SDO HMI 2014-04-10 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.28 | 0.00 | 12.14 | -20.41 | 322.11 | 8.48 | 207.41 | 0.3119 | -395.0 | -271.6 | |
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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 | 2.73 | 0.00 | 1.45 | -13.95 | 332.91 | 19.28 | 245.68 | 0.3532 | 825.0 | 640.0 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -15.30 | 332.51 | 18.88 | 241.72 | 0.3559 | 673.0 | 505.8 | |
| 0.00 | 1.94 | 0.00 | 1.04 | -19.83 | 331.92 | 18.29 | 230.32 | 0.3852 | 815.0 | 687.4 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -17.98 | 330.76 | 17.12 | 232.75 | 0.3533 | 600.0 | 436.7 | |
| 0.00 | 2.38 | 0.00 | 1.22 | -18.65 | 319.74 | 6.11 | 204.56 | 0.2436 | -676.0 | -536.9 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -21.04 | 319.12 | 5.49 | 198.88 | 0.2769 | -698.0 | -566.8 | |
| 0.00 | 2.47 | 0.00 | 1.27 | -20.89 | 318.98 | 5.35 | 198.64 | 0.2738 | -666.0 | -630.2 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -20.52 | 318.78 | 5.15 | 198.44 | 0.2668 | -895.0 | -763.3 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -23.50 | 317.18 | 3.54 | 190.64 | 0.3084 | -800.0 | -637.4 | |
| 0.00 | 2.12 | 0.00 | 1.10 | -23.72 | 316.99 | 3.35 | 189.94 | 0.3114 | -836.0 | -693.5 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -23.94 | 316.79 | 3.16 | 189.26 | 0.3145 | -817.0 | -687.1 | |
| 0.00 | 1.76 | 0.00 | 0.91 | -22.71 | 316.28 | 2.64 | 188.39 | 0.2930 | -857.0 | -689.3 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -23.60 | 316.19 | 2.56 | 187.69 | 0.3074 | -911.0 | -775.2 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -24.10 | 316.11 | 2.47 | 187.20 | 0.3155 | -918.0 | -741.1 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -24.20 | 315.02 | 1.39 | 184.03 | 0.3154 | -764.0 | -635.2 | |
| 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. | |