SDO HMI 2014-05-28 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.75 | 30.11 | 6.62 | 19.73 | -10.46 | 83.99 | 39.84 | 255.01 | 0.6535 | 329.8 | 182.3 | |
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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 |
| 9.75 | 13.99 | 6.62 | 9.50 | -9.76 | 86.66 | 42.51 | 256.86 | 0.6861 | 840.9 | 587.9 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -11.14 | 84.65 | 40.50 | 254.33 | 0.6641 | 554.0 | 424.6 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -10.43 | 84.21 | 40.06 | 255.26 | 0.6567 | 701.0 | 568.8 | |
| 0.00 | 1.53 | 0.00 | 1.01 | -11.76 | 84.18 | 40.03 | 253.27 | 0.6599 | 598.0 | 516.8 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -11.77 | 83.74 | 39.59 | 253.12 | 0.6542 | 497.0 | 404.0 | |
| 0.00 | 1.35 | 0.00 | 0.88 | -11.74 | 83.53 | 39.38 | 253.10 | 0.6515 | 628.0 | 461.3 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -10.78 | 83.30 | 39.15 | 254.47 | 0.6459 | 679.0 | 560.7 | |
| 0.00 | 1.17 | 0.00 | 0.75 | -12.19 | 82.01 | 37.86 | 251.89 | 0.6335 | 623.0 | 528.3 | |
| 0.00 | 1.17 | 0.00 | 0.75 | -12.03 | 81.91 | 37.76 | 252.09 | 0.6316 | 707.0 | 522.9 | |
| 0.00 | 2.44 | 0.00 | 1.52 | -10.16 | 80.81 | 36.66 | 254.67 | 0.6116 | -430.0 | -431.9 | |
| 0.00 | 0.90 | 0.00 | 0.56 | -10.25 | 80.63 | 36.48 | 254.46 | 0.6095 | -537.0 | -399.6 | |
| 0.00 | 1.53 | 0.00 | 0.95 | -10.23 | 79.90 | 35.75 | 254.25 | 0.5996 | -725.0 | -602.5 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -10.01 | 77.06 | 32.92 | 253.57 | 0.5601 | -801.0 | -639.7 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -14.19 | 74.10 | 29.95 | 244.70 | 0.5375 | -683.0 | -583.0 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -12.39 | 73.08 | 28.93 | 247.25 | 0.5143 | -578.0 | -507.1 | |
| 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. | |