SDO HMI 2014-06-02 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.99 | 37.71 | 9.39 | 19.70 | -18.92 | 330.36 | -1.53 | 175.52 | 0.3207 | 508.7 | 103.7 | |
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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 | 1.54 | 0.00 | 0.79 | -17.09 | 333.62 | 1.72 | 185.74 | 0.2889 | 858.0 | 607.5 | |
| 15.73 | 24.49 | 8.21 | 12.79 | -18.88 | 331.38 | -0.51 | 178.48 | 0.3173 | 1115.0 | 637.2 | |
| 2.26 | -2.00 | 1.18 | -2.00 | -18.84 | 331.13 | -0.77 | 177.70 | 0.3169 | 1077.8 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -18.59 | 330.94 | -0.96 | 177.09 | 0.3128 | 779.0 | 585.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -23.40 | 330.83 | -1.06 | 177.50 | 0.3917 | 833.0 | 621.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -19.04 | 330.52 | -1.38 | 175.92 | 0.3207 | 929.0 | 767.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -18.74 | 327.53 | -4.36 | 167.06 | 0.3232 | -901.0 | -781.6 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -18.07 | 326.36 | -5.53 | 163.14 | 0.3175 | -892.0 | -631.9 | |
| 0.00 | 2.53 | 0.00 | 1.33 | -19.03 | 326.17 | -5.73 | 163.49 | 0.3335 | -955.0 | -756.6 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -18.42 | 326.03 | -5.87 | 162.54 | 0.3246 | -841.0 | -752.1 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -18.68 | 325.89 | -6.01 | 162.40 | 0.3293 | -880.0 | -746.9 | |
| 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. | |