SDO HMI 2014-05-20 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.59 | 207.17 | 21.66 | 141.76 | -24.78 | 190.17 | 38.53 | 235.15 | 0.6914 | 526.2 | 247.8 | |
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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 |
| 0.81 | 192.50 | 0.55 | 132.14 | -24.04 | 190.39 | 38.75 | 236.28 | 0.6896 | 906.0 | 311.2 | |
| 30.78 | -1.00 | 21.11 | -1.00 | -24.63 | 190.52 | 38.88 | 235.58 | 0.6940 | 1130.7 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.75 | -26.40 | 190.37 | 38.74 | 233.21 | 0.7022 | 542.0 | 430.8 | |
| 0.00 | 1.17 | 0.00 | 0.76 | -25.72 | 185.75 | 34.11 | 231.16 | 0.6510 | -731.0 | -639.5 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -26.08 | 185.87 | 34.24 | 230.76 | 0.6547 | -591.0 | -523.1 | |
| 0.00 | 1.08 | 0.00 | 0.70 | -25.58 | 185.67 | 34.03 | 231.28 | 0.6492 | -739.0 | -622.0 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -26.22 | 185.67 | 34.04 | 230.44 | 0.6535 | -661.0 | -539.5 | |
| 0.00 | 1.62 | 0.00 | 1.06 | -26.32 | 185.54 | 33.91 | 230.22 | 0.6529 | -648.0 | -576.3 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -26.79 | 185.53 | 33.90 | 229.60 | 0.6561 | -634.0 | -517.4 | |
| 0.00 | 0.81 | 0.00 | 0.53 | -28.05 | 184.78 | 33.14 | 227.42 | 0.6575 | -571.0 | -488.4 | |
| 0.00 | 1.35 | 0.00 | 0.87 | -26.75 | 184.06 | 32.42 | 228.56 | 0.6409 | -773.0 | -577.6 | |
| 0.00 | 1.53 | 0.00 | 1.00 | -28.36 | 184.47 | 32.84 | 226.80 | 0.6569 | -556.0 | -500.9 | |
| 0.00 | 2.25 | 0.00 | 1.48 | -28.57 | 184.38 | 32.75 | 226.47 | 0.6575 | -525.0 | -466.6 | |
| 0.00 | 1.26 | 0.00 | 0.82 | -28.47 | 184.18 | 32.55 | 226.44 | 0.6549 | -769.0 | -715.5 | |
| 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. | |