SDO HMI 2014-09-09 23:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.67 | 58.97 | 20.47 | 40.90 | 9.74 | 147.33 | 44.85 | 276.51 | 0.7016 | 31.4 | -27.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.87 | 4.99 | 1.38 | 3.69 | 9.72 | 150.94 | 48.46 | 276.56 | 0.7449 | -613.4 | -509.4 | |
| 0.00 | 0.80 | 0.00 | 0.59 | 10.15 | 150.84 | 48.36 | 277.14 | 0.7437 | -528.0 | -425.0 | |
| 0.00 | 0.80 | 0.00 | 0.59 | 11.04 | 150.43 | 47.95 | 278.35 | 0.7389 | -430.0 | -388.0 | |
| 0.00 | 0.80 | 0.00 | 0.58 | 11.36 | 149.63 | 47.15 | 278.79 | 0.7296 | 462.0 | 419.9 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 11.25 | 149.55 | 47.08 | 278.64 | 0.7287 | 370.0 | 266.0 | |
| 0.00 | 1.60 | 0.00 | 1.14 | 10.20 | 148.67 | 46.19 | 277.19 | 0.7182 | -385.0 | -261.6 | |
| 0.00 | 0.89 | 0.00 | 0.63 | 10.30 | 148.60 | 46.12 | 277.32 | 0.7173 | -90.0 | -168.6 | |
| 6.59 | 19.87 | 4.65 | 14.00 | 10.13 | 148.39 | 45.91 | 277.09 | 0.7148 | -683.5 | -537.7 | |
| 2.85 | -8.00 | 2.01 | -8.00 | 10.30 | 148.24 | 45.76 | 277.33 | 0.7131 | -703.8 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.50 | 9.77 | 148.01 | 45.54 | 276.58 | 0.7103 | -563.0 | -511.0 | |
| 2.41 | -8.00 | 1.69 | -8.00 | 10.20 | 148.05 | 45.57 | 277.18 | 0.7107 | -888.0 | 999999 | |
| 12.56 | 26.37 | 8.47 | 17.75 | 9.28 | 145.61 | 43.13 | 275.84 | 0.6806 | 699.2 | 543.0 | |
| 3.39 | -12.00 | 2.27 | -12.00 | 9.17 | 145.22 | 42.74 | 275.66 | 0.6756 | 846.1 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.71 | 8.91 | 144.97 | 42.49 | 275.28 | 0.6725 | 670.0 | 545.0 | |
| 0.00 | 0.80 | 0.00 | 0.53 | 9.20 | 144.85 | 42.37 | 275.70 | 0.6708 | 518.0 | 552.1 | |
| 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. | |