SDO HMI 2014-04-14 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.66 | 109.64 | 19.29 | 61.14 | -9.30 | 242.37 | -27.25 | 99.26 | 0.4599 | 295.8 | 62.9 | |
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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 |
| 0.00 | 0.80 | 0.00 | 0.43 | -10.52 | 244.94 | -24.68 | 102.78 | 0.4227 | 765.0 | 585.6 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -9.94 | 244.01 | -25.61 | 101.12 | 0.4357 | 741.0 | 556.6 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -4.76 | 243.57 | -26.05 | 89.20 | 0.4395 | 757.0 | 547.2 | |
| 4.77 | 98.06 | 2.65 | 54.62 | -8.41 | 242.88 | -26.74 | 97.41 | 0.4507 | 1029.0 | -27.4 | |
| 2.56 | -4.00 | 1.42 | -4.00 | -8.65 | 242.83 | -26.79 | 97.94 | 0.4518 | 1031.7 | 999999 | |
| 3.01 | -4.00 | 1.67 | -4.00 | -9.97 | 242.61 | -27.01 | 100.79 | 0.4572 | -943.8 | 999999 | |
| 9.11 | -4.00 | 5.06 | -4.00 | -8.55 | 242.63 | -26.99 | 97.68 | 0.4547 | 945.2 | 999999 | |
| 12.20 | -4.00 | 6.81 | -4.00 | -9.80 | 242.29 | -27.33 | 100.34 | 0.4619 | -960.2 | 999999 | |
| 3.01 | -4.00 | 1.68 | -4.00 | -9.84 | 241.87 | -27.75 | 100.33 | 0.4683 | 958.4 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.65 | -10.00 | 241.51 | -28.11 | 100.59 | 0.4740 | 683.0 | 455.8 | |
| 0.00 | 1.50 | 0.00 | 0.85 | -10.62 | 241.03 | -28.59 | 101.74 | 0.4824 | 780.0 | 550.7 | |
| 0.00 | 3.36 | 0.00 | 1.91 | -11.57 | 240.61 | -29.01 | 103.56 | 0.4907 | 577.0 | 578.4 | |
| 0.00 | 1.06 | 0.00 | 0.61 | -9.49 | 239.07 | -30.55 | 99.06 | 0.5097 | 610.0 | 499.1 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -9.84 | 238.71 | -30.91 | 99.67 | 0.5154 | 690.0 | 596.6 | |
| 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. | |