SDO HMI 2014-03-11 06:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.34 | 27.48 | 4.36 | 26.18 | -8.89 | 298.40 | -59.13 | 96.07 | 0.8535 | 49.2 | -16.3 | |
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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 | 1.21 | 0.00 | 0.89 | -12.63 | 309.78 | -47.74 | 100.54 | 0.7370 | 517.0 | 385.0 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -9.57 | 309.59 | -47.94 | 96.38 | 0.7390 | 563.0 | 489.7 | |
| 0.00 | 0.69 | 0.00 | 0.55 | -13.88 | 305.41 | -52.11 | 102.01 | 0.7856 | 334.0 | 264.2 | |
| 0.00 | 1.30 | 0.00 | 1.08 | -6.90 | 303.79 | -53.74 | 93.24 | 0.8040 | 392.0 | 316.4 | |
| 0.00 | 1.39 | 0.00 | 1.17 | -11.13 | 302.79 | -54.74 | 98.54 | 0.8123 | 478.0 | 375.8 | |
| 0.00 | 0.69 | 0.00 | 0.59 | -9.09 | 302.89 | -54.64 | 96.02 | 0.8119 | 510.0 | 412.6 | |
| 0.00 | 1.30 | 0.00 | 1.12 | -10.72 | 301.94 | -55.58 | 98.04 | 0.8208 | 449.0 | 396.3 | |
| 0.00 | 1.30 | 0.00 | 1.21 | -6.91 | 299.30 | -58.23 | 93.63 | 0.8478 | 401.0 | 377.5 | |
| 0.00 | 2.34 | 0.00 | 2.23 | -6.51 | 298.39 | -59.14 | 93.25 | 0.8563 | 435.0 | 336.7 | |
| 0.00 | 1.21 | 0.00 | 1.18 | -6.64 | 297.65 | -59.88 | 93.47 | 0.8628 | 315.0 | 233.9 | |
| 4.34 | 12.58 | 4.36 | 12.68 | -9.46 | 296.38 | -61.15 | 96.80 | 0.8721 | -697.4 | -417.1 | |
| 0.00 | 0.61 | 0.00 | 0.62 | -9.19 | 295.89 | -61.64 | 96.53 | 0.8763 | -200.0 | -172.1 | |
| 0.00 | 0.87 | 0.00 | 0.89 | -9.41 | 295.69 | -61.84 | 96.79 | 0.8779 | -226.0 | -146.6 | |
| 0.00 | 1.04 | 0.00 | 1.06 | -6.35 | 296.04 | -61.49 | 93.27 | 0.8767 | -365.0 | -354.2 | |
| 0.00 | 0.69 | 0.00 | 0.72 | -3.62 | 295.85 | -61.67 | 90.20 | 0.8805 | 342.0 | 272.5 | |
| 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. | |