SDO HMI 2014-07-05 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.91 | 19.08 | 1.54 | 9.96 | -13.64 | 255.09 | -6.66 | 159.35 | 0.3162 | 598.7 | 534.1 | |
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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 | 1.00 | 0.00 | 0.52 | -12.65 | 259.70 | -2.05 | 172.77 | 0.2787 | 894.0 | 758.9 | |
| 0.00 | 1.09 | 0.00 | 0.56 | -12.68 | 259.29 | -2.46 | 171.38 | 0.2802 | 939.0 | 809.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -13.73 | 257.80 | -3.95 | 167.16 | 0.3022 | 792.0 | 627.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -14.28 | 257.54 | -4.21 | 166.77 | 0.3120 | 822.0 | 663.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -12.75 | 257.44 | -4.30 | 165.19 | 0.2876 | 828.0 | 668.8 | |
| 0.00 | 1.73 | 0.00 | 0.90 | -14.18 | 257.38 | -4.36 | 166.22 | 0.3111 | 786.0 | 660.5 | |
| 0.00 | 3.00 | 0.00 | 1.55 | -11.72 | 254.46 | -7.29 | 154.39 | 0.2887 | 788.0 | 574.6 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -13.88 | 253.66 | -8.09 | 155.19 | 0.3268 | 848.0 | 574.8 | |
| 0.00 | 1.64 | 0.00 | 0.86 | -13.72 | 253.54 | -8.21 | 154.65 | 0.3253 | 890.0 | 716.8 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -14.62 | 252.96 | -8.78 | 154.35 | 0.3427 | 812.0 | 567.1 | |
| 2.91 | 4.27 | 1.54 | 2.26 | -14.95 | 251.67 | -10.08 | 151.63 | 0.3572 | -967.5 | -715.9 | |
| 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. | |