SDO HMI 2014-07-10 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.72 | 0.00 | 7.75 | -23.92 | 217.27 | 17.87 | 208.83 | 0.5707 | -546.8 | -455.7 | |
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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 | 0.71 | -25.56 | 247.82 | 48.41 | 235.11 | 0.8248 | -509.0 | -419.2 | |
| 0.00 | 1.00 | 0.00 | 0.67 | -14.22 | 237.72 | 38.31 | 243.77 | 0.6722 | 645.0 | 534.3 | |
| 0.00 | 0.64 | 0.00 | 0.40 | -17.33 | 230.82 | 31.41 | 234.74 | 0.6115 | -541.0 | -517.7 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -21.48 | 216.86 | 17.45 | 213.30 | 0.5102 | -707.0 | -538.6 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -22.05 | 216.38 | 16.97 | 211.95 | 0.5133 | -719.0 | -555.8 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -22.11 | 216.15 | 16.74 | 211.53 | 0.5122 | -741.0 | -581.8 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -22.67 | 215.53 | 16.12 | 209.99 | 0.5145 | -595.0 | -555.7 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -25.70 | 211.10 | 11.70 | 200.38 | 0.5266 | -667.0 | -478.3 | |
| 0.00 | 2.27 | 0.00 | 1.34 | -28.58 | 205.12 | 5.71 | 189.26 | 0.5450 | -744.0 | -633.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -28.50 | 204.17 | 4.77 | 187.77 | 0.5418 | -783.0 | -595.6 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -27.67 | 203.03 | 3.62 | 186.12 | 0.5275 | -654.0 | -518.8 | |
| 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. | |