Observation of chromospheric evaporation during the solar maximum mission

Solar Physics ◽  
1983 ◽  
Vol 86 (1-2) ◽  
pp. 67-77 ◽  
Author(s):  
E. Antonucci ◽  
B. R. Dennis
Keyword(s):  
Solar Maximum ◽  
Solar Maximum Mission ◽  
Chromospheric Evaporation

Variations of mesospheric equatorial ozone as observed by the Solar Maximum Mission

1990 ◽  
Vol 17 (3) ◽  
pp. 299-302 ◽  
Author(s):  
Arthur C. Aikin ◽  
William Henze ◽  
David J. Kendig ◽  
Roy Nakatsuka ◽  
Henry J. P. Smith
Keyword(s):  
Solar Maximum ◽  
Solar Maximum Mission

An Ultraviolet Polarimeter For The Solar Maximum Mission

1979 ◽  
Vol 18 (3) ◽  
Author(s):  
John Calvert ◽  
Donald Griner ◽  
Justino Montenegro ◽  
Frank Nola ◽  
Frank Rutledge ◽  
...  
Keyword(s):  
Solar Maximum ◽  
Solar Maximum Mission

scholarly journals Preface

1991 ◽  
Vol 336 (1643) ◽  
pp. 323-323
Keyword(s):  
Solar Flare ◽  
Energy Release ◽  
Gamma Rays ◽  
Solar Flares ◽  
Solar Maximum ◽  
Interplanetary Space ◽  
Release Site ◽  
Solar Maximum Mission ◽  
New Information ◽  
Three Space

During the period of the 1980 solar maximum three space missions (P78-1, Solar Maximum Mission and Hinotori ) carried out extensive studies of solar flares. In their different ways all of these missions contributed significant new information to our understanding of the solar flare phenomenon. In this volume the contribution made by these three spacecraft to the study of the energy release and the related creation of high-tem perature plasma, the transport of energy from the primary release site, the production of gamma-rays at energies up to 10 MeV and the ejection of solar matter into interplanetary space are reviewed.

Atomic physics calculations relevant to solar flare spectra

1991 ◽  
Vol 336 (1643) ◽  
pp. 471-484 ◽  
Keyword(s):  
Solar Flare ◽  
Atomic Physics ◽  
Solar Flares ◽  
Solar Maximum ◽  
Emission Lines ◽  
Atomic Data ◽  
Solar Maximum Mission ◽  
X Ray ◽  
Physical Conditions ◽  
Recombination Processes

Solar flare spectra in the ultraviolet and X-ray wavelength regions are rich in emission lines from highly ionized ions, formed at temperatures around 10 7 K. These lines can be used as valuable diagnostics for probing the physical conditions in solar flares. Such analyses require accurate atomic data for excitation, ionization and recombination processes. In this paper, we present a review of work which has already been carried out, in particular for the Solar Maximum Mission observations, and we look to future requirements for Solar-A .

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