SDO HMI 2014-11-08 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.95 | 20.19 | 0.56 | 11.69 | 5.42 | 71.62 | 30.86 | 274.58 | 0.5131 | 44.5 | -103.0 | |
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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 | 5.70 | 0.00 | 3.44 | 5.52 | 75.81 | 35.04 | 274.43 | 0.5754 | -819.0 | -647.6 | |
| 0.52 | 1.81 | 0.31 | 1.08 | 5.32 | 74.92 | 34.16 | 274.11 | 0.5627 | -761.5 | -646.5 | |
| 0.00 | 0.52 | 0.00 | 0.31 | 4.44 | 74.54 | 33.78 | 272.54 | 0.5571 | -664.0 | -566.5 | |
| 0.43 | 1.90 | 0.25 | 1.12 | 4.95 | 73.57 | 32.81 | 273.49 | 0.5430 | -795.6 | -673.7 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 4.90 | 73.32 | 32.56 | 273.40 | 0.5392 | -835.0 | -679.8 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 5.85 | 71.48 | 30.72 | 275.34 | 0.5124 | 724.0 | 549.6 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 4.35 | 70.95 | 30.19 | 272.40 | 0.5038 | -530.0 | -546.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 4.21 | 67.01 | 26.25 | 272.13 | 0.4433 | 708.0 | 490.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 5.52 | 66.91 | 26.14 | 275.11 | 0.4422 | 760.0 | 599.2 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 5.64 | 66.65 | 25.88 | 275.43 | 0.4382 | 891.0 | 656.8 | |
| 0.00 | 1.98 | 0.00 | 1.09 | 6.21 | 66.58 | 25.81 | 276.74 | 0.4377 | 862.0 | 682.0 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 5.93 | 65.96 | 25.20 | 276.20 | 0.4278 | 819.0 | 731.6 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 5.67 | 64.60 | 23.84 | 275.80 | 0.4060 | 680.0 | 532.4 | |
| 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. | |