scholarly journals Task Decomposition and Role Sharing for Real-time Human-AI Swarm Collaboration

Author(s):  
Sotaro Karakama ◽  
Natsuki Matsunami ◽  
Masayuki Ito
2014 ◽  
Vol 568-570 ◽  
pp. 781-784
Author(s):  
Xiang Yun Huang ◽  
Kai Lun Shi ◽  
Qing Yuan Ren

Cloud computing is tailored to the needs of the real-time and effectiveness of the grid witch can solve complicated problems. However, using the existing algorithms may always run into the problem of local optimal solution witch will effect the accuracy. This paper use the method of IHA to reduce probability of local optimal solution by change task decomposition to feasible operation, then prove the method by using Cloudsim.


2018 ◽  
Vol 176 ◽  
pp. 01025
Author(s):  
Han Zhuangzhi ◽  
Ma Tianlin

For embedded systems, there are two cases of using an operating system and not using an operating system. When the real-time task is accomplished by the embedded system of the operating system, the task needs to meet certain conditions and occupy part of the processor's resources. Therefore, based on the method of event interruption, timed interruption and task decomposition, the real-time performance of the completion of the task of the embedded system is achieved. Finally, an embedded radar track compression scheduling algorithm is designed. It is proved through experiment that the track data can be compressed and transmitted in real time.


1979 ◽  
Vol 44 ◽  
pp. 41-47
Author(s):  
Donald A. Landman

This paper describes some recent results of our quiescent prominence spectrometry program at the Mees Solar Observatory on Haleakala. The observations were made with the 25 cm coronagraph/coudé spectrograph system using a silicon vidicon detector. This detector consists of 500 contiguous channels covering approximately 6 or 80 Å, depending on the grating used. The instrument is interfaced to the Observatory’s PDP 11/45 computer system, and has the important advantages of wide spectral response, linearity and signal-averaging with real-time display. Its principal drawback is the relatively small target size. For the present work, the aperture was about 3″ × 5″. Absolute intensity calibrations were made by measuring quiet regions near sun center.


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