SDO HMI 2014-10-04 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.64 | 374.14 | 39.36 | 200.17 | -1.38 | 154.82 | 20.67 | 249.67 | 0.3779 | 1037.5 | 373.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.61 | 321.06 | 31.40 | 172.11 | -1.40 | 155.11 | 20.96 | 249.93 | 0.3824 | 1405.9 | 374.3 | |
| 4.31 | 23.99 | 2.29 | 12.76 | -1.92 | 153.96 | 19.81 | 247.47 | 0.3683 | 960.0 | 605.6 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -2.83 | 153.88 | 19.73 | 245.14 | 0.3732 | -596.0 | -466.0 | |
| 2.90 | -2.00 | 1.54 | -2.00 | -1.74 | 153.84 | 19.68 | 247.80 | 0.3652 | 1174.8 | 999999 | |
| 1.58 | -2.00 | 0.84 | -2.00 | -1.70 | 153.68 | 19.52 | 247.72 | 0.3626 | 1148.8 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.79 | 0.02 | 153.67 | 19.52 | 252.23 | 0.3523 | 854.0 | 709.9 | |
| 0.00 | 3.69 | 0.00 | 1.96 | -1.06 | 153.64 | 19.49 | 249.32 | 0.3580 | 947.0 | 942.5 | |
| 6.24 | 12.83 | 3.29 | 6.77 | -0.23 | 153.16 | 19.01 | 251.06 | 0.3458 | 1065.7 | 753.4 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 1.65 | 152.98 | 18.83 | 256.19 | 0.3337 | 728.0 | 627.9 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -0.03 | 151.74 | 17.59 | 250.14 | 0.3227 | 660.0 | 640.1 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -1.48 | 150.18 | 16.02 | 243.89 | 0.3087 | -764.0 | -651.7 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -2.36 | 150.12 | 15.97 | 241.32 | 0.3147 | -738.0 | -663.1 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -2.26 | 149.96 | 15.81 | 241.34 | 0.3117 | -875.0 | -830.2 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -1.53 | 149.87 | 15.71 | 243.28 | 0.3044 | -872.0 | -686.4 | |
| 0.00 | 3.16 | 0.00 | 1.64 | -1.77 | 149.74 | 15.59 | 242.40 | 0.3045 | -758.0 | -772.0 | |
| 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. | |