Physics
Scientific paper
Aug 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...8011982h&link_type=abstract
Final Report Ruhr Univ., Bochum (Germany, F.R.). Lehrstuhl für Physikalische Chemie 1.
Physics
Actinometers, Ammonia, Nitric Oxide, Photolysis, Solar Flux Density, Solar Protons, Incident Radiation, Ozonosphere, Solar Terrestrial Interactions, Spacelab Payloads, Stratosphere
Scientific paper
As a possible experimental payload on board SPACELAB, the measurement of the solar photon flux in the wavelength range of from 160 to 220 nm is proposed. Emphasis is placed on the role of this flux rate in the formation of ozone in the stratosphere. It is noted that the concentration of stratospheric ozone is controlled by a complex chemical which can be influenced by human activity. The monitoring of ammonia photolysis combined with nitric oxide detection is suggested as an accurate means of determining photon flux at about 200 nm. It is also pointed out that previous determinations of the photon flux do not agree and hence there is a need to use SPACELAB for this purpose.
Hubrich C.
Stuhl F.
No associations
LandOfFree
Determination of the solar photon flux in the range of from 160 to 220 NM using the photolysis of ammonia combined with nitric oxide detection does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Determination of the solar photon flux in the range of from 160 to 220 NM using the photolysis of ammonia combined with nitric oxide detection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of the solar photon flux in the range of from 160 to 220 NM using the photolysis of ammonia combined with nitric oxide detection will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-946335