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How a Strong Solar Coronal Mass Ejection can Eject Dust from the Moon?s Surface to the Earth's Atmosphere View all abstracts by submitter

Fran De Aquino   Submitted: 2016-09-07 08:22

A solar coronal mass ejection (CME) is a massive ejection of plasma from the Sun to the space. In this article it is shown how a strong solar coronal mass ejection can eject dust from the Moon?s Surface to the space. If this ejection occurs when the Moon is in specific regions of its trajectory around the Earth, then this lunar dust can be gravitationally attracted to the Earth, forming a dust shell at the Earth's atmosphere, which can block the sunlight for some days.

Authors: Fran De Aquino
Projects: None

Publication Status: Published
Last Modified: 2016-09-07 12:10
Go to main E-Print page  Magneto-Frictional Modeling of Coronal Nonlinear Force-Free Fields: II. Application to Observations  Radio Diagnostics of Electron Acceleration Sites During the Eruption of a Flux Rope in the Solar Corona  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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