SDO HMI 2014-10-05 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.16 | 20.20 | 2.30 | 15.47 | -18.84 | 77.17 | -43.23 | 121.71 | 0.7623 | 296.0 | 270.8 | |
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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 | 1.05 | 0.00 | 0.76 | -20.86 | 82.36 | -38.05 | 127.18 | 0.7253 | 614.0 | 456.5 | |
| 0.00 | 2.20 | 0.00 | 1.61 | -21.65 | 81.20 | -39.21 | 127.32 | 0.7411 | 40.0 | 127.2 | |
| 3.16 | 7.11 | 2.30 | 5.19 | -18.21 | 79.62 | -40.78 | 122.28 | 0.7362 | 805.6 | 577.2 | |
| 0.00 | 1.41 | 0.00 | 1.00 | -15.40 | 79.54 | -40.87 | 118.76 | 0.7219 | 713.0 | 609.4 | |
| 0.00 | 1.84 | 0.00 | 1.39 | -16.84 | 76.83 | -43.58 | 119.03 | 0.7569 | 699.0 | 551.5 | |
| 0.00 | 0.88 | 0.00 | 0.69 | -19.24 | 75.80 | -44.61 | 121.32 | 0.7784 | 632.0 | 515.0 | |
| 0.00 | 0.97 | 0.00 | 0.76 | -18.96 | 75.58 | -44.83 | 120.88 | 0.7791 | 377.0 | 334.0 | |
| 0.00 | 0.79 | 0.00 | 0.60 | -16.86 | 76.12 | -44.28 | 118.69 | 0.7640 | 437.0 | 398.9 | |
| 0.00 | 0.44 | 0.00 | 0.34 | -14.55 | 74.97 | -45.43 | 115.33 | 0.7652 | 468.0 | 427.0 | |
| 0.00 | 0.53 | 0.00 | 0.48 | -24.18 | 70.74 | -49.66 | 124.27 | 0.8435 | -458.0 | -473.0 | |
| 0.00 | 0.70 | 0.00 | 0.59 | -18.96 | 72.54 | -47.87 | 119.36 | 0.8069 | -512.0 | -505.9 | |
| 0.00 | 1.23 | 0.00 | 1.08 | -20.37 | 70.79 | -49.61 | 120.13 | 0.8278 | -344.0 | -283.4 | |
| 0.00 | 1.05 | 0.00 | 0.98 | -20.27 | 68.24 | -52.17 | 118.92 | 0.8485 | -286.0 | -195.9 | |
| 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. | |