4,224 research outputs found

    Observations of the plasma flow in comet P/Swift‐Tuttle

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    We present direct ground based observations of the plasma flow sunward and tailward of the nucleus of comet P/Swift‐Tuttle. The observations are long‐slit high resolution spectra of the H_2O^+ emission centered at 6199Å with a velocity resolution of about 7 km s^(−1) (FWHM) and a spatial resolution of about 10^4 km at the comet. Emission is visible from just inside the predicted position of the cometopause on the sunward side of the nucleus out to 5 × 10^5 km on the tailward side. The deceleration of the solar plasma on the sunward side is clearly observed as is the acceleration of cometary ions into the tail. These observations show the effectiveness of ground based methods for the systematic study of cometary plasmas and point to the need for a better theoretical understanding of their acceleration mechanisms

    How Hot is the Wind from TW Hydrae?

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    It has recently been suggested that the winds from Classical T Tauri stars in general, and the wind from TW Hya in particular, reaches temperatures of at least 300,000 K while maintaing a mass loss rate of ∼10−11\sim 10^{-11} \Msol yr−1^{-1} or larger. If confirmed, this would place strong new requirements on wind launching and heating models. We therefore re-examine spectra from the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope and spectra from the Far Ultraviolet Spectroscopic Explorer satellite in an effort to better constrain the maximum temperature in the wind of TW Hya. We find clear evidence for a wind in the \ion{C}{2} doublet at 1037 \AA and in the \ion{C}{2} multiplet at 1335 \AA. We find no wind absorption in the \ion{C}{4} 1550 \AA doublet observed at the same time as the \ion{C}{2} 1335 \AA line or in observations of \ion{O}{6} observed simultaneously with the \ion{C}{2} 1037 \AA line. The presence or absence of \ion{C}{3} wind absorption is ambiguous. The clear lack of a wind in the \ion{C}{4} line argues that the wind from TW Hya does not reach the 100,000 K characteristic formation temperature of this line. We therefore argue that the available evidence suggests that the wind from TW Hya, and probably all classical T Tauri stars, reaches a maximum temperature in the range of 10,000 -- 30,000 K.Comment: 17 pages, 3 figures, Figure 1 in 2nd version fixes a small velocity scaling error and new revision adds a reference to an additional paper recently foun

    Vision infinity for food security: Dr Shashi B. Sharma

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    In the introductory abstract to ‘Vision Infinity for Food Security,’ (Sharma and Wightman 2015), co-author Dr Shashi Sharma draws our attention to the 1798 prediction by Thomas Malthus that human kind’s ability to feed itself was limited by population size. Malthus foresaw a time when human numbers would exhaust the capacity of planetary food producing resources with catastrophic consequences. After all, a secure food supply is essential for species survival. Food security can be defined as ensuring that all people, at all times, have both physical and economic access to the basic food that they need or, put more simply, for each individual to have sufficient food, each day, to provide the nutrients and energy to maintain a healthy and active life. The book calls for a fundamental and philosophical re-thinking and re-structuring of our food production, distribution and consumption. FDI has taken the opportunity to interview Professor Sharma about his book and his vision for a world perpetually free from food insecurity; that is, food security for all forever
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