SDO HMI 2011-08-09 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.75 | 0.00 | 12.86 | -16.69 | 243.42 | 23.79 | 225.25 | 0.5471 | -164.3 | -135.5 | |
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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 | 1.26 | 0.00 | 0.76 | -14.68 | 246.74 | 27.11 | 231.81 | 0.5631 | 632.0 | 551.4 | |
| 0.00 | 1.99 | 0.00 | 1.19 | -14.93 | 246.46 | 26.83 | 231.16 | 0.5620 | 726.0 | 558.3 | |
| 0.00 | 3.43 | 0.00 | 2.04 | -14.56 | 246.23 | 26.60 | 231.46 | 0.5562 | 841.0 | 657.6 | |
| 0.00 | 1.44 | 0.00 | 0.86 | -14.78 | 246.16 | 26.52 | 231.06 | 0.5573 | 895.0 | 752.9 | |
| 0.00 | 1.81 | 0.00 | 1.06 | -17.29 | 242.55 | 22.92 | 223.46 | 0.5427 | -764.0 | -646.8 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -17.74 | 242.09 | 22.46 | 222.30 | 0.5427 | -669.0 | -567.5 | |
| 0.00 | 2.80 | 0.00 | 1.64 | -17.73 | 241.85 | 22.22 | 222.01 | 0.5402 | -792.0 | -572.4 | |
| 0.00 | 2.44 | 0.00 | 1.43 | -17.52 | 241.58 | 21.95 | 221.94 | 0.5354 | -913.0 | -718.8 | |
| 0.00 | 2.89 | 0.00 | 1.70 | -17.97 | 241.40 | 21.77 | 221.12 | 0.5385 | -657.0 | -633.4 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -17.71 | 241.36 | 21.73 | 221.42 | 0.5353 | -638.0 | -516.1 | |
| 0.00 | 1.35 | 0.00 | 0.80 | -19.78 | 240.50 | 20.87 | 217.73 | 0.5499 | -468.0 | -421.6 | |
| 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. | |