Pre-Notes Notes
Schedule
please update in real-time throughout the day
Time |
Team |
9:00 AM - 9:25 AM |
Science |
9:25 AM - 9:50 AM |
Systems |
9:50 AM - 10:15 AM |
Optics |
10:15 AM - 10:25 AM |
BREAK |
10:25 AM - 10:50 AM |
Payload Mechanical |
10:50 AM -11:15 AM |
Mechanical |
11:15 AM - 11:40 AM |
Thermal |
11:40 AM - 12:15 PM |
ADCS |
12:15 PM - 12:45 PM |
LUNCH |
12:45 PM - 1:10 PM |
Electrical |
1:10 PM - 1:35 PM |
Power |
1:35 PM - 2:00 PM |
RF / Ground Station |
2:00 PM - 2:25 PM |
Mission Operations |
2:25 PM - 2:35 PM |
BREAK |
2:35 PM - 3:00 PM |
Firmware |
3:00 PM - 3:25 PM |
Command & Data Handling |
3:40 PM - 4:05 PM |
Payload Firmware |
4:05 PM - 4:15 PM |
BREAK |
4:15 PM - 4:40 PM |
Data Processing |
4:40 PM - 5:05 PM |
Regulatory |
5:05 PM - 5:30 PM |
General Q&A |
Legend (feel free to modify)
- general notes look like this
- questions asked to presenter(s) look like this
- v important advice given to presenter(s) looks like this
- answers given by presenter(s) look like this
- questions asked by presenter(s) look like this
- action items look like this
Notes
Science
Notetaker: @Riaab Zahid
- General notes
- requirements
- Have a signal to noise ratio of at least 30:1
- obtain images with sample distance ≤ 90m
- capable of conducting hyperspectral imaging
- objectives
- take and downlink and image
- downlink image of target
- process downlink image
- fit linear spectral modelling to image data
- make decisions to fit all objectives na d model the design of the satelllite to helo complete phase c
- working on building a model for crop residue
- to see if requirements make sense - some major concerns
- no satellites with SNR with 30:1
- in literature spectral feature used is well outside the range of our sensor
- may have problems mixing because soil and crop residue appea very similar
- have made noise function
- take spectral library entries and add noise function - take all library entries and re simulate data to see how FINCH will see it
- Risk management
- if SNR not viable can build algorithms into data processing pipeline and change the image capturing procedure
- ground truth failure
- selected components not optimal for scientific objectives
- Next steps
- rebuild science team
- increase complexity of linear mixing model
- choose abundance linear model
- ground truth operations
- Questions to presenters
- one of the risks may be that the SNR is too high - what is concern
- How would SNR algorithms look like
- the more data points we have of the same thing the more we do not need each pixel we can make data from multiple pixels
- possible LMM not optimal can we figure this out in advance
- no, not much literature review
- are we using full range of the blue box
- reduce amount of data which is not usable to help compression so we are not sure
- do we have a general idea of how we will be making use of the spectral imaging
- try to make a model - there is no literature
- what determines the range for the requirenent
- what decides the spectral hardware requirements
- higher level spacecraft departments decide - sensor range is blocking
- what is the action is we cant use the sensor
- rescope or find new sensor - has to occur in phase C
- Where does science have to be to be comfortable to move to phase D
- be bale to model design assembly and response to its objectives
- What will you do when in phase D
- across band spectral imaging is diverging which shows crop residue
- Do ew have efficiency graph of the sensor
- we have 60 - 70 % in our range
- Add objective levels to existing mission objectives requirements
Systems
Notetaker: @Riaab Zahid