ics viii banff canada march 27-31, 2006 to be convened by eric donovan & john samson shameless...
TRANSCRIPT
![Page 1: ICS VIII Banff Canada March 27-31, 2006 To be convened by Eric Donovan & John Samson Shameless focus on THEMIS! To be held at the Banff Center Webpage](https://reader036.vdocuments.site/reader036/viewer/2022062520/5697bfda1a28abf838cafd57/html5/thumbnails/1.jpg)
ICS VIII Banff Canada
March 27-31, 2006
To be convened by Eric Donovan & John Samson
Shameless focus on THEMIS!
To be held at the Banff Center
Webpage & First Circular coming soon.
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The local time of apogee conjunctions changes throughout the year – but it is always over central Canada.
Constellation Apogee Alignments over Central Canada
Eric Donovan
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The local time of apogee conjunctions changes throughout the year – but it is always over central Canada.
Constellation Apogee Alignments over Central Canada
Eric Donovan
![Page 4: ICS VIII Banff Canada March 27-31, 2006 To be convened by Eric Donovan & John Samson Shameless focus on THEMIS! To be held at the Banff Center Webpage](https://reader036.vdocuments.site/reader036/viewer/2022062520/5697bfda1a28abf838cafd57/html5/thumbnails/4.jpg)
The local time of apogee conjunctions changes throughout the year – but it is always over central Canada.
Constellation Apogee Alignments over Central Canada
Eric Donovan
![Page 5: ICS VIII Banff Canada March 27-31, 2006 To be convened by Eric Donovan & John Samson Shameless focus on THEMIS! To be held at the Banff Center Webpage](https://reader036.vdocuments.site/reader036/viewer/2022062520/5697bfda1a28abf838cafd57/html5/thumbnails/5.jpg)
The local time of apogee conjunctions changes throughout the year – but it is always over central Canada.
Constellation Apogee Alignments over Central Canada
Eric Donovan
![Page 6: ICS VIII Banff Canada March 27-31, 2006 To be convened by Eric Donovan & John Samson Shameless focus on THEMIS! To be held at the Banff Center Webpage](https://reader036.vdocuments.site/reader036/viewer/2022062520/5697bfda1a28abf838cafd57/html5/thumbnails/6.jpg)
Constellation Apogee Alignments over Central Canada
Eric Donovan
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THEMIS GBO array, consists of white light auroral imagers (20), as well as co-located UCLA “GMAG” fluxgate magnetometers (where deemed necessary).
THEMIS EPO (UCLA GMAG) array, consists of 10 fluxgates.
THEMIS GBOs Dedicated GB array necessary to meet objectives
Eric Donovan
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Ground-based Significant coordinated observations
• Fluxgates: CANOPUS, CANMOS, AGI, MACCS, DMI, MEASURE, IGPP-LANL, MicMac, Athabasca U., MAGIC, …
• Induction Coils: CANOPUS magnetometer array• NORSTAR multispectral ASIs, AGI multispectral ASIs • NORSTAR & Poker Flat MSPs• NORSTAR, DMI, and Alaska single beam riometers• Weatherwax imaging riometer• AMISR and the PCO• SuperDARN• PolarDARN• CADI digital ionosondes • Poker Flat Rocket Range• Athabasca Geophysical Observatory• Shiokawa MSP, panchromatic, & multispectral imagers
Eric Donovan
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Ground-based SuperDARN – Global Integrated Observation
Eric Donovan
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Ground-based Ground-based Fluxgates in the THEMIS Sector
Eric Donovan
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Ground-based Ground-based Fluxgates in the THEMIS Sector
Eric Donovan
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Ground-based Ground-based Fluxgates in the THEMIS Sector
Eric Donovan
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Ground-based Ground-based Fluxgates in the THEMIS Sector
Eric Donovan
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40 Fluxgates8 Induction Coils13 Riometers14 MSPs10 ASIs3-4 HF Radars6-8 CADIs
F10.7 Solar Flux Monitor FDAM/SSDP
Future
Ground-based Canadian GeoSpace Monitoring
National program that integrates and builds on Canadian SuperDARN, CADI, CANOPUS, CANMOS, NORSTAR, FDAM, and the F10.7 cm solar monitor.
Eric Donovan
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Ground-based Canadian GeoSpace Monitoring
Fluxgate Mags (CANMOS) David Boteler (NRCan) [email protected]
Fluxgate Mags (CANOPUS) Ian Mann (U. Alberta) [email protected]
Induction Coil Mags (CANOPUS) Ian Mann (U. Alberta) [email protected]
MSPs (NORSTAR) Eric Donovan (U. Calgary) [email protected]
ASIs (NORSTAR) Eric Donovan (U. Calgary) [email protected]
Riometers (NORSTAR) Eric Donovan (U. Calgary) [email protected]
Digisondes (CADI) John MacDougall (UWO) [email protected]
HF Radars (SuperDARN) George Sofko (U. Sask.) [email protected]
HF Radars (PolarDARN) George Sofko (U. Sask) [email protected]
FDAM/SSDP Robert Rankin (U. Alberta) [email protected]
FDAM/SSDP Robert Rankin (U. Alberta) [email protected]
Appendix – CGSM PIsEric Donovan
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CGSM CADI Polar Cap Convection
Eric Donovan
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CGSM NORSTAR ASIs & MSPs and CANOPUS Mags
Eric Donovan
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CGSM NORSTAR ASIs & MSPs
Eric Donovan
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CGSM NORSTAR ASIs & MSPs and CANOPUS Mags
Eric Donovan
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The aurora provides the only means of following the spatio-temporal evolution of (in this case) the ionospheric projection of the Earthward limit of strong pitch angle scattering in the CPS.
This provides a powerful complement to MHD simulations and empirical models [eg., Wanliss et al, 2000].
Other important boundaries :
The “Optical b2i” correlates very well with the inclination of the field.
This result is consistent with DMSP & GOES observationsas discussed by Sergeev & Newell.
• poleward border of the (bright) proton aurora
• 630 nm “polar cap shelf”
• equatorward boundary of the 630 nm brightness
Donovan et al. 2003.
CGSM MSPs
Eric Donovan
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ONSET t = 0
expa
nsio
n
t = + 2.5 min
t = + 2.7 min
t = + 6.5 min
dispersed
dispersed
CGSM Riometers
Eric Donovan
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CGSM Riometers
Eric Donovan
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Ground-based Imaging Riometer for Ionospheric Studies
Al Weatherwax to move IRIS to heart of Canadian arrays during summer 2005
Eric Donovan
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NORSTAR ASI, THEMIS ASI, Color Camera, Induction Coil, Fluxgate, meteor camera, riometer, PAI, …. your instrument here.
Instruments
Ground-based Athabasca Geophysical Observatory
New facility for multi-instrument geospace studies.
Excellent for graduate students and campaign work.
Contact Martin Connors – [email protected]
Eric Donovan
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Ground-based AMISR
Eric Donovan
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The primary objective is to understand the causal connections between specific inner magnetosphere and mid-tail events.
Ground-based Helping THEMIS Meet Mission Objectives
Secondary & tertiary objectives relate to dayside and RB physics.
Themis provides an excellent organizing theme for a coordinated and integrated multi-instrument ground-based program that will impact THEMIS and facilitate new stand-alone science.
Eric Donovan
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Appendix – CGSM Site List (not definitive)
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Ap
pen
dix
– C
GSM
Sci
en
ce T
eam
(n
ot
defi
nit
ive)
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Figure taken without permission from Chappell.
Due to our lack of understanding of the origin of the plasma sheet, and because of the real possibility that ions of ionospheric origin play a role in destabilizing the CPS, there is significant synergy between ePoP and THEMIS. See, for example, Cully et al. [JGR 2001].
ePoP Canadian Satellite to Probe Ion Outflow – Launch 2007
Eric Donovan
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ePoP Canadian Satellite to Probe Ion Outflow – Launch 2007
Instrument Institute PI
IRM Imaging rapid-scanning mass spectrometer Calgary Amerl
SEI Suprathermal electron imager Calgary Knudsen
NMS Neutral mass and velocity spectrometer ISAS Hayakawa
FAI Fast auroral imager Calgary Trondsen
RRI Radio receiver instrument CRC James
MGF Magnetic field instrument Magnametrics Wallis
GAP GPS attitude, position, and occultation exp UNB Langley
CER Coherent tri-frequency tomography beacon exp NRL Bernhardt
Eric Donovan
Contact PI Andrew Yau – [email protected]