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Phil Chamberlin
Survey Information
Institution: LASP/University of Colorado
Organizational Affiliation:
Observations
Providing Observations for WHI: No
ObservatoryNASA 36.240 Dr. Woods Sounding Rocket
Type of Observation: Solar VUV Irradiance
Coverage for WHI: Observation day/time: April 14, 2008, 17:00:05-17:05:45 UT
Temporal resolution: 10 seconds
Type: Solar VUV irradiance
Spectral Range: 0.1-105 nm, 121 nm
Spectral Resolution: 0.1 nm
Targeted Observation campaign: #4 - Quite Sun - Scott McIntosh
Observation Location for WHI:
Observation Plans for WHI:
Sample Data File
Sample Image
Modeling
Providing Modeling Support for WHI: Yes
Model Name: Flare Irradiance Spectral Model (FISM)
Model Web Site:
Type of Model: Solar UV Irradiance (0.1-190 nm)
Model Coverage: 0.1-190 nm range, 1 nm spectral resolution, 60 second temporal resolution
Sample Model Output
Sample Model Image
Data
Assisting with Data Coordination: No
Data Service:
Data Service Website:
Service Type:
Data Types or Sources:
Organizational Affiliation:
Other
Other Research Goals: We here at LASP will be launching a rocket from WSMR (P.I. Tom Woods) containing the new EVE instrument, and the primary launch date is April 10. Our main science goal is to get a definitive EUV spectrum (0.1-105 nm + Lyman Alpha) during solar minimum. We can contribute to the spectrally resolved emissions ( ~ 0.1 nm spectral resolution) and energy output of the full Sun spanning the chromosphere, transition region and corona during this times. This will only be for about 10 minutes during this day, but as you have stated this is a quite Sun measurement so it may be applicable to most of the data during the campaign. Also as a side note, we will be obtaining similar data at a 3% duty cycle over the length of this campaign from TIMED SEE, just at lower spectral resolution, and this data will also be available if needed.
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