SDO HMI 2011-10-18 06:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.10 | 38.75 | 10.59 | 31.52 | 24.18 | 331.31 | -51.17 | 63.68 | 0.7939 | -293.8 | -222.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.18 | 0.00 | 1.65 | 23.88 | 334.95 | -47.53 | 63.12 | 0.7586 | -574.0 | -526.8 | |
| 0.00 | 0.96 | 0.00 | 0.74 | 24.30 | 334.11 | -48.38 | 62.82 | 0.7682 | -614.0 | -548.1 | |
| 2.62 | 13.53 | 2.02 | 10.43 | 23.48 | 333.92 | -48.57 | 63.91 | 0.7680 | -733.5 | -451.2 | |
| 3.67 | -3.00 | 2.82 | -3.00 | 23.19 | 333.87 | -48.62 | 64.29 | 0.7678 | -681.1 | 999999 | |
| 0.00 | 2.53 | 0.00 | 1.95 | 22.87 | 333.73 | -48.76 | 64.74 | 0.7684 | -661.0 | -537.8 | |
| 0.00 | 1.05 | 0.00 | 0.83 | 24.17 | 332.41 | -50.08 | 63.43 | 0.7846 | -379.0 | -284.7 | |
| 0.00 | 1.40 | 0.00 | 1.11 | 23.54 | 332.44 | -50.05 | 64.22 | 0.7828 | -558.0 | -429.7 | |
| 0.00 | 1.13 | 0.00 | 0.91 | 23.00 | 331.69 | -50.80 | 65.07 | 0.7889 | -414.0 | -364.5 | |
| 1.66 | 2.09 | 1.34 | 1.70 | 22.93 | 331.16 | -51.33 | 65.28 | 0.7939 | 416.9 | 250.2 | |
| 0.00 | 0.79 | 0.00 | 0.64 | 22.83 | 330.63 | -51.85 | 65.52 | 0.7987 | 530.0 | 507.4 | |
| 5.15 | 8.12 | 4.41 | 6.94 | 24.65 | 328.92 | -53.56 | 63.66 | 0.8181 | -493.1 | -441.6 | |
| 0.00 | 1.48 | 0.00 | 1.34 | 26.78 | 327.02 | -55.47 | 61.55 | 0.8387 | 563.0 | 487.4 | |
| 0.00 | 1.92 | 0.00 | 1.81 | 27.64 | 325.43 | -57.05 | 60.87 | 0.8531 | 396.0 | 277.9 | |
| 0.00 | 1.57 | 0.00 | 1.47 | 26.86 | 325.56 | -56.93 | 61.75 | 0.8508 | 679.0 | 532.8 | |
| 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. | |