SDO HMI 2014-07-08 07:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.90 | 0.00 | 11.29 | -21.75 | 201.61 | -22.63 | 140.29 | 0.5587 | 183.5 | 24.0 | |
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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 | 2.00 | 0.00 | 1.15 | -21.11 | 205.57 | -18.66 | 144.31 | 0.5137 | 925.0 | 811.9 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -20.68 | 205.45 | -18.78 | 143.61 | 0.5097 | 727.0 | 670.0 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -21.18 | 205.32 | -18.92 | 144.04 | 0.5168 | 670.0 | 519.6 | |
| 0.00 | 4.72 | 0.00 | 2.78 | -22.85 | 204.77 | -19.47 | 145.25 | 0.5409 | -839.0 | -571.5 | |
| 0.00 | 1.64 | 0.00 | 0.96 | -21.83 | 203.55 | -20.68 | 142.43 | 0.5398 | 775.0 | 622.1 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -21.59 | 203.55 | -20.68 | 142.14 | 0.5372 | 668.0 | 601.8 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -21.74 | 203.00 | -21.23 | 141.61 | 0.5438 | 501.0 | 508.4 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -21.60 | 202.99 | -21.24 | 141.43 | 0.5425 | 675.0 | 475.3 | |
| 0.00 | 1.09 | 0.00 | 0.67 | -22.78 | 199.49 | -24.74 | 138.71 | 0.5871 | 712.0 | 504.2 | |
| 0.00 | 0.82 | 0.00 | 0.51 | -21.13 | 195.55 | -28.68 | 132.61 | 0.6105 | -555.0 | -507.1 | |
| 0.00 | 0.82 | 0.00 | 0.51 | -20.74 | 195.34 | -28.90 | 131.89 | 0.6093 | -548.0 | -496.1 | |
| 0.00 | 1.82 | 0.00 | 1.14 | -20.95 | 194.92 | -29.32 | 131.78 | 0.6154 | -669.0 | -548.0 | |
| 0.00 | 1.18 | 0.00 | 0.75 | -20.90 | 193.53 | -30.70 | 130.47 | 0.6293 | -656.0 | -509.6 | |
| 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. | |