SDO HMI 2011-10-18 03:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.65 | 184.13 | 14.27 | 111.13 | -26.91 | 36.07 | 11.94 | 199.02 | 0.5728 | 510.2 | 303.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.65 | 167.11 | 14.27 | 100.84 | -26.73 | 37.22 | 13.09 | 200.76 | 0.5728 | 1202.4 | 357.7 | |
| 0.00 | 3.23 | 0.00 | 1.84 | -22.47 | 33.77 | 9.64 | 198.22 | 0.4971 | 826.0 | 667.6 | |
| 0.00 | 0.44 | 0.00 | 0.26 | -27.41 | 32.50 | 8.37 | 193.34 | 0.5622 | 712.0 | 602.0 | |
| 0.00 | 0.87 | 0.00 | 0.53 | -29.12 | 30.46 | 6.34 | 189.60 | 0.5803 | 686.0 | 437.9 | |
| 0.00 | 1.66 | 0.00 | 1.00 | -28.46 | 29.71 | 5.58 | 188.67 | 0.5693 | 718.0 | 597.5 | |
| 0.00 | 1.13 | 0.00 | 0.68 | -27.86 | 26.90 | 2.77 | 184.42 | 0.5560 | -653.0 | -590.6 | |
| 0.00 | 1.48 | 0.00 | 0.90 | -29.67 | 22.51 | -1.62 | 177.56 | 0.5811 | -700.0 | -482.6 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -32.55 | 22.00 | -2.13 | 177.09 | 0.6217 | -672.0 | -587.1 | |
| 0.00 | 1.13 | 0.00 | 0.69 | -29.85 | 21.88 | -2.25 | 176.65 | 0.5842 | -708.0 | -601.7 | |
| 0.00 | 1.13 | 0.00 | 0.69 | -29.53 | 20.79 | -3.34 | 174.97 | 0.5807 | -692.0 | -542.9 | |
| 0.00 | 2.01 | 0.00 | 1.28 | -32.91 | 19.74 | -4.39 | 174.11 | 0.6289 | -601.0 | -601.8 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -29.39 | 19.21 | -4.92 | 172.59 | 0.5812 | -718.0 | -581.0 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -31.17 | 18.95 | -5.18 | 172.65 | 0.6065 | -660.0 | -549.2 | |
| 0.00 | 1.40 | 0.00 | 0.85 | -29.60 | 16.89 | -7.24 | 169.24 | 0.5894 | -783.0 | -557.8 | |
| 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. | |