Solar Particle Alert Network
Revision as of 11:09, 11 December 2006 (edit) Paul (Talk | contribs) ← Previous diff |
Revision as of 23:40, 11 December 2006 (edit) Paul (Talk | contribs) Next diff → |
||
Line 9: | Line 9: | ||
It also shared a role in the [[Carnarvon Location Project]]:<BR> | It also shared a role in the [[Carnarvon Location Project]]:<BR> | ||
- | . . . a Satellite [[Carnarvon Location Project#Tracking_Camera|Tracking Camera]] was briefly located at SPAN.<BR> | + | . . . a Satellite [[Carnarvon Location Project#Tracking_Camera|Tracking Camera]] was briefly located at SPAN;<BR> |
. . . and [[Range and Range Rate]] hosted the [[Carnarvon Location Project#Mobile_Laser|Mobile Laser]] Tracking System. | . . . and [[Range and Range Rate]] hosted the [[Carnarvon Location Project#Mobile_Laser|Mobile Laser]] Tracking System. | ||
Revision as of 23:40, 11 December 2006
SPAN systems
Back to Station Equipment
The Solar Particle Alert Network (SPAN) observatory, installed early in 1965, was critical to the safety of the Apollo astronauts. The study of the relationship between sunspot activity and intense solar flares would hopefully enable NASA to predict radiation hazards to astronauts on Apollo missions.
The three NASA multiple-telescope observatories (Boulder, USA; Canary Islands; and Carnarvon) were spaced at approximately 120° intervals around the world. They maintained continuous 24-hour monitoring of the sun with real-time reporting of flare activity, assisted by an observatory at Houston and four other observatories contracted to NASA. Several other observatories, associated with the Solar Forecast Centre, also contributed data to SPAN Control.
SPAN hosted two other facilities relatively unimportant to the main work of the station: a Riometer (Relative Ionospheric Opacity Meter)and a Jupiter Monitor.
It also shared a role in the Carnarvon Location Project:
. . . a Satellite Tracking Camera was briefly located at SPAN;
. . . and Range and Range Rate hosted the Mobile Laser Tracking System.
We are indebted to Dave Gardiner, Jim Gregg, David Johns, and Hans Lemmens for their contributions to the SPAN pages.