SDO HMI 2011-10-14 11:59:02 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 |
| 115.02 | 402.21 | 62.22 | 218.12 | 10.42 | 48.92 | -23.60 | 77.57 | 0.4041 | -78.2 | 71.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-10-14 11:59:02 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 |
| 0.00 | 1.14 | 0.00 | 0.59 | 8.48 | 55.32 | -17.19 | 80.46 | 0.2978 | -881.0 | -652.3 | |
| 9.44 | 91.17 | 4.92 | 47.50 | 9.57 | 54.60 | -17.91 | 77.28 | 0.3123 | -1045.0 | -504.0 | |
| 13.29 | -2.00 | 6.92 | -2.00 | 9.24 | 54.59 | -17.93 | 78.34 | 0.3116 | -1184.6 | 999999 | |
| 1.22 | -2.00 | 0.64 | -2.00 | 9.84 | 54.52 | -17.99 | 76.49 | 0.3144 | -879.6 | 999999 | |
| 2.97 | -2.00 | 1.55 | -2.00 | 9.56 | 54.22 | -18.29 | 77.53 | 0.3184 | -767.7 | 999999 | |
| 0.00 | 2.19 | 0.00 | 1.14 | 9.34 | 54.01 | -18.51 | 78.31 | 0.3213 | -770.0 | -568.9 | |
| 0.00 | 1.66 | 0.00 | 0.87 | 7.89 | 52.80 | -19.71 | 83.12 | 0.3380 | -801.0 | -651.6 | |
| 5.68 | 8.65 | 3.00 | 4.56 | 9.23 | 52.51 | -20.01 | 79.31 | 0.3452 | -928.2 | -772.0 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 9.86 | 52.40 | -20.11 | 77.56 | 0.3484 | -805.0 | -667.7 | |
| 0.00 | 1.84 | 0.00 | 0.97 | 9.70 | 52.28 | -20.23 | 78.06 | 0.3499 | -893.0 | -744.7 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 9.45 | 52.04 | -20.47 | 78.86 | 0.3532 | -846.0 | -723.7 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 12.05 | 51.66 | -20.86 | 71.97 | 0.3678 | -707.0 | -599.2 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 8.40 | 51.91 | -20.61 | 81.88 | 0.3532 | -785.0 | -543.9 | |
| 4.11 | 4.46 | 2.18 | 2.36 | 9.81 | 51.79 | -20.72 | 77.99 | 0.3581 | -850.9 | -890.0 | |
| 0.00 | 0.87 | 0.00 | 0.46 | 9.17 | 51.73 | -20.78 | 79.77 | 0.3575 | -644.0 | -520.1 | |
| 0.00 | 2.19 | 0.00 | 1.16 | 9.32 | 51.59 | -20.92 | 79.41 | 0.3600 | -869.0 | -706.7 | |
| 1.57 | 10.93 | 0.84 | 5.82 | 10.63 | 51.41 | -21.11 | 75.91 | 0.3665 | 570.7 | -61.0 | |
| 1.40 | -17.00 | 0.74 | -17.00 | 10.39 | 51.30 | -21.22 | 76.63 | 0.3675 | -701.9 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.65 | 8.38 | 51.42 | -21.09 | 82.06 | 0.3610 | -552.0 | -376.9 | |
| 1.40 | 2.36 | 0.74 | 1.26 | 10.09 | 51.28 | -21.23 | 77.44 | 0.3669 | -723.5 | -713.1 | |
| 1.31 | 8.74 | 0.70 | 4.66 | 9.99 | 50.96 | -21.55 | 77.86 | 0.3716 | -902.5 | -753.6 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 9.85 | 50.68 | -21.84 | 78.32 | 0.3758 | -759.0 | -661.8 | |
| 0.00 | 1.92 | 0.00 | 1.03 | 10.11 | 50.40 | -22.12 | 77.75 | 0.3809 | -345.0 | -372.2 | |
| 1.92 | 5.16 | 1.03 | 2.77 | 9.17 | 49.97 | -22.54 | 80.36 | 0.3855 | 895.7 | 877.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 8.89 | 49.89 | -22.62 | 81.09 | 0.3863 | 629.0 | 494.6 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 11.85 | 49.40 | -23.11 | 73.85 | 0.4017 | -731.0 | -604.5 | |
| 0.00 | 2.71 | 0.00 | 1.46 | 11.33 | 49.25 | -23.27 | 75.19 | 0.4024 | -732.0 | -680.5 | |
| 2.88 | 3.58 | 1.56 | 1.94 | 9.37 | 49.07 | -23.44 | 80.11 | 0.4002 | -744.1 | -509.4 | |
| 19.32 | 41.61 | 10.47 | 22.57 | 10.53 | 48.78 | -23.73 | 77.35 | 0.4073 | -908.5 | -140.9 | |
| 0.52 | -29.00 | 0.28 | -29.00 | 10.73 | 48.60 | -23.92 | 76.93 | 0.4106 | -653.2 | 999999 | |
| 0.00 | 2.27 | 0.00 | 1.23 | 9.21 | 48.68 | -23.83 | 80.62 | 0.4060 | -770.0 | -572.5 | |
| 1.40 | -29.00 | 0.76 | -29.00 | 10.48 | 48.22 | -24.29 | 77.69 | 0.4159 | -573.0 | 999999 | |
| 0.35 | 1.75 | 0.19 | 0.95 | 9.65 | 47.82 | -24.70 | 79.79 | 0.4203 | 949.8 | 837.0 | |
| 0.44 | 2.71 | 0.24 | 1.48 | 10.06 | 47.52 | -25.00 | 78.92 | 0.4258 | 1013.0 | 833.2 | |
| 1.66 | 25.70 | 0.91 | 14.11 | 9.66 | 47.32 | -25.20 | 79.90 | 0.4281 | 925.5 | 580.2 | |
| 0.00 | 2.10 | 0.00 | 1.15 | 11.93 | 47.08 | -25.44 | 74.77 | 0.4374 | 632.0 | 534.3 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 10.82 | 47.05 | -25.47 | 77.31 | 0.4347 | 573.0 | 425.5 | |
| 9.96 | -35.00 | 5.47 | -35.00 | 9.61 | 46.98 | -25.53 | 80.09 | 0.4332 | 1002.2 | 999999 | |
| 0.00 | 5.16 | 0.00 | 2.84 | 10.68 | 46.72 | -25.79 | 77.73 | 0.4394 | 911.0 | 781.9 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 9.65 | 46.51 | -26.01 | 80.12 | 0.4406 | 529.0 | 481.1 | |
| 14.95 | 77.97 | 8.29 | 43.14 | 11.68 | 46.12 | -26.40 | 75.73 | 0.4511 | 1094.2 | 533.7 | |
| 0.00 | 2.01 | 0.00 | 1.11 | 10.30 | 46.11 | -26.40 | 78.79 | 0.4479 | 910.0 | 745.8 | |
| 0.00 | 2.71 | 0.00 | 1.50 | 11.04 | 46.04 | -26.47 | 77.15 | 0.4506 | 295.0 | 265.5 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 7.51 | 46.20 | -26.32 | 85.03 | 0.4431 | 738.0 | 601.1 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 9.44 | 45.88 | -26.63 | 80.74 | 0.4499 | 669.0 | 570.7 | |
| 0.00 | 1.49 | 0.00 | 0.83 | 10.48 | 45.59 | -26.93 | 78.53 | 0.4563 | 956.0 | 837.4 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 11.26 | 45.41 | -27.11 | 76.90 | 0.4607 | 710.0 | 594.6 | |
| 0.96 | 1.92 | 0.54 | 1.07 | 10.68 | 45.40 | -27.12 | 78.14 | 0.4596 | 824.0 | 729.5 | |
| 0.00 | 1.84 | 0.00 | 1.02 | 10.35 | 45.36 | -27.15 | 78.87 | 0.4595 | 648.0 | 574.0 | |
| 2.53 | 4.11 | 1.42 | 2.30 | 11.03 | 45.09 | -27.43 | 77.49 | 0.4650 | 876.3 | 569.7 | |
| 1.05 | 64.51 | 0.59 | 36.29 | 11.46 | 44.66 | -27.85 | 76.71 | 0.4724 | 809.3 | 298.3 | |
| 12.85 | -51.00 | 7.21 | -51.00 | 11.07 | 44.64 | -27.88 | 77.55 | 0.4719 | 1048.4 | 999999 | |
| 1.84 | -51.00 | 1.03 | -51.00 | 11.23 | 44.31 | -28.21 | 77.30 | 0.4772 | 827.6 | 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. | |