SDO HMI 2014-10-10 03:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.79 | 0.00 | 8.99 | 13.87 | 92.92 | 28.59 | 288.49 | 0.4939 | 65.3 | 36.9 | |
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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 | 1.32 | 0.00 | 0.78 | 7.95 | 98.36 | 34.04 | 274.98 | 0.5586 | -751.0 | -563.6 | |
| 0.00 | 0.88 | 0.00 | 0.53 | 11.78 | 98.71 | 34.39 | 281.78 | 0.5670 | -597.0 | -439.8 | |
| 0.00 | 0.70 | 0.00 | 0.42 | 12.26 | 98.75 | 34.42 | 282.62 | 0.5682 | -695.0 | -503.4 | |
| 0.00 | 2.37 | 0.00 | 1.42 | 12.05 | 98.68 | 34.35 | 282.27 | 0.5669 | -809.0 | -621.3 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 7.64 | 96.46 | 32.13 | 274.45 | 0.5308 | -618.0 | -457.6 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 13.07 | 93.54 | 29.21 | 285.58 | 0.4956 | -754.0 | -668.2 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 17.46 | 92.93 | 28.61 | 294.42 | 0.5036 | 689.0 | 571.8 | |
| 0.00 | 1.32 | 0.00 | 0.74 | 15.09 | 92.16 | 27.84 | 290.22 | 0.4825 | 683.0 | 458.9 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 12.42 | 88.91 | 24.59 | 286.13 | 0.4248 | 682.0 | 637.0 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 15.12 | 88.92 | 24.59 | 292.21 | 0.4357 | 652.0 | 563.6 | |
| 0.00 | 1.32 | 0.00 | 0.71 | 15.11 | 87.02 | 22.69 | 293.57 | 0.4081 | 903.0 | 779.9 | |
| 0.00 | 1.75 | 0.00 | 0.97 | 21.11 | 86.71 | 22.39 | 306.65 | 0.4448 | 794.0 | 586.1 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 17.05 | 84.22 | 19.90 | 300.79 | 0.3804 | 670.0 | 610.9 | |
| 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. | |