SDO HMI 2011-01-07 17:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.76 | 0.00 | 15.48 | -13.88 | 206.18 | 39.70 | 252.90 | 0.6508 | -513.3 | -472.6 | |
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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 | 1.44 | 0.00 | 1.02 | -14.04 | 211.64 | 45.16 | 253.97 | 0.7181 | 675.0 | 520.9 | |
| 0.00 | 1.19 | 0.00 | 0.82 | -16.63 | 209.34 | 42.86 | 249.80 | 0.6969 | 585.0 | 448.1 | |
| 0.00 | 0.85 | 0.00 | 0.56 | -13.89 | 206.87 | 40.39 | 253.08 | 0.6599 | -485.0 | -424.1 | |
| 0.00 | 0.68 | 0.00 | 0.45 | -13.62 | 206.81 | 40.33 | 253.46 | 0.6585 | -441.0 | -391.8 | |
| 0.00 | 1.36 | 0.00 | 0.89 | -13.63 | 206.61 | 40.14 | 253.40 | 0.6560 | -701.0 | -506.1 | |
| 0.00 | 1.27 | 0.00 | 0.83 | -13.90 | 206.59 | 40.11 | 252.99 | 0.6564 | -567.0 | -490.9 | |
| 0.00 | 2.80 | 0.00 | 1.82 | -13.72 | 205.96 | 39.48 | 253.09 | 0.6479 | -795.0 | -560.2 | |
| 0.00 | 1.44 | 0.00 | 0.93 | -13.91 | 205.72 | 39.24 | 252.73 | 0.6454 | -640.0 | -536.9 | |
| 0.00 | 1.70 | 0.00 | 1.09 | -13.65 | 205.43 | 38.96 | 253.05 | 0.6411 | -829.0 | -637.8 | |
| 0.00 | 3.14 | 0.00 | 2.02 | -13.83 | 205.35 | 38.88 | 252.74 | 0.6405 | -727.0 | -685.9 | |
| 0.00 | 1.53 | 0.00 | 0.98 | -13.63 | 205.16 | 38.68 | 253.00 | 0.6374 | -822.0 | -609.1 | |
| 0.00 | 0.76 | 0.00 | 0.49 | -13.45 | 205.04 | 38.57 | 253.24 | 0.6356 | -612.0 | -525.3 | |
| 0.00 | 0.59 | 0.00 | 0.38 | -13.58 | 204.95 | 38.47 | 253.02 | 0.6347 | -752.0 | -693.7 | |
| 0.00 | 3.06 | 0.00 | 1.95 | -13.37 | 204.83 | 38.36 | 253.31 | 0.6326 | -735.0 | -667.6 | |
| 0.00 | 1.95 | 0.00 | 1.25 | -13.91 | 204.90 | 38.42 | 252.49 | 0.6349 | -854.0 | -740.0 | |
| 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. | |