SDO HMI 2011-06-19 09:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.97 | 43.75 | 13.30 | 55.86 | -14.83 | 245.80 | 65.83 | 253.17 | 0.9219 | 65.4 | 132.4 | |
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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 | 0.64 | 0.00 | 1.16 | -14.18 | 253.26 | 73.28 | 254.80 | 0.9634 | 159.0 | 94.7 | |
| 0.00 | 1.72 | 0.00 | 3.07 | -14.83 | 252.83 | 72.85 | 254.08 | 0.9617 | 300.0 | 238.4 | |
| 0.00 | 1.00 | 0.00 | 1.81 | -15.35 | 253.07 | 73.09 | 253.58 | 0.9631 | 213.0 | 171.2 | |
| 0.00 | 1.00 | 0.00 | 1.42 | -14.63 | 248.43 | 68.45 | 253.78 | 0.9387 | 183.0 | 143.1 | |
| 0.00 | 1.18 | 0.00 | 1.65 | -14.61 | 247.99 | 68.01 | 253.74 | 0.9362 | 405.0 | 373.1 | |
| 0.00 | 6.53 | 0.00 | 8.45 | -14.29 | 246.31 | 66.33 | 253.86 | 0.9256 | 759.0 | 603.2 | |
| 0.00 | 0.91 | 0.00 | 1.21 | -15.19 | 246.86 | 66.89 | 252.97 | 0.9299 | 361.0 | 311.1 | |
| 1.45 | 3.72 | 1.79 | 4.58 | -13.88 | 245.15 | 65.17 | 254.13 | 0.9177 | -179.1 | -173.6 | |
| 6.71 | 16.15 | 8.25 | 19.90 | -14.63 | 244.89 | 64.91 | 253.28 | 0.9167 | 400.0 | 257.2 | |
| 0.36 | -9.00 | 0.44 | -9.00 | -14.28 | 244.62 | 64.64 | 253.62 | 0.9145 | -119.5 | 999999 | |
| 0.00 | 1.18 | 0.00 | 1.40 | -13.92 | 244.06 | 64.08 | 253.93 | 0.9103 | -357.0 | -313.0 | |
| 0.00 | 0.82 | 0.00 | 0.99 | -15.60 | 244.40 | 64.43 | 252.15 | 0.9144 | -371.0 | -327.2 | |
| 0.00 | 0.82 | 0.00 | 0.93 | -15.30 | 242.59 | 62.61 | 252.17 | 0.9014 | -476.0 | -404.1 | |
| 2.45 | 5.99 | 2.82 | 6.88 | -16.23 | 242.82 | 62.85 | 251.19 | 0.9043 | -616.2 | -418.2 | |
| 0.00 | 2.09 | 0.00 | 2.41 | -16.52 | 242.85 | 62.87 | 250.88 | 0.9048 | -592.0 | -571.6 | |
| 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. | |