Deducing electron properties from hard X-ray observations
X-radiation from energetic electrons is the prime diagnostic of flare-accelerated electrons.
The observed X-ray flux (and polarization state) is fundamentally a convolution of the cross …
The observed X-ray flux (and polarization state) is fundamentally a convolution of the cross …
Solar flare hard X-ray observations
BR Dennis - Solar physics, 1988 - Springer
Recent hard X-ray observations of solar flares are reviewed with emphasis on results
obtained with instruments on the Solar Maximum Mission satellite. Flares with three different …
obtained with instruments on the Solar Maximum Mission satellite. Flares with three different …
[图书][B] The physics of solar flares
E Tandberg-Hanssen, AG Emslie - 1988 - books.google.com
Few phenomena have stirred the imaginations of solar scientists as much as the explosive
energy of solar flares. In The Physics of Solar Flares, first published in 1988, Einar Tandberg …
energy of solar flares. In The Physics of Solar Flares, first published in 1988, Einar Tandberg …
Solar hard X-ray bursts
BR Dennis - Solar physics, 1985 - Springer
The major results from SMM are presented as they relate to our understanding of the energy
release and particle transportation processes that lead to the high-energy X-ray aspects of …
release and particle transportation processes that lead to the high-energy X-ray aspects of …
Measurements of the coronal acceleration region of a solar flare
S Krucker, HS Hudson, L Glesener… - The Astrophysical …, 2010 - iopscience.iop.org
ABSTRACT The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) and
the Nobeyama Radioheliograph (NoRH) are used to investigate coronal hard X-ray and …
the Nobeyama Radioheliograph (NoRH) are used to investigate coronal hard X-ray and …
[HTML][HTML] Gas dynamics in the impulsive phase of solar flares. I Thick-target heating by nonthermal electrons
F Nagai, AG Emslie - Astrophysical Journal, Part 1 (ISSN 0004 …, 1984 - adsabs.harvard.edu
A numerical investigation is carried out of the gas dynamical response of the solar
atmosphere to a flare energy input in the form of precipitating nonthermal electrons. Rather …
atmosphere to a flare energy input in the form of precipitating nonthermal electrons. Rather …
Solar microwave bursts—A review
MR Kundu, L Vlahos - Space Science Reviews, 1982 - Springer
We review the observational and theoretical results on the physics of microwave bursts that
occur in the solar atmosphere. We particularly emphasize the advances made in burst …
occur in the solar atmosphere. We particularly emphasize the advances made in burst …
RHESSI as a hard X-ray polarimeter
Although designed primarily as a hard X-ray imager and spectrometer, the Ramaty High-
Energy Solar Spectroscopic Imager (RHESSI) is also capable of measuring the polarization …
Energy Solar Spectroscopic Imager (RHESSI) is also capable of measuring the polarization …
[HTML][HTML] Microwave signature of thick-target electron beams in solar flares
AG Emslie, DF Smith - … Journal, Part 1 (ISSN 0004-637X), vol …, 1984 - adsabs.harvard.edu
Microwave signature of thick-target electron beams in solar flares ADS Classic is now deprecated.
It will be completely retired in October 2019. This page will automatically redirect to the new …
It will be completely retired in October 2019. This page will automatically redirect to the new …
[HTML][HTML] A thermal/nonthermal model for solar microwave bursts
SG Benka, GD Holman - … Journal, Part 1 (ISSN 0004-637X), vol …, 1992 - adsabs.harvard.edu
A thermal/nonthermal model for solar microwave bursts ADS Classic is now deprecated. It will
be completely retired in October 2019. This page will automatically redirect to the new ADS …
be completely retired in October 2019. This page will automatically redirect to the new ADS …