SDO HMI 2011-01-01 01:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.28 | 179.75 | 31.42 | 114.95 | 34.00 | 267.71 | 13.45 | 342.20 | 0.6340 | -5.2 | -53.0 | |
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back to the solar disc SDO HMI 2011-01-01 01:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.65 | 104.32 | 10.67 | 66.91 | 33.61 | 269.75 | 15.49 | 339.49 | 0.6372 | -1044.8 | -316.9 | |
| 3.91 | -1.00 | 2.49 | -1.00 | 33.38 | 269.19 | 14.94 | 340.00 | 0.6318 | -742.1 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.97 | 32.94 | 268.94 | 14.68 | 340.03 | 0.6251 | -768.0 | -613.0 | |
| 2.89 | 3.65 | 1.84 | 2.33 | 33.67 | 268.70 | 14.44 | 340.79 | 0.6331 | -783.1 | -718.3 | |
| 0.00 | 2.72 | 0.00 | 1.74 | 34.49 | 266.82 | 12.56 | 343.56 | 0.6357 | -765.0 | -511.7 | |
| 2.72 | 5.61 | 1.70 | 3.51 | 33.44 | 264.93 | 10.67 | 345.39 | 0.6151 | 917.9 | 699.6 | |
| 0.00 | 1.44 | 0.00 | 0.92 | 34.77 | 265.06 | 10.81 | 345.86 | 0.6330 | 656.0 | 507.5 | |
| 1.19 | 18.26 | 0.76 | 11.74 | 35.07 | 265.03 | 10.77 | 346.05 | 0.6368 | 598.4 | 551.4 | |
| 0.00 | 1.95 | 0.00 | 1.23 | 33.65 | 264.85 | 10.59 | 345.61 | 0.6177 | 600.0 | 516.6 | |
| 1.61 | -8.00 | 1.04 | -8.00 | 35.29 | 265.02 | 10.77 | 346.16 | 0.6397 | 659.9 | 999999 | |
| 1.87 | -8.00 | 1.20 | -8.00 | 35.52 | 264.94 | 10.69 | 346.36 | 0.6423 | 698.0 | 999999 | |
| 3.91 | 40.27 | 2.48 | 25.60 | 34.32 | 264.64 | 10.38 | 346.18 | 0.6258 | 984.6 | 522.7 | |
| 14.53 | -12.00 | 9.24 | -12.00 | 34.73 | 264.40 | 10.14 | 346.67 | 0.6303 | 925.0 | 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. | |