Chapman Conference and AGU registration and housing is open
2.0 MMS Flight Dynamics and Ephemeris/Attitude
Formation maintenance maneuver scheduled for August 31/September 1 to keep at 160 km.
First formation resize maneuver scheduled for September 16/17 for 60 km.
Phase 1A Sliding Science ROI:
Recall our previous discussion RE orienting the entry/exit of ROI to optimize orientation with predicted magnetopause. This "sliding science ROI" will be implemented as soon as possible; Steve Petrinec is running an updated plan. See Steven's previous presentation for an example.
ROI is determined based on average magnetopause conditions (based on OMNI or ACE at this time in the previous solar cycle?). The instrument commanding is done at least 3 weeks in advance, so this ROI will not be based on "current conditions".
3.0 MMS Burst Memory Management
Thanks to Jim Burch for his service during the first official MMS SITL cycle.
Tom Moore is the current SITL, with Roy Torbert being the SITL on Deck for next week.
Mitsuo Oka made the following plot summarizing MMS burst memory management over time. The thin black curve shows the total number of buffers HELD for more than 3 days. If the thin black curve approaches the grey-shaded region, we are in danger of loosing segments. The table shows the number of currently pending segments. Definition of Category 0, 1, 2, etc, is here.
4.0 IMPORTANT NOTES:
If there are updates to the SITL CDF data product structure, content, or delivery schedules; please notify the Supervisory SITLs before deployment. We have had a few disruptions to the SITL process when new files were not compatible with the SITL software. Similarly, you should notify this forum for broader changes so that the broader range of codes can be smoothly updated as well.
FPI plans to release updated versions of the SITL CDF files this week (as soon as the release notes are ready). These files, with version v0.1.0, should not disrupt current display/analysis codes. The update does provide updated/corrected moments, which should be very welcome.
MMS inclusion into SPEDAS is progressing. There are crib sheets in the MMS Project folder that are of use now. As these progress and data products become available these will be expanded and inclusion in the GUI will continue to expand.
5.0 NO UPDATE FOR NOW – Tetrahedron Management:
Following is a plot with the definitive quality factor for Rev 143.
STP-MMS-P40: Spacecraft Constellation Formation Quality. A Quality Factor shall be developed that defines the usefulness of the tetrahedron formation of the four spacecraft that is the product of two functions. One function is a metric of the inner spacecraft separation, and the other is a metric of the tetrahedron shape. This Quality Factor shall be greater than or equal to 0.7 for 80% of the time in the regions of science interest. The regions of science interest are defined as geocentric distances >9 RE for Phase 1, and >15 RE for Phase 2. There is no formation requirement or region of science interest defined during the transition from Phase 1 to Phase 2.
MMS Online Data Analysis Telecon Tuesday, September 1, 2015 10:00 am | Central Daylight Time (Chicago, GMT-05:00) | 2 hrs Join WebEx meeting Meeting number: 809 629 067 Meeting password: Smart1 Join by phone 1-866-469-3239 Call-in toll-free number (US/Canada) 1-650-429-3300 Call-in toll number (US/Canada) Access code: 809 629 067
PREPARATION INSTRUCTIONS: From: <Burch>, Jim Burch <email@example.com> Date: Monday, August 31, 2015 11:53 AM Subject: Fwd: (Forward to others) WebEx meeting invitation: MMS Online Data Analysis Hi All, This is a reminder of our data analysis telecon at 10 AM CDT tomorrow. Attached is the crib_master_v3.pro, which we will use to discuss the events on Aug. 15 and Aug. 28. Summary plots for the SITL option for these dates are also attached. To use the procedure, first download the latest bleeding edge: http://themis.ssl.berkeley.edu/socware/bleeding_edge/ Select the top zip file. Install this in your SPEDAS directory. The crib_master_v3.pro is not in bleeding edge yet. Save it from this email into /spedas/projects/mms/ Please run this for the two events to make sure it works. If not, restart IDL. This way you will have the data on your local system. That will speed things up. If you want to show burst data or any analysis, please have that ready for the bouncing ball. The plan will be to discuss these events first and then possibly look at the data that comes in today if there are any magnetopause crossings. Please pass this on to others in your team. Thanks, Jim