SDO HMI 2014-01-15 04:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.69 | 431.53 | 43.47 | 221.53 | -16.39 | 12.67 | 9.75 | 218.13 | 0.2641 | 1032.3 | 400.9 | |
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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 | 1.19 | 0.00 | 0.63 | -17.07 | 18.51 | 15.60 | 229.53 | 0.3394 | -670.0 | -562.1 | |
| 42.35 | 260.96 | 21.80 | 134.35 | -16.61 | 13.45 | 10.53 | 219.85 | 0.2747 | 1343.9 | 430.9 | |
| 4.25 | -2.00 | 2.19 | -2.00 | -16.73 | 12.80 | 9.88 | 217.80 | 0.2695 | 1122.1 | 999999 | |
| 0.68 | 9.35 | 0.35 | 4.78 | -15.33 | 12.18 | 9.26 | 219.57 | 0.2447 | 980.8 | 477.4 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -15.03 | 12.07 | 9.15 | 220.07 | 0.2397 | 734.0 | 495.1 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -17.20 | 12.07 | 9.16 | 214.69 | 0.2684 | 683.0 | 482.6 | |
| 36.39 | 148.46 | 18.61 | 75.89 | -16.05 | 11.71 | 8.79 | 216.29 | 0.2494 | 1272.5 | 430.4 | |
| 0.00 | 2.21 | 0.00 | 1.12 | -14.35 | 11.36 | 8.45 | 219.81 | 0.2233 | -666.0 | -571.9 | |
| 1.02 | -7.00 | 0.52 | -7.00 | -15.70 | 11.29 | 8.38 | 215.88 | 0.2404 | 1154.7 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -16.63 | 8.08 | 5.16 | 202.39 | 0.2274 | -845.0 | -673.5 | |
| 0.00 | 2.30 | 0.00 | 1.17 | -17.23 | 7.04 | 4.12 | 197.37 | 0.2311 | -811.0 | -590.6 | |
| 0.00 | 2.21 | 0.00 | 1.12 | -16.85 | 6.14 | 3.22 | 194.18 | 0.2205 | -829.0 | -668.9 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -18.12 | 4.89 | 1.97 | 187.93 | 0.2378 | -792.0 | -624.1 | |
| 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. | |