SDO HMI 2011-10-19 10:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.68 | 403.96 | 49.05 | 315.92 | 27.58 | 55.12 | 48.01 | 301.49 | 0.7748 | -859.3 | -218.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.20 | 387.67 | 47.91 | 304.04 | 27.56 | 55.32 | 48.21 | 301.39 | 0.7767 | -1071.2 | -220.7 | |
| 0.00 | 0.70 | 0.00 | 0.56 | 30.25 | 56.19 | 49.08 | 304.39 | 0.7932 | 563.0 | 473.4 | |
| 1.48 | -1.00 | 1.14 | -1.00 | 27.50 | 54.24 | 47.13 | 301.69 | 0.7662 | -920.5 | 999999 | |
| 0.00 | 3.75 | 0.00 | 2.85 | 27.24 | 53.75 | 46.64 | 301.53 | 0.7606 | -842.0 | -780.1 | |
| 0.00 | 1.22 | 0.00 | 0.96 | 30.29 | 54.65 | 47.54 | 304.97 | 0.7797 | 351.0 | 380.4 | |
| 0.00 | 1.22 | 0.00 | 0.91 | 27.71 | 52.11 | 45.00 | 302.73 | 0.7464 | -513.0 | -476.4 | |
| 0.00 | 1.48 | 0.00 | 1.10 | 28.44 | 52.06 | 44.95 | 303.66 | 0.7488 | -389.0 | -353.8 | |
| 0.00 | 1.74 | 0.00 | 1.34 | 31.13 | 52.69 | 45.58 | 306.75 | 0.7654 | -678.0 | -557.5 | |
| 0.00 | 0.61 | 0.00 | 0.47 | 31.69 | 52.89 | 45.78 | 307.35 | 0.7695 | -513.0 | -446.4 | |
| 0.00 | 0.78 | 0.00 | 0.56 | 28.01 | 49.40 | 42.29 | 304.24 | 0.7209 | -413.0 | -374.7 | |
| 0.00 | 1.22 | 0.00 | 0.81 | 27.50 | 44.84 | 37.73 | 305.81 | 0.6717 | 468.0 | 447.3 | |
| 0.00 | 1.31 | 0.00 | 0.87 | 27.58 | 44.53 | 37.42 | 306.10 | 0.6689 | 650.0 | 498.3 | |
| 0.00 | 1.39 | 0.00 | 0.90 | 25.09 | 43.48 | 36.37 | 303.21 | 0.6441 | 667.0 | 579.2 | |
| 0.00 | 0.87 | 0.00 | 0.55 | 22.36 | 42.33 | 35.22 | 299.81 | 0.6169 | 562.0 | 562.5 | |
| 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. | |