SDO HMI 2014-04-22 10:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.39 | 0.00 | 8.90 | -16.93 | 163.89 | 2.66 | 194.58 | 0.2289 | -781.5 | -656.8 | |
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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 | 0.44 | 0.00 | 0.24 | -22.90 | 180.00 | 18.77 | 223.55 | 0.4319 | -425.0 | -399.2 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -12.30 | 171.61 | 10.38 | 233.87 | 0.2190 | -869.0 | -720.6 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -12.30 | 171.33 | 10.10 | 233.12 | 0.2151 | -982.0 | -846.3 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -16.68 | 170.80 | 9.56 | 218.00 | 0.2597 | -957.0 | -821.8 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -24.30 | 166.57 | 5.34 | 194.38 | 0.3431 | -775.0 | -610.4 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -7.21 | 165.73 | 4.50 | 243.38 | 0.0875 | -375.0 | -442.6 | |
| 0.00 | 1.33 | 0.00 | 0.66 | -9.40 | 162.91 | 1.68 | 200.61 | 0.0824 | -899.0 | -718.1 | |
| 0.00 | 1.15 | 0.00 | 0.57 | -8.46 | 162.54 | 1.31 | 200.48 | 0.0649 | -811.0 | -592.0 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -19.89 | 161.57 | 0.34 | 181.23 | 0.2584 | -876.0 | -646.1 | |
| 0.00 | 2.31 | 0.00 | 1.18 | -19.40 | 161.12 | -0.11 | 179.58 | 0.2498 | -547.0 | -602.5 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -19.58 | 160.99 | -0.24 | 179.11 | 0.2530 | -821.0 | -618.9 | |
| 0.00 | 0.80 | 0.00 | 0.41 | -17.97 | 160.14 | -1.09 | 175.39 | 0.2263 | -854.0 | -689.6 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -17.66 | 159.70 | -1.53 | 173.38 | 0.2217 | -851.0 | -616.7 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -18.30 | 159.47 | -1.76 | 172.79 | 0.2332 | -805.0 | -633.7 | |
| 0.00 | 1.07 | 0.00 | 0.56 | -23.34 | 158.26 | -2.98 | 171.39 | 0.3199 | -876.0 | -749.2 | |
| 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. | |