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Análisis cinemático de una eyección coronal de masa de 10 a 46 radios solares
Bibcode: 2022BAAA...63...24D

Cremades, H.; Balmaceda, L. A.; Di Lorenzo, L.

In this work we perform the three-dimensional reconstruction (3D) of the morphology of a coronal mass ejection (CME), in the range of heliocentric distances of approximately 10 to 46 solar radii. The event occurs on 2 April 2019, and we use observations made by LASCO-C3 aboard the Solar and Heliospheric Observatory (SOHO), SECCHI-COR2 and HI-1 abo…

2022 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
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