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This presentation deals with how one can grow green fodder in small piece of land which can provide green fodder to cattle throughout the year .
Green fodder production around the year
Green fodder production around the year
Dr Ajay Kumar Singh
-
Makhana_Report.pdf
Makhana_Report.pdf
ssuserf288df
Presented at the Pulses for Sustainable Agriculture and Human Health” on 31 May-1 June 2016 at NASC, New Delhi, India. The conference was jointly organised by the International Food Policy Research Institute (IFPRI), National Academy of Agricultural Sciences (NAAS), TCi of Cornell University (TCi-CU) and Agriculture Today.
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Non leguminous fodder- 1) Maize (Zea mays): Maize forage is more nutritious at milk stage. It is non leguminous kharif crop . it is a maintenance type fodder having 8-10% protein. 2) Jowar/sorghum (Sorghum Vulgare): Green jower contain 0.5% DCP,16% TDN, 0.13% Ca and 0.03% Phosphorus. For feeding of livestock it should be harvested at 50% flowering stage. 3) Bajra or Pearl Millet (Pennesetum typhoids) : It is harvested before flowering stage for feeding the animals. It contain 13% TDN and 0.9% DCP. 4) Oats (Avena sativa) : This is the non leguminous crop of the rabi season .It is the best crop for hay making. It is a maintenance type fodder having 7-9 % CP and 55 % TDN. Leguminous fodder : 1) Berseem (Trifolium alexandrium): Berseem is one of the most important cultivated crop of India. Kashni is the weed crop grown along with berseem. It is grown in rabi season. It contain 15% CP and 60 % TDN. But excessive intake of berseem may lead to bloat condition. 2) Lucerne (Medicago sativa) : this is the productive type fodder it contain 12-15% CP and 55- 60 % TDN 3) Lobia or Cow pea (Vigna sinensis ): It contains on an average 15% CP and 30 % crude fiber on dry matter basis. Concentrate: 1) Cereal grains- The cereal grains are high in starch and low in fibre. The DCP range between 7-10 % and TDN from 70-80%. The cereals are all deficient in Ca containing less than 1g/kg DM. the Phosphorus content is higher being 3-5g/kg . the cereal grains are deficient in Vitamin D. 2) Barley (Hordeum sativum): Barley being the second main rabi crop of India. It contains 7-8 percent DCP and 75-80 percent TDN, 0.07 percent Ca and 0.28 percent P. Barley is deficient in vitamin A, D and riboflavin but rich in niacin content. 3) Maize (Zea mays): Maize contains 7 percent DCP and 80 percent TDN. The yellow maize contains enough amount of carotene, hence good for feeding of livestock and poultry birds. It is deficient in lysine and methionine. Maize contains about 730 gm starch/ Kg DM, is very low in fibre and has a high metabolised energy value. 4) Gram: Gram contains 12 to 16 percent DCP and 78 percent TDN. Animals have great liking for this grain and so, used for preparing the concentrate mixture for feeding the livestock. 5) Jowar: Whole grains are usually fed to chickens. It contains 7 percent DCP and 74 percent TDN and high percentage of leucine.
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This presentation deals with how one can grow green fodder in small piece of land which can provide green fodder to cattle throughout the year .
Green fodder production around the year
Green fodder production around the year
Dr Ajay Kumar Singh
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Makhana_Report.pdf
Makhana_Report.pdf
ssuserf288df
Presented at the Pulses for Sustainable Agriculture and Human Health” on 31 May-1 June 2016 at NASC, New Delhi, India. The conference was jointly organised by the International Food Policy Research Institute (IFPRI), National Academy of Agricultural Sciences (NAAS), TCi of Cornell University (TCi-CU) and Agriculture Today.
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Non leguminous fodder- 1) Maize (Zea mays): Maize forage is more nutritious at milk stage. It is non leguminous kharif crop . it is a maintenance type fodder having 8-10% protein. 2) Jowar/sorghum (Sorghum Vulgare): Green jower contain 0.5% DCP,16% TDN, 0.13% Ca and 0.03% Phosphorus. For feeding of livestock it should be harvested at 50% flowering stage. 3) Bajra or Pearl Millet (Pennesetum typhoids) : It is harvested before flowering stage for feeding the animals. It contain 13% TDN and 0.9% DCP. 4) Oats (Avena sativa) : This is the non leguminous crop of the rabi season .It is the best crop for hay making. It is a maintenance type fodder having 7-9 % CP and 55 % TDN. Leguminous fodder : 1) Berseem (Trifolium alexandrium): Berseem is one of the most important cultivated crop of India. Kashni is the weed crop grown along with berseem. It is grown in rabi season. It contain 15% CP and 60 % TDN. But excessive intake of berseem may lead to bloat condition. 2) Lucerne (Medicago sativa) : this is the productive type fodder it contain 12-15% CP and 55- 60 % TDN 3) Lobia or Cow pea (Vigna sinensis ): It contains on an average 15% CP and 30 % crude fiber on dry matter basis. Concentrate: 1) Cereal grains- The cereal grains are high in starch and low in fibre. The DCP range between 7-10 % and TDN from 70-80%. The cereals are all deficient in Ca containing less than 1g/kg DM. the Phosphorus content is higher being 3-5g/kg . the cereal grains are deficient in Vitamin D. 2) Barley (Hordeum sativum): Barley being the second main rabi crop of India. It contains 7-8 percent DCP and 75-80 percent TDN, 0.07 percent Ca and 0.28 percent P. Barley is deficient in vitamin A, D and riboflavin but rich in niacin content. 3) Maize (Zea mays): Maize contains 7 percent DCP and 80 percent TDN. The yellow maize contains enough amount of carotene, hence good for feeding of livestock and poultry birds. It is deficient in lysine and methionine. Maize contains about 730 gm starch/ Kg DM, is very low in fibre and has a high metabolised energy value. 4) Gram: Gram contains 12 to 16 percent DCP and 78 percent TDN. Animals have great liking for this grain and so, used for preparing the concentrate mixture for feeding the livestock. 5) Jowar: Whole grains are usually fed to chickens. It contains 7 percent DCP and 74 percent TDN and high percentage of leucine.
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Zoology 5th semester notes( Sumit_yadav).pdf
Zoology 5th semester notes( Sumit_yadav).pdf
Sumit Kumar yadav
Applying bioinformatics and statistical genetics methods on population data to understand the mechanisms in ADHD and cocaine-dependence
Genetics and epigenetics of ADHD and comorbid conditions
Genetics and epigenetics of ADHD and comorbid conditions
bassianu17
Microscope presentation for Grade 7
Grade 7 - Lesson 1 - Microscope and Its Functions
Grade 7 - Lesson 1 - Microscope and Its Functions
OrtegaSyrineMay
Theoretical predictions and observational data indicate a class of sub-Neptune exoplanets may have water-rich interiors covered by hydrogen-dominated atmospheres. Provided suitable climate conditions, such planets could host surface liquid oceans. Motivated by recent JWST observations of K2-18 b, we self-consistently model the photochemistry and potential detectability of biogenic sulfur gases in the atmospheres of temperate sub-Neptune waterworlds for the first time. On Earth today, organic sulfur compounds produced by marine biota are rapidly destroyed by photochemical processes before they can accumulate to significant levels. Domagal-Goldman et al. suggest that detectable biogenic sulfur signatures could emerge in Archean-like atmospheres with higher biological production or low UV flux. In this study, we explore biogenic sulfur across a wide range of biological fluxes and stellar UV environments. Critically, the main photochemical sinks are absent on the nightside of tidally locked planets. To address this, we further perform experiments with a 3D general circulation model and a 2D photochemical model (VULCAN 2D) to simulate the global distribution of biogenic gases to investigate their terminator concentrations as seen via transmission spectroscopy. Our models indicate that biogenic sulfur gases can rise to potentially detectable levels on hydrogen-rich water worlds, but only for enhanced global biosulfur flux (20 times modern Earth’s flux). We find that it is challenging to identify DMS at 3.4 μm where it strongly overlaps with CH4, whereas it is more plausible to detect DMS and companion byproducts, ethylene (C2H4) and ethane (C2H6), in the mid-infrared between 9 and 13 μm. Unified Astronomy Thesaurus concepts: Exoplanet atmospheres (487); Exoplanet
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Sérgio Sacani
Cyathodium
Cyathodium bryophyte: morphology, anatomy, reproduction etc.
Cyathodium bryophyte: morphology, anatomy, reproduction etc.
Silpa
Context. WASP-76 b has been a recurrent subject of study since the detection of a signature in high-resolution transit spectroscopy data indicating an asymmetry between the two limbs of the planet. The existence of this asymmetric signature has been confirmed by multiple studies, but its physical origin is still under debate. In addition, it contrasts with the absence of asymmetry reported in the infrared (IR) phase curve. Aims. We provide a more comprehensive dataset of WASP-76 b with the goal of drawing a complete view of the physical processes at work in this atmosphere. In particular, we attempt to reconcile visible high-resolution transit spectroscopy data and IR broadband phase curves. Methods. We gathered 3 phase curves, 20 occultations, and 6 transits for WASP-76 b in the visible with the CHEOPS space telescope. We also report the analysis of three unpublished sectors observed by the TESS space telescope (also in the visible), which represents 34 phase curves. Results. WASP-76 b displays an occultation of 260±11 and 152±10 ppm in TESS and CHEOPS bandpasses respectively. Depending on the composition assumed for the atmosphere and the data reduction used for the IR data, we derived geometric albedo estimates that range from 0.05 ± 0.023 to 0.146 ± 0.013 and from <0.13 to 0.189 ± 0.017 in the CHEOPS and TESS bandpasses, respectively. As expected from the IR phase curves, a low-order model of the phase curves does not yield any detectable asymmetry in the visible either. However, an empirical model allowing for sharper phase curve variations offers a hint of a flux excess before the occultation, with an amplitude of ∼40 ppm, an orbital offset of ∼−30◦ , and a width of ∼20◦ . We also constrained the orbital eccentricity of WASP-76 b to a value lower than 0.0067, with a 99.7% confidence level. This result contradicts earlier proposed scenarios aimed at explaining the asymmetry observed in high-resolution transit spectroscopy. Conclusions. In light of these findings, we hypothesise that WASP-76 b could have night-side clouds that extend predominantly towards its eastern limb. At this limb, the clouds would be associated with spherical droplets or spherically shaped aerosols of an unknown species, which would be responsible for a glory effect in the visible phase curves.
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Sérgio Sacani
Climate Change Impacts on Terrestrial and Aquatic Ecosystems
Climate Change Impacts on Terrestrial and Aquatic Ecosystems.pptx
Climate Change Impacts on Terrestrial and Aquatic Ecosystems.pptx
DiariAli
TheCarringtoneventof1859hasbeenthestrongestsolarflareintheobservationalhistory.ItplaysacrucialroleinsheddinglightonthefrequencyandimpactsofthepastandfutureSolarEnergeticParticle(SEP)eventsonhumansocieties.WeaddresstheimpactoftheCarringtoneventbymeasuringtree‐ring14Cwithmultiplereplicationsfromhigh‐latitudelocationsaroundtheeventandbycomparingthemwithmid‐latitudemeasurements.Atransientoffsetin14Cfollowingtheeventisobservedwithhighstatisticalsignificance.Ourstate‐of‐the‐art14Cproductionandtransportmodeldoesnotreproducetheobservationalfinding,suggestingfeaturesbeyondpresentunderstanding.Particularly,ourobservationwouldrequirepartiallyfasttransportof14Cbetweenthestratosphereandtroposphereathighlatitudes.TheobservationisconsistentwiththepreviousfindingswiththeSEPeventsof774and993CEforwhichfasterintegrationof14Cintotreeringsisobservedathighlatitudes
TransientOffsetin14CAftertheCarringtonEventRecordedbyPolarTreeRings
TransientOffsetin14CAftertheCarringtonEventRecordedbyPolarTreeRings
Sérgio Sacani
The material is prepared for interested students & faculty in the areas of human & veterinary physiology of respiration
Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....
Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....
muralinath2
By:- Sumit Kumar yadav
Chemistry 5th semester paper 1st Notes.pdf
Chemistry 5th semester paper 1st Notes.pdf
Sumit Kumar yadav
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Call Girls Ahmedabad +917728919243 call me Independent Escort Service
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Cyanide resistant respiration pathway.pptx
Cyanide resistant respiration pathway.pptx
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Zoology 5th semester notes( Sumit_yadav).pdf
Zoology 5th semester notes( Sumit_yadav).pdf
Genetics and epigenetics of ADHD and comorbid conditions
Genetics and epigenetics of ADHD and comorbid conditions
Grade 7 - Lesson 1 - Microscope and Its Functions
Grade 7 - Lesson 1 - Microscope and Its Functions
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Cyathodium bryophyte: morphology, anatomy, reproduction etc.
Cyathodium bryophyte: morphology, anatomy, reproduction etc.
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Climate Change Impacts on Terrestrial and Aquatic Ecosystems.pptx
Climate Change Impacts on Terrestrial and Aquatic Ecosystems.pptx
TransientOffsetin14CAftertheCarringtonEventRecordedbyPolarTreeRings
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Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....
Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....
Chemistry 5th semester paper 1st Notes.pdf
Chemistry 5th semester paper 1st Notes.pdf
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