SDO HMI 2014-11-03 15:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.28 | 37.35 | 6.50 | 19.99 | -17.35 | 98.65 | -2.57 | 174.35 | 0.3787 | 5.4 | -123.4 | |
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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 |
| 10.03 | 15.65 | 5.31 | 8.28 | -16.41 | 103.83 | 2.61 | 187.09 | 0.3550 | 1049.4 | 696.5 | |
| 2.25 | 5.53 | 1.19 | 2.93 | -16.81 | 100.35 | -0.87 | 177.68 | 0.3593 | 1114.5 | 828.5 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -17.39 | 99.20 | -2.02 | 174.75 | 0.3699 | 689.0 | 495.9 | |
| 0.00 | 1.47 | 0.00 | 0.78 | -16.98 | 95.71 | -5.51 | 165.69 | 0.3731 | -958.0 | -769.5 | |
| 0.00 | 2.42 | 0.00 | 1.30 | -17.47 | 94.29 | -6.93 | 162.61 | 0.3870 | -906.0 | -703.9 | |
| 0.00 | 1.56 | 0.00 | 0.84 | -17.63 | 94.19 | -7.03 | 162.51 | 0.3899 | -882.0 | -749.1 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -18.09 | 93.73 | -7.49 | 161.82 | 0.3991 | -894.0 | -816.5 | |
| 0.00 | 1.30 | 0.00 | 0.69 | -16.58 | 93.73 | -7.49 | 160.51 | 0.3763 | -734.0 | -577.4 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -18.09 | 93.38 | -7.84 | 161.04 | 0.4009 | -894.0 | -693.4 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -16.26 | 91.58 | -9.64 | 155.16 | 0.3845 | -852.0 | -583.6 | |
| 0.00 | 2.68 | 0.00 | 1.48 | -19.83 | 91.21 | -10.01 | 158.02 | 0.4386 | -678.0 | -579.1 | |
| 0.00 | 1.82 | 0.00 | 1.03 | -22.88 | 89.25 | -11.97 | 157.12 | 0.4935 | -701.0 | -526.7 | |
| 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. | |