SDO HMI 2014-04-14 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.62 | 424.58 | 34.60 | 220.58 | 11.62 | 274.83 | 2.46 | 351.91 | 0.3028 | -925.1 | -389.5 | |
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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 |
| 66.62 | 409.29 | 34.60 | 212.53 | 11.54 | 275.04 | 2.67 | 351.26 | 0.3014 | -1391.1 | -428.5 | |
| 0.00 | 1.50 | 0.00 | 0.79 | 13.85 | 273.27 | 0.90 | 357.40 | 0.3368 | -764.0 | -593.8 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 13.82 | 272.43 | 0.06 | 359.82 | 0.3359 | -725.0 | -650.1 | |
| 0.00 | 1.33 | 0.00 | 0.69 | 12.88 | 269.66 | -2.71 | 8.24 | 0.3235 | 909.0 | 727.5 | |
| 0.00 | 1.59 | 0.00 | 0.83 | 12.85 | 269.47 | -2.90 | 8.81 | 0.3234 | 957.0 | 750.7 | |
| 0.00 | 1.41 | 0.00 | 0.75 | 14.54 | 269.42 | -2.95 | 8.19 | 0.3511 | 859.0 | 674.2 | |
| 0.00 | 1.15 | 0.00 | 0.61 | 14.31 | 269.33 | -3.04 | 8.54 | 0.3477 | 773.0 | 624.5 | |
| 0.00 | 1.24 | 0.00 | 0.65 | 12.72 | 269.01 | -3.36 | 10.25 | 0.3227 | 800.0 | 656.7 | |
| 0.00 | 2.83 | 0.00 | 1.49 | 14.32 | 268.30 | -4.07 | 11.34 | 0.3507 | 858.0 | 730.8 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 13.18 | 267.95 | -4.42 | 13.05 | 0.3336 | 901.0 | 822.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.02 | 266.18 | -6.19 | 19.12 | 0.3233 | 663.0 | 491.4 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 14.92 | 266.08 | -6.29 | 16.75 | 0.3691 | 716.0 | 516.9 | |
| 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. | |