SDO HMI 2014-11-01 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.73 | 101.49 | 17.17 | 51.79 | 12.72 | 114.89 | -11.05 | 51.64 | 0.2392 | -590.1 | -115.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.99 | 0.00 | 1.01 | 12.31 | 116.03 | -9.91 | 50.24 | 0.2197 | -103.0 | -159.1 | |
| 24.40 | 63.41 | 12.41 | 32.29 | 12.79 | 115.64 | -10.30 | 49.64 | 0.2298 | -1338.0 | -463.0 | |
| 1.90 | -2.00 | 0.97 | -2.00 | 13.15 | 115.63 | -10.31 | 48.47 | 0.2339 | -1036.7 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 11.85 | 115.27 | -10.66 | 53.89 | 0.2252 | 577.0 | 476.3 | |
| 1.56 | -2.00 | 0.79 | -2.00 | 13.11 | 115.01 | -10.93 | 50.20 | 0.2415 | -668.9 | 999999 | |
| 1.38 | 5.36 | 0.70 | 2.73 | 11.88 | 114.99 | -10.94 | 54.48 | 0.2293 | -848.8 | -584.6 | |
| 1.12 | 3.20 | 0.58 | 1.64 | 13.28 | 114.44 | -11.50 | 51.02 | 0.2508 | -1029.3 | -833.3 | |
| 0.69 | 6.32 | 0.35 | 3.22 | 11.93 | 114.22 | -11.72 | 56.07 | 0.2406 | 1004.5 | 261.6 | |
| 2.25 | 3.55 | 1.15 | 1.82 | 13.24 | 113.41 | -12.53 | 53.45 | 0.2641 | -636.2 | -358.3 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 11.86 | 113.44 | -12.49 | 57.93 | 0.2510 | 932.0 | 710.8 | |
| 0.00 | 5.28 | 0.00 | 2.71 | 12.87 | 113.24 | -12.70 | 54.95 | 0.2629 | 838.0 | 598.2 | |
| 0.00 | 7.53 | 0.00 | 3.87 | 12.66 | 112.78 | -13.16 | 56.56 | 0.2674 | 878.0 | 710.6 | |
| 0.43 | 3.03 | 0.22 | 1.57 | 12.82 | 111.45 | -14.48 | 58.44 | 0.2875 | 1081.4 | 864.4 | |
| 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. | |