Titlebook: Coronal Disturbances; Gordon Newkirk Book 1974 International Astronomical Union 1974 Corona.Planet.Solar flare.Variation.cosmic ray.observ

mechanical

Kidnap

Analysis of EUV Observations of a Coronal Active Region Made during the 7 March 1970 Eclipseon on the NE limb (Gabriel ., 1971). The condensation shows the existence of loop structure, which defines the local magnetic fields, and is apparent in forbidden lines including those of Si ., Si ., S ., Fe ., Fe . and Fe . which lie between 1200 Å and 2050 Å (Jordan, 1971). These lines are formed

白杨鱼

defile

Spectral Association of the 7 August 1972 Solar Radio Burst with Particle Accelerationory (Figure 1) provide a basis for correlation studies (especially timing information) of the associated white light flare, the high energy particle emission, type II bursts, and many other phenomena. This is perhaps the first time that sufficient radio coverage (i.e., data above 10000 MHz) was avai

defendant

X-Ray Emission in Absence of Flares Related to Hα Activity and Type III Burst Productiontics of the particle acceleration process operating when a Hα-flare may or may not be detectable. The Hα observations were made by Meudon Observatory with a Hα telescope fitted with a 0.75 Å band pass Lyot filter. During a 10 s period, three pictures were obtained — one at the Hα line center, one at

right-atrium

舔食

allude

Oversee

Gobble

The Flash Phase of Solar Flares: Satellite Observations of Electronsrvations support a two stage acceleration process for electrons, one stage commonly occurring at the flare flash phase and accelerating electrons up to ~ 100 keV, and a second stage occurring only in large proton flares and accelerating electrons up to relativistic energies. The location of the acce