The
Fourth Solar-B Science Meeting
--- Recent Advances in
Solar Physics and Solar-B –
Venue
ISAS
A2 Conference Room (Feb 3 - 4)
&
NAOJ
Subaru Conference Hall (Feb 5)
February
3 (Mon)
Solar-B
09:30-09:40
Welcome
(Kosugi, 10min)
Program Status and Expectations for MO&DA Phase
EIS Status
(Kosugi, Hill, Culhane, 20min)
The Outline of Solar-B
Mission Operation & Data Analysis (Ver. 0.98)
Items of special
interest include:
1) Principles of Solar-B Operations
e.g. Yohkoh vs. TRACE model,
initial phase plus operational
phase
(Tarbell)
Instruments Operations for TIMES, Cluster,
& Stereo (Holmes)
2) Definition of the Observation Planning Process including:
Presentation and discussion of Solar-B Operations Flowchart
Clarification of the roles of:
A. The Solar-B Chief Planner and Supporter
B. The Scientific Schedule Coordinators, especially in relation
to the Chief Planner
C. The Solar-B Database Coordinator and the Instrument Software
Coordinators in relation to the archiving, distribution and
analysis of Solar-B data
3) Operations Software for Solar-B and its Instruments
Items of special
interest include:
4) Scheduling and Submission of Observation Plans
5) Data Policy
Items of special
interest include:
6) Archiving, Distribution and Analysis of Solar-B Data including
Agreement on Data Classification Terminology
(Discussion of Data Processing, Archiving System and Data Providing
System Flowcharts and identification of who provides and maintains
the software through the life of the mission)
Resource Provided by ISAS Information
Analysis Center for S/C (Matuzaki)
7) Data Provision Plans at ISAS and at Other Participating Institutes
1) ISACSPLN
(Matsuzaki,
- J-side explains its
capability and effort for preparation.
2) Discussions on
Mission-Wide
Keywords
(Shimojo, DeLuca, …)
February
4 (Tue)
Recent Advances in Solar
Physics & Solar-B Observation Proposals
Instrument Developments
for Science Discussion
(Chairperson, Watanabe)
FPP capabilities
(Tarbell, 20min)
CTM: Image stabilization capability
(Nagata, 5min)
Scientific Operation: observing
tables, macrocommands, etc.(
Observational parameters: field of view,
cadence etc. (comparing
with SXT
(
XRT functions: flare detection &
AEC – update (Shimojo, 20min)
What can we see with Solar-B XRT?
(Nagata, 20min)
XRT science goals: Observations of flows
in coronal loops Golub, 20min)
EIS observing sequence
(Willock, 10min)
EIS science goals
(Harra, 20min)
Recent Advances in Solar
Physics & Solar-B Observation Proposals
Line selection and atomic physics issues (Brooks, 15min)
Observational
signatures of flows in MHD simulations (Isobe, 15min)
15:45-16:00 Results from a balloon-borne hard X-ray spectrometer
(Kobayashi, 15min)
(Chairperson,
Sakurai)
16:15-16:45
Coronal Dynamics
(Shibata, 30min)
16:45-17:00 Observations of Moreton waves with Solar-B
(Narukage, 15min)
17:00-17:15 Solar Eruption Onset: Where Does the Action Begin?
(Sterling, 15min)
17:15-17:30 Observation of sigmoids with Solar-B
(Hori, 15min)
18:00-18:15 Evolution of an emerging flux and associated active phenomena (Miyagoshi, 15min)
19:00-21:00 Conference party at ISAS cafeteria
Recent Advances in Solar Physics
& Solar-B Observation Proposals
(Chairperson, Shibata)
10:00-10:30
Coronal heating and active
regions
(Sakurai, 30min)
10:30-10:45 Corona-photosphere connection with spectropolarimeter (Katsukawa, 15min)
10:45-11:00 Observations of emerging and submerging regions with ASP and
Solar-B (Kubo,
15min)
11:00-11:15 Studies on twisted magnetic flux bundles by SOT
(Ishii, 15min)
11:15-11:45 Wave process in solar upper atmosphere
(Carlsson, 30min)
11:45-12:00 Coronal heating by
acoustic waves [Postscript file 1/2]
(Suzuki, 15min)
(Chairperson, Hoeksema)
13:00-13:15
Photospheric flows and coronal loops
(Yoshimura, 15min)
13:15-13:45 Magnetic helicity injection and flares
(Kusano, 30min)
13:45-14:00 Modeling of magnetoconvection
(Hurlburt, 15min)
14:00-14:15 Recent observations at La
Palma
(Hurlburt, 15min)
14:15-14:30 Origin of the slow solar wind
(Fujiki, 15min)
Solar-B Mission Operations and Data Analysis II
(Chairperson, Watanabe)
14:30-15:00
Discussion on Coordinated observations
A. Co-Registration/Co-Alignment of Images
(Shimizu, 10min)
B. Synoptic Observations
(DeLuca, Culhane, Ichimoto, 20min)
15:15-17:00 Planning Coordinated Observations -
Discussion led by EIS team
Examples 1. Active region loop evolution and heating
- Network and intranetwork brightenings
Development and evolution of streamers
- clarify slow solar wind
- Evolution of trans equatorial loops
5. CME onset - dimming and velocity measurements
velocity structure in ejected plasmas
6. Flare dynamics and triggering
spatially resolved studies of evaporation and
turbulence in flare plasma