SDO HMI 2014-07-07 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.45 | 21.34 | 1.25 | 10.85 | 7.37 | 252.10 | 12.44 | 287.77 | 0.2258 | 604.2 | 643.0 | |
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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 | 0.36 | 0.00 | 0.19 | 6.70 | 255.39 | 15.73 | 282.12 | 0.2766 | -376.0 | -474.8 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 6.58 | 255.16 | 15.50 | 281.85 | 0.2725 | -870.0 | -763.9 | |
| 0.00 | 2.09 | 0.00 | 1.06 | 7.79 | 252.38 | 12.72 | 289.20 | 0.2321 | 900.0 | 759.7 | |
| 0.00 | 3.00 | 0.00 | 1.53 | 8.43 | 252.31 | 12.65 | 291.91 | 0.2345 | 944.0 | 793.0 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 8.22 | 252.30 | 12.64 | 291.06 | 0.2331 | 859.0 | 722.8 | |
| 1.45 | 4.36 | 0.74 | 2.22 | 8.01 | 252.07 | 12.41 | 290.52 | 0.2283 | 1146.8 | 859.6 | |
| 1.00 | 3.72 | 0.51 | 1.89 | 7.25 | 251.74 | 12.08 | 287.74 | 0.2189 | 980.7 | 817.6 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 5.91 | 251.58 | 11.92 | 281.83 | 0.2108 | 743.0 | 615.7 | |
| 0.00 | 0.36 | 0.00 | 0.18 | 6.06 | 251.55 | 11.89 | 282.57 | 0.2108 | 716.0 | 633.5 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 7.07 | 251.42 | 11.76 | 287.36 | 0.2128 | 784.0 | 621.2 | |
| 0.00 | 2.09 | 0.00 | 1.06 | 6.13 | 251.11 | 11.45 | 283.32 | 0.2038 | 893.0 | 742.8 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 6.19 | 250.68 | 11.01 | 284.13 | 0.1968 | 856.0 | 689.1 | |
| 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. | |