1 / 9

Abstract Analysis

Abstract Analysis. BY1203127 张 翀. Abstract. Introduction.

pomona
Download Presentation

Abstract Analysis

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Abstract Analysis BY1203127 张 翀

  2. Abstract

  3. Introduction • Background: Magnetospheric line radiation (MLR) events are electromagnetic waves in the frequency range of about 1-8 kHz observed in the inner magnetosphere that, when presented in a form of frequency-time spectrograms, consist of several nearly parallel and almost equidistant intense lines. • Previous Work and Problems : Although many observations of these events have been reported using ground-based instruments and a survey of a large data set based on low-altitude satellite data has been published recently, their origin remains unclear.

  4. Method • We use low-altitude satellite observations of MLR events to study their properties. • The satellite, unlike ground observatories, is moving, it allows us to analyze the properties of the events as a function of the position, especially L-shell.

  5. Result • We show that neither the frequency spacing of the events nor their frequency drift varies significantly with the L-shell where the event is observed. • Moreover, the frequency drift is generally positive. The individual lines forming the events cannot be explained as harmonics of the base frequency equal to the frequency spacing.

  6. Conclusion • We suggest that a possible generation mechanism might be an interaction between a wave of a carrier frequency and an additional wave with the frequency equal to the observed frequency spacing. • We cannot exclude that it comes from human activity (power lines), but a magnetospheric origin is more likely. • We suggest that the emissions might be guided by the plasmasphere inner boundary before they deviate to lower L-shells at altitudes of a few thousands of kilometers.

  7. Active and Passive • This abstract prefers to use the active sentences. There are 10 sentences in total, and 5 of them begin with ‘We’. And all the 3 sentences in the conclusion part are active. • Because the background is objective, but the method and result, especially the conclusion is much more likely predicted by the author. Maybe the authors’ suggestion is not correct, it just shows a possible subsequent research direction.

  8. Thank you

More Related