SDO HMI 2011-11-24 16:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.47 | 51.69 | 26.31 | 66.54 | 18.80 | 315.69 | 66.54 | 289.71 | 0.9232 | -259.0 | -91.9 | |
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back to the solar disc SDO HMI 2011-11-24 16:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.60 | 5.65 | 4.87 | 7.64 | 17.75 | 317.13 | 67.97 | 288.42 | 0.9321 | -454.0 | -429.8 | |
| 6.93 | 21.06 | 9.70 | 29.69 | 18.79 | 317.83 | 68.68 | 289.46 | 0.9368 | -612.3 | -150.9 | |
| 0.00 | 1.63 | 0.00 | 2.05 | 18.99 | 315.27 | 66.12 | 289.94 | 0.9214 | -456.0 | -381.1 | |
| 4.37 | 6.33 | 5.48 | 7.95 | 19.27 | 315.11 | 65.95 | 290.26 | 0.9206 | -489.6 | -352.4 | |
| 0.00 | 0.34 | 0.00 | 0.42 | 18.76 | 314.33 | 65.18 | 289.80 | 0.9152 | -249.0 | -246.5 | |
| 0.00 | 1.54 | 0.00 | 1.84 | 19.00 | 313.76 | 64.61 | 290.13 | 0.9115 | -482.0 | -468.2 | |
| 1.03 | 4.45 | 1.17 | 5.07 | 18.53 | 312.50 | 63.34 | 289.78 | 0.9023 | 300.1 | 199.8 | |
| 0.68 | -7.00 | 0.78 | -7.00 | 18.72 | 312.48 | 63.33 | 289.99 | 0.9024 | 219.4 | 999999 | |
| 0.43 | 1.71 | 0.47 | 1.88 | 18.06 | 311.57 | 62.41 | 289.38 | 0.8952 | 190.4 | 166.7 | |
| 0.00 | 0.94 | 0.00 | 1.04 | 18.62 | 311.45 | 62.30 | 290.02 | 0.8949 | 236.0 | 205.0 | |
| 0.86 | 5.99 | 0.96 | 6.73 | 19.64 | 312.00 | 62.85 | 291.07 | 0.8999 | 591.4 | 374.4 | |
| 2.57 | -11.00 | 2.88 | -11.00 | 19.48 | 311.82 | 62.67 | 290.93 | 0.8985 | 539.1 | 999999 | |
| 0.00 | 2.05 | 0.00 | 2.23 | 19.48 | 310.87 | 61.72 | 291.06 | 0.8916 | 495.0 | 435.2 | |
| 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. | |