SDO HMI 2014-04-06 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.55 | 0.00 | 11.07 | 5.73 | 25.77 | 8.35 | 324.95 | 0.2626 | -81.5 | 15.3 | |
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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 | 1.23 | 0.00 | 0.63 | 2.71 | 29.54 | 12.13 | 306.21 | 0.2612 | -889.0 | -699.9 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 2.61 | 29.30 | 11.88 | 306.48 | 0.2569 | -607.0 | -446.1 | |
| 0.00 | 4.05 | 0.00 | 2.08 | 3.55 | 29.28 | 11.86 | 309.37 | 0.2665 | -982.0 | -809.0 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 1.68 | 28.40 | 10.98 | 305.61 | 0.2353 | -807.0 | -633.5 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 3.56 | 28.36 | 10.94 | 311.71 | 0.2549 | -739.0 | -594.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 2.11 | 26.76 | 9.34 | 311.65 | 0.2180 | -686.0 | -524.9 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 3.92 | 26.32 | 8.90 | 318.69 | 0.2349 | -836.0 | -647.9 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 8.14 | 25.02 | 7.60 | 332.17 | 0.2816 | 697.0 | 595.9 | |
| 0.00 | 1.50 | 0.00 | 0.77 | 7.80 | 24.76 | 7.35 | 332.38 | 0.2746 | 859.0 | 759.6 | |
| 0.00 | 4.66 | 0.00 | 2.40 | 8.26 | 24.50 | 7.08 | 333.99 | 0.2795 | 606.0 | 584.0 | |
| 0.00 | 1.50 | 0.00 | 0.77 | 8.00 | 24.07 | 6.65 | 334.99 | 0.2725 | 776.0 | 633.1 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 8.14 | 21.66 | 4.25 | 343.56 | 0.2603 | 780.0 | 597.2 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 7.32 | 17.03 | -0.39 | 1.65 | 0.2362 | 769.0 | 643.5 | |
| 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. | |