SDO HMI 2014-11-24 02:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.01 | 0.00 | 13.22 | -12.78 | 226.94 | 35.46 | 246.49 | 0.6189 | 443.8 | 261.8 | |
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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 | 1.63 | 0.00 | 1.05 | -12.63 | 228.70 | 37.22 | 247.65 | 0.6405 | 612.0 | 525.0 | |
| 0.00 | 0.86 | 0.00 | 0.55 | -13.21 | 228.69 | 37.21 | 246.78 | 0.6429 | 464.0 | 396.0 | |
| 0.00 | 1.03 | 0.00 | 0.66 | -12.81 | 228.50 | 37.02 | 247.28 | 0.6388 | 627.0 | 506.4 | |
| 0.00 | 1.29 | 0.00 | 0.83 | -12.99 | 228.42 | 36.94 | 246.97 | 0.6386 | 598.0 | 499.6 | |
| 0.00 | 2.14 | 0.00 | 1.37 | -12.68 | 228.29 | 36.81 | 247.37 | 0.6356 | 727.0 | 636.8 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -13.20 | 228.12 | 36.63 | 246.51 | 0.6357 | 672.0 | 601.2 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -12.58 | 227.86 | 36.38 | 247.30 | 0.6298 | 669.0 | 541.5 | |
| 0.00 | 1.63 | 0.00 | 1.03 | -12.67 | 227.69 | 36.20 | 247.08 | 0.6280 | 529.0 | 456.8 | |
| 0.00 | 1.89 | 0.00 | 1.20 | -13.00 | 227.55 | 36.07 | 246.50 | 0.6278 | 706.0 | 605.5 | |
| 0.00 | 1.20 | 0.00 | 0.76 | -12.87 | 227.23 | 35.75 | 246.53 | 0.6232 | 718.0 | 605.1 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -13.51 | 226.77 | 35.29 | 245.32 | 0.6205 | 398.0 | 370.1 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -13.35 | 226.52 | 35.04 | 245.42 | 0.6166 | 719.0 | 559.5 | |
| 0.00 | 3.60 | 0.00 | 2.19 | -12.88 | 224.18 | 32.69 | 244.76 | 0.5844 | -635.0 | -545.9 | |
| 0.00 | 2.06 | 0.00 | 1.24 | -11.68 | 223.87 | 32.38 | 246.50 | 0.5741 | -591.0 | -516.0 | |
| 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. | |