SDO HMI 2014-10-06 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.29 | 32.86 | 4.02 | 17.99 | 13.22 | 90.91 | -23.99 | 72.10 | 0.4171 | 204.5 | -60.6 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.48 | 0.00 | 2.32 | 12.94 | 99.25 | -15.66 | 66.00 | 0.2892 | -953.0 | -707.1 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 8.11 | 96.78 | -18.13 | 83.61 | 0.3114 | -773.0 | -651.4 | |
| 0.00 | 2.81 | 0.00 | 1.48 | 10.12 | 95.74 | -19.17 | 77.77 | 0.3322 | -712.0 | -613.8 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 8.99 | 94.45 | -20.46 | 81.55 | 0.3506 | -946.0 | -818.8 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 11.08 | 93.99 | -20.92 | 75.92 | 0.3629 | -715.0 | -582.1 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 11.00 | 93.67 | -21.24 | 76.28 | 0.3677 | -714.0 | -562.6 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 18.22 | 92.69 | -22.22 | 59.46 | 0.4188 | 708.0 | 541.3 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 15.35 | 91.32 | -23.59 | 67.00 | 0.4211 | 853.0 | 678.6 | |
| 7.29 | 10.81 | 4.02 | 5.96 | 13.38 | 89.33 | -25.58 | 72.62 | 0.4420 | 1041.8 | 735.8 | |
| 0.00 | 1.23 | 0.00 | 0.69 | 16.08 | 88.54 | -26.37 | 67.30 | 0.4645 | 673.0 | 605.4 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 15.53 | 88.55 | -26.36 | 68.43 | 0.4620 | 695.0 | 568.1 | |
| 0.00 | 1.41 | 0.00 | 0.79 | 13.27 | 87.00 | -27.91 | 73.90 | 0.4762 | 741.0 | 619.6 | |
| 0.00 | 0.70 | 0.00 | 0.41 | 15.54 | 83.93 | -30.98 | 70.73 | 0.5275 | 637.0 | 459.6 | |
| 0.00 | 2.11 | 0.00 | 1.24 | 11.87 | 82.44 | -32.47 | 78.00 | 0.5392 | -655.0 | -507.1 | |
| 0.00 | 1.32 | 0.00 | 0.81 | 20.38 | 80.75 | -34.15 | 63.81 | 0.5887 | 657.0 | 507.3 | |
| 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. | |