SDO HMI 2014-05-20 08:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.53 | 0.00 | 10.19 | -18.29 | 144.88 | -7.30 | 157.30 | 0.3116 | 402.6 | 405.4 | |
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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 | 0.27 | 0.00 | 0.14 | -22.37 | 150.11 | -2.07 | 174.49 | 0.3502 | -6.0 | -6.3 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -22.18 | 149.00 | -3.19 | 171.49 | 0.3492 | 3.0 | 4.1 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -16.58 | 148.64 | -3.55 | 166.69 | 0.2587 | 897.0 | 690.5 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -15.92 | 148.27 | -3.91 | 164.68 | 0.2495 | 809.0 | 651.7 | |
| 0.00 | 2.70 | 0.00 | 1.38 | -15.57 | 146.79 | -5.39 | 158.83 | 0.2517 | 900.0 | 769.4 | |
| 0.00 | 1.89 | 0.00 | 0.99 | -20.75 | 146.39 | -5.79 | 163.60 | 0.3356 | 1058.0 | 889.3 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -16.16 | 146.43 | -5.76 | 158.43 | 0.2633 | 919.0 | 784.1 | |
| 0.00 | 1.71 | 0.00 | 0.90 | -20.98 | 146.22 | -5.96 | 163.35 | 0.3399 | 838.0 | 675.4 | |
| 0.00 | 1.26 | 0.00 | 0.66 | -18.45 | 145.42 | -6.77 | 158.41 | 0.3050 | 873.0 | 696.3 | |
| 0.00 | 2.79 | 0.00 | 1.44 | -17.03 | 145.12 | -7.06 | 155.55 | 0.2853 | 781.0 | 648.7 | |
| 0.00 | 1.53 | 0.00 | 0.80 | -19.37 | 144.37 | -7.81 | 156.71 | 0.3256 | 336.0 | 373.2 | |
| 0.00 | 0.27 | 0.00 | 0.14 | -20.61 | 143.49 | -8.69 | 156.04 | 0.3499 | -10.0 | -8.7 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -18.32 | 135.95 | -16.23 | 136.66 | 0.3882 | -881.0 | -749.5 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -17.05 | 135.74 | -16.44 | 133.86 | 0.3768 | -881.0 | -800.8 | |
| 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. | |