An investigation has been made of the interrelationship of solar extreme ultraviolet (EUV) bursts, solar radio bursts, and terrestrial ionospheric sudden frequency deviations (SFD's). No direct general relationships between radio spectra or burst intensities and SFD incidence or magnitude (Delta f) have been found. If the EUV enhancement is greater than 3 percent at Lambda 304 or Lambda 630 A, there is an 85 percent probability of occurrence of an SFD. Time of maxima of EUV and radio bursts are found to coincide extremely well. (Author).Research supported by the Air Force Cambridge Research Laboratories, Air Force Systems Command, United States Air Force, L.G. Hanscom Field, Bedford, Massachusetts.Ionospheric Physics Laboratory Project 4643...
Observations of type II and III solar bursts indicate that while type III bursts may appear at any a...
cies derived from the 2-dimensional distribution represented in Fig. 4. Each distribution is very we...
Fiber bursts are a type of fine structure that frequently occurs in solar flares. Although observati...
High frequency sudden deviations caused by extreme ultraviolet flashes from solar flares in ionosphe...
We have reexamined the relationship between U-shaped peak-flux-density microwave spectra and solar p...
Solar radio phenomena designated as post-burst decreases, absorptions, and negative-burst events are...
Sun is the nearest star that employs us an opportunity to study the behavior of celestial bodies and...
Solar radio bursts have the potential to affect space and terrestrial navigation, communication, and...
The peak flux distribution of 40 years of solar radio burst data recorded by NOAA, as a function of ...
In this paper, some of the aspects of solar radio emission observed at frequencies 245, 410, 610, 14...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...
The solar extreme ultraviolet spectrum, in the wavelength range 226A to 1266A, is presented for data...
We have studied ionization excesses produced by enhancements of X-ray emission during solar flares u...
Context. Periodicities have frequently been reported across many wavelengths in the solar corona. Co...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
Observations of type II and III solar bursts indicate that while type III bursts may appear at any a...
cies derived from the 2-dimensional distribution represented in Fig. 4. Each distribution is very we...
Fiber bursts are a type of fine structure that frequently occurs in solar flares. Although observati...
High frequency sudden deviations caused by extreme ultraviolet flashes from solar flares in ionosphe...
We have reexamined the relationship between U-shaped peak-flux-density microwave spectra and solar p...
Solar radio phenomena designated as post-burst decreases, absorptions, and negative-burst events are...
Sun is the nearest star that employs us an opportunity to study the behavior of celestial bodies and...
Solar radio bursts have the potential to affect space and terrestrial navigation, communication, and...
The peak flux distribution of 40 years of solar radio burst data recorded by NOAA, as a function of ...
In this paper, some of the aspects of solar radio emission observed at frequencies 245, 410, 610, 14...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...
The solar extreme ultraviolet spectrum, in the wavelength range 226A to 1266A, is presented for data...
We have studied ionization excesses produced by enhancements of X-ray emission during solar flares u...
Context. Periodicities have frequently been reported across many wavelengths in the solar corona. Co...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
Observations of type II and III solar bursts indicate that while type III bursts may appear at any a...
cies derived from the 2-dimensional distribution represented in Fig. 4. Each distribution is very we...
Fiber bursts are a type of fine structure that frequently occurs in solar flares. Although observati...