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→Классификация корональных выбросов массы
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| 1 || The exposure time of the <tex dpi="130">LASCO </tex> image
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| 2 || The time interval between the current and the previous image
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| 3 || The pixel size of the LASCO image
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| 4 || The mean brightness value of the reference image
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| 5 || The mean brightness value of the current image
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| 6 || The mean brightness value of the running difference
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| 7 || The standard deviation of the running difference
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| 8 || The number of pixels for <tex dpi="130">A</tex>
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| 9 || The threshold for segmentingAfrom the running difference
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| 10 || The maximum height (arcsecs from disk center) of <tex dpi="130">A</tex>
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| 11 || The height of the center of <tex dpi="130">A</tex>
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| 12 || The minimum height of <tex dpi="130">A</tex>
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| 13 || The starting angle of <tex dpi="130">A</tex>. The angle is calculated from North 0 clockwise
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| 14 || The angle of the center of <tex dpi="130">A</tex>
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| 15 || The ending angle of <tex dpi="130">A</tex>
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| 16 || The angular width of <tex dpi="130">A</tex>
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| 17 || The height difference (<tex dpi="130">h_1</tex>) between the maximum height of <tex dpi="130">A</tex> and <tex dpi="130">A_p</tex>
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| 18 || The height of the new moving region (<tex dpi="130">h_2</tex>) which is obtained by subtracting <tex dpi="130">A_p</tex> from <tex dpi="130">A</tex>
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| 19 || The speed which is computed using <tex dpi="130">h_1</tex>, divided by the interval time cadence
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| 20 || The speed which is computed using <tex dpi="130">h_2</tex> divided by the interval time cadence
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| 21 || The span width of the new moving region
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| 22 || The center angle of the new moving region
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Работа имеет большое практическое значение, так как корональные выбросы массы могут прерывать радиопередачу, наносить повреждения спутникам и линиям электропередачи, если они направлены в сторону Земли и имеют достаточную скорость и объем, чтобы достичь ее атмосферы<ref>https://en.wikipedia.org/wiki/Coronal_mass_ejection</ref>.
