SDO HMI 2011-12-06 11:58:56 UT
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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.80 | 340.35 | 45.82 | 216.92 | 7.33 | 131.78 | 38.03 | 281.76 | 0.6244 | -32.3 | -65.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-06 11:58:56 UT
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 |
| 1.02 | 157.61 | 0.70 | 106.67 | 6.53 | 136.72 | 42.96 | 279.29 | 0.6884 | -668.7 | -295.8 | |
| 18.17 | -1.00 | 12.35 | -1.00 | 6.83 | 136.58 | 42.83 | 279.74 | 0.6872 | -946.2 | 999999 | |
| 16.80 | -1.00 | 11.22 | -1.00 | 6.71 | 135.52 | 41.77 | 279.76 | 0.6736 | -931.0 | 999999 | |
| 0.00 | 1.88 | 0.00 | 1.24 | 6.98 | 134.80 | 41.04 | 280.30 | 0.6647 | -784.0 | -615.0 | |
| 0.51 | 1.45 | 0.34 | 0.95 | 5.79 | 134.52 | 40.76 | 278.56 | 0.6593 | -709.8 | -630.7 | |
| 0.00 | 1.36 | 0.00 | 0.89 | 5.91 | 134.30 | 40.54 | 278.78 | 0.6565 | -787.0 | -701.9 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 6.95 | 134.28 | 40.52 | 280.36 | 0.6580 | -633.0 | -554.0 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 6.42 | 133.99 | 40.23 | 279.61 | 0.6533 | -773.0 | -683.0 | |
| 2.73 | 9.04 | 1.77 | 5.88 | 5.32 | 133.86 | 40.10 | 277.95 | 0.6499 | 517.8 | -103.1 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 5.38 | 133.51 | 39.76 | 278.10 | 0.6454 | -538.0 | -414.3 | |
| 0.00 | 1.02 | 0.00 | 0.65 | 5.94 | 132.14 | 38.38 | 279.23 | 0.6280 | -726.0 | -476.8 | |
| 0.00 | 1.54 | 0.00 | 0.94 | 6.99 | 129.65 | 35.89 | 281.50 | 0.5961 | -768.0 | -610.3 | |
| 0.00 | 0.43 | 0.00 | 0.26 | 6.87 | 129.53 | 35.77 | 281.34 | 0.5942 | -772.0 | -713.2 | |
| 0.00 | 0.94 | 0.00 | 0.58 | 6.75 | 129.48 | 35.73 | 281.15 | 0.5933 | -839.0 | -744.1 | |
| 0.00 | 5.88 | 0.00 | 3.61 | 7.65 | 129.23 | 35.48 | 282.71 | 0.5919 | -689.0 | -678.5 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 6.90 | 129.13 | 35.37 | 281.50 | 0.5887 | -941.0 | -765.4 | |
| 0.00 | 1.36 | 0.00 | 0.84 | 10.61 | 128.98 | 35.23 | 287.69 | 0.5974 | 467.0 | 368.2 | |
| 1.45 | 134.66 | 0.87 | 80.62 | 8.84 | 127.25 | 33.49 | 285.42 | 0.5678 | 690.5 | 234.4 | |
| 1.36 | -18.00 | 0.82 | -18.00 | 8.69 | 127.23 | 33.48 | 285.17 | 0.5671 | 710.5 | 999999 | |
| 0.00 | 0.51 | 0.00 | 0.31 | 10.88 | 127.45 | 33.69 | 288.80 | 0.5777 | 512.0 | 488.5 | |
| 26.95 | -18.00 | 16.09 | -18.00 | 8.16 | 126.89 | 33.14 | 284.36 | 0.5608 | 1076.1 | 999999 | |
| 0.00 | 2.13 | 0.00 | 1.27 | 7.53 | 126.48 | 32.73 | 283.40 | 0.5531 | 805.0 | 716.8 | |
| 0.00 | 1.96 | 0.00 | 1.16 | 7.32 | 126.46 | 32.71 | 283.04 | 0.5523 | 703.0 | 625.5 | |
| 2.81 | 3.92 | 1.66 | 2.32 | 7.98 | 125.92 | 32.16 | 284.41 | 0.5465 | 943.6 | 483.5 | |
| 0.00 | 1.19 | 0.00 | 0.70 | 6.61 | 125.53 | 31.77 | 282.06 | 0.5370 | 563.0 | 414.4 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 8.97 | 124.82 | 31.06 | 286.65 | 0.5341 | 891.0 | 701.7 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 9.00 | 124.58 | 30.82 | 286.82 | 0.5307 | 762.0 | 613.9 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 9.12 | 124.13 | 30.38 | 287.25 | 0.5249 | 721.0 | 562.0 | |
| 0.00 | 1.19 | 0.00 | 0.69 | 9.30 | 123.91 | 30.15 | 287.69 | 0.5224 | 694.0 | 536.4 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 7.63 | 123.21 | 29.46 | 284.85 | 0.5063 | 850.0 | 686.8 | |
| 0.00 | 2.30 | 0.00 | 1.32 | 6.65 | 123.11 | 29.35 | 282.98 | 0.5017 | 850.0 | 732.7 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 4.34 | 120.23 | 26.48 | 279.20 | 0.4523 | 748.0 | 555.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |