The SARA instrument (Sub-keV Atom Reflecting Analyser) comprises a low energy neutral atom (LENA) sensor for the energy range 10 eV-3.3 keV and an ion mass spectrometer (10 eV-15 keV). It is the first ever experiment to study the solar wind-planetary surface interaction via measurements of the sputtered atoms and neutralized back-scattered solar wind hydrogen. The neutral atom sensor uses conversion of the incoming neutrals to positive ions, which are then analysed via surface interaction technique. The ion mass spectrometer is based on the same principle. SARA performs LENA imaging of the Moon's elemental surface composition including that of permanently shadowed areas, and imaging of the lunar surface magnetic anomalies. It will also inve...
We present the first direct measurement of neutral oxygen in the lunar exosphere, detected by the Ch...
The Sub-keV atom reflecting analyzer instrument on board the lunar orbiter Chandrayaan-1 provided a ...
The Moon has neither a strong magnetic field nor a dense atmosphere to stand-off the solar wind. How...
This paper reports on the Sub-keV Atom Reflecting Analyzer (SARA) experiment that will be flown on t...
SARA experiment aboard the first Indian lunar mission Chandrayaan-1 had the objective to explore the...
The first Indian lunar mission Chandrayaan-1 was launched on 22 October 2008. The Sub-keV Atom Refle...
The results from the Sub-keV Atom Reflecting Analyzer (SARA) experiment onboard Chandrayaan-1 have r...
The results from the Sub-keV Atom Reflecting Analyzer (SARA) experiment onboard Chandrayaan-1 have r...
SARA experiment aboard the first Indian lunar mission Chandrayaan-1 had the objective to explore the...
The Sub-keV Atom Reflecting Analyzer (SARA) instrument on board Chandrayaan-1 was exceptionally succ...
[1] Since the Moon is not shielded by a global magnetic field or by an atmosphere, solar wind plasma...
Low-energy neutral atom (LENA) imaging is an important technique for doing planetary sciences at mag...
The Sub-keV Atom Reflecting Analyzer (SARA) instrument on the Indian Chandrayaan-1 spacecraft has pr...
Imaging of low-energy neutral atoms (LENAs) in the vicinity of the Moon can provide wide knowledge o...
Characterised by a surface bound exosphere and localised crustal magnetic fields, the Moon was consi...
We present the first direct measurement of neutral oxygen in the lunar exosphere, detected by the Ch...
The Sub-keV atom reflecting analyzer instrument on board the lunar orbiter Chandrayaan-1 provided a ...
The Moon has neither a strong magnetic field nor a dense atmosphere to stand-off the solar wind. How...
This paper reports on the Sub-keV Atom Reflecting Analyzer (SARA) experiment that will be flown on t...
SARA experiment aboard the first Indian lunar mission Chandrayaan-1 had the objective to explore the...
The first Indian lunar mission Chandrayaan-1 was launched on 22 October 2008. The Sub-keV Atom Refle...
The results from the Sub-keV Atom Reflecting Analyzer (SARA) experiment onboard Chandrayaan-1 have r...
The results from the Sub-keV Atom Reflecting Analyzer (SARA) experiment onboard Chandrayaan-1 have r...
SARA experiment aboard the first Indian lunar mission Chandrayaan-1 had the objective to explore the...
The Sub-keV Atom Reflecting Analyzer (SARA) instrument on board Chandrayaan-1 was exceptionally succ...
[1] Since the Moon is not shielded by a global magnetic field or by an atmosphere, solar wind plasma...
Low-energy neutral atom (LENA) imaging is an important technique for doing planetary sciences at mag...
The Sub-keV Atom Reflecting Analyzer (SARA) instrument on the Indian Chandrayaan-1 spacecraft has pr...
Imaging of low-energy neutral atoms (LENAs) in the vicinity of the Moon can provide wide knowledge o...
Characterised by a surface bound exosphere and localised crustal magnetic fields, the Moon was consi...
We present the first direct measurement of neutral oxygen in the lunar exosphere, detected by the Ch...
The Sub-keV atom reflecting analyzer instrument on board the lunar orbiter Chandrayaan-1 provided a ...
The Moon has neither a strong magnetic field nor a dense atmosphere to stand-off the solar wind. How...