SDO HMI 2014-04-09 10:02:48 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.66 | 0.00 | 7.70 | -14.52 | 306.37 | -26.50 | 110.81 | 0.4632 | 77.4 | 62.0 | |
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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 | 0.88 | 0.00 | 0.52 | -10.34 | 300.36 | -32.51 | 99.81 | 0.5386 | -664.0 | -562.7 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -9.42 | 312.20 | -20.67 | 100.72 | 0.3559 | 765.0 | 724.5 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -9.61 | 312.59 | -20.28 | 101.40 | 0.3501 | 20.0 | 37.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -10.14 | 312.71 | -20.16 | 102.95 | 0.3497 | 2.0 | 12.1 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -11.11 | 309.45 | -23.42 | 103.99 | 0.4037 | 792.0 | 674.2 | |
| 0.00 | 0.71 | 0.00 | 0.46 | -13.14 | 291.99 | -40.88 | 103.14 | 0.6568 | -237.0 | -274.9 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -13.62 | 299.36 | -33.51 | 105.53 | 0.5590 | -453.0 | -347.4 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -15.09 | 297.95 | -34.92 | 107.65 | 0.5822 | -578.0 | -470.9 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -16.40 | 296.26 | -36.61 | 109.27 | 0.6082 | -692.0 | -600.5 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -17.40 | 309.03 | -23.84 | 118.08 | 0.4390 | 464.0 | 451.7 | |
| 0.00 | 2.03 | 0.00 | 1.07 | -17.15 | 315.37 | -17.50 | 124.51 | 0.3503 | 13.0 | 1.7 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -18.02 | 309.42 | -23.45 | 119.74 | 0.4376 | 785.0 | 630.7 | |
| 0.00 | 1.32 | 0.00 | 0.76 | -20.63 | 305.55 | -27.32 | 121.49 | 0.5057 | 789.0 | 531.1 | |
| 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. | |