Search Publications

Redistribution of lunar polar water to mid-latitudes and its role in forming an OH veneer
DOI: 10.1016/j.pss.2013.05.009 Bibcode: 2013P&SS...89...15F

Delory, G. T.; Halekas, J. S.; Farrell, W. M. +4 more

We suggest that energization processes like ion sputtering and impact vaporization can eject/release polar water molecules residing within cold trapped regions with sufficient velocity to allow their redistribution to mid-latitudes. We consider the possibility that these polar-ejected molecules can contribution to the water/OH veneer observed as a…

2013 Planetary and Space Science
Chandrayaan-1 19
Young viscous flows in the Lowell crater of Orientale basin, Moon: Impact melts or volcanic eruptions?
DOI: 10.1016/j.pss.2013.09.001 Bibcode: 2013P&SS...87...37S

Srivastava, N.; Kumar, D.; Gupta, R. P.

Topographical, morphological and spectral reflectance studies have been carried out for a distinct resurface event inside Copernican aged Lowell crater (13.00°S 103.40°W), Orientale basin, using high resolution TC, MI-VIS, LROC-NAC, and M3 data from Kaguya, Lunar Reconnaissance Orbiter (LRO) and Chandrayaan-1 missions. The resurfacing i…

2013 Planetary and Space Science
Chandrayaan-1 17
Solar wind reflection from the lunar surface: The view from far and near
DOI: 10.1016/j.pss.2013.02.004 Bibcode: 2013P&SS...84....1S

Barabash, S.; Wurz, P.; McComas, D. J. +7 more

The Moon appears bright in the sky as a source of energetic neutral atoms (ENAs). These ENAs have recently been imaged over a broad energy range both from near the lunar surface, by India's Chandrayaan-1 mission (CH-1), and from a much more distant Earth orbit by NASA's Interstellar Boundary Explorer (IBEX) satellite. Both sets of observations hav…

2013 Planetary and Space Science
Chandrayaan-1 16
Validation of methodology to derive elemental abundances from X-ray observations on Chandrayaan-1
DOI: 10.1016/j.pss.2012.10.003 Bibcode: 2013P&SS...75..188A

Babu, B. R. S.; Narendranath, S.; Sreekumar, P. +2 more

The Chandrayaan-1 X-ray Spectrometer (C1XS) observed characteristic X-ray fluorescence (XRF) lines of major rock forming elements from the lunar surface during different solar flare conditions. As the Sun was undergoing an unusually low activity cycle during the observing period of C1XS (28th Nov. 2008-29th Aug. 2009), most observations were made …

2013 Planetary and Space Science
Chandrayaan-1 11
Experimental validation of XRF inversion code for Chandrayaan-1
DOI: 10.1016/j.pss.2013.08.022 Bibcode: 2013P&SS...89..183A

Narendranath, S.; Sreekumar, P.; Sudhakar, M. +5 more

We have developed an algorithm (x2abundance) to derive the lunar surface chemistry from X-ray fluorescence (XRF) data for the Chandrayaan-1 X-ray Spectrometer (C1XS) experiment. The algorithm converts the observed XRF line fluxes to elemental abundances with uncertainties. We validated the algorithm in the laboratory using high Z elements (20<Z…

2013 Planetary and Space Science
Chandrayaan-1 10
An algorithm for geometric correction of full pass TMC imagery of Chandrayaan-1
DOI: 10.1016/j.pss.2013.01.012 Bibcode: 2013P&SS...79...45R

Radhadevi, P. V.; Solanki, S. S.; Nagasubramanian, V. +4 more

This paper describes the development of an algorithm for geometric correction of Terrain Mapping Camera (TMC) imagery of Chandrayaan-1 (CH-1). The correction is based on a rigorous sensor model. The algorithm incorporates the camera geometry model, satellite data and lunar control points in a rigorous bundle adjustment updating the satellite model…

2013 Planetary and Space Science
Chandrayaan-1 4