Labor Cat.
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Names
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WBS Level 3
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Tasks
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WBS 2.1
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WBS 2.2
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WBS 2.3
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WBS 2.4
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WBS 2.5
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WBS 2.6
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Grand Total
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Program Coordination
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Detector Maintenance & Operations
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Computing & Data Management
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Data Processing & Simulation
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Software
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Calibration
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KE | Xinhua Bai | 2.1.1 Administration
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SDSMT Inst. Lead
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0.05
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0.05
|
|||||
2.1.4 E&O | Education & Outreach in SD/China for neutrino astronomy and IceCube | 0.05
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0.05
|
|||||||
2.5.3 Reconstruction | High energy EAS and muon bundle reconstruction | 0.10
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0.10
|
|||||||
Bai, Xinhua Total | 0.10
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0.10
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0.20
|
|||||||
GR | Emily Dvorak | 2.2.4 Detector Monitoring | IceCube operation monitoring | 0.02
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0.02
|
|||||
2.4.2 Simulation production | Filter or re-produce MC events for the IceTop and in-ice combined reconstruction tools development | 0.10
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0.10
|
|||||||
2.5.3 Reconstruction | Improve HE cosmic ray direction reconstruction resolution at higher energies: diagnosing and fixing | 0.45
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0.45
|
|||||||
Dvorak, Emily Total | 0.02
|
0.10
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0.45
|
0.57
| ||||||
South Dakota School of Mines & Technology Total | 0.10
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0.02
|
0.00
|
0.10
|
0.55
|
0.77
|
Xinhua Bai – institution lead, education & outreach , improve high energy EAS and muon bundle reconstruction, mentoring Ph.D. student
Grad Students:
Emily Dvorak (Ph.D. student) –The three foci of her work are: (1) To study the cause of the angular resolution problem in IceTop air shower reconstruction and find out a solution so that the angular resolution, after reaching its minimal value at tens of PeVs, does not degrade at higher energies up to EeV; (2) To develop software tools, jointly with researchers in the IceCube Cosmic-Ray Working Group, for the reconstruction of air shower events that trigger both the IceTop and in-ice array but with the shower core landing outside the IceTop array; (3) To search and measure prompt muon yield in high energy cosmic ray induced showers with a new method based on the stochastic energy loss by muon bundles.
Emily has passed the Ph.D. qualifying exam in August 2015. She is working 100% on IceCube starting from August 25, 2015. Support for the rest of her effort on IceCube currently comes from SD physics Ph.D. program.
SDSMT_MoU_SOW_2016.0906.docx