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Synthesis of Si-Fe Chondrule-like Dust Analogues in RF Discharge Plasmas

Synthesis of Si-Fe Chondrule-like Dust Analogues in RF Discharge Plasmas

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_969746f95e174ef8961c1fa7fa1df188

Synthesis of Si-Fe Chondrule-like Dust Analogues in RF Discharge Plasmas

About this item

Full title

Synthesis of Si-Fe Chondrule-like Dust Analogues in RF Discharge Plasmas

Publisher

Basel: MDPI AG

Journal title

Applied sciences, 2024-10, Vol.14 (19), p.8714

Language

English

Formats

Publication information

Publisher

Basel: MDPI AG

More information

Scope and Contents

Contents

Chondrules are tiny particles that occur in stony meteorites and are considered as the building blocks of early asteroids and planets. It is believed that they were formed by the fast heating of the dust in the solar nebula. To date, there is no lab-scale experimental study of the formation of chondrules from the initial gas phase precursors follow...

Alternative Titles

Full title

Synthesis of Si-Fe Chondrule-like Dust Analogues in RF Discharge Plasmas

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_969746f95e174ef8961c1fa7fa1df188

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_969746f95e174ef8961c1fa7fa1df188

Other Identifiers

ISSN

2076-3417

E-ISSN

2076-3417

DOI

10.3390/app14198714

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