The History of Sounding Rockets and Their Contribution to ... - ESA
The History of Sounding Rockets and Their Contribution to ... - ESA
The History of Sounding Rockets and Their Contribution to ... - ESA
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- a further experiment (RN 104) by Dr. Atzei <strong>of</strong> the IAP team was fl own by <strong>ESA</strong> in Oc<strong>to</strong>ber 1967. It<br />
measured the vertical distribution <strong>of</strong> pressure, temperature <strong>and</strong> density at altitudes between 20 <strong>and</strong><br />
90 km. Pressure was measured at the surface <strong>of</strong> the rocket <strong>and</strong> at the stagnation point using a<br />
gauge<br />
- the IAP team also performed studies <strong>of</strong> meteoric aerosols above 80 km altitude.<br />
B. <strong>The</strong> experiment by the CEN Saclay group, led by Pr<strong>of</strong>. J. Labeyrie, had the objective <strong>of</strong> performing<br />
X-ray spectroscopy from space. For this task, the group used proportional counters with an au<strong>to</strong>-coincidence<br />
facility <strong>to</strong> eliminate particular radiation.<br />
<strong>The</strong> group also performed other sounding-rocket experiments such as:<br />
- spectrometry <strong>of</strong> gamma-rays in space, for which scintillation spectrographs were used: a pho<strong>to</strong>multiplier<br />
collected gamma-ray scintillations from sodium-iodide (NaI) crystals <strong>and</strong> from a plastic<br />
scintillation counter<br />
- measurement <strong>of</strong> the intensity <strong>of</strong> solar X-ray spectra during a solar-fl are event: for this, a proportional<br />
counter was used, which provided 100 channels for amplitude analysis.<br />
C. <strong>The</strong> experiment by a team from Toulouse University, led by Pr<strong>of</strong>. F. Cambou, had the objective <strong>of</strong> performing<br />
spectroscopy <strong>of</strong> auroral pro<strong>to</strong>ns <strong>and</strong> determining their contribution <strong>to</strong> auroral phenomena. <strong>The</strong><br />
pro<strong>to</strong>ns’ energy distribution throughout the rocket trajec<strong>to</strong>ry was measured using solid lithium detec<strong>to</strong>rs,<br />
as was magnetic defl ection.<br />
A further experiment conducted by the University group involved measuring the intensity <strong>of</strong> the 3914 A<br />
nitrogen line <strong>and</strong> the hydrogen line in an aurora with the help <strong>of</strong> two pho<strong>to</strong>multipliers <strong>and</strong> fi lters centred<br />
on these two lines.<br />
D. An experiment by a research team from the Cosmic Physics Labora<strong>to</strong>ry at Meudon, led by Pr<strong>of</strong>. J.E.<br />
Blamont, <strong>to</strong>ok measurements <strong>of</strong> local temperatures in the upper atmosphere by observing vibration <strong>and</strong><br />
rotational spectra <strong>of</strong> aluminium oxide, ejected by an explosion <strong>of</strong> TNT carried by a rocket.<br />
Franco - American Cooperation<br />
Rocket type Altitude Range/year Research centre/objectives<br />
2 Aerobee 150 280 km Wallops Isl<strong>and</strong> / Oct. 1963 CNET, Ionosphere irregularities via parallel<br />
VLF fi eld strength <strong>and</strong> local<br />
2 Aerobee 150 280 km Wallops Isl<strong>and</strong> / Sept. 1965 Electron density measurements<br />
2 Dragon 400 km Hammaguir, CNES & Goddard Space Flight Center,<br />
2 Centaure 190 km Algeria / 4 in April 1964 Charged particles & neutral gas temp.<br />
1 Aerobee 150 280 km White S<strong>and</strong>s / Nov. 1964 CNRS: One <strong>of</strong> several experiments providing<br />
1 Aerobee 150 280 km White S<strong>and</strong>s / Nov. 1965 special sample surfaces <strong>to</strong> collect <strong>and</strong> analyse<br />
1 Aerobee 150 280 km White S<strong>and</strong>s / June 1967 extraterrestrial dust particles as part <strong>of</strong> the<br />
Luster project