SDO HMI 2014-04-21 12:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.46 | 85.72 | 16.48 | 76.67 | -23.16 | 117.70 | -55.65 | 114.51 | 0.8362 | 459.0 | 352.9 | |
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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 |
| 12.78 | 69.75 | 11.30 | 61.55 | -23.16 | 118.37 | -54.97 | 114.63 | 0.8304 | 833.7 | 414.3 | |
| 4.26 | -1.00 | 3.82 | -1.00 | -23.41 | 117.81 | -55.54 | 114.82 | 0.8357 | 411.8 | 999999 | |
| 0.00 | 1.86 | 0.00 | 1.67 | -22.56 | 117.59 | -55.76 | 113.77 | 0.8363 | 517.0 | 373.1 | |
| 0.00 | 0.89 | 0.00 | 0.81 | -22.88 | 117.15 | -56.20 | 114.07 | 0.8406 | 179.0 | 193.7 | |
| 0.00 | 1.06 | 0.00 | 0.95 | -22.05 | 117.61 | -55.74 | 113.16 | 0.8353 | 553.0 | 361.2 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -22.10 | 117.40 | -55.94 | 113.19 | 0.8372 | 359.0 | 322.3 | |
| 0.00 | 1.15 | 0.00 | 1.06 | -22.71 | 116.54 | -56.80 | 113.76 | 0.8455 | 352.0 | 284.5 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -22.88 | 116.25 | -57.10 | 113.92 | 0.8482 | 245.0 | 250.3 | |
| 0.00 | 2.84 | 0.00 | 2.71 | -23.95 | 115.39 | -57.95 | 115.02 | 0.8569 | 571.0 | 382.4 | |
| 0.00 | 1.95 | 0.00 | 1.88 | -24.09 | 115.04 | -58.31 | 115.12 | 0.8599 | 312.0 | 260.6 | |
| 0.00 | 0.89 | 0.00 | 0.85 | -23.81 | 115.24 | -58.10 | 114.83 | 0.8579 | -173.0 | -114.2 | |
| 1.42 | 2.93 | 1.36 | 2.81 | -22.72 | 114.94 | -58.41 | 113.52 | 0.8589 | -556.6 | -422.1 | |
| 0.00 | 0.62 | 0.00 | 0.65 | -22.54 | 112.06 | -61.29 | 112.92 | 0.8815 | -366.0 | -373.0 | |
| 0.00 | 1.24 | 0.00 | 1.24 | -20.16 | 113.14 | -60.21 | 110.34 | 0.8708 | -172.0 | -109.6 | |
| 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. | |