.45 | 0.00 | 0.95 | 16.85 | 104.74 | -37.89 | 65.15 | 0.6501 | 616.0 | 528.4 | |
| 0.00 | 1.11 | 0.00 | 0.73 | 16.63 | 104.32 | -38.31 | 65.66 | 0.6542 | 534.0 | 396.3 | |
| 0.00 | 2.48 | 0.00 | 1.64 | 16.83 | 103.55 | -39.07 | 65.71 | 0.6642 | 546.0 | 511.0 | |
| 0.00 | 0.86 | 0.00 | 0.57 | 16.45 | 102.64 | -39.98 | 66.64 | 0.6736 | 572.0 | 555.5 | |
| 0.00 | 0.94 | 0.00 | 0.63 | 16.36 | 102.67 | -39.96 | 66.76 | 0.6730 | 751.0 | 601.0 | |
| 0.00 | 0.86 | 0.00 | 0.57 | 16.57 | 102.33 | -40.29 | 66.60 | 0.6777 | 501.0 | 402.1 | |
| 0.00 | 1.20 | 0.00 | 0.81 | 15.77 | 101.84 | -40.79 | 67.94 | 0.6807 | 691.0 | 569.2 | |
| 0.00 | 2.57 | 0.00 | 1.73 | 15.61 | 101.63 | -40.99 | 68.24 | 0.6826 | 432.0 | 404.4 | |
| 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. | |