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IMPRS June 2003 S pace Instrum entation (4) Lectures for the IM PRS June 23 to June 27 at M PA e Lindau Com piled/organized by Rainer S chw enn,M PA e, supported by D rs.Curdt,G andorfer,H ilchenbach,H oekzem a,Richter,S chühle T ue,24.6., 15:00 M odern particle analyzers in planetary research: TO F,EN A (RS )

The principle of time-of-flight (TOF) instruments

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The principle of time-of-flight (TOF) instruments. From the 3 independently measured quantities (E/q, τ, E total ) the 3 desired quantities E, q, m can be uniquely derived. Ulysses SWICS. - PowerPoint PPT Presentation

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Page 1: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

Space Instrumentation (4)

Lectures f or the I MPRS J une 23 to J une 27 at MPAe Lindau Compiled/ organized by Rainer Schwenn, MPAe,

supported by Drs. Curdt, Gandorfer, Hilchenbach, Hoekzema, Richter, Schühle

Tue, 24.6., 15:00 Modern particle analyzers in planetary research: TOF, ENA (RS)

Page 2: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

The principle of time-of-flight (TOF) instruments

From the 3 independently measured quantities (E/q, τ, Etotal) the 3 desired quantities E, q, m can be uniquely

derived.

Ulysses SWICS

Page 3: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

The first TOF measurements revealed: There are two populations of oxygen ions in the magnetosphere: highly

ionized (from solar wind) and singly ionized (from the ionosphere)

Page 4: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

The SWICS instrument on Ulysses

Page 5: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

The CTOF instrument on SOHO

Page 6: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

The CTOF instrument on SOHO

Page 7: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

Electrostatic analyzer

TOF analyzer

Page 8: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

The solar wind element composition as revealed by modern TOF instrumentation on SOHO

Page 9: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

The solar wind element composition as revealed by modern TOF instrumentation on SOHO

http://umtof.umd.edu/pm/instrument.html

Page 10: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

Elemental abundances and the FIP effect

The solar wind element composition as revealed by modern TOF instrumentation on SOHO

Page 11: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

ROSINA/RTOF auf ROSETTAReflektron-Time-of-Flight-Spektrometer

Instrument parameters

• Mass range: 1-1000 amu

• Mass resolution m/m=500 (1% Level)

• High time resolution by simultaneous mesurement of different masses

http://www.phim.unibe.ch/rosina/rosina.html

Page 12: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

ROSINA/RTOF auf ROSETTAReflektron-Time-of-Flight-Spektrometer

Comparison of a mass spectrum obtained with the IMS-HIS sensor at

comet Halley with a laboratory spectrum obtained by RTOF on the

Rosetta mission

Page 13: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

Time-of-flight analyzer with a floatable drift tube

Simultaneous energy distribution and ion/neutral fraction measurements using a linear time-of-flight

Page 14: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

E!!B energy-mass spectrograph for measurement of ions and neutral atoms

Page 15: The principle of time-of-flight (TOF) instruments

IMPRS June 2003

Mass spectroscopy using a rotating electric field

time-of-flight phase

E