SDO HMI 2014-10-05 04:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.93 | 0.00 | 11.20 | -18.35 | 102.02 | -27.72 | 132.78 | 0.6077 | -190.5 | -141.0 | |
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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 | 1.14 | 0.00 | 0.79 | -33.12 | 109.87 | -19.88 | 155.76 | 0.6959 | -364.0 | -367.5 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -15.21 | 110.98 | -18.76 | 139.57 | 0.4806 | 825.0 | 690.3 | |
| 0.00 | 1.14 | 0.00 | 0.71 | -23.86 | 107.39 | -22.36 | 145.07 | 0.6097 | 658.0 | 579.2 | |
| 0.00 | 1.58 | 0.00 | 0.94 | -17.43 | 106.03 | -23.72 | 135.96 | 0.5542 | 796.0 | 629.8 | |
| 0.00 | 2.73 | 0.00 | 1.59 | -14.97 | 105.83 | -23.91 | 132.36 | 0.5320 | 812.0 | 667.5 | |
| 0.00 | 1.32 | 0.00 | 0.83 | -17.38 | 99.57 | -30.18 | 129.15 | 0.6208 | -797.0 | -737.1 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -17.40 | 99.20 | -30.55 | 128.84 | 0.6249 | -791.0 | -621.4 | |
| 0.00 | 1.49 | 0.00 | 0.95 | -17.61 | 99.09 | -30.66 | 129.01 | 0.6277 | -563.0 | -462.1 | |
| 0.00 | 1.49 | 0.00 | 0.95 | -17.56 | 98.84 | -30.90 | 128.72 | 0.6299 | -633.0 | -509.8 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -17.62 | 98.31 | -31.43 | 128.34 | 0.6360 | -433.0 | -370.4 | |
| 0.00 | 2.02 | 0.00 | 1.29 | -17.07 | 98.24 | -31.51 | 127.56 | 0.6326 | -778.0 | -652.0 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -17.10 | 97.23 | -32.52 | 126.75 | 0.6435 | -601.0 | -541.4 | |
| 0.00 | 1.41 | 0.00 | 0.91 | -16.14 | 96.00 | -33.75 | 124.51 | 0.6500 | -608.0 | -561.4 | |
| 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. | |