SDO HMI 2011-10-19 19:09:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.60 | 184.82 | 38.48 | 140.07 | -12.24 | 48.68 | 46.07 | 248.49 | 0.7579 | -200.2 | -261.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.11 | 46.08 | 11.62 | 38.11 | -12.11 | 52.89 | 50.28 | 250.31 | 0.8010 | 738.8 | 82.3 | |
| 0.00 | 3.92 | 0.00 | 3.18 | -11.70 | 52.36 | 49.75 | 250.62 | 0.7945 | 470.0 | 479.4 | |
| 0.00 | 0.78 | 0.00 | 0.64 | -12.62 | 52.60 | 49.99 | 249.59 | 0.7997 | 375.0 | 329.4 | |
| 0.78 | -1.00 | 0.64 | -1.00 | -12.36 | 52.48 | 49.87 | 249.86 | 0.7977 | 628.7 | 999999 | |
| 0.96 | 1.13 | 0.74 | 0.88 | -9.84 | 50.74 | 48.13 | 252.33 | 0.7723 | 612.9 | 588.0 | |
| 0.00 | 1.31 | 0.00 | 1.00 | -11.64 | 49.53 | 46.92 | 249.64 | 0.7654 | 730.0 | 582.1 | |
| 0.00 | 2.09 | 0.00 | 1.60 | -11.81 | 49.30 | 46.69 | 249.34 | 0.7636 | 668.0 | 574.9 | |
| 0.00 | 2.53 | 0.00 | 1.91 | -12.13 | 48.53 | 45.92 | 248.63 | 0.7565 | -498.0 | -403.1 | |
| 1.39 | 1.74 | 1.06 | 1.32 | -13.03 | 48.48 | 45.87 | 247.48 | 0.7593 | -281.6 | -306.8 | |
| 0.00 | 1.74 | 0.00 | 1.32 | -13.17 | 48.25 | 45.63 | 247.20 | 0.7574 | -372.0 | -323.5 | |
| 4.18 | 19.42 | 3.11 | 14.46 | -11.89 | 47.78 | 45.17 | 248.62 | 0.7476 | -700.1 | -273.4 | |
| 0.00 | 2.35 | 0.00 | 1.76 | -13.09 | 47.92 | 45.31 | 247.17 | 0.7536 | -480.0 | -488.6 | |
| 0.00 | 0.78 | 0.00 | 0.59 | -13.31 | 47.97 | 45.36 | 246.91 | 0.7550 | -457.0 | -379.8 | |
| 4.18 | -11.00 | 3.10 | -11.00 | -12.16 | 47.66 | 45.05 | 248.22 | 0.7474 | -705.7 | 999999 | |
| 4.53 | 100.95 | 3.34 | 73.30 | -12.80 | 47.03 | 44.42 | 247.13 | 0.7430 | -514.8 | -496.7 | |
| 6.27 | -15.00 | 4.58 | -15.00 | -12.40 | 46.64 | 44.03 | 247.47 | 0.7372 | -718.9 | 999999 | |
| 14.20 | -15.00 | 10.29 | -15.00 | -12.19 | 46.25 | 43.64 | 247.57 | 0.7322 | -923.8 | 999999 | |
| 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. | |