SDO HMI 2011-06-19 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.44 | 46.63 | 8.06 | 61.08 | -14.83 | 245.94 | 66.51 | 253.27 | 0.9262 | 94.4 | 213.9 | |
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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 |
| 0.45 | 2.99 | 0.83 | 5.50 | -14.85 | 252.83 | 73.40 | 254.13 | 0.9642 | 312.0 | 231.4 | |
| 0.00 | 1.00 | 0.00 | 1.88 | -15.33 | 253.17 | 73.74 | 253.66 | 0.9660 | 439.0 | 344.5 | |
| 0.00 | 1.18 | 0.00 | 1.69 | -14.63 | 248.04 | 68.61 | 253.80 | 0.9397 | 370.0 | 312.3 | |
| 0.00 | 9.25 | 0.00 | 12.24 | -14.24 | 246.28 | 66.85 | 253.98 | 0.9288 | 748.0 | 567.3 | |
| 0.00 | 3.27 | 0.00 | 4.13 | -13.83 | 245.25 | 65.83 | 254.28 | 0.9219 | 30.0 | 51.2 | |
| 0.00 | 4.45 | 0.00 | 5.70 | -14.31 | 245.53 | 66.10 | 253.80 | 0.9241 | 359.0 | 310.7 | |
| 2.54 | 11.70 | 3.19 | 14.64 | -14.74 | 244.85 | 65.42 | 253.24 | 0.9201 | 389.3 | 260.5 | |
| 0.00 | 1.09 | 0.00 | 1.37 | -15.12 | 245.00 | 65.57 | 252.85 | 0.9215 | 283.0 | 252.7 | |
| 0.00 | 1.18 | 0.00 | 1.43 | -13.93 | 244.09 | 64.67 | 254.00 | 0.9143 | -399.0 | -318.6 | |
| 0.00 | 1.54 | 0.00 | 1.93 | -15.56 | 244.80 | 65.37 | 252.35 | 0.9207 | 1.0 | -33.4 | |
| 0.00 | 0.54 | 0.00 | 0.69 | -15.82 | 244.96 | 65.53 | 252.09 | 0.9220 | 400.0 | 359.0 | |
| 3.45 | 8.44 | 4.04 | 9.88 | -16.24 | 242.77 | 63.34 | 251.27 | 0.9078 | -524.9 | -496.1 | |
| 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. | |