SDO HMI 2014-03-05 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.02 | 45.79 | 10.01 | 42.26 | 7.69 | 135.04 | 55.72 | 283.98 | 0.8453 | -36.5 | 285.4 | |
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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 |
| 8.12 | 10.54 | 8.32 | 10.80 | 7.26 | 138.80 | 59.48 | 282.47 | 0.8772 | -470.6 | -321.1 | |
| 0.00 | 1.90 | 0.00 | 1.77 | 6.78 | 135.53 | 56.21 | 282.76 | 0.8483 | -412.0 | -413.4 | |
| 0.00 | 3.89 | 0.00 | 3.62 | 6.99 | 135.51 | 56.19 | 283.01 | 0.8486 | -293.0 | -372.1 | |
| 0.00 | 0.78 | 0.00 | 0.73 | 8.24 | 135.44 | 56.12 | 284.46 | 0.8506 | 231.0 | 166.0 | |
| 0.00 | 0.60 | 0.00 | 0.56 | 7.13 | 135.05 | 55.73 | 283.29 | 0.8447 | 343.0 | 271.9 | |
| 0.00 | 0.52 | 0.00 | 0.48 | 8.44 | 135.05 | 55.74 | 284.80 | 0.8477 | 387.0 | 332.2 | |
| 0.69 | 1.73 | 0.63 | 1.58 | 7.40 | 134.73 | 55.41 | 283.69 | 0.8424 | 302.2 | 246.2 | |
| 0.00 | 1.38 | 0.00 | 1.24 | 6.70 | 134.23 | 54.92 | 283.02 | 0.8363 | 321.0 | 264.4 | |
| 0.00 | 1.38 | 0.00 | 1.25 | 7.13 | 134.26 | 54.94 | 283.51 | 0.8375 | 547.0 | 487.0 | |
| 0.00 | 2.42 | 0.00 | 2.17 | 8.79 | 133.65 | 54.33 | 285.61 | 0.8358 | 450.0 | 339.9 | |
| 0.00 | 0.78 | 0.00 | 0.69 | 8.72 | 133.33 | 54.01 | 285.63 | 0.8326 | 454.0 | 384.0 | |
| 0.00 | 0.86 | 0.00 | 0.75 | 6.93 | 132.93 | 53.61 | 283.66 | 0.8246 | 388.0 | 320.0 | |
| 1.21 | 19.01 | 1.06 | 16.62 | 8.19 | 132.91 | 53.59 | 285.14 | 0.8274 | 546.4 | 593.1 | |
| 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. | |