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Pulling G : human responses to high and low gravity / / Erik Seedhouse



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Autore: Seedhouse Erik Visualizza persona
Titolo: Pulling G : human responses to high and low gravity / / Erik Seedhouse Visualizza cluster
Pubblicazione: New York, : Springer, 2012
Edizione: 1st ed. 2013.
Descrizione fisica: 1 online resource (229 p.)
Disciplina: 531.14
612/.014532
Soggetto topico: Gravity - Physiological effect
Note generali: Description based upon print version of record.
Nota di bibliografia: Includes bibliographical references and index.
Nota di contenuto: Preface -- Acknowledgments -- About the Author -- List of figures -- List of tables -- List of abbreviations and acronyms -- Chapter 1: Project MX981 -- Chapter 2: To black out or not to black out -- Chapter 3: The wobblies -- Chapter 4: The G machine -- Chapter 5: Formula One -- Chapter 6: Punching out -- Chapter 7: Launch and re-entry -- Chapter 8: Microgravity -- Chapter 9: Artificial gravity -- Index.
Sommario/riassunto: Formula 1 racing drivers, fighter pilots, astronauts - G forces are an integral part of their lives - How do racing drivers sustain high G loads and not pass out? - What accelerative forces are unleashed when a fighter pilot ejects from a high-performance jet? - What is it like being launched into space and what are the effects on astronauts living in zero G on board the International Space Station? - How do aircraft simulate zero G? Pulling G gives a unique insight into how G forces affect people working in the high and low G environments. It examines the risks of high and low acceleration and explains the physiology of surviving in these environments. The history of G-related research is described, together with present-day and future development of methods to cope with the effects of increased and reduced G.
Titolo autorizzato: Pulling G  Visualizza cluster
ISBN: 1-283-90790-9
1-4614-3030-5
Formato: Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione: Inglese
Record Nr.: 9910438124303321
Lo trovi qui: Univ. Federico II
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Serie: Popular Science, . 2626-6113