SDO HMI 2014-10-05 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.61 | 34.18 | 5.22 | 20.13 | 13.26 | 92.15 | -32.12 | 75.71 | 0.5364 | 69.7 | 16.2 | |
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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 | 1.41 | 0.00 | 0.75 | 9.92 | 103.20 | -21.07 | 79.22 | 0.3620 | -737.0 | -579.2 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 9.81 | 102.72 | -21.55 | 79.69 | 0.3695 | -705.0 | -507.8 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 10.63 | 99.30 | -24.96 | 78.73 | 0.4248 | -758.0 | -621.0 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 13.84 | 98.74 | -25.53 | 71.67 | 0.4426 | -773.0 | -586.4 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 13.71 | 98.62 | -25.65 | 72.01 | 0.4440 | -747.0 | -591.2 | |
| 0.00 | 0.79 | 0.00 | 0.44 | 10.26 | 97.20 | -27.07 | 80.12 | 0.4564 | -788.0 | -744.4 | |
| 0.00 | 1.76 | 0.00 | 0.98 | 6.76 | 97.02 | -27.25 | 87.82 | 0.4569 | -766.0 | -574.7 | |
| 0.00 | 1.32 | 0.00 | 0.74 | 8.18 | 96.55 | -27.72 | 84.73 | 0.4643 | -716.0 | -630.2 | |
| 0.00 | 3.16 | 0.00 | 1.80 | 10.99 | 95.01 | -29.26 | 79.06 | 0.4906 | -708.0 | -596.1 | |
| 0.00 | 1.23 | 0.00 | 0.73 | 17.60 | 92.40 | -31.87 | 67.45 | 0.5470 | 681.0 | 490.6 | |
| 0.00 | 1.23 | 0.00 | 0.76 | 19.42 | 88.92 | -35.35 | 65.95 | 0.5998 | 656.0 | 540.4 | |
| 0.00 | 0.97 | 0.00 | 0.59 | 16.76 | 89.26 | -35.01 | 70.18 | 0.5862 | 652.0 | 517.5 | |
| 0.00 | 2.11 | 0.00 | 1.33 | 21.22 | 87.76 | -36.51 | 63.63 | 0.6213 | 642.0 | 439.1 | |
| 8.61 | 15.37 | 5.22 | 9.32 | 13.25 | 89.19 | -35.08 | 76.16 | 0.5783 | 904.5 | 585.4 | |
| 0.00 | 0.88 | 0.00 | 0.54 | 13.43 | 88.18 | -36.09 | 76.08 | 0.5926 | 685.0 | 563.5 | |
| 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. | |