SDO HMI 2014-10-14 18:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.13 | 458.15 | 41.91 | 262.70 | -21.01 | 17.14 | 13.81 | 206.35 | 0.5043 | 1037.0 | 374.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.49 | 0.00 | 0.84 | -17.98 | 20.14 | 16.81 | 214.46 | 0.4882 | 878.0 | 723.2 | |
| 0.00 | 1.75 | 0.00 | 0.99 | -19.12 | 18.87 | 15.54 | 211.10 | 0.4921 | 787.0 | 621.8 | |
| 0.00 | 0.87 | 0.00 | 0.50 | -18.96 | 18.79 | 15.46 | 211.16 | 0.4893 | 877.0 | 704.7 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -19.28 | 17.61 | 14.28 | 208.84 | 0.4846 | -510.0 | -307.0 | |
| 36.26 | 433.87 | 20.84 | 248.91 | -21.15 | 17.58 | 14.25 | 206.94 | 0.5090 | 1233.2 | 384.9 | |
| 0.00 | 1.31 | 0.00 | 0.74 | -18.88 | 17.15 | 13.82 | 208.49 | 0.4758 | 1077.0 | 924.2 | |
| 35.56 | -5.00 | 20.33 | -5.00 | -20.90 | 16.96 | 13.64 | 206.17 | 0.5015 | 1466.5 | 999999 | |
| 0.26 | -5.00 | 0.15 | -5.00 | -20.72 | 16.49 | 13.16 | 205.54 | 0.4959 | 1105.3 | 999999 | |
| 0.00 | 4.19 | 0.00 | 2.39 | -21.51 | 14.85 | 11.52 | 202.05 | 0.4969 | 877.0 | 655.5 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -18.71 | 14.48 | 11.15 | 203.83 | 0.4554 | -809.0 | -597.1 | |
| 0.00 | 4.98 | 0.00 | 2.82 | -20.90 | 14.28 | 10.95 | 201.55 | 0.4850 | 377.0 | 689.3 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -22.34 | 14.16 | 10.83 | 200.22 | 0.5047 | -790.0 | -548.5 | |
| 0.00 | 1.22 | 0.00 | 0.70 | -22.00 | 13.84 | 10.51 | 199.92 | 0.4982 | -862.0 | -706.4 | |
| 0.00 | 0.87 | 0.00 | 0.50 | -21.79 | 13.76 | 10.43 | 199.93 | 0.4949 | -688.0 | -637.5 | |
| 1.05 | 3.49 | 0.59 | 1.97 | -21.01 | 13.41 | 10.08 | 199.90 | 0.4820 | -964.2 | -730.9 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -27.64 | 6.57 | 3.24 | 185.17 | 0.5569 | -491.0 | -390.2 | |
| 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. | |