SDO HMI 2014-04-11 04:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.57 | 130.80 | 57.33 | 179.79 | 4.35 | 241.57 | -68.20 | 82.99 | 0.9335 | -9.5 | -91.5 | |
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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 |
| 3.18 | 76.61 | 3.94 | 95.72 | 4.94 | 244.11 | -65.66 | 81.98 | 0.9184 | -898.0 | -336.3 | |
| 4.50 | -1.00 | 5.55 | -1.00 | 4.44 | 244.20 | -65.57 | 82.50 | 0.9173 | -752.1 | 999999 | |
| 2.03 | -1.00 | 2.52 | -1.00 | 4.73 | 244.08 | -65.70 | 82.21 | 0.9184 | -904.5 | 999999 | |
| 3.62 | -1.00 | 4.56 | -1.00 | 5.01 | 243.65 | -66.13 | 81.97 | 0.9216 | -408.7 | 999999 | |
| 2.21 | -1.00 | 2.80 | -1.00 | 4.84 | 243.53 | -66.24 | 82.17 | 0.9222 | -274.6 | 999999 | |
| 3.88 | -1.00 | 4.91 | -1.00 | 4.50 | 243.59 | -66.18 | 82.53 | 0.9215 | -413.3 | 999999 | |
| 3.44 | -1.00 | 4.37 | -1.00 | 4.15 | 243.43 | -66.35 | 82.93 | 0.9223 | -246.7 | 999999 | |
| 0.00 | 0.53 | 0.00 | 0.76 | 5.56 | 240.89 | -68.89 | 81.83 | 0.9395 | -111.0 | -77.5 | |
| 1.24 | 2.82 | 1.80 | 4.10 | 3.13 | 240.17 | -69.61 | 84.50 | 0.9417 | 331.1 | 282.8 | |
| 1.15 | 44.22 | 1.70 | 67.81 | 3.57 | 239.75 | -70.03 | 84.09 | 0.9445 | 628.6 | 206.3 | |
| 4.85 | -10.00 | 7.32 | -10.00 | 3.98 | 239.58 | -70.19 | 83.68 | 0.9457 | 763.8 | 999999 | |
| 0.62 | -10.00 | 0.94 | -10.00 | 3.54 | 239.39 | -70.39 | 84.17 | 0.9465 | 355.0 | 999999 | |
| 9.97 | -10.00 | 15.40 | -10.00 | 3.91 | 239.05 | -70.73 | 83.83 | 0.9487 | 449.6 | 999999 | |
| 0.88 | 3.80 | 1.52 | 6.55 | 5.19 | 237.18 | -72.60 | 82.76 | 0.9592 | 322.7 | 197.2 | |
| 0.00 | 2.82 | 0.00 | 4.85 | 4.83 | 237.18 | -72.60 | 83.14 | 0.9590 | 275.0 | 208.5 | |
| 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. | |