Add to ORKGAbstract. The Transition Region and Coronal Explorer (TRACE) gave us the highest EUV spatial resolution and the Ramaty High Energy Solar Spec-trometric Imager (RHESSI) gave us the highest hard X-ray and gamma-ray spectral resolution to study solar flares. We review a number of recent highlights obtained from both missions that either enhance or challenge our physical understanding of solar flares, such as: 1. Multi-thermal Diagnostic of 6.7 and 8.0 keV Fe and Ni lines, 2. Multi-thermal Conduction Cooling Delays
The 3.8–10 keV solar flare spectrum includes lines of highly stripped Ca, Fe, and Ni ions, as well a...
International audienceThe main goal of the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mi...
The 4-10 keV solar flare spectrum includes highly excited lines of stripped Ca, Fe, and Ni ions as w...
Observations of solar flares in X-rays and gamma-rays provide the most direct information about the ...
Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays at 100 MeV. Th...
Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays beyond 1 GeV. ...
Solar flares can release ~1e33 ergs of power, accelerate particles to relativistic speeds, heat plas...
We investigate the X-ray and UV emission detected by RHESSI and TRACE in the context of a solar flar...
We investigate the X-ray and UV emission detected by RHESSI and TRACE in the context of a solar flar...
We investigate the X-ray and UV emission detected by RHESSI and TRACE in the context of a solar flar...
The Transition Region And Coronal Explorer Satellite, TRACE, launched in 1998, has proved a valuable...
The Transition Region And Coronal Explorer Satellite, TRACE, launched in 1998, has proved a valuable...
Solar flares are huge explosions on the Sun that release a tremendous amount of energy from the coro...
Abstract. Recent results of solar flare imaging at X-ray and γ-ray energies are briefly summarized u...
International audienceThe main goal of the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mi...
The 3.8–10 keV solar flare spectrum includes lines of highly stripped Ca, Fe, and Ni ions, as well a...
International audienceThe main goal of the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mi...
The 4-10 keV solar flare spectrum includes highly excited lines of stripped Ca, Fe, and Ni ions as w...
Observations of solar flares in X-rays and gamma-rays provide the most direct information about the ...
Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays at 100 MeV. Th...
Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays beyond 1 GeV. ...
Solar flares can release ~1e33 ergs of power, accelerate particles to relativistic speeds, heat plas...
We investigate the X-ray and UV emission detected by RHESSI and TRACE in the context of a solar flar...
We investigate the X-ray and UV emission detected by RHESSI and TRACE in the context of a solar flar...
We investigate the X-ray and UV emission detected by RHESSI and TRACE in the context of a solar flar...
The Transition Region And Coronal Explorer Satellite, TRACE, launched in 1998, has proved a valuable...
The Transition Region And Coronal Explorer Satellite, TRACE, launched in 1998, has proved a valuable...
Solar flares are huge explosions on the Sun that release a tremendous amount of energy from the coro...
Abstract. Recent results of solar flare imaging at X-ray and γ-ray energies are briefly summarized u...
International audienceThe main goal of the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mi...
The 3.8–10 keV solar flare spectrum includes lines of highly stripped Ca, Fe, and Ni ions, as well a...
International audienceThe main goal of the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) mi...
The 4-10 keV solar flare spectrum includes highly excited lines of stripped Ca, Fe, and Ni ions as w...