ISSI International Team

Sub-millimeter Solar Flare Observations


Scientific Aims - Proposal - Team Members - Meetings - Overview paper - Library - Notes



Scientific Aims

We will systematize our knowledge of the emission of solar flares in the THz range (submillimeter wavelengths). This is essentially a new field of solar flare research, with substantial ambiguities of interpretation but potentially great significance because of the implications for high-energy particle acceleration. It is also a timely topic due to the potential for future observations in the THz domain with the new instrumentation at SST (the Solar Submillimer-wave Telescope) and ALMA (the Atacama Large Millimeter Array) and proposed space instrumentation. We therefore anticipate good discussions of current observations, vigorous debate of the theories in the context of the broad coverage of solar flares now available at other wavelengths, and the potential of the new instruments to address the questions arising. The output of the team will be an overview paper setting out the properties of the existing observations and their interpretations, and goals for new observations.


Proposal

Original proposal (pdf file)


Team Members

Säm Krucker (team leader), UC Berkeley, USA
Hugh Hudson (team leader), UC Berkeley, USA
T.S. Bastian, NRAO, USA
C.G. Gimenez de Castro, CRAAE, Brazil
G.D. Cristiani, IAFE, Argentina
A.S. Hales, NRAO, USA
Jana Kasparova, Ondrejov, Czech Republic
Ludwig Klein, LESIA, France
M. Kretzschmar, LPCEE Orleans, France
T. Lüthi, Leica, Switzerland
S. Pohjolainen, University of Turku, Finland
Alec MacKinnon, U. of Glasgow, UK
Gerard Trottet, LESIA, France
Steven White, AFRL, USA

Meetings

First: November 9-11, 2009 (Mon-Wed)
Second: June 9-11, 2010 (Wed-Fri)

First meeting (presentations are availalbe in ppt or pdf):

MONDAY November 9:
INSTRUMENTATION & OBSERVATIONS:
SST: instrument and summary of observations including present Mid-IR observations (Gimenez de Castro)
KOSMA: instrument and summary of observations (Luethi)

TUESDAY November 10:
THEORY: Possible explanations for an increasing spectrum
thermal continua (IR-WL-UV) (Hudson)
thermal submillimeter emission (Bastian)
synchrotron (White)
Other mechanisms (MacKinnon)
quantitative comparison: Theory & Observations (Trottet)

WEDNESDAY November 11:
FUTURE INSTRUMENTS & COORDINATED OBSERVATIONS:
ALMA (Hales)
far infrared observations (Klein)
Mid and Far IR (Brazil) (Gimenez de Castro)
Mid-IR (Scotland) (Hudson)
Tuorla (Pohjolainen)

Table of events:

Table of events with submillimeter observations

Overview plot of events:

Overview plot

Summary (doc file):

Table of discussed emission mechanisms and outline of review paper

Second meeting (June 2010)

Paper draft:

The beginnings of a paper are on this directory (updated 6-Sep-2010)

Editorial rotation and publication plan

We have decided to experiment with a new scheme for contributions to the overview paper. In the following list each author has been assigned a specific week for input to the manscript. This could either be by copying the files and emailing any new ones to Hugh and Sa"m, or else by marking up a .pdf and sending that. We intend to update the working directory each weekend during this cycle and send an informational email out.

13 June nil
20 June First draft available in A&A Review style
27 June Giménez de Castro
4 July Trottet
11 July White
18 July Lüthi 25 July Kretzschmar
1 Aug Bastian
8 Aug MacKinnon
15 Aug Kasparova
22 Aug Klein

29 Aug Hales
5 Sep Krucker, Hudson
12 Sep Send to Pierre Kaufmann for pre-review
19 Sep
26 Sep Submit to journal

The current version (20 July 2010) is HERE as a big .tar file.