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Internal jugular pressure increases during parabolic flight

One hypothesized contributor to vision changes experienced by >75% of International Space Station astronauts is elevated intracranial pressure (ICP). While no definitive data yet exist, elevated ICP might be secondary to the microgravity‐induced cephalad fluid shift, resulting in venous congestio...

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Autores principales: Martin, David S., Lee, Stuart M. C., Matz, Timothy P., Westby, Christian M., Scott, Jessica M., Stenger, Michael B., Platts, Steven H.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2016
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5210371/
https://www.ncbi.nlm.nih.gov/pubmed/28039409
http://dx.doi.org/10.14814/phy2.13068
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author Martin, David S.
Lee, Stuart M. C.
Matz, Timothy P.
Westby, Christian M.
Scott, Jessica M.
Stenger, Michael B.
Platts, Steven H.
author_facet Martin, David S.
Lee, Stuart M. C.
Matz, Timothy P.
Westby, Christian M.
Scott, Jessica M.
Stenger, Michael B.
Platts, Steven H.
author_sort Martin, David S.
collection PubMed
description One hypothesized contributor to vision changes experienced by >75% of International Space Station astronauts is elevated intracranial pressure (ICP). While no definitive data yet exist, elevated ICP might be secondary to the microgravity‐induced cephalad fluid shift, resulting in venous congestion (overfilling and distension) and inhibition of cerebrospinal and lymphatic fluid drainage from the skull. The objective of this study was to measure internal jugular venous pressure (IJVP) during normo‐ and hypo‐gravity as an index of venous congestion. IJVP was measured noninvasively using compression sonography at rest during end‐expiration in 11 normal, healthy subjects (3 M, 8 F) during normal gravity (1G; supine) and weightlessness (0G; seated) produced by parabolic flight. IJVP also was measured in two subjects during parabolas approximating Lunar (1/6G) and Martian gravity (1/3G). Finally, IJVP was measured during increased intrathoracic pressure produced using controlled Valsalva maneuvers. IJVP was higher in 0G than 1G (23.9 ± 5.6 vs. 9.9 ± 5.1 mmHg, mean ± SD P < 0.001) in all subjects, and IJVP increased as gravity levels decreased in two subjects. Finally, IJVP was greater in 0G than 1G at all expiration pressures (P < 0.01). Taken together, these data suggest that IJVP is elevated during acute exposure to reduced gravity and may be elevated further by conditions that increase intrathoracic pressure, a strong modulator of central venous pressure and IJVP. However, whether elevated IJVP, and perhaps consequent venous congestion, observed during acute microgravity exposure contribute to vision changes during long‐duration spaceflight is yet to be determined.
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spelling pubmed-52103712017-01-05 Internal jugular pressure increases during parabolic flight Martin, David S. Lee, Stuart M. C. Matz, Timothy P. Westby, Christian M. Scott, Jessica M. Stenger, Michael B. Platts, Steven H. Physiol Rep Original Research One hypothesized contributor to vision changes experienced by >75% of International Space Station astronauts is elevated intracranial pressure (ICP). While no definitive data yet exist, elevated ICP might be secondary to the microgravity‐induced cephalad fluid shift, resulting in venous congestion (overfilling and distension) and inhibition of cerebrospinal and lymphatic fluid drainage from the skull. The objective of this study was to measure internal jugular venous pressure (IJVP) during normo‐ and hypo‐gravity as an index of venous congestion. IJVP was measured noninvasively using compression sonography at rest during end‐expiration in 11 normal, healthy subjects (3 M, 8 F) during normal gravity (1G; supine) and weightlessness (0G; seated) produced by parabolic flight. IJVP also was measured in two subjects during parabolas approximating Lunar (1/6G) and Martian gravity (1/3G). Finally, IJVP was measured during increased intrathoracic pressure produced using controlled Valsalva maneuvers. IJVP was higher in 0G than 1G (23.9 ± 5.6 vs. 9.9 ± 5.1 mmHg, mean ± SD P < 0.001) in all subjects, and IJVP increased as gravity levels decreased in two subjects. Finally, IJVP was greater in 0G than 1G at all expiration pressures (P < 0.01). Taken together, these data suggest that IJVP is elevated during acute exposure to reduced gravity and may be elevated further by conditions that increase intrathoracic pressure, a strong modulator of central venous pressure and IJVP. However, whether elevated IJVP, and perhaps consequent venous congestion, observed during acute microgravity exposure contribute to vision changes during long‐duration spaceflight is yet to be determined. John Wiley and Sons Inc. 2016-12-30 /pmc/articles/PMC5210371/ /pubmed/28039409 http://dx.doi.org/10.14814/phy2.13068 Text en Published 2016. This article is a U.S. Government work and is in the public domain in the USA. Physiological Reports published by Wiley Periodicals, Inc. on behalf of The Physiological Society and the American Physiological Society This is an open access article under the terms of the Creative Commons Attribution (http://creativecommons.org/licenses/by/4.0/) License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
spellingShingle Original Research
Martin, David S.
Lee, Stuart M. C.
Matz, Timothy P.
Westby, Christian M.
Scott, Jessica M.
Stenger, Michael B.
Platts, Steven H.
Internal jugular pressure increases during parabolic flight
title Internal jugular pressure increases during parabolic flight
title_full Internal jugular pressure increases during parabolic flight
title_fullStr Internal jugular pressure increases during parabolic flight
title_full_unstemmed Internal jugular pressure increases during parabolic flight
title_short Internal jugular pressure increases during parabolic flight
title_sort internal jugular pressure increases during parabolic flight
topic Original Research
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5210371/
https://www.ncbi.nlm.nih.gov/pubmed/28039409
http://dx.doi.org/10.14814/phy2.13068
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