Radar observations and the extent of coronal heating.
Coronal heating extent placed at 1.6 solar radii by 38 MHz radar investigation studies, noting agreement with coronal density calculation
MAGNETOHYDRODYNAMIC WAVE↗
Engineering topics
Brandt, J. C.
Publications and source records attributed to Brandt, J. C..
Interplanetary gas. XIV.
Super-Alfvenic point or distance of effective corotation for loss of angular momentum in solar wind plasma
SOLAR ROTATION↗
The search for solar M-regions.
Search for solar M-regions complicated by velocity decrease near active sun, considering corpuscular streams as enhanced solar wind
SOLAR ACTIVITY EFFECT↗
Temperature of the Solar Corona from Intensity Gradients Measured During the May 30, 1965 Total Eclipse
Solar corona temperature from intensity gradients measured during total eclipse of May 30, 1965
SOLAR ECLIPSE↗
Temperature of the Solar Corona from Intensity Gradients Measured During the May 30, 1965 Total Eclipse
Corona temperature and logarithmic intensity gradients determined by pointwise three-color photoelectric photometry during solar eclipse
TEMPERATURE MEASUREMENT↗
Interplanetary gas. XIII.
Cometary tails relationship to interplanetary gas properties and solar wind velocities deduced from observation of type I ionic cometary tails
SOLAR WIND↗
A five colour photometry and polarimetry of the zodiacal light - A preliminary report
Five color photometry and polarimetry of the zodiacal light
Brandt, J. C.↗
On mass models of the galactic system.
Discrepancies between various mass models of galactic systems, commenting on rotation curves
GALACTIC EVOLUTION↗
Interplanetary gas. XIII - Gross plasma velocities from the orientations of ionic comet tails
Interplanetary gas and solar wind plasma velocities from orientations of ionic comet tails
VELOCITY↗
Interplanetary gas. viii - on the importance of radiative losses.
Radiative losses for all ions in the extended solar corona
INTERPLANETARY GAS↗
INTERPLANETARY GAS. VIII. ON THE ROLE OF RADIATIVE LOSSES INTERPLANETARY GAS. VIII. ON THE ROLE OF RADIATIVE LOSSES
Radiative losses evaluated for all significant ions present in interplanetary gas from 4 to 215 radii - solar corona energy balance
INTERPLANETARY GAS↗