Bhoochetana: Building Resilience and Livelihoods through Integrated Watershed Management

Rainfed areas are hotspots of poverty and malnutrition, and are prone to severe land degradation of natural resources. Globally, 80% of agriculture is rainfed providing 62% of the world’s staple food. With increasing population over the years, per capita availability and quality of land and water resources have declined substantially resulting to water scarcity. Agriculture is the major consumer of water, accounting for 70-80% of water withdrawal. With the impacts of climate change, existing water and land scarcity will be aggravated further. Producing food for the ever growing population to achieve food and nutrition security, and improving rural livelihoods are challenges to be met today as well as in the near future. Agriculture is the major contributor in the growth of the state of Karnataka, India and is still the mainstay for a large number of population in the state economy. However, trends are showing that the agriculture and allied sectors’ contribution to Karnataka’s GDP was around 43% in 1980-1981 that came down to 26% in 2001-2002, which further came down to 16.8% in 2007-2008, remaining stagnant in 2009-2010. This declining contribution of agriculture in the state GDP was a big concern for the state government

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta