NASA LogoNTRSNTRS - NASA Technical Reports ServerSearchmore_vertCollectionsAboutNewsHelpLogin Back to ResultsSolar Flares and Coronal Physics Using P/OF as a Research ToolThis NASA Conference Publication contains the proceedings of the Workshop on Solar High-Resolution Astrophysics Using the Pinhole/Occulter Facility held at NASA Marshall Space Flight Center, Alabama, on May 8 to 10, 1985. These proceedings include primarily the invited tutorial papers, extended abstracts of contributed poster papers, and summaries of subpanel (X-Ray and Coronal Physics) discussions. Both observational and theoretical results are presented. Although the emphasis of the Workshop was focused primarily on topics peculiar to solar physics, one paper is included that discusses the P/0F as a tool for X-ray astronomy.Document ID19860015143Acquisition SourceLegacy CDMSDocument TypeConference ProceedingsAuthorsTandberg, E.*(NASA Marshall Space Flight Center Huntsville, AL, United States)*Wilson, R. M.*(NASA Marshall Space Flight Center Huntsville, AL, United States)*Hudson, R. M.*(California Univ. San Diego, La Jolla, United States)*Date AcquiredSeptember 5, 2013Publication DateApril 1, 1986Subject CategorySolar PhysicsReport/Patent NumberM-523NASA-CP-2421NAS 1.55:2421Accession Number86N24614Distribution LimitsPublicCopyrightWork of the US Gov. Public Use Permitted.Available DownloadsNameType19860015143.pdfSTIcloud_downloadcontent_copyvisibilityRelated RecordsIDRelationTitle19860015153WorkWhy P/OF should look for evidences of over-dense structures in solar flare hard X-ray sources19860015145WorkThe Sun at high spatial resolution:  The physics of small spatial structures in a magnetized medium19860015157WorkThe solar radio corona:  Manifestations of energetic electrons19860015155WorkHard X-ray imaging and the relative contribution of thermal and nonthermal emission in flares19860015151WorkTheoretical motivation for high spatial resolution, hard X-ray observations during solar flares19860015149WorkInterplanetary energetic particles, coronal flares and hard X-ray microflares19860015159WorkHigh-spectral resolution solar microwave observations19860015168WorkThe Pinhole/Occulter as a tool for X-ray astronomy19860015146WorkThe flare kernel in the impulsive phase19860015144WorkThe concept of the Pinhole/Occulter Facility19860015158WorkRadio imaging of flares19860015167WorkOn the formation of coronal cavities19860015165WorkInterpretation of coronal synoptic observations19860015156WorkSuper active regions and production of major solar flares19860015166WorkWave speeds in the corona and the dynamics of mass ejections19860015148WorkResults from the solar maximum mission19860015154WorkThe heating of the thermal plasma with energetic electrons in small solar flares19860015150WorkOptical imaging spectroscopy19860015152WorkThe role of high resolution observations in determining energy release and transport processes19860015164WorkSolwind observations of coronal mass ejections during 1979-198519860015163WorkCorona and solar wind19860015147WorkX-ray imaging of flare loops and coronal arches19860015161WorkShort-lived solar burst spectral component at f approximately 100 GHz19860015162WorkPolar-cap and coronal-hole-associated brightenings of the Sun at millimeter wavelengths19860015160WorkSingle-dish high sensitivity determination of solar limb emission at 22 and 44 GHzvisibility_offNo Preview Available
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