Imaging spectroscopy of solar radio burst fine structures
Current Language EN
English English Türkçe Türkçe Español Español Português Português Pусский Pусский Filipino Filipino Tiếng Việt Tiếng Việt हिन्दी हिन्दी العربية العربية বাংলা বাংলা Deutsch Deutsch 中文 中文

Imaging spectroscopy of solar radio burst fine structures

Kontar, E. P.;Yu, S.;Kuznetsov, A. A.;Emslie, A. G.;Alcock, B.;Jeffrey, N. L. S.;Melnik, V. N.;Bian, N. H.;Subramanian, P.;
Nature communications 2017 Vol. 8 pp. 1-9
206
kontar2017imagingnature

Abstract

Radio observations of the solar atmosphere provide a unique view on the non-thermal processes in the outer atmosphere. Here the authors use LOFAR observations to demonstrate that the observed radio burst characteristics are dominated by propagation effects rather than underlying emission variations.

Keywords

Engineering (General). Civil engineering (General) Science physics astronomy

Access

URL:
http://link.springer.com/article/10.1038/s41467-01...

Citation

ID: 99532
Ref Key: kontar2017imagingnature
Use this key to autocite in SciMatic or Thesis Manager

References

References

No Bibliography

Blockchain Verification

Account:
NFT Contract Address:
0x95644003c57E6F55A65596E3D9Eac6813e3566dA
Article ID:
99532
Unique Identifier:
e4223937a32e6ce5b590aeeb0da7772a
Network:
Scimatic Chain (ID: 481)
Blockchain Readiness Checklist
Authors
Abstract
Journal Name
Year
Title
5/5
Creates 1,000,000 NFT tokens for this article
Token Features:
  • ERC-1155 Standard NFT
  • 1 Million Supply per Article
  • Transferable via MetaMask
  • Permanent Blockchain Record
Blockchain QR Code
Scan with Saymatik Web3.0 Wallet
Gas fees required in SCI Coins
Buy SCI

Saymatik Web3.0 Wallet

Google Play
App Store