SDO HMI 2014-10-01 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.33 | 105.05 | 14.58 | 72.40 | -10.14 | 140.60 | -40.83 | 112.13 | 0.6971 | 472.9 | 266.8 | |
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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 | 1.76 | 0.00 | 1.29 | -16.67 | 139.89 | -41.54 | 120.14 | 0.7369 | 554.0 | 408.4 | |
| 0.00 | 0.44 | 0.00 | 0.32 | -15.53 | 139.97 | -41.46 | 118.78 | 0.7301 | 549.0 | 424.6 | |
| 21.33 | 94.57 | 14.58 | 64.64 | -9.66 | 140.93 | -40.50 | 111.67 | 0.6913 | 1005.9 | 346.9 | |
| 0.00 | 1.41 | 0.00 | 1.04 | -14.61 | 138.26 | -43.17 | 116.71 | 0.7434 | -732.0 | -616.4 | |
| 0.00 | 0.44 | 0.00 | 0.32 | -13.40 | 138.25 | -43.18 | 115.19 | 0.7380 | -655.0 | -481.6 | |
| 0.00 | 1.23 | 0.00 | 0.90 | -13.54 | 138.18 | -43.25 | 115.32 | 0.7393 | -662.0 | -568.1 | |
| 0.00 | 0.62 | 0.00 | 0.45 | -13.29 | 137.72 | -43.71 | 114.79 | 0.7430 | -383.0 | -458.0 | |
| 0.00 | 2.29 | 0.00 | 1.73 | -13.88 | 136.76 | -44.67 | 115.05 | 0.7557 | -85.0 | -125.3 | |
| 0.00 | 1.06 | 0.00 | 0.79 | -12.64 | 136.79 | -44.64 | 113.52 | 0.7501 | -626.0 | -549.7 | |
| 0.00 | 0.44 | 0.00 | 0.33 | -12.80 | 136.71 | -44.72 | 113.69 | 0.7516 | -472.0 | -477.8 | |
| 0.00 | 0.79 | 0.00 | 0.59 | -12.48 | 136.44 | -44.99 | 113.16 | 0.7532 | -530.0 | -458.6 | |
| 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. | |