SDO HMI 2014-04-13 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.50 | 47.08 | 4.39 | 27.59 | -9.46 | 242.29 | -32.29 | 98.66 | 0.5352 | 261.8 | 426.5 | |
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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 | 1.50 | 0.00 | 0.86 | -10.40 | 244.70 | -29.88 | 100.92 | 0.5010 | 912.0 | 752.4 | |
| 0.79 | 11.39 | 0.46 | 6.64 | -8.70 | 242.81 | -31.77 | 97.31 | 0.5267 | 1025.8 | 721.9 | |
| 0.00 | 3.36 | 0.00 | 1.95 | -8.97 | 242.75 | -31.83 | 97.81 | 0.5279 | 754.0 | 526.8 | |
| 0.00 | 1.06 | 0.00 | 0.62 | -9.30 | 242.65 | -31.93 | 98.41 | 0.5297 | 359.0 | 195.8 | |
| 6.71 | 16.96 | 3.93 | 9.94 | -9.77 | 242.42 | -32.16 | 99.27 | 0.5337 | -917.5 | -8.4 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -9.49 | 242.27 | -32.31 | 98.72 | 0.5355 | -60.0 | -94.7 | |
| 0.00 | 2.74 | 0.00 | 1.61 | -9.26 | 241.86 | -32.72 | 98.23 | 0.5412 | 342.0 | 358.8 | |
| 0.00 | 1.50 | 0.00 | 0.88 | -9.61 | 241.71 | -32.87 | 98.87 | 0.5437 | 648.0 | 622.5 | |
| 0.00 | 1.24 | 0.00 | 0.73 | -9.87 | 241.50 | -33.08 | 99.32 | 0.5471 | 682.0 | 554.5 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -11.10 | 240.69 | -33.90 | 101.39 | 0.5604 | 716.0 | 514.4 | |
| 0.00 | 2.21 | 0.00 | 1.31 | -9.08 | 240.86 | -33.73 | 97.80 | 0.5555 | 756.0 | 647.9 | |
| 0.00 | 1.41 | 0.00 | 0.85 | -11.54 | 240.48 | -34.10 | 102.13 | 0.5641 | 676.0 | 606.2 | |
| 0.00 | 1.77 | 0.00 | 1.05 | -9.21 | 240.55 | -34.03 | 98.01 | 0.5601 | 615.0 | 522.2 | |
| 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. | |