X-ray Structures of the Sun during the Importance 1N Flare of 8 June 1968
- 9 August 1968
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 161 (3841), 564-567
- https://doi.org/10.1126/science.161.3841.564
Abstract
High-resolution solar x-ray images were obtained with a rocket-borne grazing incidence telescope. The x-ray flare is large in extent, has fine strulctuire, and follows a neutral magnetic line. X-ray emitting coronal links interconnect active regions. The general coronal emission at the limb and several faint regions on the disc are observed.Keywords
This publication has 12 references indexed in Scilit:
- The X-Ray Emission Spectrum of a Solar Active RegionThe Astrophysical Journal, 1968
- Study of X-Ray Images of the Sun at Solar MinimumThe Astrophysical Journal, 1968
- Observation of the Solar Flare X-Ray Emission-Line Spectrum of Iron from 1.3 to 20 ÅThe Astrophysical Journal, 1967
- Solar X-Ray Spectrum from 1.9 to 25 ÅThe Astrophysical Journal, 1967
- A Functioning Model of the Soft X-ray Slitless SpectrometerApplied Optics, 1966
- X-ray emission of the SunSpace Science Reviews, 1965
- Spectral and Photometric Measurements of Solar X-Ray Emission Below 60 ÅThe Astrophysical Journal, 1965
- Soft X-ray Image of the SunNature, 1965
- The Heating of the Solar Chromosphere, Plages, and Corona by Magnetohydrodynamic Waves.The Astrophysical Journal, 1961
- A “telescope” for soft X-ray astronomyJournal of Geophysical Research, 1960