SDO HMI 2014-04-10 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.26 | 0.00 | 12.53 | -20.05 | 322.80 | -1.82 | 181.06 | 0.2769 | -100.9 | 33.5 | |
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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 | 1.50 | 0.00 | 0.76 | -15.51 | 332.24 | 7.61 | 217.54 | 0.2104 | 747.0 | 607.2 | |
| 0.00 | 4.76 | 0.00 | 2.40 | -14.39 | 332.17 | 7.54 | 220.91 | 0.1950 | 1024.0 | 845.4 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -21.13 | 330.54 | 5.91 | 200.18 | 0.2798 | 607.0 | 471.9 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -17.77 | 329.25 | 4.62 | 200.60 | 0.2192 | 952.0 | 845.1 | |
| 0.00 | 1.59 | 0.00 | 0.81 | -18.02 | 329.00 | 4.38 | 199.20 | 0.2217 | 792.0 | 556.2 | |
| 0.00 | 1.50 | 0.00 | 0.76 | -17.50 | 328.30 | 3.67 | 197.01 | 0.2096 | 811.0 | 673.6 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -23.85 | 317.06 | -7.56 | 158.61 | 0.3315 | -623.0 | -629.2 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -23.62 | 316.45 | -8.18 | 156.77 | 0.3319 | -558.0 | -469.8 | |
| 0.00 | 3.35 | 0.00 | 1.76 | -23.31 | 316.43 | -8.19 | 156.32 | 0.3272 | -844.0 | -687.6 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -23.12 | 316.41 | -8.21 | 156.01 | 0.3246 | -973.0 | -752.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -22.55 | 316.35 | -8.28 | 155.06 | 0.3166 | -810.0 | -617.2 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -23.27 | 316.11 | -8.52 | 155.44 | 0.3289 | -628.0 | -490.2 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -21.24 | 314.57 | -10.06 | 148.37 | 0.3117 | -503.0 | -384.1 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -23.84 | 312.80 | -11.83 | 148.70 | 0.3624 | -719.0 | -522.1 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -25.60 | 311.81 | -12.82 | 149.35 | 0.3941 | -789.0 | -642.3 | |
| 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. | |