SDO HMI 2011-10-10 23:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.62 | 170.15 | 21.24 | 106.77 | 23.43 | 153.66 | 34.99 | 300.97 | 0.6156 | -441.5 | -275.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.23 | 152.55 | 5.21 | 96.30 | 23.00 | 154.68 | 36.01 | 299.65 | 0.6251 | -763.5 | -377.4 | |
| 0.61 | -1.00 | 0.39 | -1.00 | 22.57 | 154.51 | 35.84 | 299.09 | 0.6210 | -568.9 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.69 | 26.57 | 155.75 | 37.08 | 304.29 | 0.6550 | -628.0 | -496.2 | |
| 24.78 | -1.00 | 15.64 | -1.00 | 23.25 | 154.28 | 35.61 | 300.23 | 0.6214 | -1088.4 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.79 | 25.04 | 149.50 | 30.83 | 305.95 | 0.5758 | 663.0 | 553.9 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 25.28 | 148.49 | 29.82 | 307.09 | 0.5659 | 641.0 | 503.3 | |
| 0.00 | 2.28 | 0.00 | 1.37 | 25.67 | 148.33 | 29.66 | 307.82 | 0.5668 | 552.0 | 486.4 | |
| 0.00 | 0.61 | 0.00 | 0.36 | 23.51 | 147.77 | 29.10 | 304.81 | 0.5454 | 627.0 | 555.4 | |
| 0.00 | 1.23 | 0.00 | 0.73 | 25.95 | 147.95 | 29.28 | 308.55 | 0.5644 | 515.0 | 443.6 | |
| 0.00 | 1.23 | 0.00 | 0.74 | 26.79 | 147.91 | 29.24 | 309.85 | 0.5702 | 616.0 | 460.3 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 26.20 | 146.01 | 27.34 | 310.58 | 0.5447 | 719.0 | 577.5 | |
| 0.00 | 3.15 | 0.00 | 1.85 | 26.78 | 145.25 | 26.58 | 312.17 | 0.5411 | 716.0 | 491.8 | |
| 0.00 | 1.93 | 0.00 | 1.13 | 26.77 | 144.95 | 26.28 | 312.43 | 0.5377 | 700.0 | 527.0 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 26.30 | 144.65 | 25.98 | 311.99 | 0.5304 | 790.0 | 631.5 | |
| 0.00 | 1.40 | 0.00 | 0.79 | 23.91 | 141.66 | 22.99 | 311.16 | 0.4763 | 761.0 | 542.9 | |
| 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. | |