Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Malcolm Druett"'
Autor:
Malcolm Druett, Eamon Scullion, Valentina Zharkova, Sarah Matthews, Sergei Zharkov, Luc Rouppe Van der Voort
Publikováno v:
Nature Communications, Vol 8, Iss 1, Pp 1-13 (2017)
The dynamic of plasma heating in solar flares can be effectively derived from observations of optical hydrogen H-α line emissions. Here the authors report the observation of a C1.5 class flare that produced two H-α ribbons, interpreted combining ra
Externí odkaz:
https://doaj.org/article/9d4dd231977a43d5a387f2d64c8712d9
Autor:
Connor Macrae, Sergei Zharkov, Sarah A. Matthews, Malcolm Druett, Satoshi Inoue, Valentina Zharkova, Ingolf Dammasch
Aims.The 6 September 2017 X9.3 solar flare produced very unique observations of magnetic field transients and a few seismic responses, or sunquakes, detected by the Helioseismic and Magnetic Imager (HMI) instrument aboard Solar Dynamic Observatory (S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6f6e0fd74c6b700306607c950ac0b66
https://nrl.northumbria.ac.uk/id/eprint/43079/9/NRL_43079.pdf
https://nrl.northumbria.ac.uk/id/eprint/43079/9/NRL_43079.pdf
Autor:
Malcolm Druett, Valentina Zharkova
Aims. Hydrogen Lyman continuum emission is greatly enhanced in the impulsive kernels of solar flares, with observations of Lyman lines showing impulsive brightening and both red and blue wing asymmetries, based on the images with low spatial resoluti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5350cf26fc9451c407bea1de67ceb98a
https://nrl.northumbria.ac.uk/id/eprint/37683/9/aa32427-17.pdf
https://nrl.northumbria.ac.uk/id/eprint/37683/9/aa32427-17.pdf
Autor:
Ben Snow, Malcolm Druett
Publikováno v:
Astronomy & Geophysics. 62:2.34-2.39
An RAS Specialist Discussion Meeting organized by Malcolm Druett and Ben Snow on 13 November 2020 drew a broad international audience to explore a tricky layer of the Sun
Publikováno v:
Astronomy & Astrophysics. 639:A79
In this paper we present the interpretation of the observations of the flare from 6 September 2017 reported in Paper I. These include gamma-ray (GR), hard X-ray (HXR), soft X-rays, Lyαline, extreme ultraviolet (EUV), Hα, and white light (WL) emissi
Autor:
Valentina Zharkova, Malcolm Druett
Publikováno v:
Astronomy & Astrophysics. 610:A68
Aim.Sharp rises of hard X-ray (HXR) emission accompanied by Hαline profiles with strong red-shifts up to 4 Å from the central wavelength, often observed at the onset of flares with the Specola Solare Ticinese Telescope (STT) and the Swedish Solar