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| 1 | 1984MNRAS.209..719C |
| 1.000 | 08/1984 | F G C O U |
| Cowsik, R.; Sarkar, S. |
| Erratum - the Evolution of Supernova Remnants as Radio Sources |
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| 2 | 1984MNRAS.207..745C |
| 1.000 | 04/1984 | A F G R C O U |
| Cowsik, R.; Sarkar, S. |
| The evolution of supernova remnants as radio sources |
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| 3 | 1983ICRC....2..306C |
| 1.000 | 08/1983 | |
| Cowsik, R.; Sarkar, S. |
| Acceleration of Electrons in Supernova Remnants |
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| 4 | 1983IAUS..101..187C |
| 1.000 | 00/1983 | F G T R C |
| Cowsik, R.; Sarkar, S. |
| The Evolution of Supernova Remnants as Radio Sources |
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| 5 | 1982MNRAS.199...97S |
| 1.000 | 04/1982 | A F G R C |
| Sarkar, S. |
| Does the galactic synchrotron radio background originate in old supernova remnants |
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| 6 | 1982BASI...10...49C |
| 1.000 | 03/1982 | |
| Cowsik, R.; Sarkar, S. |
| The evolution of the radio spectra of supernova remnants. |
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| 7 | 1980BASI....8..159S |
| 1.000 | 12/1980 | F G |
| Sarkar, S. |
| Report on the I.A.U. Symp. on the Origin of Cosmic Rays |
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| 8 | 1980ICRC....1..277B |
| 1.000 | 10/1980 | A |
| Biawas, S.; Durgaprasad, N.; Sarkar, S.; Venkatavaradan, V. S. |
| Abundances of the anomalous component of nitrogen to argon ions in low energy /8-50 MeV/amu/ cosmic rays in the SKYLAB experiment |
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| 9 | 1980MNRAS.191..855C |
| 1.000 | 06/1980 | A F G R C U |
| Cowsik, R.; Sarkar, S. |
| A lower limit to the magnetic field in Cassiopeia-A |
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| 10 | 1980spre.conf..259D |
| 1.000 | 00/1980 | A |
| Durgaprasad, N.; Venkatavaradan, V. S.; Sarkar, S.; Biswas, S. |
| Energy spectra and charge states of low energy cosmic rays in the SKYLAB experiment |
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| 11 | 1980nsgr.symp...57C |
| 1.000 | 00/1980 | A T C |
| Cowsik, R.; Sarkar, S. |
| Gamma ray emission from supernova remnants |
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| 12 | 1979IJRSP...8..226B |
| 1.000 | 12/1979 | A |
| Biswas, S.; Durgaprasad, N.; Kajarekar, P. J.; Sarkar, S.; Venkatavaradan, V. S. |
| Detection of relativistic iron nuclei in the plastic track detector CR-39 |
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| 13 | 1979IJRSP...8..222D |
| 1.000 | 12/1979 | A |
| Durgaprasad, N.; Venkatavaradan, V. S.; Sarkar, S.; Biswas, S. |
| Charge states of low energy cosmic rays in the SKYLAB experiment |
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| 14 | 1979ICRC...12..341S |
| 1.000 | 00/1979 | |
| Sarkar, S.; Durgaprasad, N.; Biswas, S.; Venkatavaradan, V. S. |
| Obsevations of Relativistic Cosmic Ray Iron Groupe Nuclei in the Track Detector Allyl Diglycol Carbonate |
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| 15 | 1979ICRC...11...95B |
| 1.000 | 00/1979 | |
| Biswas, S.; Durgaprasad, N.; Sarkar, S.; Venkatavaradan, V. S. |
| Observations of Relativistic Iron Group Nuclei of Cosmic Rays in CR-39 Track Detection |
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| 16 | 1979ICRC....1..296D |
| 1.000 | 00/1979 | |
| Durgaprasad, N.; Venkatavaradan, V. S.; Sarkar, S.; Biswas, S. |
| Energy Dependence of the Ratio of Calcium Group to Iron Group Nuclei in Low Energy (50 - 150 Mev/amu) Cosmic Rays |
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| 17 | 1979ICRC....1..282B |
| 1.000 | 00/1979 | U |
| Biswas, S.; Durgaprasad, N.; Sarkar, S. |
| On the Origin of the Anomalous Component in the Low Energy Cosmic Rays |
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| 18 | 1979ICRC....1..277B |
| 1.000 | 00/1979 | |
| Biswas, S.; Durgaprasad, N.; Sarkar, S.; Venkatavaradan, V. S. |
| Abundances of the Anomalous Component of Nitrogen to Argon Ions in Low Energy (8-50 Mev/amu) Cosmic Rays in the SKYLAB Experiment |
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| 19 | 1979ICRC....1..202C |
| 1.000 | 00/1979 | U |
| Cowsik, R.; Sarkar, S.; Cassé, M. |
| Are Gamma Ray Sources also Cosmic Ray Sources? |
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| 20 | 1978ICRC....2..327B |
| 1.000 | 00/1978 | |
| Biswas, S.; Durgaprasad, N.; Nevatia, J.; Sarkar, S.; Venkatavaradan, V. S. |
| Energy spectra and abundances of carbon to nickel ions in the low energy 8-100 MeV/amu cosmic rays observed in the SKYLAB experiment |
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| 21 | 1977IJRSP...6..209B |
| 1.000 | 09/1977 | A |
| Biswas, S.; Durgaprasad, N.; Sarkar, S.; Venkatavaradan, V. S. |
| Properties of low energy ions observed in the SKYLAB cosmic ray experiment |
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| 22 | 1977ICRC....2..327B |
| 1.000 | 00/1977 | |
| Biswas, S.; Durgaprasad, N.; Vatia, J. Ne; Sarkar, S.; Venkatavaradan, V. S. |
| Energy Spectra and Abundances of Carbon to Nickel Ions in the Low Energy (8-100 MeV/amu) Cosmic Rays Observed in the Skylab Experiment |
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