SDO HMI 2014-10-06 08:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.91 | 0.00 | 9.02 | -18.09 | 99.65 | -14.71 | 150.40 | 0.4846 | -189.5 | -140.2 | |
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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 | 1.23 | 0.00 | 0.71 | -23.45 | 109.41 | -4.95 | 170.97 | 0.5063 | 763.0 | 649.5 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -15.33 | 107.51 | -6.85 | 162.73 | 0.3893 | 750.0 | 651.6 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -16.91 | 106.25 | -8.11 | 161.15 | 0.4195 | 781.0 | 815.8 | |
| 0.00 | 1.49 | 0.00 | 0.81 | -15.70 | 106.27 | -8.09 | 160.18 | 0.4013 | 808.0 | 563.4 | |
| 0.00 | 2.20 | 0.00 | 1.23 | -17.54 | 99.97 | -14.39 | 149.54 | 0.4695 | -861.0 | -714.2 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -16.03 | 97.98 | -16.38 | 144.35 | 0.4670 | -637.0 | -577.2 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -17.80 | 97.79 | -16.57 | 146.23 | 0.4906 | -780.0 | -590.5 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -16.43 | 95.88 | -18.48 | 141.57 | 0.4911 | -769.0 | -620.4 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -16.71 | 95.39 | -18.97 | 141.20 | 0.4990 | -612.0 | -524.5 | |
| 0.00 | 0.53 | 0.00 | 0.32 | -21.36 | 93.55 | -20.81 | 144.25 | 0.5685 | -672.0 | -576.2 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -22.35 | 93.36 | -21.00 | 145.08 | 0.5812 | -507.0 | -440.3 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -19.15 | 93.56 | -20.80 | 141.71 | 0.5436 | -659.0 | -546.8 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -18.15 | 93.55 | -20.81 | 140.48 | 0.5327 | -69.0 | -60.1 | |
| 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. | |