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SPP group involvement in rocket and balloon experiments
- Cascades-2 sounding rocket- PoGO Lite astrophysical balloon
Hardware solutions- SMILE magnetometer- SMILE 2.0- “Silverbox” and photometers
Timeline- Cascades-2 campaign- PoGO Lite launch
(Applications in progress- SPIDER- SEPAM)
Cascades2 ~reflight of ~
The Changing Aurora: in Situ and Camera Analysis of
Dynamic Electron precipitation Structures
PI: – Kristina A Lynch, Dartmouth Kevin RhoadsLead CoIs: – Paul Kintner, Cornell Steve Powell – Marc Lessard, UNH Paul Riley – Hans Stenbaek-Nielsen, UAF/GI CoIs: – James LaBelle, Dartmouth – Mark Psiaki, Cornell – Tom Hallinan, UAF/GI Collaborators: – John Bonnell and Chris Chaston, SSL/UCB – Goran Marklund and Nickolay Ivchenko, KTH, Sweden – Charles Seyler, Cornell – Craig Heinselman, SRI
March 2005PFRR3rd stage failure
Another chance
Same team, same goals
KTH:1. Magnetometer2. Ground Camera
Bo
PFRRAMISR Kaktovic
E and B along Bo
e- across Bo
Fast e- down Bo
Image down Bo
Ground cameras
Radar
Science Questions:space vs time
(1) Does dynamic aurora move with respect to the background ionosphere? How much? Does it matter?
(2) What is the spatial (as opposed to temporal)variation of auroral parameters like B and E?What does this mean for theories of energy transfer?
(3) Alfven waves carry disturbances and changes down to and through the auroral zone, giving us structured anddancing aurora. They are pretty: do they matter? Are these structures significant for magnetosphere/ionosphere coupling? Do direct observations of these motions validate
theories and models?
PoGOLite is a balloon-borne experiment which stands to open a new observational window on the Universe through measurements of the polarisation of gamma-rays in the energy range 25 - 80 keV from compact astrophysical objects, such as pulsars, and accreting black holes. Thepolarisation is reconstructed using the modulation of Compton scattering angles in the segmented sensitive volume of the instrument composed of plastic scintillators.
Lead PI in Sweden: prof. Mark Pearce (Astroparticle Physics, KTH)
PoGOLite detectors
PoGOLite first flight
Location: Esrange, Kiruna
Time: mid-August 2010
Duration: 12-24 hours
Objective: test payload,characterise background
Targets:Crab (RA: 05h 34m, DEC: +22 00)Cyg X-1 (RA: 19h 58m DEC: +35 12)
PoGOLite Auroral Background
Millan, 2002. MAXIS balloon X rays.
PoGOLite Auroral Background
Petrinec, 2000. Polar PIXIE observations of 2-12 keV X rays and AKR.
PoGOLite auroral diagnostics
- Astrophysicists want to know when there is aurora, andwhat are its parameters (energy flux, characteristic energies).
- We want to know whether auroral X-rays are polarised
- The diagnostic package will consist of photometers (a la ASK) and a magnetometer (a la Cascades-2).
- From photometer ratios the energies can be esimated.
Challenges:
Strong background → only red, IR emissions filter width?cooling?background channelorfilter tilting?
SMILE – digital fluxgate magnetometer
Sensor: dimension 20x20x21 mmweight 21gcable weight 4 g/m
Electronics+box: dimension 70x70x25 mmweight <200 gpower <500 mW
Prototype electronics PCB:120x88 mm, 80 g
SMILE diagram
FPGA
Processor
SMILE 2.0 diagram
FPGA
Processor PC RS-232
NASATM LVDS serial
Memory
GPS
1PPS, (UTC)
Sensor
Electronicsbox
FPGA
Processor PC RS-232
Memory
GPS
1PPS, (UTC)
Photometer counter for PoGOLite
Photometer
ASK timing - old system
”Black Box” for ASK timing
ASK timing - new system
”Silver Box” for ASK timing
FPGA
Processor PC RS-232
Memory
GPS
1PPS, (UTC)
”Silver Box” diagram
Photometer
Camera Camera
Camera
- better and faster synchronisation to GPS time
- eliminates possible hangup of NI driver software
- allows synchronisation of instruments at different locations
- reduces the number of cables!
- thermal control loop and light-sensitive switchcan be implemented independently of the PC
- run photometers as fast as you want!
- store data in memory, and read out later
- timetag data unambiguously
”Silver Box” advantages
It takes a while to make it!
but …
We will make several!
”Silver Box” drawbacks
- ASK system
- PoGOLite system & new EMCCD
- SIF photometers?
- ???
October 20 – get ASK up and running for the season
October 29 – heating campaign at Tromsø, with new camera, PoGOLite photometers
February – Cascades-2 campaign in Alaska, with newcamera, PoGOLite photometers, (othercameras)?
HD and GM will be at Toolik lake.
Heating at HAARP, a campaign at AMISR?
The plan