HRTS/SKYLAB Database



Profiles on C IV 1548 and 1550 Angstrom
transition zone lines in a sunspot (center)
bordered by an active region. The spatial
variations in the emission correspond to
the vertical direction where the spatial
resolution of the spectra are on the order
of 1" (725 km on the Sun). Doppler
shifts (horizontal direction) over sunspot
reveal down flows of up to 150 km/s.

HRTS Project
Solar Physics Branch
Naval Research Laboratory


The HRTS/SKYLAB Database is comprized of data from the HRTS experiment flown on HRTS rockets and the HRTS experiment on Spacelab-2 as well as data from the NRL SO82B Ultraviolet Spectrograph flown on the SKYLAB Mission. This database is the under sponsorship of NASA's Space Physics Data System.

Data is organized by mission:




Naval Research Laboratory (NRL)
Solar Physics Branch / Code 7660

Last revised 04 October 1996
For more information send mail to Ken Dere