SDO HMI 2014-10-05 12:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.83 | 233.91 | 22.15 | 123.83 | -13.64 | 121.37 | -4.00 | 169.00 | 0.3534 | 440.0 | 253.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.43 | 186.74 | 17.13 | 98.65 | -13.59 | 122.32 | -3.05 | 171.42 | 0.3485 | 1219.8 | 386.4 | |
| 0.00 | 1.05 | 0.00 | 0.54 | -9.08 | 121.82 | -3.55 | 167.17 | 0.2763 | 804.0 | 593.3 | |
| 0.00 | 1.76 | 0.00 | 0.93 | -13.69 | 120.67 | -4.69 | 167.01 | 0.3552 | 834.0 | 675.8 | |
| 0.00 | 2.72 | 0.00 | 1.44 | -13.41 | 120.40 | -4.96 | 166.09 | 0.3517 | 1028.0 | 770.8 | |
| 0.00 | 3.34 | 0.00 | 1.76 | -13.12 | 120.22 | -5.14 | 165.40 | 0.3479 | 978.0 | 788.3 | |
| 2.02 | 4.22 | 1.08 | 2.25 | -14.47 | 120.01 | -5.36 | 165.78 | 0.3700 | 845.2 | 664.3 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -12.41 | 118.85 | -6.52 | 161.07 | 0.3431 | 910.0 | 746.8 | |
| 0.00 | 1.49 | 0.00 | 0.81 | -15.73 | 117.34 | -8.03 | 160.37 | 0.4020 | -731.0 | -617.5 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -15.63 | 117.28 | -8.09 | 160.15 | 0.4009 | -912.0 | -641.8 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -14.96 | 116.99 | -8.38 | 158.89 | 0.3923 | -888.0 | -711.9 | |
| 1.49 | 9.05 | 0.80 | 4.82 | -13.42 | 116.99 | -8.38 | 157.33 | 0.3693 | -1075.3 | -837.7 | |
| 0.00 | 1.76 | 0.00 | 0.93 | -13.10 | 116.88 | -8.49 | 156.71 | 0.3653 | -1036.0 | -882.9 | |
| 5.89 | 8.52 | 3.14 | 4.55 | -13.39 | 116.52 | -8.85 | 156.18 | 0.3719 | -989.9 | -745.1 | |
| 0.00 | 5.18 | 0.00 | 2.78 | -14.17 | 115.80 | -9.57 | 155.37 | 0.3882 | -894.0 | -746.9 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -15.30 | 115.75 | -9.62 | 156.45 | 0.4050 | -964.0 | -784.5 | |
| 0.00 | 2.11 | 0.00 | 1.15 | -15.76 | 115.60 | -9.77 | 156.59 | 0.4126 | -672.0 | -614.0 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -15.63 | 115.55 | -9.82 | 156.34 | 0.4111 | -832.0 | -639.6 | |
| 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. | |