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  • 1
    In: INTERNATIONAL JOURNAL OF EXPERIMENTAL RESEARCH AND REVIEW, International Journal of Experimental Research and Review, Vol. 18 ( 2019-4-30), p. 6-14
    Abstract: Many important varieties of field, horticultural and forestry species are conserved as Field Gene Banks (FGB). FGBs provide easy and ready access to conserved material for research as well as for use. Plant breeders are in need of a continuous supply of diverse and novel genetic diversity to produce new crop varieties able to cope with the impacts of changing cultivation conditions and climate change. FGB is one of the options of a complementary strategy for the conservation of germplasm of many plant species. Murshidabad and Malda, the once famous districts for Mango (Mangifera indica L.) diversity, districts of West Bengal are now facing tremendous genetic erosion of the mango germplasm. The Field gene bank will be an ex situ conservation approach. 25 (Twenty five) mango varieties were collected from Malda and Murshidabad districts and cuttings transferred to Gurudas College, Kolkata 700054 for conservation as Field Gene Bank. The mango germplasm accessions were collected with the assistance of the West Bengal Biodiversity Board (WBBB). Some of the valuable mango varieties viz. Bimli, Churmur, Dobani, Do Phala, Golap Bhog, Golap Khash, Molam Jam, collected from orchards of Malda and Murshidabad districts. As a field Gene Bank these varieties are readily accessible and useable for characterization and evaluation. These field gene banks will aid in documentation of the rich mango legacy of West Bengal and help in mango crop improvement.
    Type of Medium: Online Resource
    ISSN: 2455-4855
    Language: Unknown
    Publisher: International Journal of Experimental Research and Review
    Publication Date: 2019
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  • 2
    Online Resource
    Online Resource
    American Physical Society (APS) ; 1998
    In:  Physical Review Letters Vol. 80, No. 4 ( 1998-1-26), p. 728-731
    In: Physical Review Letters, American Physical Society (APS), Vol. 80, No. 4 ( 1998-1-26), p. 728-731
    Type of Medium: Online Resource
    ISSN: 0031-9007 , 1079-7114
    RVK:
    RVK:
    Language: English
    Publisher: American Physical Society (APS)
    Publication Date: 1998
    detail.hit.zdb_id: 1472655-5
    detail.hit.zdb_id: 208853-8
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1999
    In:  Journal of Geophysical Research: Space Physics Vol. 104, No. A6 ( 1999-06), p. 12683-12693
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 104, No. A6 ( 1999-06), p. 12683-12693
    Abstract: Recent space missions such as FAST and Freja report highly structured plasma flows along the magnetic field. Electrostatic fluctuations that can be supported by such inhomogeneous parallel flows are investigated. It is found that even a small transverse gradient in parallel flow can significantly reduce the critical value of the relative ion‐electron field‐aligned drift for the current‐driven electrostatic ion acoustic modes. It is also shown that the shear‐modified ion acoustic mode can be excited without any relative field‐aligned drift provided that the flow gradient is sufficiently strong. The instability mechanism can be described in a local limit. The new shear‐modified ion‐acoustic modes considered in this paper are shown to be different from both the nonresonant mode due to a velocity shear in the parallel flow [ D'Angelo , 1965] and the resonant classical current‐driven ion‐acoustic mode [ Fried and Gould , 1961]. The new modes discussed in this paper can be excited for typical ionospheric conditions and a wide range of ion‐electron temperature ratios. The reported results may explain ionospheric observations of low‐frequency ion‐acoustic‐like waves, especially for ion‐electron temperature ratios of the order of unity and larger when the critical current for the homogeneous current‐driven ion acoustic mode is significantly above the observed values. Other possible applications of our results to space plasmas are also discussed.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1999
    detail.hit.zdb_id: 161666-3
    SSG: 16,13
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  • 4
    Online Resource
    Online Resource
    American Physical Society (APS) ; 2013
    In:  Physical Review Letters Vol. 111, No. 14 ( 2013-10-2)
    In: Physical Review Letters, American Physical Society (APS), Vol. 111, No. 14 ( 2013-10-2)
    Type of Medium: Online Resource
    ISSN: 0031-9007 , 1079-7114
    RVK:
    RVK:
    Language: English
    Publisher: American Physical Society (APS)
    Publication Date: 2013
    detail.hit.zdb_id: 1472655-5
    detail.hit.zdb_id: 208853-8
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  • 5
    Online Resource
    Online Resource
    Japan Society for Aeronautical and Space Sciences ; 2012
    In:  TRANSACTIONS OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, AEROSPACE TECHNOLOGY JAPAN Vol. 10, No. ists28 ( 2012), p. Pr_23-Pr_27
    In: TRANSACTIONS OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, AEROSPACE TECHNOLOGY JAPAN, Japan Society for Aeronautical and Space Sciences, Vol. 10, No. ists28 ( 2012), p. Pr_23-Pr_27
    Type of Medium: Online Resource
    ISSN: 1884-0485
    Language: English
    Publisher: Japan Society for Aeronautical and Space Sciences
    Publication Date: 2012
    detail.hit.zdb_id: 2953256-5
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  • 6
    Online Resource
    Online Resource
    Springer Science and Business Media LLC ; 2018
    In:  Scientific Reports Vol. 8, No. 1 ( 2018-11-21)
    In: Scientific Reports, Springer Science and Business Media LLC, Vol. 8, No. 1 ( 2018-11-21)
    Abstract: The unprecedented high-resolution data from the Magnetospheric Multi-Scale (MMS) satellites is revealing the physics of dipolarization fronts created in the aftermath of magnetic reconnection in extraordinary detail. The data shows that the fronts contain structures on small spatial scales beyond the scope of fluid framework. A new kinetic analysis, applied to MMS data here, predicts that global plasma compression produces a unique particle distribution in a narrow boundary layer with separation of electron and ion scale physics. Layer widths on the order of an ion gyro-diameter lead to an ambipolar potential across the magnetic field resulting in strongly sheared flows. Gradients along the magnetic field lines create a potential difference, which can accelerate ions and electrons into beams. These small-scale kinetic effects determine the plasma dynamics in dipolarization fronts, including the origin of the distinctive broadband emissions.
    Type of Medium: Online Resource
    ISSN: 2045-2322
    Language: English
    Publisher: Springer Science and Business Media LLC
    Publication Date: 2018
    detail.hit.zdb_id: 2615211-3
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2012
    In:  Geophysical Research Letters Vol. 39, No. 16 ( 2012-08-28)
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 39, No. 16 ( 2012-08-28)
    Abstract: Nonlinear scattering generates a long‐lasting wave cavity in radiation belts Smaller obliqueness of waves can be maintained by induced nonlinear scattering Multi‐pass whistler gain leads to rapid electron precipitation
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2012
    detail.hit.zdb_id: 2021599-X
    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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  • 8
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2007
    In:  Journal of Geophysical Research: Space Physics Vol. 112, No. A6 ( 2007-06)
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 112, No. A6 ( 2007-06)
    Abstract: It is shown that intense ion cyclotron turbulence can be induced in the near‐Earth space by shaped release of neutral gas of materials such as lithium, cesium, etc. Release of 1 ton of neutral lithium gas in the Earth's equatorial plane at L = 2 can introduce about 30 GJ of energy which can be used to excite waves around the lithium ion cyclotron harmonics that readily evolves into the turbulent state. The energy is obtained by converting the orbital kinetic energy of the neutral lithium atoms into free energy for the electromagnetic waves through photoionization and creation of a ring distribution in the lithium ion velocity perpendicular to the ambient magnetic field. This distribution function is highly unstable and can spontaneously trigger large amplitude shear Alfven waves near lithium cyclotron harmonics with unique nonlinear properties. These waves lead to pitch angle scattering of the trapped electrons in a broad energy band.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2007
    detail.hit.zdb_id: 161666-3
    SSG: 16,13
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  • 9
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2001
    In:  Journal of Geophysical Research: Space Physics Vol. 106, No. A2 ( 2001-02), p. 1807-1815
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 106, No. A2 ( 2001-02), p. 1807-1815
    Abstract: We have recently performed a detailed characterization of ion Joule heating perpendicular to an axial magnetic field in the laboratory in a simulated ionospheric plasma environment which contains localized electric field structuring. Since Joule heating is often regarded as an important mechanism contributing to energization of outflowing heavy ions observed by higher‐altitude auroral satellites, this work has particular relevance to space physics issues, and, to our knowledge, has not been investigated systematically in a controlled environment. Since transverse (to B ) ionospheric electric fields are often spatially and temporally structured, with scale lengths often as small as an ion gyroradius, the ability to systematically vary the spatial extent and magnitude of an electric field region and to observe the effect on ion energy is important. The experiment makes use of a concentric set of separately biasable ring anodes which generate a radial electric field with controllable scale length perpendicular to an ambient axial magnetic field. Joule heating results from ion‐neutral collisions occurring within this transverse, dc electric field. Until there is sufficient neutral pressure to raise the ion‐neutral collision frequency ( v in ) to an observable Joule heating threshold, ion cyclotron wave heating, which is induced by shear in E × B rotation, can be the primary channel for ion energization. We have discussed in earlier papers the conditions under which this occurs, and we have treated the transition between the two forms of ion heating. We concentrate primarily in this work on constructing the fields themselves and on the relationship between the subsequent collisional heating and the Pedersen conductivity as an initial indication of the validity of the measurement results. We are able to demonstrate that measurable heating is produced by even relatively small scale structures of the order of the ion gyroradius. In addition, we show that measured heating is consistent with predictions of Joule heating as a function of ion‐neutral collisions. Finally, this work can have major implications for ionospheric studies where large‐scale electric fields are often assumed in the calculation of Joule heating.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2001
    detail.hit.zdb_id: 161666-3
    SSG: 16,13
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  • 10
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2002
    In:  Journal of Geophysical Research: Space Physics Vol. 107, No. A8 ( 2002-08)
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 107, No. A8 ( 2002-08)
    Abstract: In an earlier work we described a laboratory‐based experimental series that demonstrated the transition from velocity‐shear‐driven ion cyclotron wave heating to ion Joule heating as a function of ion‐neutral collision frequency. As part of this effort, we demonstrated the ability to control the magnitude and direction of the electric field (or the sign of potential change) in space in a simulated ionospheric environment. In the results presented here we have calculated the electric field by differentiation of a fit to the potential profile and have used the full width at half maximum of this field as a marker for the size of the region. In the case of the ion temperature measurements, which are derived from energy analyzer data by conventional techniques, we demonstrate increased ion temperature consistent with increasing electric field region length. We also have been able to demonstrate a peak in the ion temperature as a function of collision frequency and the Joule heating rate. The data suggest that for approximately constant pressure and electric field strength, the normalized ion temperature increase will be limited for a given scale size. Finally, we argue that these observations are consistent with the notion of a limit to ion heating based on a comparison of the scale length of the region to the mean free path for ion‐neutral collisions.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2002
    detail.hit.zdb_id: 161666-3
    SSG: 16,13
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