SDO HMI 2014-04-14 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.95 | 270.46 | 26.14 | 141.90 | 12.17 | 263.03 | -6.59 | 19.73 | 0.3291 | -969.0 | -382.1 | |
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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 |
| 7.96 | 258.98 | 4.17 | 135.52 | 12.37 | 263.79 | -5.83 | 17.78 | 0.3265 | -1191.4 | -426.0 | |
| 22.63 | -1.00 | 11.84 | -1.00 | 12.12 | 263.70 | -5.92 | 18.28 | 0.3229 | -1506.4 | 999999 | |
| 18.39 | -1.00 | 9.62 | -1.00 | 12.00 | 263.33 | -6.29 | 19.46 | 0.3230 | -1460.6 | 999999 | |
| 0.97 | -1.00 | 0.51 | -1.00 | 12.10 | 262.83 | -6.79 | 20.76 | 0.3274 | -646.6 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 12.60 | 260.77 | -8.85 | 25.65 | 0.3484 | -735.0 | -569.8 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 14.44 | 259.66 | -9.96 | 26.04 | 0.3830 | -756.0 | -578.4 | |
| 0.00 | 1.24 | 0.00 | 0.69 | 17.13 | 255.05 | -14.57 | 31.99 | 0.4556 | 534.0 | 382.1 | |
| 0.00 | 1.50 | 0.00 | 0.83 | 16.10 | 253.83 | -15.79 | 35.42 | 0.4529 | 785.0 | 685.4 | |
| 0.00 | 1.50 | 0.00 | 0.82 | 12.70 | 252.98 | -16.64 | 41.89 | 0.4200 | 631.0 | 424.2 | |
| 0.00 | 1.41 | 0.00 | 0.80 | 15.62 | 250.43 | -19.19 | 41.47 | 0.4799 | 802.0 | 702.7 | |
| 0.00 | 1.68 | 0.00 | 0.92 | 9.33 | 249.42 | -20.20 | 53.39 | 0.4263 | 559.0 | 446.4 | |
| 0.00 | 1.33 | 0.00 | 0.77 | 11.23 | 243.62 | -26.01 | 56.82 | 0.5159 | 791.0 | 738.0 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 10.74 | 243.46 | -26.16 | 57.80 | 0.5140 | 522.0 | 482.1 | |
| 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. | |