Photodestruction of hydrogen molecules in H I regions.
Photodissociation of hydrogen molecules in H I regions of interstellar medium, evaluating lifetime and density
Engineering topics
Publications and source records attributed to Stecher, T. P..
Photodissociation of hydrogen molecules in H I regions of interstellar medium, evaluating lifetime and density
Far UV extinction curve and wavelength dependence of interstellar polarization by graphite grains
Interstellar molecule formation as result of chemical exchange reactions between atoms of interstellar gas and atoms chemically bound to interstellar grains
Graphite grain formation in cool stars examined on basis of molecular equilibrium data for stellar atmospheres
Interstellar molecule formation by chemical exchange reactions between interstellar gas atoms and atoms chemically bound to interstellar grains
Interstellar molecular hydrogen abundance and possible source from giant stars
Mie scattering calculation to support theory that interstellar extinction is caused by graphite particles
Interstellar extinction in UV by measurement of stellar energy distributions between 3000 and 1200 angstroms
Geometrical UV reflectivity of Jupiter in terms of Rayleigh scattering determined from objective-grating rocket spectrometer
Jupiter photoelectric spectral scan in UV REPRODUCED as geometric reflectivity vs wavelength, using Aerobee rocket
Measurements from UV objective grating stellar spectrophotometers rocket flown to obtain stellar spectra
Graphite particles and interstellar extinction
Ultraviolet reflectivity of Jupiter from spectral scanning by Aerobee rocket spectrometers
Jupiter photoelectric spectral scan in UV REPRODUCED as geometric reflectivity vs wavelength, using Aerobee rocket
Stellar spectra and ultraviolet auroral observations by aerobee rockets in the 1,300-1,800 angstrom region
Ultraviolet aurora with north-south asymmetry and stellar spectra taken from aerobee rocket flight
Continuous absorption in solar atmosphere by quasi-hydrogen molecule