SDO HMI 2014-04-12 13:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.31 | 0.00 | 8.84 | -20.16 | 325.30 | 33.66 | 241.46 | 0.5907 | 34.4 | 107.4 | |
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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 | 1.06 | 0.00 | 0.71 | -15.86 | 333.92 | 42.28 | 252.83 | 0.6796 | 412.0 | 313.1 | |
| 0.00 | 1.50 | 0.00 | 0.99 | -14.82 | 332.95 | 41.31 | 254.16 | 0.6657 | 623.0 | 436.4 | |
| 0.00 | 1.15 | 0.00 | 0.76 | -16.87 | 332.63 | 40.98 | 251.03 | 0.6660 | 474.0 | 461.2 | |
| 0.00 | 1.06 | 0.00 | 0.71 | -21.01 | 332.25 | 40.61 | 244.88 | 0.6734 | 571.0 | 488.0 | |
| 0.00 | 1.50 | 0.00 | 1.00 | -21.26 | 332.25 | 40.60 | 244.51 | 0.6743 | 421.0 | 344.5 | |
| 0.00 | 1.68 | 0.00 | 1.02 | -19.69 | 325.16 | 33.51 | 243.79 | 0.5816 | 839.0 | 718.1 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -19.58 | 324.94 | 33.29 | 243.86 | 0.5783 | 668.0 | 609.5 | |
| 0.00 | 1.15 | 0.00 | 0.66 | -21.04 | 318.46 | 26.82 | 237.04 | 0.5038 | -773.0 | -570.5 | |
| 0.00 | 0.53 | 0.00 | 0.31 | -23.61 | 317.97 | 26.33 | 232.17 | 0.5165 | -616.0 | -525.0 | |
| 0.00 | 1.77 | 0.00 | 1.01 | -23.87 | 317.11 | 25.47 | 230.94 | 0.5085 | -712.0 | -621.9 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -22.74 | 316.23 | 24.59 | 232.01 | 0.4889 | -753.0 | -518.9 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -25.48 | 306.78 | 15.14 | 214.75 | 0.4154 | -741.0 | -618.0 | |
| 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. | |