SDO HMI 2014-09-10 13:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.26 | 52.64 | 18.41 | 42.16 | 9.65 | 147.13 | 52.34 | 276.61 | 0.7874 | 277.3 | -67.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.25 | 3.12 | 1.10 | 2.75 | 9.88 | 151.24 | 56.45 | 277.06 | 0.8294 | -463.9 | -307.1 | |
| 0.00 | 1.78 | 0.00 | 1.57 | 10.65 | 151.23 | 56.44 | 277.99 | 0.8291 | -538.0 | -413.4 | |
| 0.00 | 0.89 | 0.00 | 0.76 | 10.23 | 149.96 | 55.17 | 277.43 | 0.8168 | -132.0 | -176.9 | |
| 0.62 | 12.92 | 0.52 | 10.73 | 10.33 | 148.97 | 54.18 | 277.53 | 0.8068 | -311.9 | -568.2 | |
| 2.41 | -4.00 | 2.00 | -4.00 | 10.19 | 148.83 | 54.04 | 277.35 | 0.8054 | -619.6 | 999999 | |
| 1.87 | -4.00 | 1.56 | -4.00 | 10.40 | 148.88 | 54.09 | 277.61 | 0.8059 | -490.8 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.86 | 9.50 | 147.53 | 52.73 | 276.43 | 0.7921 | -609.0 | -580.6 | |
| 0.00 | 1.60 | 0.00 | 1.29 | 9.72 | 147.43 | 52.63 | 276.71 | 0.7910 | -650.0 | -615.6 | |
| 0.00 | 4.99 | 0.00 | 3.91 | 8.85 | 146.09 | 51.30 | 275.54 | 0.7770 | 524.0 | 366.7 | |
| 17.11 | 22.45 | 13.23 | 17.36 | 9.27 | 145.49 | 50.70 | 276.06 | 0.7703 | 720.4 | 465.1 | |
| 0.00 | 1.69 | 0.00 | 1.31 | 10.09 | 145.52 | 50.73 | 277.13 | 0.7704 | 522.0 | 459.8 | |
| 0.00 | 0.53 | 0.00 | 0.41 | 9.94 | 145.49 | 50.69 | 276.94 | 0.7701 | 576.0 | 505.0 | |
| 0.00 | 0.62 | 0.00 | 0.47 | 8.59 | 144.07 | 49.28 | 275.10 | 0.7547 | 527.0 | 523.3 | |
| 0.00 | 0.98 | 0.00 | 0.74 | 9.96 | 144.01 | 49.21 | 276.93 | 0.7535 | 528.0 | 466.0 | |
| 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. | |