SDO HMI 2011-11-24 09:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.18 | 178.68 | 32.37 | 181.76 | 19.18 | 193.38 | -59.61 | 68.93 | 0.8739 | -300.8 | -138.2 | |
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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 |
| 0.77 | 155.04 | 0.76 | 152.30 | 19.41 | 194.39 | -58.60 | 68.50 | 0.8673 | -217.9 | -191.2 | |
| 23.56 | -1.00 | 23.11 | -1.00 | 18.76 | 194.52 | -58.47 | 69.22 | 0.8653 | -733.9 | 999999 | |
| 0.94 | 2.40 | 0.97 | 2.47 | 18.62 | 192.81 | -60.19 | 69.66 | 0.8789 | -188.3 | -328.3 | |
| 0.00 | 1.71 | 0.00 | 1.79 | 19.18 | 192.41 | -60.59 | 69.10 | 0.8826 | -296.0 | -244.4 | |
| 0.00 | 0.94 | 0.00 | 1.03 | 19.74 | 191.12 | -61.87 | 68.68 | 0.8930 | 512.0 | 436.0 | |
| 1.54 | 4.28 | 1.88 | 5.22 | 21.36 | 188.11 | -64.88 | 67.34 | 0.9155 | 458.8 | 484.3 | |
| 0.77 | -6.00 | 0.94 | -6.00 | 21.14 | 188.07 | -64.92 | 67.59 | 0.9155 | 404.0 | 999999 | |
| 1.54 | 2.23 | 1.94 | 2.79 | 21.76 | 187.39 | -65.61 | 67.02 | 0.9205 | 491.0 | 474.6 | |
| 0.00 | 0.94 | 0.00 | 1.21 | 21.68 | 186.75 | -66.25 | 67.19 | 0.9244 | 526.0 | 476.8 | |
| 0.00 | 1.03 | 0.00 | 1.30 | 21.34 | 187.06 | -65.94 | 67.52 | 0.9222 | 419.0 | 447.4 | |
| 0.00 | 0.94 | 0.00 | 1.25 | 22.11 | 186.11 | -66.89 | 66.81 | 0.9287 | 245.0 | 302.2 | |
| 0.00 | 0.86 | 0.00 | 1.15 | 22.28 | 185.60 | -67.40 | 66.69 | 0.9318 | 192.0 | 172.6 | |
| 2.06 | 6.08 | 2.77 | 8.23 | 21.93 | 185.61 | -67.39 | 67.06 | 0.9315 | 319.6 | 88.5 | |
| 0.00 | 0.77 | 0.00 | 1.04 | 21.58 | 185.53 | -67.47 | 67.45 | 0.9316 | 314.0 | 277.1 | |
| 0.00 | 1.46 | 0.00 | 1.98 | 21.38 | 185.30 | -67.70 | 67.68 | 0.9329 | 174.0 | 160.3 | |
| 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. | |