SDO HMI 2011-12-15 12:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.29 | 357.57 | 31.70 | 194.47 | -18.15 | 352.20 | 17.58 | 224.03 | 0.4149 | 1123.6 | 422.4 | |
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back to the solar disc SDO HMI 2011-12-15 12:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.93 | 329.32 | 26.59 | 179.12 | -17.93 | 352.31 | 17.69 | 224.58 | 0.4136 | 1399.5 | 409.1 | |
| 2.89 | -1.00 | 1.58 | -1.00 | -19.08 | 352.43 | 17.81 | 222.78 | 0.4274 | 825.9 | 999999 | |
| 3.23 | -1.00 | 1.77 | -1.00 | -19.01 | 352.26 | 17.64 | 222.62 | 0.4249 | 1020.9 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -15.15 | 351.05 | 16.43 | 227.94 | 0.3695 | -941.0 | -675.4 | |
| 1.62 | 2.30 | 0.88 | 1.25 | -18.93 | 351.27 | 16.65 | 221.19 | 0.4134 | 1009.8 | 876.9 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -19.86 | 351.17 | 16.55 | 219.49 | 0.4232 | 634.0 | 473.4 | |
| 1.62 | 14.72 | 0.88 | 8.01 | -19.33 | 350.99 | 16.37 | 220.04 | 0.4151 | 948.4 | 710.2 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -16.86 | 350.66 | 16.03 | 223.84 | 0.3833 | -718.0 | -640.2 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -19.58 | 350.82 | 16.20 | 219.35 | 0.4163 | 803.0 | 602.8 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -20.96 | 350.97 | 16.35 | 217.44 | 0.4342 | 760.0 | 578.5 | |
| 0.00 | 0.68 | 0.00 | 0.37 | -20.99 | 350.67 | 16.05 | 216.91 | 0.4318 | 717.0 | 514.8 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -20.05 | 350.41 | 15.79 | 217.90 | 0.4179 | 836.0 | 695.7 | |
| 0.00 | 2.13 | 0.00 | 1.15 | -19.52 | 350.26 | 15.64 | 218.49 | 0.4100 | 783.0 | 763.0 | |
| 0.00 | 0.85 | 0.00 | 0.47 | -20.90 | 350.27 | 15.65 | 216.37 | 0.4268 | 808.0 | 688.5 | |
| 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. | |