SDO HMI 2014-06-02 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.63 | 47.74 | 8.68 | 24.91 | -18.67 | 330.30 | -2.70 | 172.02 | 0.3185 | 359.0 | 171.9 | |
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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 | 2.44 | 0.00 | 1.26 | -17.10 | 333.62 | 0.61 | 182.04 | 0.2876 | 904.0 | 676.7 | |
| 15.00 | 26.66 | 7.83 | 13.92 | -18.86 | 331.34 | -1.66 | 175.02 | 0.3179 | 1125.2 | 683.8 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -17.16 | 331.10 | -1.90 | 173.70 | 0.2902 | -708.0 | -506.4 | |
| 1.63 | -2.00 | 0.85 | -2.00 | -18.79 | 331.05 | -1.95 | 174.14 | 0.3172 | 1016.5 | 999999 | |
| 0.00 | 2.62 | 0.00 | 1.36 | -18.34 | 330.96 | -2.04 | 173.70 | 0.3100 | 386.0 | 422.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -19.34 | 330.40 | -2.61 | 172.44 | 0.3275 | 660.0 | 513.4 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -19.08 | 329.82 | -3.18 | 170.67 | 0.3246 | 820.0 | 574.4 | |
| 0.00 | 2.26 | 0.00 | 1.18 | -18.53 | 329.64 | -3.36 | 169.83 | 0.3163 | 867.0 | 572.0 | |
| 0.00 | 1.63 | 0.00 | 0.85 | -18.72 | 327.96 | -5.04 | 165.12 | 0.3254 | -884.0 | -766.7 | |
| 0.00 | 1.72 | 0.00 | 0.90 | -18.69 | 327.45 | -5.55 | 163.65 | 0.3271 | -893.0 | -727.0 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -18.05 | 326.41 | -6.59 | 160.12 | 0.3224 | -935.0 | -710.1 | |
| 0.00 | 2.35 | 0.00 | 1.24 | -19.52 | 326.12 | -6.88 | 160.91 | 0.3468 | -671.0 | -375.3 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -18.43 | 326.01 | -7.00 | 159.45 | 0.3306 | -822.0 | -598.8 | |
| 0.00 | 1.63 | 0.00 | 0.85 | -18.62 | 325.90 | -7.10 | 159.39 | 0.3342 | -974.0 | -779.5 | |
| 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. | |