SDO HMI 2014-11-24 01:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.43 | 0.00 | 13.17 | -12.10 | 225.75 | 33.72 | 246.61 | 0.5934 | 82.7 | 49.8 | |
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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 | 1.29 | 0.00 | 0.82 | -12.64 | 228.68 | 36.65 | 247.34 | 0.6335 | 586.0 | 520.9 | |
| 0.00 | 0.77 | 0.00 | 0.49 | -13.00 | 228.48 | 36.45 | 246.70 | 0.6326 | 510.0 | 498.8 | |
| 0.00 | 2.40 | 0.00 | 1.52 | -12.69 | 228.24 | 36.21 | 247.04 | 0.6281 | 735.0 | 622.6 | |
| 0.00 | 1.80 | 0.00 | 1.14 | -12.62 | 228.00 | 35.97 | 247.02 | 0.6249 | 714.0 | 603.0 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -13.24 | 228.10 | 36.07 | 246.15 | 0.6290 | 619.0 | 551.0 | |
| 0.00 | 1.20 | 0.00 | 0.75 | -12.85 | 227.22 | 35.18 | 246.25 | 0.6160 | 774.0 | 556.7 | |
| 0.00 | 0.77 | 0.00 | 0.48 | -13.10 | 227.14 | 35.11 | 245.84 | 0.6163 | 760.0 | 645.9 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -13.03 | 226.95 | 34.91 | 245.83 | 0.6135 | 663.0 | 616.6 | |
| 0.00 | 3.86 | 0.00 | 2.33 | -12.85 | 224.14 | 32.11 | 244.41 | 0.5768 | -682.0 | -568.0 | |
| 0.00 | 1.20 | 0.00 | 0.72 | -10.38 | 223.79 | 31.76 | 248.28 | 0.5595 | -702.0 | -485.9 | |
| 0.00 | 1.11 | 0.00 | 0.67 | -11.69 | 223.84 | 31.81 | 246.12 | 0.5667 | -674.0 | -554.3 | |
| 0.00 | 1.11 | 0.00 | 0.67 | -11.60 | 223.69 | 31.66 | 246.18 | 0.5642 | -624.0 | -591.3 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -12.82 | 223.78 | 31.75 | 244.24 | 0.5719 | -798.0 | -652.9 | |
| 0.00 | 2.57 | 0.00 | 1.51 | -8.56 | 223.19 | 31.15 | 251.09 | 0.5429 | -52.0 | -90.0 | |
| 0.00 | 0.60 | 0.00 | 0.36 | -13.13 | 222.23 | 30.19 | 242.66 | 0.5536 | -589.0 | -457.6 | |
| 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. | |