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Altered Intracellular Trafficking as a Mechanism for Prolonged Duration of G Protein-Coupled Receptor Activation. [PDF]
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Venus Monitoring Camera for Venus Express
Planetary and Space Science, 2007Abstract The Venus Express mission will focus on a global investigation of the Venus atmosphere and plasma environment, while additionally measuring some surface properties from orbit. The instruments PFS and SPICAV inherited from the Mars Express mission and VIRTIS from Rosetta form a powerful spectrometric and spectro-imaging payload suite.
David Crisp +2 more
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Venus Express—Science observations experience at Venus
Acta Astronautica, 2009Abstract The Venus Express mission is the European Space Agency's (ESA) first spacecraft at Venus. It was launched in November 2005 by a Soyuz–Fregat launcher and arrived at Venus in April 2006. The mission covers a broad range of scientific goals including physics, chemistry, dynamics and structure of the atmosphere as well as atmospheric ...
Hoofs, R. +5 more
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Journal of Pain & Palliative Care Pharmacotherapy, 2011
This is the story of a man in India who is among millions denied access to pain relief all over the developing world. He was in agonizing pain and pleaded to a doctor for pain relief, adding that he had not slept for several days. Not only was pain relief denied to him, but he was also insulted by a doctor with the words, "What do you want me to do ...
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This is the story of a man in India who is among millions denied access to pain relief all over the developing world. He was in agonizing pain and pleaded to a doctor for pain relief, adding that he had not slept for several days. Not only was pain relief denied to him, but he was also insulted by a doctor with the words, "What do you want me to do ...
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Science, 1995
The Magellan imagery shows that Venus has a crater abundance equivalent to a surface age of 300 million to 500 million years and a crater distribution close to random. Hence, the tectonics of Venus must be quiescent compared to those of Earth in the last few 100 million years.
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The Magellan imagery shows that Venus has a crater abundance equivalent to a surface age of 300 million to 500 million years and a crater distribution close to random. Hence, the tectonics of Venus must be quiescent compared to those of Earth in the last few 100 million years.
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Nature, 1970
VENERA 4, 5 and 6 indicate that the surface layers and atmosphere of Venus are considerably dryer than corresponding regions on Earth. The water content of the atmosphere is in the region of 0.1 to 1 per cent of the total atmospheric gases by volume1, and at the Venus surface temperatures of about 700 K this is very dry indeed.
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VENERA 4, 5 and 6 indicate that the surface layers and atmosphere of Venus are considerably dryer than corresponding regions on Earth. The water content of the atmosphere is in the region of 0.1 to 1 per cent of the total atmospheric gases by volume1, and at the Venus surface temperatures of about 700 K this is very dry indeed.
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Uspekhi Fizicheskih Nauk, 1971
CONTENTS 1. Chemical Composition 317 2. Temperature, Pressure, Density 319 3. Cloud Layer 325 4. Thermal Regime 328 5. General Circulation 331 6. Upper Atmosphere 332 7. Origin and Evolution 335 8.
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CONTENTS 1. Chemical Composition 317 2. Temperature, Pressure, Density 319 3. Cloud Layer 325 4. Thermal Regime 328 5. General Circulation 331 6. Upper Atmosphere 332 7. Origin and Evolution 335 8.
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