SDO HMI 2011-09-04 13:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.21 | 127.60 | 22.01 | 140.43 | 23.22 | 303.17 | 63.80 | 292.55 | 0.8923 | -166.6 | 1.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.61 | 98.02 | 1.91 | 114.85 | 22.59 | 305.60 | 66.22 | 291.59 | 0.9104 | 271.6 | -116.1 | |
| 15.99 | -1.00 | 18.70 | -1.00 | 22.60 | 305.20 | 65.83 | 291.62 | 0.9077 | -704.3 | 999999 | |
| 0.00 | 1.61 | 0.00 | 1.43 | 25.68 | 295.25 | 55.88 | 296.15 | 0.8333 | 384.0 | 284.9 | |
| 0.00 | 1.70 | 0.00 | 1.49 | 25.07 | 294.77 | 55.39 | 295.51 | 0.8282 | 552.0 | 489.6 | |
| 0.00 | 1.88 | 0.00 | 1.66 | 25.57 | 294.99 | 55.62 | 296.07 | 0.8310 | 565.0 | 377.1 | |
| 0.00 | 1.79 | 0.00 | 1.57 | 25.84 | 294.64 | 55.27 | 296.45 | 0.8283 | 309.0 | 253.8 | |
| 0.00 | 2.32 | 0.00 | 2.01 | 25.58 | 293.94 | 54.57 | 296.26 | 0.8217 | 635.0 | 550.6 | |
| 1.61 | 2.77 | 1.40 | 2.41 | 25.89 | 294.09 | 54.72 | 296.61 | 0.8236 | 455.9 | 494.5 | |
| 0.00 | 3.22 | 0.00 | 2.82 | 26.62 | 294.37 | 55.00 | 297.43 | 0.8272 | 534.0 | 364.1 | |
| 0.00 | 1.52 | 0.00 | 1.30 | 25.78 | 293.61 | 54.23 | 296.56 | 0.8191 | 637.0 | 547.9 | |
| 0.00 | 1.16 | 0.00 | 0.99 | 25.33 | 293.19 | 53.82 | 296.09 | 0.8146 | 563.0 | 472.7 | |
| 0.00 | 8.04 | 0.00 | 6.86 | 26.11 | 293.25 | 53.88 | 297.03 | 0.8165 | 605.0 | 553.1 | |
| 0.00 | 0.98 | 0.00 | 0.84 | 26.99 | 293.28 | 53.91 | 298.09 | 0.8184 | 402.0 | 310.8 | |
| 0.00 | 1.61 | 0.00 | 1.37 | 26.72 | 293.04 | 53.67 | 297.81 | 0.8157 | 629.0 | 464.9 | |
| 0.00 | 0.98 | 0.00 | 0.83 | 26.22 | 292.70 | 53.33 | 297.28 | 0.8118 | 534.0 | 497.4 | |
| 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. | |