SDO HMI 2011-09-06 12:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.71 | 30.69 | 8.65 | 24.73 | -19.69 | 258.75 | 45.24 | 238.00 | 0.7901 | 378.9 | 293.2 | |
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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 | 0.98 | 0.00 | 0.89 | -23.05 | 262.68 | 49.17 | 236.31 | 0.8389 | 594.0 | 456.5 | |
| 0.00 | 0.71 | 0.00 | 0.61 | -20.86 | 260.84 | 47.34 | 237.79 | 0.8143 | 540.0 | 444.5 | |
| 0.00 | 1.16 | 0.00 | 0.98 | -21.89 | 260.27 | 46.77 | 236.36 | 0.8142 | 525.0 | 402.9 | |
| 10.71 | 14.28 | 8.65 | 11.53 | -19.41 | 259.06 | 45.55 | 238.49 | 0.7920 | 647.2 | 478.4 | |
| 0.00 | 1.16 | 0.00 | 0.93 | -19.21 | 258.76 | 45.25 | 238.55 | 0.7884 | 854.0 | 636.9 | |
| 0.00 | 2.05 | 0.00 | 1.67 | -20.03 | 258.92 | 45.41 | 237.71 | 0.7937 | 508.0 | 412.8 | |
| 0.00 | 1.52 | 0.00 | 1.22 | -19.60 | 258.63 | 45.12 | 238.04 | 0.7890 | 732.0 | 634.1 | |
| 0.00 | 0.80 | 0.00 | 0.65 | -19.77 | 258.64 | 45.13 | 237.86 | 0.7900 | 537.0 | 514.4 | |
| 0.00 | 1.79 | 0.00 | 1.42 | -19.18 | 258.38 | 44.88 | 238.39 | 0.7848 | 798.0 | 683.4 | |
| 0.00 | 1.70 | 0.00 | 1.40 | -21.50 | 259.07 | 45.57 | 236.15 | 0.8022 | 432.0 | 308.7 | |
| 0.00 | 0.89 | 0.00 | 0.69 | -19.00 | 257.25 | 43.74 | 237.97 | 0.7734 | -410.0 | -337.8 | |
| 0.00 | 0.80 | 0.00 | 0.62 | -18.48 | 256.99 | 43.48 | 238.43 | 0.7683 | -648.0 | -608.1 | |
| 0.00 | 0.98 | 0.00 | 0.75 | -19.22 | 255.91 | 42.40 | 236.95 | 0.7620 | -430.0 | -349.5 | |
| 0.00 | 0.98 | 0.00 | 0.74 | -19.20 | 255.69 | 42.18 | 236.84 | 0.7598 | -621.0 | -480.6 | |
| 0.00 | 0.89 | 0.00 | 0.63 | -15.59 | 253.31 | 39.80 | 239.73 | 0.7162 | -426.0 | -461.2 | |
| 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. | |