When we look at a solar flare we observe at relatively close hand a sample of the most energetic phenomena in the universe. These dynamic eruptions can only truly be appreciated from time-lapse movies or spectra. They fill the interplanetary medium with cosmic rays and shock waves, and produce plasmas with temperatures of 50 million degrees. They are rewarding both from the astrophysical and aesthetic points of view
Analysis is made of observations of the August, 1972 flares at Big Bear and Tel Aviv, involving mono...
The Sun offers a convenient nearby laboratory to study the physical processes of particle accelerati...
Solar eruptive phenomena correspond to various kind of transient activities occurring in the solar a...
Optical observationd now present considerable information on the flare process. It is always associa...
Because the Earth resides in the atmosphere of our nearest stellar neighbor, events occurring on the...
We present, in general, the solar flare phenomenon going through several aspects: a brief historical...
The observation of solar flares in visual light is mostly made in the light of hydrogen-α, which sho...
I have studied a number of flares for which good X-ray and optical data were available. An average l...
We analyze large-scale H-alpha movies of the large spot group of Sept. 13–26, 1963, together with ra...
Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays beyond 1 GeV. ...
Space-based observations of high-energy emission from solar flares have contributed greatly to our u...
We describe observations of the class 3+ flare of August 28, 1966, made at the Mount Wilson Observat...
accepted in Nature PhysicsInternational audienceFlares are powerful energy releases occurring in ste...
As one of the most intense activities on the solar surface, flares have been extensively observed an...
Study of rapid fluctuations in the emission of radiation from solar flares provides a promising appr...
Analysis is made of observations of the August, 1972 flares at Big Bear and Tel Aviv, involving mono...
The Sun offers a convenient nearby laboratory to study the physical processes of particle accelerati...
Solar eruptive phenomena correspond to various kind of transient activities occurring in the solar a...
Optical observationd now present considerable information on the flare process. It is always associa...
Because the Earth resides in the atmosphere of our nearest stellar neighbor, events occurring on the...
We present, in general, the solar flare phenomenon going through several aspects: a brief historical...
The observation of solar flares in visual light is mostly made in the light of hydrogen-α, which sho...
I have studied a number of flares for which good X-ray and optical data were available. An average l...
We analyze large-scale H-alpha movies of the large spot group of Sept. 13–26, 1963, together with ra...
Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays beyond 1 GeV. ...
Space-based observations of high-energy emission from solar flares have contributed greatly to our u...
We describe observations of the class 3+ flare of August 28, 1966, made at the Mount Wilson Observat...
accepted in Nature PhysicsInternational audienceFlares are powerful energy releases occurring in ste...
As one of the most intense activities on the solar surface, flares have been extensively observed an...
Study of rapid fluctuations in the emission of radiation from solar flares provides a promising appr...
Analysis is made of observations of the August, 1972 flares at Big Bear and Tel Aviv, involving mono...
The Sun offers a convenient nearby laboratory to study the physical processes of particle accelerati...
Solar eruptive phenomena correspond to various kind of transient activities occurring in the solar a...