The contribution of OSO-8 to solar physics from data analyzed as of May 1979 II - An optically thick region of the chromosphere-corona transition region observed with OSO 8 Line formation in the solar chromosphere. OSO 8 observations of the K2 component of the Ca II K line between the solar center and limb The high energy X-ray spectrum of 4U 1700-37 observed from OSO 8ĭUMONT, S. Observations of chromospheric lines from OSO-8ĭOLAN, J. F. Impulsive EUV bursts observed in C IV with OSO-8 Temporal and spatial fluctuations in strengths and widths of C IV and Si II lines observed with OSO 8ĪTHAY, R. G. Analysis of data from the mapping X-ray heliometer experimentĭata reduction and analysis for the graphite crystal X-ray spectrometer and polarimeter experiment flown aboard OSO-8 spacecraft Task 2: Analysis of data from the high resolution ultraviolet spectrometer experimentĪCTON, L. W. Steady flows in the chromosphere and transition-zone above active regions as observed by OSO-8 The contribution of OSO-8 to our knowledge of the chromosphere and transition region OSO-8 observations of Ca II H and K, Mg II h and k, L-alpha and L-beta above a sunspot OSO-8 observations of the impulsive phase of solar flares in the transition-zone and corona L alpha, L beta /of H I/, k and h /of Mg II/, K and H /of Ca II/ observations in a quiescent prominence with the OSO-8 LPSP instrument Transition-zone observations of rapid flare events as observed by OSO-8Ĭontinued analysis of OSO-8 and Kitt Peak data on solar faculae OSO 8 observational limits to the acoustic coronal heating mechanism The high energy X-ray spectrum of 4U 0900-40 observed from OSO 8 High energy X-ray observations of CYG X-3 from from OSO-8: Further evidence of a 34.1 day periodĭOLAN, J. F. High energy X-ray observations of Cyg X-3 from OSO-8 - Further evidence of a 34.1 day period Optically thick lines in a quiescent prominence - Profiles of Lyman-alpha, Lyman-beta /H I/, k and h /Mg II/, and K and H /Ca II/ lines with the OSO 8 LPSP instrument I - Principles and observational procedures from ground-based instruments and OSO-8 satelliteĮvidence of redshifts in the average solar line profiles of C IV and Si IV from OSO-8 observationsĮVIDENCE OF REDSHIFTS IN THE AVERAGE SOLAR LINE PROFILES OF CIV AND SIIV FROM OSO-8 OBSERVATIONS ORWIG, L. E.ĮRRATUM - THE HIGH ENERGY SPECTRUM OF 4U0900-40 OBSERVED FROM OSO-8Ī model of a sunspot chromosphere based on OSO 8 observationsĭUMONT, S.

Vertical flows of supergranular and mesogranular scale observed on the sun with OSO 8ĭOLAN, J. F.

Solar H-Lyman-alpha flux and profile relative measurements from OSO-8 - January 1976 to March 1978 OSO-8 observations of a quiescent prominence - A comparison of Lyman-alpha with theoretical intensities Simultaneous H and K Ca II, h and k Mg II, L-alpha and L-beta H I profiles of the Apsolar flare observed with the OSO-8/L.P.S.P. The high-energy X-ray spectrum of Centaurus XR-3 observed from OSO 8 High energy X-ray observations of COS-B gamma-ray sources from OSO-8ĭOLAN, J. F. Modernizing the OSO-8 High-Energy Celestial X-ray Data SetĭOLAN, J. F. Retrieved 258 abstracts, starting with number 1. Astrophysics Data System (ADS) Query Results from Astronomy Database

Per frost henriksen