Transcript Kein Folientitel

S p a c e I n stru m e n ta tio n (5 )
L e ctu r e s f o r th e I M P R S J u n e 2 3 to J u n e 2 7 a t M P A e L in d a u
C o m p ile d / o r g a n iz e d b y R a in e r S ch w e n n , M P A e ,
s u p p o r te d b y D r s . C u r d t, G a n d o r f e r , H ilch e n b a ch , H o e k z e m a , R ich te r , S ch ü h le
T u e , 2 4 .6 .,
16 :0 0
E n e rg e tic p a rtic le s. D e te c tio n o f in t e rste lla r g a s. (R S )
IMPRS June 2003
Energetic particles in the solar system
The heliosphere is flooded with those particles, from at least 6 different sources!
IMPRS June 2003
Galactic Cosmic Rays hitting the Earth
Spaceship Earth as a spectrometer for GCRs!
In order to penetrate the magnetic shield of the Earth down to the
atmosphere, GCRs must have energies above 1 GeV (polar latitudes)
and 20 GeV (at the equator)
IMPRS June 2003
Galactic Cosmic Rays hitting the Earth
Spaceship Earth as a spectrometer for GCRs!
„Forbush decreases“
of GCRs are known since
the 1940s
The GCRs are effectively
shielded by magnetic clouds
following coronal mass
ejections (CMEs)
IMPRS June 2003
SCR and GCR through the solar cycle
Minimum
Maximum
Minimum
Sunspots
Neutron flux at Earth
Galactic cosmic rays
Solar cosmic rays
1974
1986
IMPRS June 2003
The Helios E6 cosmic
ray detector (Uni Kiel)
IMPRS June 2003
The High Energy Telescope HET on Ulysses
http://ulysses.uchicago.edu/WWW/Simpson/UlyDocs/HETsktch.html
IMPRS June 2003
Ulysses COSPIN HET: de/dx vs E spectra
IMPRS June 2003
Solid state detectors (SSD):
• Elektrons and Ions with energies of 10 keV to MeV
• High time and spacial reolution
IMPRS June 2003
Micro-Calorimeter
Stacks will be used for the
Advanced Cosmic-Ray Composition
Experiment for the Space Station
(ACCESS 2005)
IMPRS June 2003
Focussing of interstellar neutral gas by the Sun
IMPRS June 2003
How to measure neutral particles
with low energies? Ionize them
first!
For example, by letting them pass
through extreme electric fields.
IMPRS June 2003
Interstellar helium
Detector:
GAS on Ulysses
NIHEAD
Interplanetary
Pathfinder 1998
IMPRS June 2003
Interstellar neutral gas flow into the
heliosphere
Velocity:
25.3 ± 0.4 km/s
Flow Direction
ecliptic longitude : 73.9 ± 0.8o
ecliptic latitude:
-5.6 ± 0.4o
Temperature:
7000 ± 600K
The flow of neutral gas into
the solar system can be
interpreted as the solar
system moving through the
interstellar medium in a
direction about towards the
star Antares (Alpha-Scorpii).
IMPRS June 2003
Neutral Particle Detectors
ASPERA-3
Mars Express
2003
Cheng 1993
MENA
IMAGE
2000
IMPRS June 2003
ENA Imaging at Saturn/Titan
by Cassini/MIMI
Measured MIMI/INCA images during the
Cassini flyby at Jupiter
http://saturn.jpl.nasa.gov/index.cfm
IMPRS June 2003