
The NRL Solar Physics Branch
GREAT SOLAR
HELIUM ERUPTION
This photograph of the sun
was taken using the extreme
ultraviolet radiation from ionized
helium, 304 Angstom wavelength.
It was taken on December 19, 1992
using the Solar Physics Branch's
SO82A Spectroheliograph
onboard the Skylab ATM.
The Solar Physics Branch is in the
Naval Research Laboratory (NRL) ,
Space Science Divison.
Researchers in the Solar Physics Branch have been involved in observational
and theoretical studies of the solar atmosphere since the early years of the
space age. Experiments developed at NRL have flown on NASA missions
such as Skylab/ATM, the OSO satellite series, the Space Shuttle STS-3,
Spacelab-2 and Atlas missions.
There are three active experimental programs in the Solar Physics Branch:
The Branch also maintains two database projects:
- The Space Physics Data System's HRTS/SKYLAB database with solar data from the Solar Physics Baranch's spectrograph and spectroheliograph instruments flown as part of the HRTS , Spacelab 2 and SKYLAB missions. This database is the under sponsorship of NASA's Space Physics Data System.
- The CHIANTI database for the calculation of astrophysical spectra. This database contains the most recent atomic data for calculating a collisionally dominated spectrum and is maintained by an international consortium of scientists.
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Late Breaking News and Other Items of Interest:
You can also visit the
NRL Space Science Division home page.
Naval Research Laboratory (NRL)
Solar Physics Branch / Code 7660
Last revised 25 September 1996
For more information send mail to
Ken Dere