SDO HMI 2014-04-22 04:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.38 | 0.00 | 11.44 | -16.20 | 164.80 | 0.28 | 183.02 | 0.2146 | -720.9 | -641.9 | |
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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 | 0.62 | 0.00 | 0.32 | -5.56 | 177.15 | 12.64 | 267.03 | 0.2190 | 696.0 | 531.3 | |
| 0.00 | 2.04 | 0.00 | 1.03 | -11.72 | 173.22 | 8.71 | 231.61 | 0.1899 | -769.0 | -656.6 | |
| 0.00 | 0.80 | 0.00 | 0.41 | -18.45 | 170.74 | 6.22 | 203.86 | 0.2554 | -858.0 | -689.0 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -29.57 | 169.21 | 4.69 | 189.71 | 0.4234 | -797.0 | -530.1 | |
| 0.00 | 0.98 | 0.00 | 0.50 | -17.72 | 168.02 | 3.50 | 194.82 | 0.2284 | -761.0 | -547.8 | |
| 0.00 | 0.89 | 0.00 | 0.46 | -20.52 | 167.95 | 3.43 | 191.84 | 0.2742 | -833.0 | -700.7 | |
| 0.00 | 1.42 | 0.00 | 0.73 | -20.39 | 167.72 | 3.20 | 191.17 | 0.2714 | -901.0 | -665.5 | |
| 0.00 | 0.98 | 0.00 | 0.51 | -24.22 | 166.55 | 2.03 | 185.61 | 0.3317 | -651.0 | -497.1 | |
| 0.00 | 3.02 | 0.00 | 1.50 | -7.41 | 165.49 | 0.97 | 202.07 | 0.0450 | -763.0 | -633.4 | |
| 0.00 | 1.51 | 0.00 | 0.75 | -9.40 | 162.75 | -1.77 | 158.17 | 0.0824 | -903.0 | -690.6 | |
| 0.00 | 1.51 | 0.00 | 0.75 | -8.58 | 162.69 | -1.83 | 153.02 | 0.0699 | -886.0 | -679.2 | |
| 0.00 | 1.86 | 0.00 | 0.97 | -21.64 | 161.52 | -3.00 | 170.34 | 0.2914 | -717.0 | -612.1 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -19.45 | 160.76 | -3.76 | 166.08 | 0.2578 | -825.0 | -670.5 | |
| 0.00 | 1.42 | 0.00 | 0.71 | -10.07 | 159.37 | -5.15 | 134.95 | 0.1254 | -947.0 | -747.2 | |
| 0.00 | 3.29 | 0.00 | 1.72 | -23.38 | 158.18 | -6.34 | 162.20 | 0.3327 | -898.0 | -841.9 | |
| 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. | |