SDO HMI 2014-11-01 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 |
| 8.40 | 26.60 | 5.20 | 16.92 | -16.69 | 100.20 | -32.86 | 123.95 | 0.6264 | 210.4 | 197.7 | |
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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 | 1.13 | 0.00 | 0.69 | -16.92 | 104.18 | -28.88 | 127.47 | 0.5844 | -713.0 | -576.8 | |
| 0.00 | 1.04 | 0.00 | 0.64 | -16.35 | 102.49 | -30.58 | 125.16 | 0.5993 | 705.0 | 606.2 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -16.45 | 102.33 | -30.74 | 125.16 | 0.6019 | 463.0 | 566.7 | |
| 3.03 | 6.76 | 1.87 | 4.17 | -16.17 | 102.34 | -30.72 | 124.77 | 0.5996 | 989.2 | 828.8 | |
| 0.52 | -4.00 | 0.32 | -4.00 | -15.94 | 102.38 | -30.69 | 124.48 | 0.5975 | 993.2 | 999999 | |
| 0.00 | 1.13 | 0.00 | 0.69 | -15.82 | 102.26 | -30.81 | 124.20 | 0.5981 | 626.0 | 568.8 | |
| 4.85 | 10.65 | 3.01 | 6.60 | -16.12 | 101.99 | -31.08 | 124.40 | 0.6033 | 850.5 | 552.9 | |
| 0.00 | 0.87 | 0.00 | 0.57 | -15.73 | 96.96 | -36.11 | 120.17 | 0.6584 | -700.0 | -555.1 | |
| 0.00 | 1.47 | 0.00 | 1.03 | -19.21 | 94.46 | -38.61 | 123.12 | 0.7058 | -178.0 | -225.4 | |
| 0.00 | 0.87 | 0.00 | 0.61 | -18.71 | 93.99 | -39.08 | 122.20 | 0.7079 | -698.0 | -544.7 | |
| 0.00 | 0.95 | 0.00 | 0.69 | -19.47 | 91.74 | -41.33 | 121.83 | 0.7351 | -703.0 | -548.5 | |
| 0.00 | 0.78 | 0.00 | 0.57 | -19.68 | 91.59 | -41.48 | 121.99 | 0.7376 | -727.0 | -636.3 | |
| 0.00 | 0.69 | 0.00 | 0.50 | -16.80 | 91.35 | -41.72 | 118.28 | 0.7257 | -388.0 | -346.2 | |
| 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. | |