SDO HMI 2011-11-27 10:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.48 | 193.87 | 20.69 | 126.86 | 14.44 | 251.98 | 39.07 | 290.79 | 0.6551 | -604.8 | -316.2 | |
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back to the solar disc SDO HMI 2011-11-27 10:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.34 | 179.23 | 19.29 | 117.81 | 14.26 | 252.42 | 39.51 | 290.31 | 0.6598 | -1102.9 | -364.2 | |
| 2.14 | -1.00 | 1.40 | -1.00 | 14.51 | 251.80 | 38.89 | 290.92 | 0.6530 | -908.1 | 999999 | |
| 0.00 | 2.74 | 0.00 | 1.80 | 17.21 | 251.63 | 38.72 | 294.94 | 0.6612 | -672.0 | -490.7 | |
| 0.00 | 1.20 | 0.00 | 0.79 | 17.39 | 251.55 | 38.64 | 295.24 | 0.6611 | -609.0 | -427.4 | |
| 0.00 | 0.51 | 0.00 | 0.34 | 17.03 | 251.22 | 38.31 | 294.87 | 0.6557 | -542.0 | -582.5 | |
| 0.00 | 1.03 | 0.00 | 0.63 | 11.91 | 247.53 | 34.62 | 288.58 | 0.5888 | 715.0 | 599.7 | |
| 0.00 | 1.03 | 0.00 | 0.63 | 16.10 | 246.85 | 33.94 | 295.70 | 0.5975 | 661.0 | 450.5 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 12.96 | 245.25 | 32.34 | 291.41 | 0.5622 | 599.0 | 500.3 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 17.48 | 244.94 | 32.03 | 299.04 | 0.5808 | 572.0 | 384.0 | |
| 0.00 | 1.80 | 0.00 | 1.08 | 17.62 | 243.95 | 31.03 | 299.93 | 0.5692 | 600.0 | 495.7 | |
| 0.00 | 1.28 | 0.00 | 0.75 | 13.56 | 242.92 | 30.01 | 293.78 | 0.5334 | 732.0 | 565.1 | |
| 0.00 | 1.54 | 0.00 | 0.92 | 17.81 | 243.55 | 30.64 | 300.52 | 0.5654 | 683.0 | 650.6 | |
| 0.00 | 1.45 | 0.00 | 0.87 | 18.86 | 243.32 | 30.41 | 302.37 | 0.5693 | 640.0 | 521.2 | |
| 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. | |