SDO HMI 2014-05-19 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.58 | 59.83 | 7.69 | 31.45 | 9.87 | 180.18 | 15.32 | 308.73 | 0.3359 | -214.0 | -238.7 | |
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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 | 1.80 | 0.00 | 0.95 | 7.31 | 183.06 | 18.20 | 297.73 | 0.3515 | -877.0 | -729.2 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 9.55 | 182.01 | 17.15 | 304.72 | 0.3553 | 687.0 | 530.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 9.02 | 181.66 | 16.80 | 304.00 | 0.3458 | -764.0 | -588.9 | |
| 9.45 | 36.07 | 4.99 | 19.02 | 9.60 | 181.34 | 16.48 | 305.92 | 0.3468 | -1016.2 | -692.8 | |
| 5.13 | -4.00 | 2.70 | -4.00 | 9.26 | 181.23 | 16.36 | 305.28 | 0.3421 | -1148.8 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 10.67 | 179.00 | 14.14 | 312.66 | 0.3278 | -808.0 | -615.6 | |
| 0.00 | 5.94 | 0.00 | 3.13 | 12.13 | 178.56 | 13.70 | 316.74 | 0.3394 | -471.0 | -234.2 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 10.75 | 178.27 | 13.41 | 314.36 | 0.3200 | 543.0 | 436.3 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 10.10 | 178.12 | 13.25 | 313.16 | 0.3108 | 664.0 | 539.2 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 10.91 | 178.12 | 13.26 | 315.03 | 0.3200 | 775.0 | 595.7 | |
| 0.00 | 2.25 | 0.00 | 1.16 | 6.74 | 177.96 | 13.10 | 304.37 | 0.2739 | 817.0 | 687.8 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 10.10 | 177.89 | 13.03 | 313.64 | 0.3081 | 781.0 | 549.4 | |
| 0.00 | 1.53 | 0.00 | 0.80 | 10.13 | 177.64 | 12.78 | 314.26 | 0.3054 | 936.0 | 711.6 | |
| 0.00 | 2.79 | 0.00 | 1.46 | 12.49 | 176.04 | 11.17 | 323.15 | 0.3169 | 662.0 | 613.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 11.60 | 174.14 | 9.28 | 326.39 | 0.2866 | 800.0 | 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. | |