| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.86 | 510.49 | 39.95 | 284.17 | -20.90 | 17.31 | 3.00 | 186.18 | 0.4569 | 922.0 | 354.5 | |
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back to the solar disc SDO HMI 2014-10-13 22:00:31 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.66 | 0.00 | 0.91 | -18.07 | 20.87 | 6.56 | 194.95 | 0.4230 | 948.0 | 789.5 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -21.79 | 20.25 | 5.94 | 191.66 | 0.4772 | -732.0 | -545.1 | |
| 0.00 | 2.54 | 0.00 | 1.43 | -21.82 | 19.83 | 5.52 | 190.85 | 0.4764 | -655.0 | -623.3 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -19.47 | 19.49 | 5.18 | 191.21 | 0.4396 | 724.0 | 573.8 | |
| 0.00 | 1.31 | 0.00 | 0.71 | -18.15 | 19.20 | 4.89 | 191.21 | 0.4182 | 901.0 | 723.6 | |
| 19.85 | 488.81 | 11.05 | 272.00 | -20.93 | 17.84 | 3.53 | 187.24 | 0.4579 | 1342.9 | 385.8 | |
| 50.97 | -6.00 | 28.33 | -6.00 | -20.85 | 17.23 | 2.92 | 186.01 | 0.4557 | 1417.5 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -25.10 | 17.08 | 2.77 | 184.85 | 0.5200 | 609.0 | 434.5 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -23.91 | 16.01 | 1.70 | 183.12 | 0.5010 | 464.0 | 395.1 | |
| 0.52 | 1.84 | 0.28 | 1.00 | -18.03 | 15.89 | 1.58 | 183.68 | 0.4094 | -916.0 | -785.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -18.03 | 15.60 | 1.30 | 183.02 | 0.4092 | -787.0 | -690.2 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -19.91 | 13.80 | -0.51 | 178.91 | 0.4385 | -727.0 | -584.3 | |
| 0.52 | 3.23 | 0.29 | 1.80 | -21.08 | 12.87 | -1.44 | 177.05 | 0.4574 | -920.0 | -823.5 | |
| 0.00 | 1.84 | 0.00 | 1.07 | -25.41 | 11.13 | -3.18 | 174.50 | 0.5252 | -769.0 | -533.4 | |
| 0.00 | 1.31 | 0.00 | 0.73 | -20.89 | 10.28 | -4.03 | 171.72 | 0.4583 | -610.0 | -474.1 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -25.59 | 9.79 | -4.52 | 172.27 | 0.5302 | -799.0 | -505.8 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -27.78 | 7.49 | -6.82 | 169.29 | 0.5672 | -541.0 | -492.4 | |
| 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. | |