SDO HMI 2014-07-17 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.27 | 0.00 | 8.33 | -21.14 | 148.61 | 46.23 | 238.42 | 0.7917 | -87.8 | -36.5 | |
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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 | 1.48 | -20.50 | 156.66 | 54.27 | 242.71 | 0.8577 | 320.0 | 279.2 | |
| 0.00 | 0.82 | 0.00 | 0.68 | -17.67 | 151.83 | 49.45 | 244.09 | 0.8070 | 407.0 | 393.4 | |
| 0.00 | 0.73 | 0.00 | 0.61 | -18.59 | 151.84 | 49.45 | 243.02 | 0.8103 | 197.0 | 307.4 | |
| 0.00 | 0.82 | 0.00 | 0.67 | -18.02 | 150.59 | 48.21 | 243.17 | 0.7967 | 333.0 | 285.3 | |
| 0.00 | 0.73 | 0.00 | 0.57 | -16.91 | 149.49 | 47.11 | 244.03 | 0.7820 | 568.0 | 526.9 | |
| 0.00 | 0.27 | 0.00 | 0.22 | -18.66 | 148.73 | 46.35 | 241.59 | 0.7816 | 227.0 | 342.3 | |
| 0.00 | 0.82 | 0.00 | 0.64 | -22.93 | 146.19 | 43.80 | 235.32 | 0.7774 | -544.0 | -433.0 | |
| 0.00 | 0.73 | 0.00 | 0.53 | -18.27 | 144.33 | 41.95 | 239.86 | 0.7362 | -549.0 | -440.5 | |
| 0.00 | 1.18 | 0.00 | 0.93 | -24.26 | 145.54 | 43.16 | 233.45 | 0.7785 | -437.0 | -381.3 | |
| 0.00 | 1.36 | 0.00 | 1.04 | -24.09 | 143.84 | 41.46 | 232.66 | 0.7625 | -506.0 | -450.5 | |
| 0.00 | 0.73 | 0.00 | 0.55 | -24.61 | 143.25 | 40.86 | 231.70 | 0.7601 | -433.0 | -377.9 | |
| 0.00 | 0.54 | 0.00 | 0.41 | -27.02 | 140.47 | 38.08 | 227.22 | 0.7509 | -637.0 | -488.2 | |
| 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. | |