作者: M. Hegde , K. M. Hiremath , Vijayakumar H. Doddamani , Shashanka R Gurumath
DOI: 10.1007/S12036-015-9338-9
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摘要: Present study probes temporal changes in the area and radiative flux of near equatorial coronal hole associated with solar wind parameters such as speed, density, magnetic field temperature. Using high resolution data from SDO/AIA for two wavelengths 193 A 211 A, holes are extracted examined association speed parameters. We find a strong between different wind. For both wavelength bands, we also compute energy earth it is found to be similar order that energy. However, owing almost magnitudes emitted by due wind, conjectured might have originated around same height where line formed corona.