TERMIUM Plus^®

Record 1,  Textual support,  English

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An expandable device introduced in the stomach as a temporary obesity treatment to reduce the stomach’s capacity, thus reducing food intake and body weight.  5, record 1, English, - gastric%20balloon

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The Heliosphere Intragastric Balloon System is a temporary non-surgical obesity treatment that induces short-term weight loss by partially filling the stomach to achieve satiety.... The deflated balloon is inserted into the stomach through the mouth using an endoscope. It is then filled with air to a final volume of 650 mL to 750 mL and released to float freely in the stomach. The balloon is used with a supervised calorie-restricted diet, and must be removed after six months. Another type of intragastric balloon is the BioEnterics Intragastric Balloon System[, ] a silicone balloon filled with saline.  6, record 1, English, - gastric%20balloon

Record 1,  Textual support,  French

Record number: 1, Textual support number: 1 DEF

Dispositif gonflable implanté [temporairement] dans l'estomac comme adjonction à la thérapie de l'obésité [afin de réduire le volume de l'estomac et, par conséquent, la prise alimentaire et le poids].  5, record 1, French, - ballon%20intragastrique

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Le ballon intra-gastrique Héliosphère est un traitement temporaire non chirurgical de l'obésité qui permet une perte de poids à court terme en occupant du volume dans l'estomac afin de provoquer la sensation de satiété. [...] Le ballon sans air est introduit dans l'œsophage jusqu'à l'estomac à l'aide d'un endoscope. Il est gonflé par la suite pour occuper un volume final de 650 ml à 750 ml et libéré pour flotter librement dans l'estomac. Le ballon est utilisé de pair avec un régime d'amaigrissement surveillé et doit être retiré dans un délai de six mois. Un autre type de ballon intra-gastrique est le ballon intra-gastrique BioEnterics[,] un ballon en silicone qui se remplit de sérum physiologique.  4, record 1, French, - ballon%20intragastrique

Record 1,  Textual support,  Spanish

Record 2,  Textual support,  English

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... the heliopause... marks the end of a region created by our Sun that is called the heliosphere. The Sun creates this heliosphere by sending a constant flow of particles and a magnetic field out into space at over 670, 000 miles per hour.  2, record 2, English, - heliosphere

Record 2,  Textual support,  French

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Un peu comme l'huile ne se mélange pas à l'eau, le vent solaire et le milieu interstellaire ne sont pas tout à fait miscibles, le vent solaire crée donc une bulle dans le milieu interstellaire baptisée héliosphère. [...] l'héliosphère agit comme un bouclier pour tout ce qu'elle renferme et protège notamment notre fragile ADN des radiations les plus intenses de la galaxie. La limite extérieure de l'héliosphère porte le nom d'héliopause et marque le début de l'espace interstellaire.  2, record 2, French, - h%C3%A9liosph%C3%A8re

Record 2,  Textual support,  Spanish

Record 3,  Textual support,  English

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Scientists define the beginning of interstellar space as the place where the Sun's constant flow of material and magnetic field stop affecting its surroundings. This place is called the heliopause. It marks the end of a region created by our Sun that is called the heliosphere.  2, record 3, English, - interstellar%20space

Record 3,  Textual support,  French

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La limite extérieure de l'héliosphère porte le nom d'héliopause et marque le début de l'espace interstellaire. La compréhension de cette limite peut nous aider à mieux cerner le voyage effectué par le Soleil à travers la galaxie, ce qui en retour nous permettra d'en apprendre plus sur la situation des autres étoiles dispersées dans l'univers.  2, record 3, French, - espace%20interstellaire

Record 3,  Textual support,  Spanish

Record 4,  Textual support,  English

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Vestiges of the interstellar wind flowing into what's called the heliosphere-the vast bubble filled by the Sun's own constant flow of particles, the solar wind – is one of the ways scientists can observe what lies just outside of our own home, in the galactic cloud through which the solar system travels.  2, record 4, English, - interstellar%20wind

Record 4,  Textual support,  French

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[...] les deux sondes ont atteint les limites [de] l'héliosphère à environ la même distance, soit 120 unités astronomiques [...] L'héliosphère est la zone du système solaire où le vent en provenance de notre Soleil empêche la propagation du vent interstellaire en provenance d'autres étoiles.  2, record 4, French, - vent%20interstellaire

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Record 5,  Textual support,  English

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After this acceleration an as yet unknown fraction diffuses backwards into the inner heliosphere against the solar wind, i. e. the anomalous component is subjected to the effects of solar modulation.  2, record 5, English, - anomalous%20component

Record 5,  Textual support,  French

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Présence anormale de particules de grande énergie dans l'héliosphère.  2, record 5, French, - composante%20anormale

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Le lent éloignement d'Ulysse des régions équatoriales, jusqu'à une distance radiale d'environ 5 AU à l'aphélie, couplée à la très faible activité solaire constatée pendant la majeure partie de l'année 1997, ont fourni une occasion unique de mesurer la variation radiale réelle de la composante anormale du rayonnement cosmique (ACR) décelée dans l'héliosphère interne, à l'abri d'effets latitudinaux.  3, record 5, French, - composante%20anormale

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Record 6,  Textual support,  English

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The Sun emits a steady flow of electrically-charged particles called the solar wind. As the solar wind expands supersonically into space, it creates a magnetized bubble around the Sun--the heliosphere. Eventually, the solar wind runs into the electrically-charged particles and magnetic field in the interstellar gas. The solar wind abruptly slows down from supersonic to subsonic speed, creating a termination shock. Before both spacecraft travel beyond the heliopause into interstellar space, they must pass through that shockwave.  2, record 6, English, - termination%20shock

Record 6,  Textual support,  French

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Record 7,  Textual support,  English

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Previous studies of the Sun have only been done in the Ecliptic, and are thus a small glimpse of the dynamic solar environment. Although it will get no closer to the Sun than it was the day it was launched, the Ulysses spacecraft will provide a unique opportunity to explore the Heliosphere in total. It carries a 55 kg(121 lbm) instrument payload to collect data on the solar magnetic field, solar radiation such as radio and plasma waves and X-rays, and the solar wind, as well as cosmic radiation and dust entering the solar system. There are nine instruments :... Unified Radio and Plasma Wave Experiment(URAP) to measure high frequency radio waves and lower frequency plasma waves...  2, record 7, English, - unified%20radio%20and%20plasma%20wave%20experiment

Record 7,  Textual support,  French

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Record 8,  Textual support,  English

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The energy eruptions in the solar atmosphere can lead to the acceleration of local gas particles to extremely high energies and their injection into the interplanetary space. These fast moving streams of particles are recorded by ERNE. At times, when there is no energetic particle production at the Sun, ERNE is observing the continuous flux of energetic particles from Milky Way(galactic cosmic rays), and from the boundary of the heliosphere accelerated by the termination shock(anomalous cosmic rays).  3, record 8, English, - energetic%20and%20relativistic%20nuclei%20and%20electron%20experiment

Record 8,  Textual support,  French

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Record 9,  Textual support,  English

Record number: 9, Textual support number: 1 OBS

IAU : International Astronomical Union  1, record 9, English, - IAU%20Commission%20on%20Interplanetary%20Plasma%20and%20the%20Heliosphere

Record 9,  Textual support,  French

Record 9,  Textual support,  Spanish