SDO HMI 2010-11-18 20:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.97 | 325.77 | 74.45 | 481.26 | 13.70 | 173.84 | 70.24 | 283.77 | 0.9402 | -47.3 | 4.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.55 | 172.87 | 8.09 | 301.14 | 12.77 | 177.59 | 73.99 | 282.60 | 0.9618 | 298.2 | -111.0 | |
| 22.05 | -1.00 | 38.04 | -1.00 | 12.98 | 176.98 | 73.39 | 282.83 | 0.9590 | -651.5 | 999999 | |
| 0.00 | 2.75 | 0.00 | 4.14 | 12.59 | 174.49 | 70.89 | 282.49 | 0.9460 | -558.0 | -469.2 | |
| 0.00 | 1.63 | 0.00 | 2.50 | 13.19 | 174.80 | 71.20 | 283.11 | 0.9478 | -415.0 | -317.0 | |
| 0.00 | 4.12 | 0.00 | 5.94 | 13.48 | 173.51 | 69.92 | 283.47 | 0.9407 | 18.0 | -221.9 | |
| 1.46 | 4.80 | 1.96 | 6.46 | 12.84 | 171.99 | 68.39 | 282.85 | 0.9314 | 246.9 | 299.7 | |
| 0.43 | 2.32 | 0.59 | 3.17 | 13.53 | 172.32 | 68.72 | 283.57 | 0.9336 | 280.2 | 140.4 | |
| 0.00 | 3.09 | 0.00 | 4.17 | 13.57 | 172.01 | 68.41 | 283.63 | 0.9317 | 527.0 | 409.6 | |
| 0.00 | 1.12 | 0.00 | 1.48 | 13.07 | 171.62 | 68.02 | 283.11 | 0.9292 | 455.0 | 348.8 | |
| 0.00 | 0.86 | 0.00 | 1.09 | 14.30 | 170.50 | 66.90 | 284.51 | 0.9224 | 316.0 | 248.0 | |
| 2.49 | 3.00 | 2.98 | 3.60 | 14.72 | 168.99 | 65.39 | 285.07 | 0.9124 | 178.0 | 112.0 | |
| 19.99 | 128.35 | 22.79 | 146.58 | 15.29 | 167.51 | 63.91 | 285.83 | 0.9023 | 754.1 | 242.1 | |
| 0.00 | 0.86 | 0.00 | 0.99 | 17.79 | 167.61 | 64.02 | 288.57 | 0.9048 | -186.0 | -255.2 | |
| 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. | |