English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

The purpose of this work is to draw attention of readers to a problem ofpossible differences in generation of magnetic storms induced by various largescale solar wind (SW) streams: CIR, Sheath and ICME (including MC and Ejecta).Recently we showed that when using a modification of formula by Burton et al.[1975] for connection of interplanetary conditions with Dst and Dst* indicesthe efficiency of storm generation by Sheath and CIR is about 50 percent higherthan generation by ICME [Nikolaeva et al., 2013, 2015]. In the literature thereare many various functions coupling (FC) various interplanetary parameters withmagnetospheric state. In this work we study the efficiency of main phase stormgeneration by different SW streams when using 12 another FCs on the basis ofOMNI data during 1976 ... 2000. Obtained results show that for most part of FCsSheaths have the highest efficiency and MCs have the lowest efficiency inaccordance with our previous results. The reliability of the obtained data andpossible reasons of divergences for various FCs and various SW types requirefurther researches.

Does generation of magnetic storm depend on type of solar wind?