SDO HMI 2014-03-06 15:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.68 | 143.11 | 32.41 | 134.36 | -9.99 | 359.61 | -58.86 | 97.29 | 0.8518 | 519.4 | 258.3 | |
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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 | 1.30 | 0.00 | 1.16 | -9.32 | 1.63 | -56.85 | 96.40 | 0.8336 | -219.0 | -241.2 | |
| 17.64 | 118.30 | 16.41 | 109.63 | -10.35 | 359.97 | -58.50 | 97.71 | 0.8486 | 720.9 | 307.9 | |
| 13.58 | -2.00 | 12.56 | -2.00 | -9.56 | 0.20 | -58.28 | 96.76 | 0.8468 | 714.5 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.21 | -8.10 | 360.00 | -58.48 | 95.05 | 0.8493 | -263.0 | -223.3 | |
| 0.00 | 0.95 | 0.00 | 0.91 | -9.91 | 358.98 | -59.50 | 97.24 | 0.8576 | 325.0 | 275.5 | |
| 0.00 | 1.90 | 0.00 | 1.88 | -10.90 | 357.81 | -60.67 | 98.44 | 0.8675 | 523.0 | 358.1 | |
| 0.00 | 0.86 | 0.00 | 0.88 | -12.59 | 356.84 | -61.63 | 100.41 | 0.8751 | 406.0 | 317.5 | |
| 0.43 | 1.38 | 0.43 | 1.37 | -10.14 | 357.69 | -60.79 | 97.56 | 0.8688 | 434.0 | 397.6 | |
| 0.00 | 0.69 | 0.00 | 0.69 | -10.32 | 357.44 | -61.04 | 97.78 | 0.8708 | 245.0 | 207.6 | |
| 0.00 | 0.52 | 0.00 | 0.52 | -9.81 | 357.48 | -61.00 | 97.20 | 0.8707 | 194.0 | 175.8 | |
| 3.03 | 10.12 | 3.01 | 10.06 | -9.08 | 357.64 | -60.84 | 96.34 | 0.8696 | 440.7 | 268.9 | |
| 0.00 | 1.12 | 0.00 | 1.13 | -9.84 | 357.16 | -61.32 | 97.24 | 0.8734 | -152.0 | -78.1 | |
| 0.00 | 2.77 | 0.00 | 2.85 | -10.25 | 356.57 | -61.91 | 97.75 | 0.8781 | -476.0 | -437.6 | |
| 0.00 | 0.78 | 0.00 | 0.80 | -9.40 | 356.78 | -61.70 | 96.77 | 0.8767 | 208.0 | 132.6 | |
| 0.00 | 1.12 | 0.00 | 1.27 | -14.42 | 353.62 | -64.86 | 102.55 | 0.9000 | -474.0 | -341.3 | |
| 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. | |