The top documents tagged [plasma flows]

Magnetic sail braking vs two-stage fusion rockets
Technology Magnetic sail braking vs two-stage fusion rockets

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Plasma Wind Tunnel
Documents Plasma Wind Tunnel

1.345 views

Lynda and Abyle products. Blood pump Moves blood in all the therapies. In CRRT the blood flow is between 0.30 and 450 ml/min. In CRRT the blood flow
Documents Lynda and Abyle products. Blood pump Moves blood in all the therapies. In CRRT the blood flow is between 0.30 and 450 ml/min. In CRRT the blood flow

220 views

Charge-Exchange Spectroscopy at the University of Wisconsin-Madison Mark Nornberg Santhosh Kumar, Daniel Den Hartog Alexis Briesemeister 2012 ADAS Workshop
Documents Charge-Exchange Spectroscopy at the University of Wisconsin-Madison Mark Nornberg Santhosh Kumar, Daniel Den Hartog Alexis Briesemeister 2012 ADAS Workshop

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STORM Annual Meeting - Graz, November 25-26, 2013 A brief overview of magnetosheath physics Maria Federica Marcucci INAF-IAPS STORM Annual Meeting - Graz,
Documents STORM Annual Meeting - Graz, November 25-26, 2013 A brief overview of magnetosheath physics Maria Federica Marcucci INAF-IAPS STORM Annual Meeting - Graz,

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Chapter 3. Transport Equations The plasma flows in planetary ionospheres can be in equilibrium (d/dt = 0), like the midlatitude terrestrial ionosphere,
Documents Chapter 3. Transport Equations The plasma flows in planetary ionospheres can be in equilibrium (d/dt = 0), like the midlatitude terrestrial ionosphere,

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Lynda and “Abyle” products. Blood pump Moves blood in all the therapies. In CRRT the blood flow is between 0.30 and 450 ml/min. In CRRT the blood flow
Documents Lynda and “Abyle” products. Blood pump Moves blood in all the therapies. In CRRT the blood flow is between 0.30 and 450 ml/min. In CRRT the blood flow

222 views

Solar Physics & Space Plasma Research Center (SP 2 RC) The role of partial ionisation in the stability of prominences structures Istvan Ballai SP 2 RC,
Documents Solar Physics & Space Plasma Research Center (SP 2 RC) The role of partial ionisation in the stability of prominences structures Istvan Ballai SP 2 RC,

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EISCAT-Cluster observations of quiet-time near-Earth magnetotail fast flows and their signatures in the ionosphere Nordic Cluster Meeting, Uppsala, Sweden,
Documents EISCAT-Cluster observations of quiet-time near-Earth magnetotail fast flows and their signatures in the ionosphere Nordic Cluster Meeting, Uppsala, Sweden,

214 views

Lecture 9 Solar Wind-Magnetosphere Interaction Structure of the Magnetosphere
Documents Lecture 9 Solar Wind-Magnetosphere Interaction Structure of the Magnetosphere

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5 th RHESSI workshop, Locarno. WG 4 Report Participants: Steven ChristeSäm Krucker Brian DennisMonique Pick Lyndsay FletcherEd Schmahl Peter GallagherManuela
Documents 5 th RHESSI workshop, Locarno. WG 4 Report Participants: Steven ChristeSäm Krucker Brian DennisMonique Pick Lyndsay FletcherEd Schmahl Peter GallagherManuela

218 views

The goal of the study : To localize sources of the quasi-stationary slow solar wind. Method:
Documents The goal of the study : To localize sources of the quasi-stationary slow solar wind. Method:

32 views