SDO HMI 2014-05-16 06:00:38 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 |
| 92.20 | 379.73 | 52.75 | 217.34 | 10.31 | 178.90 | -27.29 | 64.19 | 0.5025 | -92.7 | -52.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-05-16 06:00:38 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 |
| 3.59 | 6.38 | 2.00 | 3.56 | 10.43 | 182.05 | -24.13 | 61.24 | 0.4606 | -1021.2 | -747.7 | |
| 0.00 | 0.81 | 0.00 | 0.45 | 9.87 | 182.06 | -24.12 | 62.33 | 0.4565 | -845.0 | -741.8 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 10.38 | 181.55 | -24.64 | 61.82 | 0.4671 | -740.0 | -659.8 | |
| 0.00 | 1.35 | 0.00 | 0.76 | 10.64 | 181.29 | -24.90 | 61.58 | 0.4724 | -786.0 | -623.6 | |
| 4.31 | 185.90 | 2.41 | 104.24 | 9.21 | 181.34 | -24.85 | 64.31 | 0.4622 | -1210.1 | -496.4 | |
| 2.52 | -5.00 | 1.41 | -5.00 | 10.33 | 180.98 | -25.21 | 62.45 | 0.4746 | -807.0 | 999999 | |
| 8.00 | -5.00 | 4.48 | -5.00 | 9.31 | 181.02 | -25.16 | 64.39 | 0.4672 | -1142.9 | 999999 | |
| 3.23 | -5.00 | 1.82 | -5.00 | 10.77 | 180.90 | -25.28 | 61.69 | 0.4785 | -822.7 | 999999 | |
| 18.24 | -5.00 | 10.24 | -5.00 | 9.99 | 180.94 | -25.25 | 63.14 | 0.4729 | -1126.4 | 999999 | |
| 2.16 | -5.00 | 1.22 | -5.00 | 10.56 | 180.58 | -25.61 | 62.38 | 0.4815 | -611.8 | 999999 | |
| 8.63 | -5.00 | 4.85 | -5.00 | 9.47 | 180.64 | -25.55 | 64.40 | 0.4736 | -970.2 | 999999 | |
| 1.53 | -5.00 | 0.86 | -5.00 | 9.38 | 180.37 | -25.82 | 64.80 | 0.4768 | -548.1 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.81 | 8.58 | 180.33 | -25.86 | 66.40 | 0.4726 | -676.0 | -544.1 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 8.24 | 180.11 | -26.07 | 67.22 | 0.4737 | -706.0 | -508.0 | |
| 0.00 | 1.71 | 0.00 | 0.97 | 10.29 | 179.71 | -26.48 | 63.62 | 0.4916 | -645.0 | -471.3 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 10.51 | 179.62 | -26.57 | 63.29 | 0.4942 | -485.0 | -421.6 | |
| 0.36 | 4.85 | 0.20 | 2.75 | 9.06 | 179.50 | -26.68 | 66.11 | 0.4870 | 483.5 | 40.2 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 8.79 | 178.87 | -27.32 | 67.09 | 0.4943 | 855.0 | 671.5 | |
| 0.00 | 1.98 | 0.00 | 1.13 | 8.62 | 178.57 | -27.61 | 67.64 | 0.4975 | 544.0 | 412.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 9.87 | 177.98 | -28.21 | 65.76 | 0.5127 | 750.0 | 600.3 | |
| 2.70 | 53.91 | 1.57 | 31.40 | 11.24 | 177.67 | -28.52 | 63.55 | 0.5251 | 1090.4 | 428.2 | |
| 1.80 | -21.00 | 1.05 | -21.00 | 11.46 | 177.61 | -28.58 | 63.21 | 0.5273 | 1064.4 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.16 | 10.41 | 177.47 | -28.72 | 65.17 | 0.5228 | 614.0 | 704.7 | |
| 6.74 | -21.00 | 3.93 | -21.00 | 11.41 | 177.29 | -28.89 | 63.55 | 0.5311 | 941.2 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.74 | 10.95 | 176.85 | -29.34 | 64.67 | 0.5343 | 756.0 | 605.8 | |
| 3.05 | 107.91 | 1.79 | 63.45 | 10.46 | 176.72 | -29.46 | 65.62 | 0.5331 | 1022.2 | 395.2 | |
| 8.18 | -26.00 | 4.80 | -26.00 | 10.80 | 176.44 | -29.75 | 65.21 | 0.5389 | 1120.4 | 999999 | |
| 0.27 | -26.00 | 0.16 | -26.00 | 10.53 | 176.40 | -29.79 | 65.72 | 0.5379 | 994.7 | 999999 | |
| 1.44 | 7.01 | 0.85 | 4.12 | 10.35 | 176.13 | -30.06 | 66.22 | 0.5405 | 919.6 | 632.6 | |
| 15.45 | -26.00 | 9.11 | -26.00 | 10.81 | 176.01 | -30.18 | 65.49 | 0.5447 | 998.5 | 999999 | |
| 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. | |