SDO HMI 2014-04-11 18:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.62 | 0.00 | 10.13 | -22.19 | 319.10 | 17.01 | 221.83 | 0.4104 | -112.2 | -337.1 | |
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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 | 1.06 | 0.00 | 0.62 | -17.31 | 332.59 | 30.50 | 246.40 | 0.5309 | 741.0 | 668.5 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -17.26 | 331.06 | 28.97 | 245.63 | 0.5099 | 624.0 | 549.2 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -17.36 | 329.51 | 27.41 | 244.45 | 0.4891 | 571.0 | 618.4 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -16.89 | 329.08 | 26.99 | 245.09 | 0.4807 | 736.0 | 660.9 | |
| 0.00 | 1.15 | 0.00 | 0.65 | -16.74 | 328.91 | 26.82 | 245.27 | 0.4777 | 936.0 | 754.1 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -17.58 | 325.59 | 23.50 | 240.97 | 0.4366 | 723.0 | 664.6 | |
| 0.00 | 1.50 | 0.00 | 0.81 | -23.61 | 317.08 | 14.98 | 217.59 | 0.3901 | -786.0 | -595.9 | |
| 0.00 | 1.76 | 0.00 | 0.95 | -24.19 | 316.63 | 14.54 | 215.83 | 0.3929 | -823.0 | -674.3 | |
| 0.00 | 1.94 | 0.00 | 1.04 | -24.20 | 316.26 | 14.17 | 215.14 | 0.3896 | -809.0 | -738.1 | |
| 0.00 | 3.00 | 0.00 | 1.59 | -21.91 | 315.92 | 13.83 | 218.48 | 0.3579 | -915.0 | -794.5 | |
| 0.00 | 2.03 | 0.00 | 1.09 | -24.27 | 316.00 | 13.90 | 214.54 | 0.3880 | -955.0 | -800.4 | |
| 0.00 | 2.47 | 0.00 | 1.32 | -25.03 | 314.45 | 12.36 | 210.42 | 0.3846 | -783.0 | -690.9 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -27.18 | 306.89 | 4.79 | 191.55 | 0.3728 | -718.0 | -441.6 | |
| 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. | |