SDO HMI 2014-07-03 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.98 | 0.00 | 9.03 | 4.68 | 265.26 | -26.24 | 85.68 | 0.4387 | 100.2 | 68.0 | |
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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 | 1.09 | 0.00 | 0.55 | 1.66 | 279.46 | -12.05 | 96.56 | 0.2109 | -908.0 | -729.4 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 8.34 | 279.28 | -12.23 | 66.18 | 0.2301 | -751.0 | -646.9 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 3.41 | 278.45 | -13.06 | 88.26 | 0.2267 | -876.0 | -684.7 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 0.79 | 278.31 | -13.20 | 99.66 | 0.2326 | -919.0 | -757.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 3.24 | 274.65 | -16.85 | 89.05 | 0.2907 | -690.0 | -515.7 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 10.55 | 267.70 | -23.81 | 71.31 | 0.4206 | 791.0 | 669.0 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 8.71 | 261.14 | -30.36 | 78.12 | 0.5126 | 834.0 | 656.1 | |
| 0.00 | 0.55 | 0.00 | 0.32 | 1.61 | 259.51 | -31.99 | 91.92 | 0.5320 | 717.0 | 593.3 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -1.20 | 258.35 | -33.15 | 96.90 | 0.5528 | 660.0 | 581.9 | |
| 0.00 | 1.09 | 0.00 | 0.65 | 7.48 | 257.72 | -33.79 | 81.18 | 0.5601 | 615.0 | 474.0 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 7.82 | 257.50 | -34.00 | 80.64 | 0.5636 | 589.0 | 472.6 | |
| 0.00 | 1.36 | 0.00 | 0.89 | 5.49 | 250.81 | -40.69 | 85.18 | 0.6536 | 584.0 | 457.5 | |
| 0.00 | 1.36 | 0.00 | 0.92 | 4.42 | 248.88 | -42.63 | 86.84 | 0.6785 | 656.0 | 586.1 | |
| 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. | |