SDO HMI 2014-07-03 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.73 | 22.99 | 0.49 | 14.57 | -13.67 | 253.30 | -34.92 | 116.74 | 0.6235 | 332.2 | 78.3 | |
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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 | 1.36 | 0.00 | 0.81 | -12.82 | 258.05 | -30.17 | 118.63 | 0.5604 | 394.0 | 416.7 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -12.93 | 257.82 | -30.40 | 118.62 | 0.5640 | 802.0 | 650.0 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -12.36 | 257.71 | -30.50 | 117.63 | 0.5618 | 813.0 | 664.6 | |
| 0.00 | 0.73 | 0.00 | 0.44 | -10.69 | 256.50 | -31.72 | 114.07 | 0.5679 | 445.0 | 372.1 | |
| 0.00 | 1.73 | 0.00 | 1.05 | -12.56 | 256.19 | -32.03 | 116.86 | 0.5825 | 754.0 | 653.8 | |
| 0.00 | 1.36 | 0.00 | 0.84 | -13.14 | 255.73 | -32.49 | 117.45 | 0.5916 | 667.0 | 560.5 | |
| 0.00 | 1.64 | 0.00 | 1.00 | -12.14 | 255.36 | -32.86 | 115.65 | 0.5906 | 568.0 | 440.6 | |
| 0.00 | 3.00 | 0.00 | 1.84 | -12.62 | 255.25 | -32.97 | 116.32 | 0.5946 | 707.0 | 518.7 | |
| 0.00 | 2.09 | 0.00 | 1.37 | -15.10 | 251.24 | -36.98 | 117.48 | 0.6568 | 675.0 | 421.6 | |
| 0.00 | 2.54 | 0.00 | 1.70 | -15.11 | 249.92 | -38.30 | 116.75 | 0.6723 | -794.0 | -628.5 | |
| 0.73 | 6.00 | 0.49 | 4.00 | -14.73 | 249.76 | -38.46 | 116.14 | 0.6723 | -815.0 | -701.2 | |
| 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. | |