WorldCat Identities

Badhwar, G. D.

Overview
Works: 13 works in 15 publications in 1 language and 126 library holdings
Genres: Conference proceedings 
Roles: Editor
Classifications: QC801,
Publication Timeline
Key
Publications about  G. D Badhwar Publications about G. D Badhwar
Publications by  G. D Badhwar Publications by G. D Badhwar
Most widely held works about G. D Badhwar
 
Most widely held works by G. D Badhwar
Radiological assessment for Space Station Freedom ( Book )
1 edition published in 1993 in English and held by 78 WorldCat member libraries worldwide
A semi-automatic technique for multitemporal classification of a given crop by G. D Badhwar ( Book )
2 editions published between 1979 and 1980 in English and held by 2 WorldCat member libraries worldwide
The energy dependence of the abundance of lithium, beryllium, and boron in the primary cosmic radiation: Observations at Ft. Churchill by G. D Badhwar ( Book )
1 edition published in 1964 in English and held by 1 WorldCat member library worldwide
The relative abundance of Lithium, Beryllium, Boron, and the S-group nuclei has been determined at two different energies with the help of a pure nuclear emulsion stack flown from Fort Churchill, Canada (lambda = 70.5) on 4 August, 1962 under a total of 4.7 g/sq. cm of residual atmosphere. The ratio of the L to S nuclei, LS, at the top of the atmosphere between 200-700 Mev/n and> 700 Mev/n was determined as 0.41 = 0.08 and 0.19 = 0.03 respectively. The results of both the absolute flux values of L and S-group nuclei as well as their ratios are in accord with other investigations. Combined with the evidence from the measurements of He3He in the same stack, our results indicate that low energy cosmic ray nuclei have traversed about twice as much hydrogen as high energy particles. The results rule out an accelerating mechanism of the Fermi type but may be explained by a source-trapping mechanism. (Author)
The energy dependence of the abundance of lithium, beryllium, and boron in the primary cosmic radiation: observations at fort churchill ( Book )
1 edition published in 1964 in English and held by 1 WorldCat member library worldwide
The relative abundance of Lithium, Beryllium, Boron, and the S-group nuclei has been determined at two different energies with the help of a pure nuclear emulsion stack flown from Fort Churchill, Canada (lambda = 70.5) on 4 August, 1962 under a total of 4.7 g/sq. cm of residual atmosphere. The ratio of the L to S nuclei, LS, at the top of the atmosphere between 200-700 Mev/n and> 700 Mev/n was determined as 0.41 = 0.08 and 0.19 = 0.03 respectively. The results of both the absolute flux values of L and S-group nuclei as well as their ratios are in accord with other investigations. Combined with the evidence from the measurements of He3He in the same stack, our results indicate that low energy cosmic ray nuclei have traversed about twice as much hydrogen as high energy particles. The results rule out an accelerating mechanism of the Fermi type but may be explained by a source-trapping mechanism. (Author)
Crop emergence date determination from spectral data by G. D Badhwar ( )
1 edition published in 1980 in English and held by 1 WorldCat member library worldwide
Argentina spectral-agronomic multitemporal data set ( Book )
1 edition published in 1983 in English and held by 1 WorldCat member library worldwide
Development stage estimation of corn from spectral data : an initial model by G. D Badhwar ( Book )
1 edition published in 1980 in English and held by 1 WorldCat member library worldwide
Isotopic composition of low energy hydrogen nuclei in the primary cosmic radiation by G. D Badhwar ( Book )
1 edition published in 1964 in English and held by 1 WorldCat member library worldwide
The abundance of low energy deuterons and tritons was determined in a nuclear emulsion stack exposed at Fort Churchill, Manitoba, Canada on August 4, 1962 under 4.2 g/sq cm of residual atmosphere. Using the grain density vs. residual range method for the identification of tracks produced by particles, the differential flux of deuterons and tritons was determined. The results appear to be consistent with the absence of deuterons and tritons in the primary cosmic radiation. An upper limit on the amount of hydrogen traversed by low energy cosmic ray particles has been placed. (Author)
Isotopic composition of low energy hydrogen nuclei in the primary cosmic radiation ( Book )
1 edition published in 1964 in English and held by 1 WorldCat member library worldwide
The abundance of low energy deuterons and tritons was determined in a nuclear emulsion stack exposed at Fort Churchill, Manitoba, Canada on August 4, 1962 under 4.2 g/sq cm of residual atmosphere. Using the grain density vs. residual range method for the identification of tracks produced by particles, the differential flux of deuterons and tritons was determined. The results appear to be consistent with the absence of deuterons and tritons in the primary cosmic radiation. An upper limit on the amount of hydrogen traversed by low energy cosmic ray particles has been placed. (Author)
 
moreShow More Titles
fewerShow Fewer Titles
Audience Level
0
Audience Level
1
  Kids General Special  
Audience level: 0.85 (from 0.00 for Crop emerg ... to 1.00 for A semi-aut ...)
Languages
English (15)
Covers