SDO HMI 2014-06-30 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.97 | 371.13 | 106.45 | 614.82 | -20.24 | 258.93 | -70.09 | 112.27 | 0.9542 | 73.6 | -79.0 | |
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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 |
| 6.36 | 25.08 | 8.55 | 33.83 | -21.18 | 263.51 | -65.51 | 114.10 | 0.9312 | 607.5 | 281.3 | |
| 0.27 | 145.73 | 0.38 | 225.30 | -21.33 | 262.40 | -66.63 | 114.03 | 0.9377 | 471.0 | -302.4 | |
| 4.09 | -2.00 | 5.82 | -2.00 | -21.24 | 262.14 | -66.88 | 113.89 | 0.9390 | 287.2 | 999999 | |
| 5.91 | -2.00 | 8.95 | -2.00 | -21.50 | 260.85 | -68.17 | 113.91 | 0.9462 | -616.5 | 999999 | |
| 0.00 | 1.18 | 0.00 | 1.88 | -21.97 | 259.90 | -69.12 | 114.22 | 0.9514 | -581.0 | -527.0 | |
| 2.36 | -2.00 | 3.62 | -2.00 | -21.22 | 260.51 | -68.52 | 113.55 | 0.9476 | -591.1 | 999999 | |
| 1.09 | 3.54 | 1.58 | 5.15 | -20.22 | 261.46 | -67.56 | 112.68 | 0.9415 | 3.8 | -189.5 | |
| 7.09 | -2.00 | 11.21 | -2.00 | -21.61 | 259.92 | -69.10 | 113.85 | 0.9510 | -474.3 | 999999 | |
| 2.73 | 6.81 | 4.46 | 11.18 | -22.17 | 259.31 | -69.71 | 114.32 | 0.9545 | -292.4 | -217.6 | |
| 0.00 | 1.45 | 0.00 | 2.59 | -23.14 | 257.85 | -71.17 | 115.06 | 0.9620 | 32.0 | 78.6 | |
| 2.73 | -2.00 | 4.61 | -2.00 | -21.64 | 258.64 | -70.38 | 113.65 | 0.9571 | -302.5 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.96 | -20.93 | 257.41 | -71.61 | 112.72 | 0.9621 | 213.0 | 185.7 | |
| 32.34 | 186.25 | 57.27 | 332.93 | -19.20 | 257.37 | -71.65 | 110.93 | 0.9610 | 290.1 | 47.1 | |
| 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. | |