SDO HMI 2014-04-14 03:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.12 | 418.93 | 34.40 | 218.03 | 11.63 | 274.87 | 4.16 | 346.56 | 0.3080 | -942.1 | -393.4 | |
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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 |
| 66.12 | 404.78 | 34.40 | 210.60 | 11.57 | 275.07 | 4.36 | 345.92 | 0.3072 | -1445.7 | -433.1 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 13.55 | 272.45 | 1.73 | 354.92 | 0.3325 | -757.0 | -610.9 | |
| 0.00 | 2.30 | 0.00 | 1.21 | 13.81 | 269.79 | -0.93 | 2.70 | 0.3358 | 789.0 | 515.5 | |
| 0.00 | 2.03 | 0.00 | 1.06 | 12.86 | 269.57 | -1.14 | 3.50 | 0.3203 | 900.0 | 733.7 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 13.84 | 269.51 | -1.21 | 3.51 | 0.3366 | 764.0 | 595.4 | |
| 0.00 | 1.15 | 0.00 | 0.61 | 14.52 | 269.16 | -1.55 | 4.35 | 0.3481 | 518.0 | 487.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 12.83 | 269.11 | -1.61 | 4.92 | 0.3203 | 851.0 | 648.5 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 15.13 | 268.94 | -1.78 | 4.81 | 0.3583 | 710.0 | 620.6 | |
| 0.00 | 1.33 | 0.00 | 0.69 | 12.51 | 268.74 | -1.97 | 6.14 | 0.3157 | 654.0 | 519.4 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 14.26 | 268.27 | -2.45 | 6.93 | 0.3454 | 808.0 | 671.4 | |
| 0.00 | 2.03 | 0.00 | 1.07 | 13.12 | 268.03 | -2.69 | 8.07 | 0.3271 | 1033.0 | 813.5 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 12.02 | 266.10 | -4.62 | 14.52 | 0.3156 | 691.0 | 530.3 | |
| 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. | |