SDO HMI 2014-04-03 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.52 | 0.00 | 7.12 | -26.78 | 82.20 | 30.68 | 229.75 | 0.5891 | -243.5 | -189.8 | |
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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 |
| 0.00 | 0.97 | 0.00 | 0.68 | -22.09 | 95.53 | 44.01 | 245.06 | 0.7123 | 594.0 | 503.7 | |
| 0.00 | 1.14 | 0.00 | 0.83 | -25.12 | 96.79 | 45.27 | 241.40 | 0.7349 | 563.0 | 418.7 | |
| 0.00 | 0.88 | 0.00 | 0.62 | -22.14 | 95.28 | 43.75 | 244.91 | 0.7096 | 565.0 | 543.2 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -30.23 | 84.52 | 33.00 | 228.29 | 0.6327 | 657.0 | 513.9 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -27.31 | 76.73 | 25.21 | 225.93 | 0.5288 | -692.0 | -602.7 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -29.03 | 76.82 | 25.30 | 223.48 | 0.5452 | -564.0 | -476.8 | |
| 0.00 | 2.02 | 0.00 | 1.19 | -28.78 | 76.53 | 25.01 | 223.54 | 0.5400 | -973.0 | -723.6 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -27.46 | 75.50 | 23.98 | 224.43 | 0.5172 | -589.0 | -489.7 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -27.95 | 75.50 | 23.98 | 223.70 | 0.5218 | -645.0 | -568.7 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -27.01 | 74.66 | 23.14 | 224.20 | 0.5042 | -792.0 | -636.3 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -27.60 | 70.98 | 19.46 | 218.79 | 0.4731 | -802.0 | -561.5 | |
| 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. | |