Participation of HEND in the Program of Interplanetary Network of localization of cosmic gammaray bu - PowerPoint PPT Presentation

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Participation of HEND in the Program of Interplanetary Network of localization of cosmic gammaray bu

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Title: Participation of HEND in the Program of Interplanetary Network of localization of cosmic gammaray bu


1
Participation of HEND in the Program of
Interplanetary Network of localization of cosmic
gamma-ray bursts
2
What is Gamma-Ray Burst?
3
Gamma-Ray Burst Coordinate Network
4
Participations in GCN
  • Ulysses, heliocentric orbit,
  • 650 light sec from Earth
  • HEND, Mars orbit, 1200
  • light sec from Earth
  • Spacecrafts near Earth,
  • WIND (KONUS experiment)
  • HETE-2
  • BeppoSax ( up to end of April
  • 2002)

5
Gamma-Ray Burst HEND Subsystem
  • Size of CsI crystal
  • - height 5.5 cm
  • - external diameter 5.5 cm
  • wall thickness 1 cm
  • Resolution
  • 0.25 sec, 1 sec.
  • Spectral range
  • from 39keV up to 1.2MeV
  • Continue data flow

6
HEND counterpart to IPN Time Profile and
Interplanetary Point
Event
TIME Position of S/C
THEND
TCEB
TUT
Odyssey Coordinate
Odyssey SPICE support
7
HEND autoburst data distribution system
Event
HEND
CEB
Odyssey
Data Request
JPL
UofA
Distribution to community
IKI
8
GRB020405
Error Box for GRB020405
  • Observed by Ulysses, Mars Odyssey (HEND),
    BeppoSAX, and Wind
  • Triangulated to a 75 square arcminute error box
    and circulated to astronomers within 17 hours
  • Optical transient source identified less than one
    hour later

Ulysses/HEND
Ulysses/BeppoSax
9
Optical counterpart for GRB020405
10
Statistic of of HEND Gamma Ray-Bursts
Free space Cruise stage
Orbital Stage
16 detected GRB (4 events/month)
9 detected GRB (2events/month)
3 events localized
5 events localized
3 have optical afterglow
3 have optical afterglow
11
Temporal properties of HEND Gamma-Ray Bursts
  • time duration distribution of long
  • GRB in a good agreement with
  • BATSE GRB time duration
  • distribution
  • there is a absence of short GRB in
  • common HEND KONUS events

12
Conclusions
  • HEND is the member of Interplanetary Gamma-Ray
    Burst Coordinate Network
  • during the year of operation 25 GRB were
    detected
  • 8 GRB were localized
  • GRB part of HEND work became more important
    after finish of BeppoSax scientific operation
    stage in the end of April 2002
  • farther development of HEND burst facility is
    necessary for own HEND GRB triggering.
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