SDO HMI 2014-07-07 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.27 | 17.09 | 1.59 | 11.86 | 12.12 | 278.12 | 43.94 | 283.88 | 0.7009 | -221.8 | -168.8 | |
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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 | 0.82 | 0.00 | 0.63 | 10.47 | 283.94 | 49.76 | 280.71 | 0.7662 | -375.0 | -386.1 | |
| 0.00 | 0.73 | 0.00 | 0.53 | 11.04 | 281.52 | 47.34 | 281.74 | 0.7395 | -599.0 | -516.9 | |
| 0.00 | 0.64 | 0.00 | 0.46 | 7.63 | 280.86 | 46.69 | 277.14 | 0.7291 | -532.0 | -408.4 | |
| 0.00 | 1.45 | 0.00 | 1.03 | 10.86 | 279.54 | 45.36 | 281.74 | 0.7161 | -549.0 | -387.3 | |
| 0.00 | 0.36 | 0.00 | 0.26 | 10.80 | 279.30 | 45.13 | 281.70 | 0.7132 | -525.0 | -424.2 | |
| 0.00 | 0.91 | 0.00 | 0.64 | 10.88 | 278.92 | 44.75 | 281.87 | 0.7087 | -490.0 | -425.6 | |
| 2.27 | 4.09 | 1.59 | 2.87 | 11.50 | 278.96 | 44.78 | 282.73 | 0.7100 | -758.6 | -560.1 | |
| 0.00 | 1.09 | 0.00 | 0.75 | 11.51 | 278.09 | 43.91 | 282.88 | 0.6994 | -731.0 | -681.6 | |
| 0.00 | 1.27 | 0.00 | 0.89 | 12.83 | 278.32 | 44.15 | 284.71 | 0.7044 | -565.0 | -342.8 | |
| 0.00 | 1.27 | 0.00 | 0.88 | 12.99 | 278.10 | 43.92 | 284.99 | 0.7020 | -311.0 | -337.9 | |
| 0.00 | 0.91 | 0.00 | 0.61 | 12.93 | 275.78 | 41.60 | 285.41 | 0.6735 | 772.0 | 644.0 | |
| 0.00 | 0.91 | 0.00 | 0.61 | 14.03 | 275.51 | 41.33 | 287.09 | 0.6726 | 503.0 | 422.0 | |
| 0.00 | 1.73 | 0.00 | 1.12 | 14.33 | 273.54 | 39.37 | 288.08 | 0.6488 | 766.0 | 588.2 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 16.98 | 272.23 | 38.06 | 292.56 | 0.6407 | 606.0 | 468.8 | |
| 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. | |